Lectures on The Riemann Zeta–Function By K. Chandrasekharan Tata Institute of Fundamental Research, Bombay 1953 Lectures on the Riemann Zeta-Function By K. Chandrasekharan Tata Institute of Fundamental Research 1953 The aim of these lectures is to provide an intorduction to the theory of the Riemann Zeta-function for students who might later want to do research on the subject. The Prime Number Theorem, Hardy’s theorem on the Zeros of ζ(s), and Hamburger’s theorem are the principal results proved here. The exposition is self-contained, and required a preliminary knowledge of only the elements of function theory. Contents 1 The Maximum Principle 1 2 The Phragmen-Lindelof principle 9 3 Schwarz’s Lemma 17 4 Entire Functions 25 5 Entire Functions (Contd.) 35 6 The Gamma Function 1 Elementary Properties . . . . . . . . . . . . . . . . . . . 2 Analytic continuation of Γ(z) . . . . . . . . . . . . . . . 3 The Product Formula . . . . . . . . . . . . . . . . . . . 45 45 49 51 7 The Gamma Function: Contd 4 The Bohr-Mollerup-Artin Theorem . . . . . . . . . . . . 5 Gauss’s Multiplication Formula . . . . . . . . . . . . . 6 Stirling’s Formula . . . . . . . . . . . . . . . . . . . . . 55 55 58 59 8 The Zeta Function of Riemann 63 1 Elementary Properties of ζ(s) . . . . . . . . . . . . . . . 63 9 The Zeta Function of Riemann (Contd.) 69 2 Elementary theory of Dirichlet Series . . . . . . . . . . 69 v vi Contents 10 The Zeta Function of Riemann (Contd) 75 2 (Contd). Elementary theory of Dirichlet series . . . . . . 75 11 The Zeta Function of Riemann (Contd) 87 3 Analytic continuation of ζ(s). First method . . . . . . . 87 4 Functional Equation (First method) . . . . . . . . . . . . 90 5 Functional Equation (Second Method) . . . . . . . . . . 92 12 The Zeta Function of Riemann (Contd) 97 6 Some estimates for ζ(s) . . . . . . . . . . . . . . . . . . 97 7 Functional Equation (Third Method) . . . . . . . . . . . 99 13 The Zeta Function of Riemann (Contd) 105 8 The zeros of ζ(s) . . . . . . . . . . . . . . . . . . . . . 105 14 The Zeta Function of Riemann (Contd) 113 9 Riemann-Von Magoldt Formula . . . . . . . . . . . . . 113 15 The Zeta Function of Riemann (Contd) 121 10 Hardy’s Theorem . . . . . . . . . . . . . . . . . . . . . 121 16 The Zeta Function of Riemann (Contd) 127 17 The Zeta Function of Riemann (Contd) 12 The Prime Number Theorem . . . . . . . . . . . . . . . 13 Prime Number Theorem and the zeros of ζ(s) . . . . . . 14 Prime Number Theorem and the magnitude of pn . . . . 135 135 145 146 Lecture 1 The Maximum Principle Theorem 1. If D is a domain bounded by a contour C for which Cauchy’s 1 theorem is valid, and f is continuous on C regular in D, then “| f | ≤ M on C” implies “| f | ≤ M in D”, and if | f | = M in D, then f is a constant. Proof. (a) Let zo ∈ D, n a positive integer. Then 1 Z { f (z)}n dz n | f (zo )| = 2πi z − zo C lc · M n , ≤ 2πδ where lc = length of C, δ = distance of zo from C. As n → ∞ | f (z)| ≤ M. (b) If | f (zo )| = M, then f is a constant. For, applying Cauchy’s inte d gral formula to { f (z)}n , we get dz 1 Z f n dz |n{ f (zo )}n−1 · f ′ (zo )| = 2πi (z − zo )2 ≤ 1 C n M lC 2πδ2 , 1. The Maximum Principle 2 so that | f ′ (zo )| ≤ lc M 1 · → 0, as n → ∞ 2πδ2 n Hence | f ′ (zo )| = 0. 2 (c) If | f (zo )| = M, and | f ′ (zo )| = 0, then f ′′ (zo ) = 0, for d2 { f (z)}n = n(n − 1){ f (z)}n−2 { f ′ (z)}2 + n{ f (z)}n−1 f ′′ (z). 2 dz At zo we have so that d2 { f (z)}n z=zo = n f n−1 (Z0 ) f ′′ (z0 ), 2 dz 2! Z { f (z)}n dz |nM n−1 f ′′ (z0 )| = 2πi (z − zo )3 C ≤ 2!lc n M , 2πδ3 and letting n → ∞, we see that f ′′ (zo ) = 0. By a similar reasoning we prove that all derivatives of f vanish at z0 (an arbitrary point of D). Thus f is a constant. Remark. The above proof is due to Landau [12, p.105]. We shall now show that the restrictions on the nature of the boundary C postulated in the above theorem cab be dispensed with. Theorem 2. If f is regular in a domain D and is not a constant, and M = max | f |, then z∈D | f (zo )| < M, zo ∈ D. For the proof of this theorem we need a 1. The Maximum Principle 3 Lemma. If f is regular in |z − z0 | ≤ r, r > 0, then | f (z0 )| ≤ Mr , 3 where Mr = max | f (z)|, and | f (zo )| = Mr only if f (z) is constant for |z − zo | = r. |z−zo |=r Proof. On using Cauchy’s integral formula, we get Z f (z) 1 dz f (zo ) = 2πi z − z0 |z−zo |=n 1 = 2π Z2π f (zo + reiθ )dθ. (1) 0 Hence | f (zo )| ≤ Mr . Further, if there is a point ζ (such that) |ζ − zo | = r, and | f (ζ)| < Mr , then by continuity, there exists a neighbourhood of ζ, on the circle |z − zo | = r, in which | f (z)| ≤ Mr − ε, ε > 0 and we should have | f (zo )| < Mr ; so that “| f (zo )| = Mr ” implies “| f (z)| = Mr everywhere on |z − zo | = r”. That is | f (zo + reiθ )| = | f (zo )| for 0 ≤ θ ≤ 2π, or f (zo + reiθ ) = f (zo )eiϕ , 0 ≤ ϕ ≤ 2π On substituting this in (1), we get 1 1= 2π Z2π cos ϕdθ 0 Since ϕ is a continuous function of θ and cos ϕ ≤ 1, we get cos ϕ · 1 for all θ, i.e. ϕ = 0, hence f (s) is a constant. Remarks . The Lemma proves the maximum principle in the case of a 4 circular domain. An alternative proof of the lemma is given below [7, Bd 1, p.117]. 1. The Maximum Principle 4 Aliter. If f (z0 + reiθ ) = φ(θ) (complex valued) then 1 f (z0 ) = 2π Z2π φ(θ)dθ 0 Now, if a and b are two complex numbers, |a| ≤ M, |b| ≤ M and a , b, then |a + b| < 2M. Hence if φ(θ) is not constant for 0 ≤ θ < 2π, then there exist two points θ1 , θ2 such that |φ(θ1 ) + φ(θ2 )| = 2Mr − 2ε, say, where ε > 0 On the other hand, by regularity, |φ(θ1 + t) − φ(θ1 )| < ε/2, for 0 < t < δ |φ(θ2 + t) − φ(θ2 )| < ε/2, for 0 < t < δ Hence |φ(θ1 + t) + φ(θ2 + t)| < 2Mr − ε, for 0 < t < δ. Therefore Z2π φ(θ)dθ = 0 Zθ1 0 | Z2π θ1 θ1 +δ θ2 θ2 +δ θ Zδ Z 1 Zθ2 Z2π + = + φ(θ)dθ + [φ(θ1 + t) + φ(θ2 + t)] dt 0 Hence θ1 +δ Zθ2 θ2 +δ Z2π Z Z + + + + θ1 +δ θ2 +δ 0 φ(θ) dθ| ≤ Mr (2π − 2δ) + (2Mr − ε)δ = 2πMr − εδ 0 1 | 2π Z2π 0 φ(θ)dθ| < Mr 1. The Maximum Principle 5 5 Proof of Theorem 2. Let zo ∈ D. Consider the set G1 of points z such that f (z) , f (zo ). This set is not empty, since f is non-constant. It is a proper subset of D, since zo ∈ D, zo < G1 . It is open, because f is continuous in D. Now D contains at least one boundary point of G1 . For if it did not, G′1 ∩ D would be open too, and D = (G1 ∪ G′1 )D would be disconnected. Let z1 be the boundary point of G1 such that z1 ∈ D. Then z1 < G1 , since G1 is open. Therefore f (z1 ) = f (zo ). Since z1 ∈ BdG1 and z1 ∈ D, we can choose a point z2 ∈ G1 such that the neighbourhood of z1 defined by |z − z1 | ≤ |z2 − z1 | lies entirely in D. However, f (z2 ) , f (z1 ), since f (z2 ) , f (zo ), and f (zo ) = f (z1 ). Therefore f (z) is not constant on |z − z1 | = r, (see (1) on page 3) for, if it were, then f (z2 ) = f (z1 ). Hence if M ′ = max | f (z)|, then |z−z1 |=|z2 −z1 | | f (z1 )| < M ′ ≤ M = max | f (z)| z∈D i.e. | f (zo )| < M Remarks. The above proof of Theorem 2 [7, Bd I, p.134] does not make use of the principle of analytic continuation which will of course provide an immediate alternative proof once the Lemma is established. Theorem 3. If f is regular in a bounded domain D, and continuous in D̄, then f attains its maximum at some point in Bd D, unless f is a constant. Since D is bounded, D̄ is also bounded. And a continuous function on a compact set attains its maximum, and by Theorem 2 this maximum 6 cannot be attained at an interior point of D. Note that the continuity of | f | is used. Theorem 4. If f is regular in a bounded domain D, is non-constant, and if for every sequence {zn }, zn ∈ D, which converges to a point ξ ∈ Bd D, we have lim sup | f (zn )| ≤ M, n→∞ then | f (z)| < M for all z ∈ D. [17, p.111] 1. The Maximum Principle 6 Proof. D is an Fσ , for define sets Cn by the property: Cn consists of all z such that |z| ≤ n and such that there exists an open circular neighbourhood of radius 1/n with centre z, which is properly contained in D. Then Cn ⊂ Cn+1 , n = 1, 2, . . .; and Cn is compact. Define max | f (z)| ≡ mn . Z∈Cn By Theorem 2, there exists a zn ∈ Bd Cn such that | f (zn )| = mn . The sequence {mn } is monotone increasing, by the previous results; and the sequence {zn } is bounded, so that a subsequence {zn p } converges to a limit ξ ∈ Bd D. Hence lim| f (zn p )| ≤ M i.e. or i.e. 7 lim mn p ≤ M mn < M for all n | f (z)| < M. z ∈ D. N.B. That ξ ∈ Bd D can be seen as follows. If ξ ∈ D, then there exists an No such that ξ ∈ C No ⊂ D, and | f (ξ)| < mNo ≤ lim mn , whereas we have f (zn p ) → f (ξ), so that | f (zn p )| → | f (ξ)|, or lim mn = | f (ξ)|. Corollaries. (1) If f is regular in a bounded domain D and continuous in D, then by considering e f (z) and e−i f (z) instead of f (z), it can be seen that the real and imaginary parts of f attain their maxima on Bd D. (2) If f is an entire function different from a constant, then M(r) ≡ l.u.b | f (z)|, and |z|=r A(r) ≡ l.u.b Re{ f (z)} |z|=r are strictly increasing functions of r. Since f (z) is bounded if M(r) is, for a non-constant function f , M(r) → ∞ with r. 1. The Maximum Principle 7 (3) If f is regular in D, and f , 0 in D, then f cannot attain a minimum in D. Further if f is regular in D and continuous in D̄, and f , 0 in D̄, and m = min | f (z)|, then | f (z)| > m for all z ∈ D unless f is a z∈Bd D constant. [We see that m > 0 since f , 0, and apply the maximum principle to 1/ f ]. (4) If f is regular and , 0 in D and continuous in D̄, and | f | is a constant γ on Bd D, then f = γ in D. For, obviously γ , 0, and, by Corollary 3, | f (z)| ≥ γ for z ∈ D, se that f attains its maximum in D, and hence f = γ. (5) If f is regular in D and continuous in D̄, and | f | is a constant on 8 Bd D, then f is either a constant or has a zero in D. (6) Definition: If f is regular in D, then α is said to be a boundary value of f at ξ ∈ Bd D, if for every sequence zn → ξ ∈ Bd D, zn ∈ D, we have lim f (zn ) = α n→∞ (a) It follows from Theorem 4 that if f is regular and non - constant in D, and has boundary-values {α}, and |α| ≤ H for each α, then | f (z)| < H, z ∈ D. Further, if M ′ = max |α| then α∈b.v M ′ = M ≡ max | f (z)| z∈D For, |α| is a boundary value of | f |, so that |α| ≤ M, hence M ′ ≤ M. On the other hand, there exists a sequence {zn }, zn ∈ D, such that | f (zn )| → M. We may suppose that zn → zo (for, in any case, there exists a subsequence {zn p } with the limit zo , say, and one can then operate with the subsequence). Now zo < D, for otherwise by continuity f (zo ) = lim f (zn ) = M, which contradicts the maximum n→∞ principle. Hence zo ∈ Bd D, and M is the boundary-value of | f | at zo . Therefore M ≤ M ′ , hence M = M ′ . (b) Let f be regular and non-constant in D, and have boundaryvalues {α} on Bd D. Let m = min | f |; m′ = min |α| > 0. z∈D α∈b.v. 1. The Maximum Principle 8 Then, if f , 0 in D, by Corollary (6)a, we get max z∈D 9 1 1 1 = ′ = ; | f (z)| m m so that | f | > m = m′ in D. Thus if there exists a point zo ∈ D such that | f (zo )| ≤ m′ , then f must have a zero in D, so that m′ > 0 = m. We therefore conclude that, if m′ > 0, then m′ = m if and only if f , 0 in D [6, Bd. I, p.135]. Lecture 2 The Phragmen-Lindelof principle We shall first prove a crude version of the Phragmen-Lindelof theorem 10 and then obtain a refined variant of it. The results may be viewed as extensions of the maximum-modulus principle to infinite strips. Theorem 1. [6, p.168] We suppose that (i) f is regular in the strip α < x < β; f is continuous in α ≤ x ≤ β (ii) | f | ≤ M on x = α and x = β (iii) f is bounded in α ≤ x ≤ β Then, | f | ≤ M in α < x < β; and | f | = M in α < x < β only if f is a constant. Proof. (i) If f (x + iy) → O as y → ±∞ uniformly in x, α ≤ x ≤ β, then the proof is simple. Choose a rectangle α ≤ x ≤ β, |y| ≤ η with η sufficiently large to imply | f |(x ± iη) ≤ M for α ≤ x ≤ β. Then, by the maximum-modulus principle, for any zo in the interior of the rectangle, | f (zo )| ≤ M. 9 2. The Phragmen-Lindelof principle 10 (ii) If | f (x + iy)| 6→ 0, as y → ±∞, consider the modified function 2 fn (z) = f (z)ez /n . Now | fn (z)| → 0 as y → ±∞ uniformly in x, and 2 /n | fn (z)| ≤ Mec 11 on the boundary of the strip, for a suitable constant c. Hence 2 | fn (zo )| ≤ Mec /n for an interior point zo of the rectangle, and letting n → ∞, we get | f (zo )| ≤ M. If | f (zo )| = M, then f is a constant. For, if f were not a constant, in the neighbourhood of zo we would have points z, by the maximum-modulus principle, such that | f (z)| > M, which is impossible. Theorem 1 can be restated as: Theorem 1′ : Suppose that (i) f is continuous and bounded in α ≤ x ≤ β (ii) | f (α + iy)| ≤ M1 , | f (β + iy)| ≤ M2 for all y Then | f (xo + iyo )| ≤ M1L(xo ) M21−L(xo ) for α < xo < β, |yo | < ∞, where L(t) is a linear function of t which takes the value 1 at α and 0 at β. If equality occurs, then f (z) = cM1L(z) M21−L(z) ; |c| = 1. Proof. Consider f1 (z) = 12 f (z) M1L(z) M21−L(z) and apply Theorem 1 to f1 (z). More generally we have [12, p.107] 2. The Phragmen-Lindelof principle 11 Theorem 2. Suppose that (i) f is regular in an open half-strip D defined by: z = x + iy, α < x < β, y>η (ii) lim| f | ≤ M, for ξ ∈ Bd D z→ξ in D θπ|z| (iii) f = O exp e β−α , θ < D uniformly in D. Then, | f | ≤ M in D; and | f | < M in D unless f is a constant. Proof. Without loss of generality we can choose π α=− , 2 β = +π/2, η=0 Set g(z) = f (z). exp(−σe−ikz ) ≡ f (z).{ω(z)}σ , say, where σ > 0, θ < k < 1. Then, as y → +∞, " ( # kπ θ|z| ky g = O exp e − σe cos 2 uniformly in x, and 13 eθ|z| − σeky cos kπ kπ ≤ eθ(y+π/2) − σeky cos 2 2 → −∞, as y → ∞, uniformly in x, since θ < k. Hence |g| → 0 uniformly as y → ∞, so that |g| ≤ M, for y > y′ , α < x < β. 2. The Phragmen-Lindelof principle 12 Let zo ∈ D. We can then choose H so that |g(z)| ≤ M for y = H, α < x < β, and we may also suppose that H > y0 = im(zo ). Consider now the rectangle defined by α < x < β, y = 0, y = H. Since |ωσ | ≤ 1 we have lim |g| ≤ M z→ξ in D for every point ξ on the boundary of this rectangle. Hence, by the maximum-modulus principle, |g(zo )| < M, unless g is a constant; −ikzo | f (zo )| < M|eσe or | Letting σ → 0, we get 14 | f (zo )| < M. Remarks. The choice of ω in the above proof is suggested by the critical case θ = 1 of the theorem when the result is no longer true. For take α = −π/2, θ = 1, Then −iz β = π/2, −iz ) |ee | = eRe(e y−ix } = eRe{e η = 0, y = ee −iz f = ee cos x So | f | = 1 on x = ±π/2, y and f = ee on x = 0. Corollary 1. If f is regular in D, continuous on Bd D, | f | ≤ M on Bd D, and |z|πθ f = O ee β−α , θ < 1, then | f | ≤ M in D. 2. The Phragmen-Lindelof principle 13 Corollary 2. Suppose that hypotheses (i) and (iii) of Theorem 2 hold; suppose further that f is continuous on Bd D, f = O(ya ) on x = α, f = O(yb ) on x = β. Then f = O(yc ) on x = γ, uniformly in γ, where c = pγ + q, and px + q is the linear function which equals a at x = α and b at x = β. Proof. Let η > 0. Define ϕ(z) = f (z)ψ(z), where ψ is the single-valued 15 branch of (−zi)−(pz+q) defined in D, and apply Theorem 2 to ϕ. We first observe that ϕ is regular in D and continuous in D̄. Next |ψ(z)| = |(y − ix)−(px+q)−ipy | log y − ix ) = |y − ix|−(px+q) exp(py im y ! " ( !)# x 1 O(1) 1 −(px+q) =y |1 + O | exp py − + O 2 y y y ! 1 }, = y−(px+q) e−px {1 + O y the O’s being uniform in the x′ s. Thus ϕ = O(1) on x = α and x = β. Since ψ = O(yk ) = O(|z|k ), we see that condition (iii) of Theorem 2 holds for ϕ if θ is suitably chosen. Hence ϕ = O(1) uniformly in the strip, which proves the corollary. Theorem 3. [12, p.108] Suppose that conditions (i) and (iii) of Theorem 2 hold. Suppose further that f is continuous in Bd D, and lim | f | ≤ M on x = α, y→∞ x=β Then lim | f | ≤ M uniformly in α ≤ x ≤ β. y→∞ P Proof. f is bounded in D̄, by the previous theorem. Let η ≥ 0, > 0. 16 Let H = H(ε) be the ordinate beyond which | f | < M +ε on x = α, x = β. 2. The Phragmen-Lindelof principle 14 Let h > 0 be a constant. Then z <1 z + hi in the strip. Choose h = h(H) so large that z f (z) · < M + ε on y = H z + hi z ≤ | f | < M). Then the function (possible because f · z + hi z g(z) = f · z + hi satisfies the conditions of Theorem 2 (with M + ε in place of M) in the strip above y = H. Thus |g| ≤ M + ε in this strip and so lim |g| ≤ M + ε uniformly. y→∞ That is, lim| f | ≤ M + ε, since z → 1 uniformly in x. Hence z + hi lim| f | ≤ M. 17 Corollary 1. If conditions (i) and (iii) of Theorem 2 hold, if f is continuous on Bd D, and if a on x = α, lim| f | ≤ b on x = β, where a , 0, b , 0, then lim | f | ≤ e px+q , y→∞ uniformly, p and q being so chosen that e px+q = a for x = α and = b for x = β. 2. The Phragmen-Lindelof principle Proof. Apply Theorem 3 to g = f e−(pz+q) 15 Corollary 2. If f = O(1) on x = α, f = o(1) on x = β, then f = o(1) on x = γ, α < γ ≤ β. [if conditions (i) and (iii) of Theorem 2 are satisfied]. Proof. Take b = ε in Corollary 1, and note that e pγ+q → 0 as ε → 0 for fixed γ, provided p and q are chosen as specified in Corollary 1. Lecture 3 Schwarz’s Lemma Theorem 1. Let f be regular in |z| < 1, f (o) = 0. If, for |z| < 1, we have | f (z)| ≤ 1, then | f (z)| ≤ |z|, for |z| < 1. Here, equality holds only if f (z) ≡ c z and |c| = 1. We further have | f ′ (o)| ≤ 1. f (z) is regular for |z| < 1. Given o < r < 1 choose ρ such that z r < ρ < 1; then since | f (z)| ≤ 1 for |z| = ρ, it follows by the maximum modulus principle that f (z) 1 ≤ , z ρ Proof. also for |z| = r. Since the L.H.S is independent of ρ → 1, we let ρ and obtain | f (z)| ≤ |z|, for |z| < 1. f (z0 ) = 1, (by the If for z0 , (|z0 | < 1), we have | f (z0 )| = |z0 |, then z0 f (z) ) hence f = cz, |c| = 1. maximum principle applied to z Since f (z) = f ′ (o)z + f ′′ (o)z2 + · · · in a neighbourhood of the origin, f (z) ≤ 1 in z 1, we get | f ′ (o)| ≤ 1. More generally, we and since z have 17 18 3. Schwarz’s Lemma 18 19 Theorem 1′ : Let f be regular and | f | ≤ M in |z| < R, and f (o) = 0. Then M|z| , |z| < R. | f (z)| ≤ R In particular, this holds if f is regular in |z| < R, and continuous in |z| ≤ R, and | f | ≤ M on |z| = R. Theorem 2 (Caratheodory’s Inequality). [12, p.112] Suppose that (i) f is regular in |z| < R f is non-constant (ii) f (o) = 0 (iii) Re f ≤ ∪ in |z| < R. (Thus ∪ > 0, since f is not a constant). Then, |f| ≤ 2∪ρ , for |z| = ρ < R. R−ρ Proof. Consider the function ω(z) = f (z) . f (z) − 2∪ We have Re{ f − 2∪} ≤ −∪ < 0, so that ω is regular in |z| < R. If f = u + iv, we get s u2 + v2 |ω| = (2 ∪ −u)2 + v2 so that |ω| ≤ 1, since 2 ∪ −u ≥ |u|. But ω(o) = o, since f (o) = o. Hence by Theorem 1, |ω(z)| ≤ 20 |z| , R |z| < R. 2∪ω But f = − . Now take |z| = ρ < R. 1−ω Then, we have, 3. Schwarz’s Lemma 19 |f| ≤ N.B. If 2 ∪ |ω| 2 ∪ ρ ≤ 1 − |ω| R − ρ 2∪ρ , for |zo | < R, then R−ρ 2U · cz f (z) = , |c| = 1. 1 − cz | f (zo )| = More generally, we have Theorem 2′ : Let f be regular in |z| < R; f non-constant f (o) = ao = β + iγ Re f ≤ ∪(|z| < R), so that ∪ ≥ β Then 2(∪ − β)ρ | f (z) − ao | ≤ R−ρ for |z| = ρ < R Remark . If f is a constant, then Theorem 2 is trivial. We shall now prove Borel’s inequality which is sharper than Theorem 2. Theorem 3 (Borel’s Inequality). [12, p.114] Let f (z) = regular in |z| < 1. Let Re f ≤ ∪. f (o) = ao = β + iγ. Then |an | ≤ 2(∪ − β) ≡ 2 ∪1 , say, n > 0. ∞ P an zn , be n=0 Proof. We shall first prove that |a1 | < ∪1 , and then for general an . (i) Let f1 ≡ ∞ P n=1 an zn . Then Re f1 ≤ ∪1 . For |z| = ρ < 1, we have, by Theorem 2, 2 ∪1 ρ | f1 | ≤ 1−ρ 2∪1 f1 (z) ≤ i.e. z 1−ρ 21 3. Schwarz’s Lemma 20 Now letting z → 0, we get |a1 | ≤ 2∪1 (ii) Define ω = e2πi/k , k a +ve integer. Then k X v=1 We have ω νm if m , 0 =o & if m , a multiple of k if m = 0 =k or if m = a multiple of k. ∞ k−1 X 1X f1 (ωr z) = ank znk = g1 (zk ) ≡ g1 (ζ), say. k r=0 n=1 22 The series for g1 is convergent for |z| < 1, and so for |ζ| < 1. Hence g1 is regular for |ζ| < 1. Since Re g1 ≤ ∪1 , we have | coefficient of ζ| ≤ 2∪1 by the first part of the proof i.e. |ak | ≤ 2∪1 . Corollary 1. Let f be regular in |z| < R, and Re{ f (z)− f (o)} ≤ ∪1 . Then | f ′ (z)| ≤ 2 ∪1 R , (R − ρ)2 |z| = ρ < R Proof. Suppose R = 1. Then X X | f ′ (z)| ≤ n|an |ρn−1 ≤ 2 ∪1 nρn−1 This argument can be extended to the nth derivative. Corollary 2. If f is regular for every finite z, and k e f (z) = O(e|z| ), as |z| → ∞, then f (z) is a polynomial of degree ≤ k. 3. Schwarz’s Lemma Proof. Let f (z) = P 21 an zn . For large R, and a fixed ζ, |ζ| < 1, we have Re{ f (Rζ)} < cRk . By Theorem 3, we have |an Rn | ≤ 2(2Rk − Re ao ), n > 0. Letting R → ∞, we get an = 0 if n > k. Apropos Schwarz’s Lemma we give here a formula and an inequality which are useful. Theorem 4. Let f be regular in |z − zo | ≤ r 23 f = P(r, θ) + Q(r, θ). Then 1 f ′ (zo ) = πr Z2π P(r, θ)e−iθ dθ. o Proof. By Cauchy’s formula, (i) 1 f (zo ) = 2πi Z |z−zo |=r f (z)dz 1 = 2 2πr (z − zo ) Z2π (P + iQ)e−iθ dθ 0 By Cauchy’s theorem, (ii) 1 1 0= 2 · r 2πi Z 1 f (z)dz = 2πr |z−zo |=r Z2π (P + iQ)eiθ dθ 0 We may change i to −i in this relation, and add (i) and (ii). Then Z2π 1 ′ f (zo ) = P(r, θ)e−iθ dθ πr 0 3. Schwarz’s Lemma 22 Corollary. If f is regular, and | Re f ≤ M in |z − z0 | ≤ r, then | f ′ (zo )| ≤ 24 2M . r Aliter: We have obtained a series of results each of which depended on the preceding. We can reverse this procedure, and state one general result from which the rest follow as consequences. ∞ P Theorem 5. [11, p.50] Let f (z) ≡ cn (z−z0 )n be regular in |z−z0 | < R, n=0 and Re f < ∪. Then 2(∪ − Re co ) , Rn and in |z − zo | ≤ ρ < R, we have |en | ≤ n = 1, 2, 3, . . . 2ρ | f (z) − f (z0 )| ≤ {∪ − Re f (zo )} R−ρ (n) f (z) 2R {∪ − Re f (zo )} n = 1, 2, 3, . . . ≤ n! (R − ρ)n+1 (5.1) (5.2) (5.3) Proof. We may suppose zo = 0. Set φ(z) = ∪ − f (z) = ∪ − c0 − ≡ ∞ X 0 bn zn , ∞ X cn zn 1 |z| < R. Let γ denote the circle |z| = ρ < R. Then 1 bn = 2πi Z 1 φ(z)dz = n+1 2πρn z γ Zπ −π (P + iQ)e−inθ dθ, n ≥ 0, (5.4) where φ(r, θ) = P(r, θ) + iQ(r, θ). Now, if n ≥ 1, then φ(z)zn−1 is regular is γ, so that ρn 0= 2r Zπ −π (P + iQ)einθ dθ, n ≥ 1 (5.5) 3. Schwarz’s Lemma 23 Changing i to −i in (5.5) and adding this to (5.4) we get 1 bn ρn = π Zπ Pe−nθi dθ, −π n ≥ 1. But P = ∪ − Re f ≥ 0 in |z| < R and so in γ. Hence, if n ≥ 1, 1 |bn |ρn ≤ π Zπ −π 1 |Pe−nθi |dθ = π Zπ Pdθ = 2 Re bo , 25 (5.6) −π on using (5.4) with n = 0. Now letting ρ → R, we get |bn |Rn ≤ 2βo ≡ 2 Re bo . Since bo = ∪ − co , and bn = −cn , n ≥ 1, we at once obtain (5.1). We then deduce, for |z| ≤ ρ < R |φ(z) − φ(o)| = | ∞ X 1 n bn z | ≤ ∞ X 2β0 1 ρ n R = 2βo ρ R−ρ (5.7) and if n ≥ 1, (n) |φ (z)| ≤ ∞ X r=n r(r − 1) . . . (r − n + 1) d = dρ !n X ∞ 2β0 n=0 !n 2βe R d dρ R − ρ βo R · n! =2 (R − ρ)n+1 = 2β0 ρr−n Rr ρ r R (5.8) (5.7) and (5.8) yield the required results on substituting φ = ∪ − f and β0 = ∪ − Re f (0). Lecture 4 Entire Functions An entire function is an analytic function (in the complex plane) which 26 has no singularities except at ∞. A polynomial is a simple example. A polynomial f (z) which has zeros at z1 , . . . , zn can be factorized as ! ! z z f (z) = f (0) 1 − ... 1 − z1 zn The analogy holds for entire functions in general. Before we prove this, we wish to observe that if G(z) is an entire function with no zeros it can G′ (z) ; every be written in the form eg(z) where g is entire. For consider G(z) (finite) point is an ‘ordinary point’ for this function, and so it is entire and equals g1 (z), say. Then we get ) Zz1 G(z) log = g1 (ζ)dζ = g(z) − g(z0 ), say, G(z0 ) ( z0 so that G(z) = G(z0 )eg(z)−g(z0 ) = eg(z)−g(z0 )+log G(zo ) As a corollary we see that if G(z) is an entire function with n zeros, distinct or not, then G(z) = (z − z1 ) . . . (z − zn )eg(z) 25 4. Entire Functions 26 where g is entire. We wish to uphold this in the case when G has an infinity of zeros. 27 Theorem 1 (Weierstrass). [15, p.246] Given a sequence of complex numbers an such that 0 < |a1 | ≤ |a2 | ≤ . . . ≤ |an | ≤ . . . whose sole limit point is ∞, there exists an entire function with zeros at these points and these points only. Proof. Consider the function 1− ! z Qν (z) e , an where Qν (z) is a polynomial of degree q. This is an entire function which does not vanish except for z = an . Rewrite it as ! z z Qν (z) 1− e = eQν (z)+log 1− an an − azn − =e and choose Qν (z) = z2 ...+Qν (z) 2a2 , z zν + ... + ν an νa n so that ν+1 ! − azn 1 ... z Qν (z) ν+1 1− e =e an ≡ 1 + ∪n (z), say. We wish to determine ν in such a way that ∞ Y 1 28 ! z Qν (z) e 1− an is absolutely and uniformly convergent for |z| < R, however large R may 4. Entire Functions 27 be. Choose an R > 1, and an α such that 0 < α < 1; then there exists a q (+ ve integer) such that |aq | ≤ R , α R . α |aq+1 | > Then the partial product q Y 1 ! z Qν (Z) e 1− an is trivially an entire function of z. Consider the remainder ∞ Y q+1 ! z Qν (z) e 1− an for |z| ≤ R. R z We have, for n > q, |an | > or < α < 1. Using this fact we α an shall estimate each of the factors {1 + ∪n (z)} in the product, for n > q. ν+1 z 1 | ∪n (z)| = e− ν+1 an −... − 1 1 z ν+1 ... ν+1 a ≤e n −1 Since |em − 1| ≤ e|m| − 1, for em − 1 = m + |m| + |m2 | . . . = e|m| − 1. 2 ν+1 z 1+ azn +... an |Un (z)| ≤ e − 1, ν+1 z (1+α+α2 +··· ) an ≤e =e ν+1 1 z 1−α an −1 −1 m2 + . . . or |em − 1| ≤ 29 2! 4. Entire Functions 28 real, ex −1 ≤ · · · ) = xe x Hence xe x , 1 1 z ν+1 1−α · e ≤ 1 − α an for ex , since if x is ! x2 x2 x + · · · ≤ x(1 + x + + −1 = x 1+ + 2! 3! 2! |Un (z)| ≤ 30 ν+1 z an 1 e 1−α z ν+1 1 − α an Now arise two cases: (i) either there exists an integer p > 0 such ∞ P 1 < ∞ or (ii) there does not. In case (i) take ν = p − 1, so that p n=1 |an | that 1 e 1−a Rp · , since |z| ≤ R; |Un (z)| ≤ |an | p 1 − α and hence P |Un (z)| < ∞ for |z| ≤ R, i.e. uniformly convergent for |z| ≤ R. In case (ii) take ν = n − 1, so that |Un (z)| < ∞ Q (1 + Un (z)) is absolutely and q+1 1 e 1−α z n ,n>q 1 − α an z < 1 an |z| ≤ R |an | → ∞ P Then by the ‘root-test’ |Un (z)| < ∞, and the same result follows as before. Hence the product ∞ Y 1 31 1− ! z Qν (z) e an is analytic in |z| ≤ R; since R is arbitrary and ν does not depend on R we see that the above product represents an entire function. 4. Entire Functions 29 Remark. If in addition z = 0 is also a zero of G(z) then G(z) has no zmG(z) zeros and equals eg(z) , say, so that g(z) G(z) = e ·z m ∞ Y n=1 ! z Qν (z) 1− e an In the above expression for G(z), the function g(z) is an arbitrary entire function. If G is subject to further restrictions it should be possible to say more about g(z); this we shall now proceed to do. The class of entire functions which we shall consider will be called “entire functions of finite order”. Definition. An entire function f (z) is of finite order if there exists a conλ stant λ such that | f (z)| < er for |z| = r > r0 . For a non-constant f , of finite order, we have λ > 0. If the above inequality is true for a certain λ, it is also true for λ′ > λ. Thus there are an infinity of λ′ s o satisfying this. The lower bound of such λ′ s is called the “order of f ”. Let us denote it by ρ. Then, given ε > 0, there exists an ro such that | f (z)| < er ρ+ε for |z| = r > r0 . This would imply that ρ+ε M(r) = max | f (z)| < er , r > r0 , |z|=r while 32 rρ−ε M(r) > e for an infinity of values of r tending to +∞ Taking logs. twice, we get log log M(r) <ρ+ε log r and log log M(r) > ρ − ε for an infinity of values of r → ∞ log r 4. Entire Functions 30 Hence log log M(r) r→∞ log R ρ = lim Theorem 2. If f (z) is an entire function of order ρ < ∞, and has an infinity of zeros, f (0) , 0, then given ε > 0, there exists an R◦ such that for R ≥ Ro , we have ρ+ε eR 1 n · log ≤ 3 log 2 | f (o)| R Here n(R) denotes the number of zeros of f (z) in |z| ≤ R. Proof. We first observe that if f (z) is analytic in |z| ≤ R, and a1 . . . an are the zeros of f inside |z| < R/3, then for 33 we get the inequality g(z) = 1− z a1 f (z) ... 1 − |g(z)| ≤ z an M 2n where M is defined by: | f (z)| ≤ M for |z| = R. For, if |z| = R, then since z R z |a p | ≤ , p = 1 . . . n, we get ≥ 3 or 1 − ≥ 2 ap 3 ap By the maximum modules theorem, |g(o)| ≤ M M , i.e. | f (o)| ≤ 2n 2n or 1 M ≤ · log n≡n 3 log 2 f (o) R ! If, further, f is of order ρ, then for r > r◦ , we have M < er gives the required results. N.B. The result is trivial if the number of zeros is finite. ρ+ε which 4. Entire Functions 31 Corollary. n(R) = O(Rρ+ε ). For 1 ≤ · Rρ+ε − log | f (o)| , 3 log 2 − log | f (0)| < Rρ+ε , say. n and R Then for R ≥ R′ n and hence the result. R 3 2 ρ+ε R log 2 < Theorem 3. If f (z) is of order ρ < ∞, has an infinity of zeros X 1 <∞ a1 , a2 , . . . , f (o) , 0, σ > ρ, then |an |σ 34 Proof. Arrange the zeros in a sequence: |a1 | ≤ |a2 | ≤ . . . Let α p = |a p | Then in the circle |z| ≤ r = αn , there are exactly n zeros. Hence ρ+ε n < c αn , for n ≥ N or 1 1 1 > · n c αρ+ε n Let σ > ρ + ε (i.e. choose 0 < ε < σ − ρ). Then 1 nσ/ρ+ε or Hence > 1 cσ/ρ+ε · 1 , ασn 1 1 < cσ/ρ+ε · σ/ρ+ε for n ≥ N σ αn n P 1 < ∞. ασn 32 35 4. Entire Functions Remark. (i) There cannot be too dense a distribution of zeros, since ρ+ε n < c < αn . Nor can their moduli increase too slowly, since, for P 1 does not converge. instance, (log n) p (ii) The result is of course trivial if there are only a finite number of zeros. 1 < ∞, |an |σ is called the exponent of convergence of {an }. We shall denote it by ρ1 . Then X 1 X 1 < ∞, = ∞, ε > 0 |an |ρ1 +ε |an |ρ1 −ε Definition. The lower bound of the numbers ‘σ’ for which P By Theorem 1, we have ρ1 ≤ ρ N.B. If the a′n s are finite in number or nil, then ρ1 = 0. Thus ρ1 > 0 implies that f has an infinity of zeros. Let f (z) be entire, of order ρ < ∞; f (o) , 0, and f (zn ) = 0, n = 1, 2, 3, . . .. Then there exists an integer P 1 (p + 1) such that <∞ |zn |ρ+1 (By Theorem 1, any integer > ρ will serve for ρ + 1). Thus, by Weierstrass’s theorem, we have ! ∞ Y z zzn + 2zz2n 2 +···+ νzzνν Q(z) n, e f (z) = e 1− z n 1 36 where ν = p (cf. proof of Weierstrass’s theorem). P Definition. The smallest integer p for which |z |1p+1 < ∞ is the ‘genus’ n ! p z zzn +···+ pzz p n , with zeros zn . If z′ s e of the ‘canonical product’ Π 1 − n zn are finite in number, !we (including nil) define p = 0, and we define the z product as Π 1 − zn Examples. (i) zn = n, p = 1 (ii) zn = en , p = 0 (iii) z1 = 12 log 2, zn = log n, n ≥ 2, no finite p. 4. Entire Functions Remark. If σ > ρ1 , then Also, But 33 P 1 <∞ |zn |σ X 1 <∞ |zn | p+1 X 1 =∞ |zn | p Thus, if ρ1 is not an integer, p = [ρ1 ], and if ρ1 is an integer, then either P 1 P 1 < ∞ or = ∞; in the first case, p + 1 = ρ1 , which in the ρ 1 |zn | |zn |ρ1 second case p = ρ1 . Hence, φ ≤ ρ1 But ρ1 ≤ ρ. Thus p ≤ ρ1 ≤ ρ Also p ≤ ρ1 ≤ p + 1, since X 1 < ∞. |zn | p+1 Lecture 5 Entire Functions (Contd.) Theorem 1 (Hadamard). [8] Let f be an entire function with zeros |z1 | ≤ |z2 | ≤ . . . → ∞{zn } such that Let f (o) , 0. Let f be of order ρ < ∞. Let G(z) be the canonical product with the given zeros. Then f (z) = eQ(z)G(z), where Q is a polynomial of degree ≤ ρ. We shall give a proof without using Weierstrass’s theorem. The proof f ′ (z) 1 will depend on integrating the function . over a sequence f (z) zµ (z − x) of expending circles. Given R > 0, let N be defined by the property: |zN | ≤ R, |zN+1 | > R. We need the following Lemma. Let 0 < ε < 1. Then N f ′ (z) X 1 < cRρ−1+ε − f (z) n+1 z − zn for |z| = R R > R0 , and |z| = is free from any zn . 2 2 35 37 5. Entire Functions (Contd.) 36 For we can choose an R0 such that for |z| = R > R0 , 38 ρ+ε (i) | f (z)| < eR , (ii) no zn lies on |z| = (iii) log R , and 2 1 < (2R)ρ+ε | f (0)| For such an R > R0 , define N f (z) Y z gR (z) = 1− f (0) n=1 zn !−1 Then for |z| = 2R, we have |gR (z)| < 1 (2R)ρ+ε e | f (o)| z | ≥ 1 for 1 ≤ n ≤ N. zn Hence, by the maximum modulus principle, ρ+ε since | f | < e(2R) , and |1 − |gR (z)| < 1 (2R)ρ+ε e for |z| = R. f (0) That is log |gR (z)| < 2ρ+2 Rρ+ε . (0 < ε < 1) If hR (z) ≡ log gR (z), and the log vanishes for z = 0, then, since gR (z) is analytic and gR (z) , 0 for |z| ≤ R, we see that hR (z) is analytic for |z| ≤ R, and hR (0) = 0. Further, for |z| = R, Re hR (z) = log |gR (z)| < 2ρ+2 Rρ+ε 39 Hence, by the Borel-Caratheodory inequality, we have for |z| = R/2, |h′R (z)| < cRρ−1+ε , which gives the required lemma. 5. Entire Functions (Contd.) 37 Proof of theorem. Let µ = [ρ] Then consider I≡ Z 1 f ′ (z) · dz f (z) zµ (z − x) R taken along |z| = R/2, where |x| < . The only poles of the inte4 grand are: 0, x and those z′n s which lie inside |z| = R/2. Calculating the residues, we get 1 2πi Z |z|=R/2 X 1 1 f ′ (z) dz = µ µ f (z) z (z − x) z · (zn − x) |Z |<R/2 n n f ′ (x) 1 · f (x) xµ ! 1 1 f ′ (z) µ−1 − D + z=0 f (z) (µ − 1)! z−x + We shall prove that the l.h.s tends to o as R → ∞ in such a way that |z| = R/2 is free from any zn . Rewriting I as Z ′ X N N Z X f 1 dz dz 1 + · µ I= µ − f z − zn z (z − x) z − zn z (z − x) 1 1 ≡ I1 + I2 , we get for |z| = R/2 (by the Lemma), 40 |I1 | = O(Rρ−µ−1+ε ) = O(1). Let k denote the number of z′n s lying inside |z| = R/2 Then I2 = Z k X ... + n=1|z|=R/2 ≡ I2,1 + I2,2 , say. N Z X n=k+1 ... 5. Entire Functions (Contd.) 38 The value of I2,1 remains unaltered when we integrate along |z| = 3R/4, and along the new path, |z − zn | ≥ R/4 since n ≤ k. Since N = O(Rρ+ε ) we get I2,1 = O(Rρ−µ−1+ε ) = O(1) Similarly integrating I2,2 over |z| = R/4, we get I2,2 = O(1) Thus I = o(1). Hence ! ∞ f ′ (x) 1 X 1 h iµ−1 f ′ 1 1 D =0 + · z=0 f (x) xµ n=1 zµn (z − x) (µ − 1)! f z−x i.e. i.e. 41 f ′ (x) f (x) + f ′ (x) = f (x) µ−1 X 0 µ−1 X 0 bn xn ∞ X x−1 µ zn (z n=1 ! = 0, bn = aµ−n , an = − − x) ∞ X xµ−1 xµ−2 1 n µ + + ··· + cn x + µ−1 x − zn zn zn n=1 h f ′ i(µ−n) f z=0 (µ − n)! Integrating and raising to the power of e we get the result: µ P f (x) = e 0 dn x n ∞ Y 1 ! x x/z p +·+xµ /µzµn cn−1 1− , dn = e . zn n If f is an entire functions of order ρ, which is not a constant, and such that f (o) , 0, and f (zn ) = 0, n = 1, 2, 3, . . . |zn | ≤ |zn+1 |, then f (z) = eQ1 (z)G1 (z), where Q1 (z) is a polynomial of degree q ≤ ρ and ! ∞ Y z zz +···+ 1p zz p n , G1 (z) = 1− en zn n=1 where p + 1 is the smallest integer for which existing, since f is of finite order. P 1 < ∞, this integer |zn | p+1 5. Entire Functions (Contd.) 39 Remark. This follows at once from Weierstrass’s theorem but can also be deduced from the infinite-product representation derived in the proof of Hadamard’s theorem (without the use of Weierstrass’s theorem). One has only to notice that Y 1 e− p+1 µ z p+1 −...− µ1 zzn zn is convergent, where p is the genus of the entire function in question, so 42 that f (z) = eQ(z)G(z) may be multiplied by this product yielding f (z) = eQ1 (z)G1 (z), where Q1 is again of degree ≤ µ. We recall the convention that if the z′n s are finite in number (or if there are no z′n s), then p = 0 and ρ1 = 0. We have also seen that q ≤ ρ, ρ1 ≤ ρ i.e. max(q, ρ1 ) ≤ ρ We shall now prove the following Theorem 2. ρ ≤ max(q, ρ1 ) Let up u2 +···+ p E(u) ≡ (1 − u)e 2 u+ If |u| ≤ 21 , then p+1 p+2 −u up u |E(u)| = elog(1−u)+u+...+ p = e p+1 − p+2 −··· ≤ e|u| p+1 (1+ 1 + 1 +··· ) 2 4 = e2|u| p+1 τ ≤ e|2u| p+1 ≤ e|2u| , if τ ≤ p + 1 If |u| > 12 , then |E(u)| ≤ (1 + |u|)e|u|+···+ ≤ (1 + |u|)e|u| ≤ (1 + |u|)e|u| |u| p p p ·(|u|1−p +···+1) p (2 p−1 +···+1) 5. Entire Functions (Contd.) 40 < e|2u| p +log(1+|u|) τ +log(1+|u|) ≤ e|2u| , if p ≤ τ, since |2u| > 1. 43 Hence, for all u, we have τ +log(1+|u|) |E(u)| ≤ e|2u| , if p ≤ τ ≤ p + 1. It is possible to choose τ in such a way that (i) p ≤ τ ≤ p + 1, (ii) τ > 0, (iii) P 1 < ∞, (if there are an infinity of z′n s) and |zn |τ (iv) ρ1 ≤ τ ≤ ρ1 + ε P 1 < ∞ (if the series is infinite this would imply that |zn |ρ1 ρ1 > 0), we have only to take τ = ρτ > 0. And in all other cases we must P 1 < ∞] and so we have p ≤ ρ1 < p + 1, [for, if ρ1 = p + 1, then |zn |ρ1 P 1 choose τ such that ρ1 < τ < p + 1; this implies again that <∞ |zn |τ and τ > 0. For such a τ we can write the above inequality as For, if τ |E(u)| ≤ ec1 |u| , c1 is a constant. 44 Hence | f (z)| ≤ e|Q(z)|+c1 · c2 rq +c3 rτ i.e. M(r) < e Hence ∞ τ X z zn n=1 , |z| = r > 1, and c1 X |1/zn |τ = c3 . log M(r) = O(rq ) + O(rτ ), as r → ∞, 5. Entire Functions (Contd.) 41 = O(rmax(q,τ) ), as r → ∞ (2.1) so that ρ ≤ max(q, τ) Since τ is arbitrarily near ρ1 , we get ρ ≤ max(q, ρ1 ), and this proves the theorem. Theorem 3. If the order of the canonical product G(z) is ρ′ , then ρ′ = ρ1 Proof. As in the proof of Theorem 2, we have p ≤ τ ≤ p + 1; τ τ>0 |E(u)| ≤ ec1 |u| P 1 <∞ |zn |τ ρ1 ≤ τ ≤ ρ + ε, ε>0 Hence ∞ τ X z c1 zn n=1 |G(z)| ≤ e τ ≤ ec3 r , |z| = r. If M(r) = max |G(z)| , then 45 |z|=r M(r) < ec3 r τ Hence ρ′ ≤ τ which implies ρ′ ≤ ρ1 ; but ρ1 ≤ ρ′ . Hence ρ′ = ρ1 Theorem 4. If, either 5. Entire Functions (Contd.) 42 (i) ρ1 < q or (ii) then P 1 < ∞ (the series being infinite), |zn |ρ1 log M(r) = O(rβ ), for β = max(ρ1 , q). Proof. (i) If ρ1 < q, then we take τ < q and from (2.1) we get log M(r) = O(rq ) = O(rmax(ρ1 ,q) ) ∞ P 1 < ∞, then we may take τ = ρ1 > 0 and from (2.1) we n=1 |zn |ρ1 get (ii) If log M(r) = O(rq ) + O(rρ1 ) = O(rβ ) Theorem 5. (i) We have ρ = max(ρ1 , q) (The existence of either side implies the other) 46 (ii) If ρ > 0, and if log M(r) = O(rρ ) does not hold, then ρ1 = ρ, f (z) P has an infinity of zeros zn , and |zn |−τ is divergent. Proof. The first part is merely an affirmation of Hadamard’s theorem, ρ1 ≤ ρ and Theorem 2. For the second part, we must have ρ1 = ρ; for if ρ1 < ρ, then ρ = q by the first part, so that ρ1 < q, which implies, by Theorem 4, that logM(r) = O(rq ) = O(rρ ) in contradiction with our hypothesis. Since ρ > 0, and ρ1 = ρ we have therefore ρ1 > 0, which implies that f (z) has ∞ P P an infinity of zeros. Finally |zn |−ρ1 is divergent, for if |zn |ρ1 < ∞, 1 then by Theorem 4, we would have log M(r) = O(rρ ) which contradicts the hypothesis. 5. Entire Functions (Contd.) 43 Remarks. (1) ρ1 is called the ‘real order’ of f (z), and ρ the ‘apparent order Max (q, p) is called the ‘genus’ of f (z). (2) If ρ is not an integer, then ρ = ρr , for q is an integer and ρ = max(ρ1 , q). In particular, if ρ is non-integral, then f must have an infinity of zeros. Lecture 6 The Gamma Function 1 Elementary Properties [15, p.148] 47 Define the function Γ by the relation. Z∞ Γ(x) = t x−1 e−t dt, x real. 0 (i) This integral converges at the ‘upper limit’ ∞, for all x, since t x−1 e−t = t−2 t x+1 e−t = O(t−2 ) as t → ∞; it converges at the lower limit o for x > 0. (ii) The integral converges uniformly for 0 < a ≤ x ≤ b. For ∞ 1 Z∞ Z1 Z∞ Z Z t x−1 e−t dt = + = O ta−1 dt + O tb−1 e−t dt 0 0 0 1 1 = O(1), independently of x. Hence the integral represents a continuous function for x > 0. (iii) If z is complex, R∞ tz−1 e−t dt is again uniformly convergent over any 0 finite region in which Re z ≥ a > 0. For if z = x + iy, then |tz−1 | = t x−1 , 45 6. The Gamma Function 46 and we use (ii). Hence Γ(z) is an analytic function for Re z > 0 (iv) If x > 1, we integrate by parts and get Γ(x) = h i∞ −t x−1 e−t 0 + (x − 1) Z∞ t x−2 e−t dt 0 = (x − 1)Γ(x − 1). 48 However, Z∞ Γ(1) = e−t dt = 1; hence 0 Γ(n) = (n − 1)!, if n is a +ve integer. Thus Γ(x) is a generalization of n! (v) We have 1 log Γ(n) = (n − ) log n − n + c + O(1), 2 where c is a constant. log Γ(n) = log(n − 1)! = n−1 X log r. r=1 We estimate log r by an integral: we have 1 r+ 2 Z log t dt = r− 12 1 1 Z2 Z2 log(s + r)ds = − 21 = Z1/2 0 0 + Z0 − 12 log(t + r) + log(r − t) dt 1. Elementary Properties 47 !# Z1/2" t2 2 log r + log 1 − 2 dt = r 0 ! 1 = log r + cr , where cr = O 2 . r Hence log Γ(n) = r+ 12 Z n−1 X r=1 r− 12 1 = n− 2 Z log t dt − cr log t dt − 1 2 = ( n−1 X cr r=1 ! ! ) 1 1 1 1 1 1 − log − (n − ) + n − log n − 2 2 2 2 2 2 ∞ ∞ X X − cr + Cr n r=1 1 = (n − ) log n − n + c + o(1), where c is a constant. 2 49 Hence, also 1 (n!) = a.e−n nn+ 2 eo(1) , where ‘a’ is a constant such that c = log a (vi) We have Γ(x)Γ(y) = Γ(x + y) Z∞ O ty−1 dt, x > 0, y > 0. (1 + t) x+y For Γ(x)Γ(y) = Z∞ 0 t x−1 −t e dt · Z∞ 0 sy−1 e−s ds, x > o, y > 0 6. The Gamma Function 48 Put s = tv; then Γ(x)Γ(y) = Z∞ = Z∞ 0 Z∞ = Z∞ Z∞ dt vy−1 dv t x+y−1 e−t(1+v) dt vy−1 dv u x+y−1 e−u du (1 + v) x+y t e 0 ty vy−1 e−tv dv 0 0 0 = Γ(x + y) 0 Z∞ 0 50 Z∞ x−1 −t vy−1 dv. (1 + v) x+y The inversion of the repeated integral is justified by the use of the fact that the individual integrals converge uniformly for x ≥ ε > 0, y ≥ ε > 0. (vii) Putting x = y = tan2 θ] 1 in (vii), we get [using the substitution t = 2 1 {Γ( )}2 = 2Γ(1) 2 Zπ/2 dθ = π. 0 √ Since Γ( 12 ) > 0, we get Γ( 21 ) = π Putting y = 1 − x, on the other hand, we get the important relation Γ(x)Γ(1 − x) = Z∞ 0 u−x π du = , 0 < x < 1, 1+u sin(1 − x)π since Z∞ 0 π xa−1 dx = for 0 < a < 1, by contour 1+x sin aπ 2. Analytic continuation of Γ(z) 49 integration. Hence Γ(x)Γ(1 − x) = π , sin xπ 0 < x < 1. 2 Analytic continuation of Γ(z) [15, p. 148] We have seen that the function Γ(z) = Z∞ e−t tz−1 dt o is a regular function for Re z > 0. We now seek to extend it analytically into the rest of the complex z-plane. Consider Z I(z) ≡ e−ζ (−ζ)z−1 dζ, C where C consists of the real axis from ∞ to δ > 0, the circle |ζ| = δ in 51 the ‘positive’ direction x and again the real axis from δ to ∞. We define (−ζ)z−1 = e(z−1) log(−ζ) by choosing log(−ζ) to be real when ζ = −δ The integral I(z) is uniformly convergent in any finite region of the Z-plane, for the only possible difficulty is at ζ = ∞, but this was covered by case (iii) in § 1. Thus I(z) is regular for all finite values of z. We shall evaluate I(z). For this, set ζ = ρeiϕ so that log(−ζ) = log ρ + i(ϕ − π) on the contour [so as to conform with the requirement that log(−ζ) is real when ζ = −δ] Now the integrals on the portion of C corresponding to (∞, δ) and (δ, ∞) give [since ϕ = 0 in the first case, and ϕ = 2π in the second]: Zδ ∞ −ρ+(z−1)·(log ρ−iπ) e dρ + Z∞ δ e−ρ+(z−1)(log ρ+iπ) dρ 6. The Gamma Function 50 = Z∞ h δ = Z∞ δ i −e−ρ+(z−1)(log ρ−iπ) + e−ρ+(z−1)(log ρ+iπ) dρ h i e−ρ+(z−1) log ρ e(z−1)iπ − e−(z−1)iπ dρ = −2i sin zπ Z∞ e−ρ · ρz−1 dρ δ On the circle |ζ| = δ, we have |(−ζ)z−1 | = |e(z−1) log(−ζ)| = |e(z−1)[log δ+i(ϕ−π)] | = e(x−1) log δ−y(ϕ−π) = O(δ x−1 ). 52 The integral round the circle |ζ| = δ therefore gives O(δ x ) = O(1), as δ → 0, if x > 0. Hence, letting δ → 0, we get I(z) = −2i sin πz Z∞ e−ρ ρz−1 dρ, Re z > 0 0 = −2i sin πzΓ(z), Re z > 0. We have already noted that I(z) is regular for all finite z; so 1 iI(z) cosec πz 2 is regular for all finite z, except (possibly) for the poles of cosec πz namely, z = 0, ±1, ±2, . . .; and it equals Γ(z) for Re z > 0. Hence - 21 iI(z) cosec zπ is the analytic continuation of Γ(z) all over the z-plane. 3. The Product Formula 51 We know, however, by (iii) of § 1, that Γ(z) is regular for z = 1 1, 2, 3, . . .. Hence the only possible poles of iI(z) cosec πx are z = 2 0, −1, −2, . . .. These are actually poles of Γ(z), for if z is one of these numbers, say −n, then (−ζ)z−1 is single-valued in 0 and I(z) can be evaluated directly by Cauchy’s theorem. Actually Z −ζ e −2πi 2πi n+1 (−1) (−1)n+n+1 = dζ = n+1 n! n! ζ C i.e. I(−n) = − −2πi . n! So the poles of cosec πz, at z = 0, −n, are actually poles of Γ(z). The 53 residue at z = −n is therefore ! −2πi z + n (−1)n lim = z→−n n! −2i sin zπ n! The formula in (viii) of § 1 can therefore be upheld for complex values. Thus Γ(z) · Γ(1 − z) = π cosec πz for all non-integral values of z. Hence, also, 1 is an entire function. Γ(z) (Since the poles of Γ(1 − z) are cancelled by the zeros of sin πz) 3 The Product Formula 1 is an entire function of order 1. Γ(z) Since I(z) = −2i sin zπ Γ(z), and We shall prove that Γ(z) · Γ(1 − z) = π , sin πz we get I(1 − z) = −2i sin(π − zπ)Γ(1 − z) 6. The Gamma Function 52 = −2i sin zπ or 54 Now π 1 · sin πz Γ(z) =− 2iπ Γ(z) 1 I(1 − z) = . Γ(z) −2iπ Z1 Z∞ π|z| −t x−1 −t x−1 e t dt + e t dt I(z) = O e 0 1 Z∞ π|z| −t |z| = O e 1 + e t dt 1 1+|z| Z∞ Z + 1 + = O eπ|z| 1 1+|z| i h = O eπ|z| (|z| + 1)|z|+1 h 1+ε i = O e|z| , ε > 0. 1 is of order ≤ 1. However, the exponent of convergence Γ(z) of its zeros equals 1. Hence the order is = 1, and the genus of the canonical product is also equal to 1. Thus ∞ Y z −z 1 az+b = z, e (1 + )e n Γ(z) n n=1 Hence 1 = 1 and z→0+ zΓ(z) by Hadamard’s theorem. However, we know that lim Γ(1) = 1. These substitutions give b = 0, and ! 1 −1/n 1 = ea Π 1 + e π or, ! # ∞ " X 1 1 0=a+ − log 1 + n n 1 3. The Product Formula 53 m " ! # 1 1 X − = a − lim log 1 + m→∞ n n 1 m m X 1 X = a + lim log(n + 1) − log n − m→∞ n 1 1 m X 1 = a + lim log(m + 1) − m→∞ n 1 = a − γ, where γ is Euler’s constant. 55 Hence ∞ Y 1 z = eγz z 1 + e−z/n Γ(z) n n=1 As a consequence of this we can derive Gauss’s expression for Γ(z). For ez/n ez/1 . . . · Γ(z) = lim e n→∞ z 1 + 1z 1+ z " # n 1 1 2 n = lim nz · · · ... n→∞ z z+1 z+2 z+n " # nz · n! = lim n→∞ z(z + 1) . . . (z + n) " z(log n−1− 12 −...− n1 ) 1 # We shall denote nz · n! ≡ Γn (z), z(z + 1) . . . (z + n) so that 56 Γ(z) = lim Γn (z). n→∞ Further, we get by logarithmic-differentiation, ! ∞ Γ′ (z) 1 X 1 1 = −γ − − − . Γ(z) z n=1 z + n n 6. The Gamma Function 54 Thus Hence ∞ X 1 d2 [log Γ(z)] = ; 2 dz2 (n + z) n=0 d2 [log Γ(z)] > 0 for real, positive z. dz2 Lecture 7 The Gamma Function: Contd 4 The Bohr-Mollerup-Artin Theorem [7, Bd.I, p.276] We shall prove that the functional equation of Γ(x), namely Γ(x + 1) = 57 d2 xΓ(x), together with the fact that 2 [log Γ(x)] > 0 for x > 0, deterdx mines Γ(x) ‘essentially’ uniquely-essentially, that is, except for a constant of proportionality. If we add the normalization condition Γ(1) = 1, then these three properties determine Γ uniquely. N.B. The functional equation alone does not define Γ uniquely since g(x) = p(x)Γ(x), where p is any analytic function of period 1 also satisfies the same functional equation. We shall briefly recall the definition of ‘Convex functions’. A realvalued function f (x), defined for x > 0, is convex, if the corresponding function f (x + y) − f (x) φ(y) = , y defined for all y > −x, y , 0, is monotone increasing throughout the range of its definition. If 0 < x1 < x < x2 are given, then by choosing y1 = x1 − x and 55 7. The Gamma Function: Contd 56 y2 = x2 − x, we can express the condition of convexity as: f (x) ≤ 58 x2 − x x − x1 f (x1 ) + f (x2 ) x2 − x1 x2 − x1 Letting x → x1 , we get f (x1 + 0) ≤ f (x1 ); and letting x2 → x, we get f (x) ≤ f (x + 0) and hence f (x1 + 0) = f (x1 ) for all x1 . Similarly f (x1 − 0) = f (x1 ) for all x1 . Thus a convex function is continuous. Next, if f (x) is twice (continuously) differentiable, we have ϕ′ (y) = y f ′ (x + y) − f (x + y) + f (x) y2 and writing x + y = u, we get f (x) = f (u − y) = f (u) − y f ′ (u) + y2 ′′ f [u − (1 − θ)y], 0 ≤ θ ≤ 1 2 which we substitute in the formula for ϕ′ (y) so as to obtain ϕ′ (y) = 1 ′′ f [x + θy]. 2 Thus if f ′′ (x) ≥ 0 for all x > 0, then ϕ′ (y) is monotone increasing and f is convex. [The converse is also true]. Thus log Γ(x) is a convex function; by the last formula of the previous section we may say that Γ(x) is ‘logarithmically convex’ for x > 0. Further Γ(x) > 0 for x > 0. Theorem. Γ(x) is the positive function uniquely defined for x > 0 by the conditions: (1.) Γ(x + 1) = xΓ(x) (2.) Γ(x) is logarithmically convex (3.) Γ(1) = 1. 4. The Bohr-Mollerup-Artin Theorem 59 57 Proof. Let f (x) > 0 be any function satisfying the above three conditions satisfied by Γ(x). Choose an integer n > 2, and 0 < x ≤ 1. Let n − 1 < n < n + x ≤ n + 1. By logarithmic convexity, we get log f (n − 1) − log f (n) log f (n + x) − log f (n) < (n − 1) − n (n + x) − n log f (n + 1) − log f (n) ≤ (n + 1) − n Because of conditions 1 and 3, we get f (n − 1) = (n − 2)!, f (n) = (n − 1)!, f (n + 1) = n! and f (n + x) = x(x + 1) . . . (x + n − 1) f (x). Substituting these in the above inequalities we get log(n − 1) x < log f (n + x) ≤ log n x , (n − 1)! which implies, since log is monotone, f (n + x) ≤ nx (n − 1)! (n − 1)!(n − 1) x (n − 1)!n x < f (x) ≤ x(x + 1) . . . (x + n − 1) x(x + 1) . . . (x + n − 1) or (n − 1) x < Replacing (n − 1) by n in the first inequality, we get x+n , n = 2, 3, . . . Γn (x) < f (x) ≤ Γn (x) · n where Γn is defined as in Gauss’s expression for Γ. Letting n → ∞, we get f (x) = Γ(x), 0 < x ≤ 1. For values of x > 1, we uphold this relation by the functional equation. 7. The Gamma Function: Contd 58 5 Gauss’s Multiplication Formula. [7, Bd.I, p.281] 60 Let p be a positive integer, and ! ! ! x x+1 x+ p−1 x f (x) = p Γ Γ ...Γ p p p [If p = 1, then f (x) = Γ(x)]. For x > 0, we then have dx [log f (x)] > 0. dx2 Further f (x + 1) = x f (x). Hence by the Bohr-Artin theorem, we get f (x) = a p Γ(x). Put x = 1. Then we get ! ! ! 2 p 1 ·Γ ...Γ a p = pΓ p p p (5.1) [a1 = 1, by definition]. Put k = 1, 2, . . . p, in the relation ! k nk/p n!pn+1 Γn , = p k(k + p) . . . (k + np) and multiply out and take the limit as n → ∞. We then get from (5.1), a p = p. lim n n→∞ p+1 2 (n!) p pnp+p (np + p)! However ! ! !# " 2 p 1 1+ ... 1 + (np + p)! = (np)!(np) p 1 + np np np Thus, for fixed p, as n → ∞, we get (n!) p pnp n→∞ (np)!n(p−1)/2 a p = p lim 6. Stirling’s Formula 61 59 Now by the asymptotic formula obtained in (v) of § 1, [see p.49] (n!) p = a p nnp+p/2 e−np eo(1) 1 1 (np)! = annp+ 2 pnp+ 2 e−np eo(1) Hence ap = √ p · a p−1 . Putting p = 2 and using (5.1) we get ! √ 1 1 1 Γ(1) = 2π a = √ , a2 = √ 2Γ 2 2 2 Hence ap = √ (5.2) p(2π)(p−1)/2 . Thus ! ! √ x x+ p−1 p Γ ...Γ = p(2π)(p−1)/2 Γ(x) p p x For p = 2 and p = 3 we get: √ x x + 1! x + 2! x x + 1! π 2π Γ Γ(x). Γ = x−1 Γ(x); Γ Γ Γ = 1 2 2 3 3 3 2 3 x− 2 6 Stirling’s Formula [15, p.150] From (v) of § 1, p.49 and (5.2) we get √ 1 (n!) = 2π · e−n · nn+ 2 eo(1) , which is the same thing as ! √ 1 log(n − 1)! = n − log n − n + log 2π + o(1) 2 (6.1) Further 62 1+ 1 1 + ··· + − log N = γ + 0(1), as N → ∞ 2 N−1 (6.2) 7. The Gamma Function: Contd 60 and z log(N + z) = log N + log 1 + N ! z 1 = log N + + O 2 , as N → ∞. N N (6.3) We need to use (6.1)-(6.3) for obtaining the asymptotic formula for Γ(z) where z is complex. From the product-formula we get log Γ(z) = ∞ X z n=1 z − γz − log z, − log 1 + n n each logarithm having its principal value. Now ZN 0 N−1 X [u] − u + 21 du = u+z n=0 N−1 X Zn+1 1 n + 2 + z − 1 du u+z n 1 + z)[log(n + 1 + z) − log(n − z)] − N 2 n=0 ! N−1 N−1 X 1 X = n[log(n + 1 + z) − log(n + z)] + z + 2 n=0 n=0 log(n + 1 + z) − log(n + z) − N ! N−1 X 1 = (N − 1) log(N + z) − log(n + z) + z + log(N + z) 2 n=1 ! 1 − z + log z − N 2 ! ! 1 1 = N − + z log(N + z) − z + log z 2 2 N−1 X z −N− log n + log 1 + n n=1 = (n + (6.4) 6. Stirling’s Formula 61 ! ! 1 1 = N − + z log(N + z) − z + log z − N − log(N − 1)! 2 2 N−1 N−1 X1 X z z −z − log 1 + + n n n 1 n=1 63 Now substituting for log(N + z) etc., from (6.1)-(6.3), we get ZN 0 !) ! ( [u] − u + 21 1 1 z 1 du = (N − + z) log N + + O 2 − z + u+z 2 N 2 N ! 1 log z − N − N − log N + N − c + O(1)+ 2 N−1 N−1 X1 Xz z − log 1 + −z n n n 1 n=1 N−1 X 1 √ + z + O(1) − log 2π = z log N − n 1 − z− N−1 Xz 1 z log z − log z + − log 1 + 2 n n n=1 ! Now letting N → ∞, and using (6.4), and (6.2), we get Z∞ 0 ! [u] − u + 12 1 1 du + log 2π − z + z − log z = log Γ(z) u+z 2 2 Ru If ϕ(u) = ([v] − v + 12 )dv, then 0 ϕ(u) = O(1), since ϕ(n + 1) = ϕ(n), if n is an integer. Hence Z∞ Z∞ Z∞ [u] − u + 21 dϕ(u) ϕ(u) du = = u+z u+z (u + z)2 0 0 0 64 (6.5) 7. The Gamma Function: Contd 62 ∞ Z dv = O |u + z|2 0 If we write z = reiθ , and u = ru1 , then ∞ Z∞ Z [u] − u + 21 1 du 1 du = O r u+z |u1 + θiθ |2 0 0 The last integral is finite if θ , π. Hence Z∞ 0 ! [u] − u + 21 1 du = O , uniformly for |arg z| ≤ π − ε < π u+z r Thus we get from (6.5): ! ! 1 1 1 log Γ(z) = z − log z − z + log 2π + O 2 2 |z| for |arg z| ≤ π − ε < π 65 Corollaries. (1) log Γ(z + α) = (z + α − 12 ) log z − z + 12 log 2π + O as |z| → ∞ uniformly for |arg z| ≤ π − ε < π. α bounded. (2) For any fixed x, as y → ±∞ 1 1 |Γ(x + iy)| ∼ e− 2 π|y| |y| x− 2 1 |z| √ 2π ! Γ′ (z) 1 1 (3) = log z − + O 2 , |arg z| ≤ π − ε < π [11, p.57] Γ(z) 2z |z| This may be deduced from (1) by using Z 1 f (ζ) ′ dζ, f (z) = 2πi (ζ − z)2 C where f (z) = log Γ(z) − z − 21 log z + z − 21 log 2π and C is a circle with centre at ζ = z and radius |z| sin ε/2. Lecture 8 The Zeta Function of Riemann 1 Elementary Properties of ζ(s) [16, pp.1-9] We define ζ(s), for s complex, by the relation ζ(s) = ∞ X 1 , s = σ + it, σ > 1. ns n=1 66 (1.1) We define x s , for x > 0, as e s log x , where log x has its real determination. Then |n s | = nσ , and the series converges for σ > 1, and uniformly in any finite region in which σ ≥ 1 + δ > 1. Hence ζ(s) is regular for σ ≥ 1 + δ > 1. Its derivatives may be calculated by termwise differentiation of the series. We could express ζ(s) also as an infinite product called the Euler Product: !−1 Y 1 ζ(s) = 1− s , σ > 1, (1.2) p p where p runs through all the primes (known to be infinite in number!). It is the Euler product which connects the properties of ζ with the properties of primes. The infinite product is absolutely convergent for σ > 1, 63 64 8. The Zeta Function of Riemann since the corresponding series X 1 X 1 = < ∞, σ > 1 ps pσ p p Expanding each factor of the product, we can write it as ! Y 1 1 1 + s + 2s + · · · p p p 67 Multiplying out formally we get the expression (1.1) by the unique factorization theorem. This expansion can be justified as follows: ! Y 1 1 1 1 1 + s + 2s + · · · = 1 + s + s + · · · , p n n p 1 2 p≤p where n1 , n2 , . . . are those integers none of whose prime factors exceed P. Since all integers ≤ P are of this form, we get !−1 X ∞ X Y ∞ 1 1 1 1 1 = 1 − − − 1 − − − · · · n s p≤P n1s n2s p2 n=1 n s n=1 1 1 + + ··· ≤ (P + 1)σ (P + 2)σ → 0, as P → ∞, if σ > 1. Hence (1.2) has been established for σ > 1, on the basis of (1.1). As an immediate consequence of (1.2) we observe that ζ(s) has no zeros for σ > 1, since a convergent infinite product of non-zero factors is non-zero. We shall now obtain a few formulae involving ζ(s) which will be of use in the sequel. We first have ! X 1 (1.3) log ζ(s) = − log 1 − 2 , σ > 1. p p 1. Elementary Properties of ζ(s) If we write π(x) = P 65 1, then p≤x ∞ X ! 1 log ζ(s) = − {π(n) − π(n − 1)} log 1 − s n n=2 " ! !# ∞ X 1 1 =− π(n) log 1 − s − log 1 − n (n + 1) s n=2 = ∞ X n=2 π(n) Zn+1 n s dx x(x s − 1) 68 Hence log ζ(s) = s Z∞ 2 π(x) dx, σ > 1. x(x s − 1) (1.4) It should be noted that the rearrangement of the series preceding the above formula is permitted because ! 1 π(n) ≤ n and log 1 − s = O(n−σ ). n A slightly different version of (1.3) would be log ζ(s) = XX p m 1 , mpms σ>1 (1.3)′ where p runs through all primes, and m through all positive integers. Differentiating (1.3), we get − ζ ′ (s) X p−s log p X X log ρ = = , ζ(s) 1 − p−s pms p p,m or ∞ ζ ′ (s) X ∧(n) = , σ>1 s ζ(s) n n=1 , (1.5) 8. The Zeta Function of Riemann 66 log p, if n is a + ve power of a prime p where ∧(n) = 0, otherwise. Again ! Y 1 1 = 1− s ζ(s) p p = ∞ X µ(n) ns n=1 , σ>1 69 (1.6) (1.6) where µ(1) = 1, µ(n) = (−1)k if n is the product of k different primes, µ(n) = 0 if n contains a factor to a power higher than the first. We also have ∞ X d(n) , σ>1 ζ 2 (s) = ns n=1 where d(n) denotes the number of divisors of n, including 1 and n. For ζ 2 (s) = ∞ ∞ ∞ X 1 X 1 X 1 X 1 · = s s s m n µ mn=µ m=1 n=1 µ=1 More generally k ζ (s) = ∞ X dk (n) ns n=1 70 , σ>1 (1.7) where k = 2, 3, 4, . . ., and dk (n) is the number of ways of expressing n as a product of k factors. Further ζ(s) · ζ(s − a) = = ∞ ∞ X 1 X na , m s n=1 n s m=1 ∞ X 1 X a · n , µ s mn=µ µ=1 so that ζ(s) · ζ(s − a) = ∞ X σ2 (µ) µ=1 µδ (1.8) 1. Elementary Properties of ζ(s) 67 where σa (µ) denotes the sum of the ath powers of the divisors of µ. If a , 0, we get, from expanding the respective terms of the Euler products, ! ! Y pa p2a 1 1 1 + s + 2s + · · · 1 + s + 2a + · · · ζ(a)ζ(s − a) = p p p p p ! Y 1 + pa 1 + pa + p2a 1+ = + + ··· ps p2s p ! Y 1 − p2a 1 · + ··· 1+ = 1 − pa p s p Using (1.8) we thus get 1 +1)a 1 − p(m 1 − pr(mr +1)a 1 σ2 (n) = . . . 1 − pa1 1 − par (1.9) 1 m2 mr 1 if n = pm 1 , p2 . . . pr by comparison of the coefficients of n s . More generally, we have 1 − p−2s+a+b ζ(s) · ζ(s − a) · ζ(s − b) · ζ(s − a − b) Y = ζ(2s − a − b) (1 − p−s )(1 − p−s+a )(1 − p−s+b ) p (1 − p−s+a+b ) for σ > max {1, Re a + 1, Re b + 1, Re(a + b) + 1}. Putting p−s = z, we get the general term in the right hand side equal to 1 − pa+b z2 (1 − z) · (1 − pa z) · (1 − pb z)(1 − pa+b z) ( ) pa+b 1 1 pa pb + = − − (1 − pa )(1 − pb ) 1 − z 1 − pa z 1 − pb z 1 − pa+b z ∞ n X o 1 (m+1)a (m+1)b (m+1)(a+b) m 1 − p − p + p z = (1 − pa )(1 − pb ) m=0 = ∞ n X on o 1 (m+1)a (m+1)b m 1 − p 1 − p z (1 − pa )(1 − pb ) m=o 71 8. The Zeta Function of Riemann 68 Hence 72 ζ(s) · ζ(s − a)ζ(s − b) · ζ(s − a − h) ζ(2s − a − b) ∞ YX 1 − p(m+1)a 1 − p(m+1)b 1 = · · ms 1 − pa p 1 − pb p m=0 Now using (1.9) we get ∞ ζ(s) · ζ(s − a) · ζ(s − b)ζ(s − a − b) X σa (n)σb (n) = ζ(2s − a − b) ns n=1 (1.10) σ > max{1, Re a + 1, Re b + 1, Re(a + b) + 1} If a = b = 0, then ∞ {ζ(s)}4 X {d(n)2 } = , ζ(2s) ns n=1 get σ > 1. (1.11) If α is real, and α , 0, we write αi for a and −αi for b in (1.10), and ∞ ζ 2 (s)ζ(s − αi)ζ(s + αi) X |σαi (n)|2 = , σ > 1, ζ(2s) ns n=1 P αi d . where σαi (n) = d/n (1.12) Lecture 9 The Zeta Function of Riemann (Contd.) 2 Elementary theory of Dirichlet Series [10] 73 The Zeta function of Riemann is the sum-function associated with the P 1 . We shall now study, very briefly, some of the Dirichlet series ns elementary properties of general Dirichlet series of the form ∞ X n=1 an e−λn s , o ≤ λ1 < λ2 < . . . → ∞ Special cases are: λn = log n; λn = n, e−s = x. We shall first prove a lemma applicable to the summation of Dirichlet series. Lemma. Let A(x) = P λn ≤x an , where an may be real or complex. Then, if x ≥ λ1 , and φ(x) has a continuous derivative in (0, ∞), we have X λn ≤ω an φ(λn ) = − Zω A(x)φ′ (x)dx + A(ω)φ(ω). λ1 69 9. The Zeta Function of Riemann (Contd.) 70 If A(ω)φ(ω) → 0 as ω → ∞, then ∞ X n=1 an φ(λn ) = − Z∞ A(x)φ′ (x)dx, λ1 provided that either side is convergent. Proof. A(ω)φ(ω) − = X X λn ≤ω = an φ(λn ) λn ≤ω an {φ(ω) − φ(λn )} ω XZ an φ′ (x)dx λn ≤ω λ n = Zω A(x)φ′ (x)dx λ1 74 Theorem 1. If ∞ P n=1 an e−λn s converges for s = s0 ≡ σ0 + ito , then it converges uniformly in the angular region defined by |am(s − s0 )| ≤ θ < π/2, for 0 < θ < π/2 Proof. We may suppose that so = 0. For X X X ′ an e−λn s = an e−λn s0 e−λn(s−s0 ) ≡ bn e−λn s , say, and the new series converges at s′ = 0. By the above lemma, we get ν X µ+1 −λn s an e ν µ X X s = − an e−λn 1 1 2. Elementary theory of Dirichlet Series = Zλν 71 A(x) · e−xs · sdx + A(λν )e−λν s − A(λµ )e−λµ s λµ =s Zλν {A(x) − A(λµ )}e−xs dx + [A(λν ) − A(λµ )]e−λν s λµ P We have assumed that an converges, therefore, given ǫ > 0, there 75 exists an n0 such that for x > λµ ≥ n0 , we have |A(x) − A(λµ )| < ε Hence, for such µ, we have Zλν ν X an e−λn s ≤ ε|s| e−xσ dx + εe−λν σ µ+1 λµ |s| +ε σ < 2ε (sec θ + 1), ≤ 2ε |s| < sec θ, and this proves the theorem. As a conseif σ , 0, since σ quence of Theorem 1, we deduce P s Theorem 2. If an e−λn converges for s = s0 , then it converges for Re s > σo , and uniformly in any bounded closed domain contained in the half-plane σ > σo . We also have P Theorem 3. If an e−λn s converges for s = s0 to the sum f (s0 ), then f (s) → f (s0 ) as s → s0 along any path in the region |am(s − s0 )| ≤ θ < π/2. A Dirichlet series may converge for all values of s, or some values of s, or no values of s. Ex.1. P an n−s , an = 1 converges for all values of s. n! 9. The Zeta Function of Riemann (Contd.) 72 Ex.2. Ex.3. 76 P P an n−s , an = n! converges for no values of s. n−s converges for Re s > 1, and diverges for Re s ≤ 1. If a Dirichlet series converges for some, but not all, values of s, and if s1 is a point of convergence while s2 is a point of divergence, then, on account of the above theorems, we have σ1 > σ2 . All points on the real axis can then be divided into two classes L and U; σ ∈ U if the series converges at σ, otherwise σ ∈ L. Then any point of U lies to the right of any point of L, and this classification defines a number σo such that the series converges for every σ > σo and diverges for σ < σo , the cases σ = σ0 begin undecided. Thus the region of convergence is a half-plane. The line σ = σ0 is called the line of convergence, and the number σo is called the abscissa of convergence. We have seen that σ0 may be ±∞. On the basis of Theorem 2 we can establish Theorem 4. A Dirichlet series represents in its half-plane of convergence a regular function of s whose successive derivatives are obtained by termwise differentiation. We shall now prove a theorem which implies the ‘uniqueness’ of Dirichlet series. P s Theorem 5. If an e−λn converges for s = 0, and its sum f (s) = 0 for an infinity of values of s lying in the region: σ ≥ ε > 0, |am s| ≤ θ < π/2, then an = 0 for all n. 77 Proof. f (s) cannot have an infinite number of zeros in the neighbourhood of any finite point of the giver region, since it is regular there. Hence there exists an infinity of valves sn = σn + itn , say, with σn+1 > ση , lim σn = ∞ such that f (sn ) = 0. However, g(s) ≡ eλ1 s f (s) = a1 + ∞ X 2 an e−(λn −λ1 )s , 2. Elementary theory of Dirichlet Series 73 (here we are assuming λ1 > 0) converges for s = 0, and is therefore uniformly convergent in the region given; each term of the series on the right → 0, as s → ∞ and hence the right hand side, as a whole, tends to a1 as s → ∞. Thus g(s) → a1 as s → ∞ along any path in the given region. This would contradict the fact that g(sn ) = 0 for an infinity of sn → ∞, unless a1 = 0. Similarly a2 = 0, and so on. Remark . In the hypothesis it is essential that ε > 0, for if ε = 0, the origin itself may be a limit point of the zeros of f , and a contradiction does not result in the manner in which it is derived in the above proof. P The above arguments can be applied to an e−λn s so as to yield the existence of an abscissa of absolute convergence σ̄, etc. In general, σ̄ ≥ σ0 . The strip that separates σ̄ from σo may comprise the whole plane, or may be vacuous or may be a half-plane. Ex.1. σ0 = 0, σ̄ = 1 1−s (1 − 2 Ex.2. ! ! 1 1 1 1 1 )ζ(s) = s + s + s + · · · − 2 s + s + · · · 1 2 3 2 4 ! 1 1 1 1 = s − s + s − s + ··· 1 2 3 4 P (−1)n √ (log n)−s converges for all s but never absolutely. In the 78 n simple case λn = log n, we have Theorem 6. σ̄ − σ0 ≤ 1. P P |an | For if an n−s < ∞, then |an | · n−σ = O(1), so that <∞ n s+1+ε for ε > 0 While we have observed that the sum-function of a Dirichlet series is regular in the half-plane of convergence, there is no reason to assume that the line of convergence contains at least one singularity of the function (see Ex 1. above!). In the special case where the coefficients are positive, however we can assert the following Theorem 7. If an ≥ 0, then the point s = σ0 is a singularity of the function f (s). 9. The Zeta Function of Riemann (Contd.) 74 Proof. Since an ≥ 0, we have σ0 = σ̄, and we may assume, without loss of generality, that σ0 = 0. Then, if s = 0 is a regular point, the Taylor series for f (s) at s = 1 will have a radius of convergence > 1. (since the circle of convergence of a power series must have at least one singularity). Hence we can find a negative value of s for which f (s) = ∞ X (s − 1)ν ν=0 79 ν! f (ν) (1) = ∞ ∞ X (1 − s)ν X ν=0 ν1 an λνn e−λn n=1 Here every term is positive, so the summations can be interchanged and we get ∞ ∞ ∞ X X (1 − s)ν λνn X s f (s) = an e−λn = an e−λn ν! n=1 ν=0 n=1 Hence the series converges for a negative value of s which is a contradiction. Lecture 10 The Zeta Function of Riemann (Contd) 2 (Contd). Elementary theory of Dirichlet series 80 We wish to prove a formula for the partial sum of a Dirichlet series. We shall give two proofs, one based on an estimate of the order of the sumfunction [10], and another [14, Lec. 4] which is independent of such an estimate. We first need the following Lemma 1. If σ > 0, then σ+i∞ Z 1 2πi σ−i∞ where σ+i∞ R σ−1∞ = lim T →∞ σ+iT R . 1, eus ds = 0, s 1, 2 if u > 0 if u < 0 if u = 0 σ−iT Proof. The case u = 0 is obvious. We shall therefore study only the cases u ≷ 0. Now σ+iT Z σ−iT eus ds eus = s us σ+iT Z σ−iT 75 + σ+iT Z σ−iT eus ds us2 10. The Zeta Function of Riemann (Contd) 76 However |eu(σ+iT ) | = euσ and |s| > T ; hence, letting T → ∞, we get σ+i∞ Z eus ds = s eus ds ≡ I, say. us2 σ−i∞ σ−i∞ 81 σ+i∞ Z We shall evaluate I on the contour suggested by the diagram. If u < 0 , we use the contour L + CR ; and if u > 0, we use L + C L . If u < 0, we have, on CR , us uσ e ≤ e , since Re s > σ. s2 r2 If u > 0, we have, on C L , us uσ e ≤ e , since Re s < σ. s2 r2 Hence Z us euσ e ds → 0, as r → ∞. ≤ 2πr · 2 2 us |u|γ R ,C L C By Cauchy’s theorem, however, we have Z Z =− ; L CR 2. (Contd). Elementary theory of Dirichlet series 77 hence 1 2πi (1) σ+i∞ Z eus ds = 0, us2 if u < 0. σ−i∞ If, however, u > 0, the contour L + C L encloses a pole of the second order at the origin, and we get Z Z = − +1, L CL so that 1 2πi (2) σ+i∞ Z eus ds = 1, us2 if u > 0. σ−i∞ Remarks. We can rewrite the Lemma as: if a > 0, a+i∞ 0, if λ < λn Z (λ−λn )s e 1 ds = 1, if λ > λn 2πi s 1 a−i∞ if λ = λn 2, Formally, therefore, we should have 1 2πi a+i∞ Z a−i∞ a+i∞ Z (λ−λn )s ∞ 1 X e eλs ds f (s) ds = an s 2πi 1 s a−i∞ X′ an = λn ≤λ the dash denoting that if λ = λn the last term should be halved. We wish now to establish this on a rigorous basis. We proceed to prove another lemma first. 82 10. The Zeta Function of Riemann (Contd) 78 Lemma 2. Let P an e−λn s converge for s = β real. Then n X aν e−λν s = o(|t|), 1 the estimate holding uniformly both in σ ≥ β + ε > β and in n. In particular, for n = ∞, f (s) = o(|t|) uniformly for σ ≥ β + ε > β Proof. Assume that β = 0, without loss of generality. Then aν = O(1) and A(λν ) − A(λµ ) = O(1) for all ν and µ If 1 < N < n, then n X −λν s aν e 1 N n X X = + aν e−λν s 1 = N+1 N X −λν s aν e 1 +s Zλn {A(x) − A(λN )}e−xs dx λN s 83 {A(λn ) − A(λN )}e−λn λ Z n = O(N) + O(1) + O |s| e−xσ dx λN ! |s| −λN σ = O(N) + O e σ = O(N) + O |t|e−λN ε since |s|2 = t2 + σ2 and σ ≥ ε. Hence n X aν e−λν s = O(N) + O(|t|e−λN ε ), if 1 < N < n 1 If N ≥ n, then, trivially, n X 1 aν e−λν s = O(N). 2. (Contd). Elementary theory of Dirichlet series 79 If we choose N as a function of |t|, tending to ∞ more slowly than |t|, we get n X aν e−λν s = O(|t|) 1 in either case. 84 Theorem (Perron’s Formula). Let σ0 be the abscissa of convergence of P an e−λn s whose sum-function is f (s). Then for σ > σ0 and σ > 0, we have σ+i∞ Z ′ X f (s) ωs 1 e ds, an = 2πi s λ ≤ω ν σ−i∞ where the dash denotes the fact that if ω = λn the last term is to be halved. Proof. Let λm ≤ ω < λm+1 , and m X −λn s f (s) − a e n ωs g(s) = e 1 (This has a meaning since Re s ≡ σ > σ0 ). Now 1 2πi σ+i∞ Z g(s) ds s σ−i∞ 1 = 2πi σ+i∞ Z σ−i∞ X′ f (s)eωs ds − an s λ ≤ω n by the foregoing lemma. We have to show that the last expression is zero. Applying Cauchy’s theorem to the rectangle σ − iT 1 , σ + iT 2 , Ω + iT 2 , Ω − iT 1 , 10. The Zeta Function of Riemann (Contd) 80 where T 1 , T 2 > 0, and Ω > σ, we get 1 2πi σ+i∞ Z g(s) ds = 0, s σ−i∞ 85 for 1 2πi σ+iT Z 2 σ−iT 1 Ω−iT Ω+iT σ+iT Z 1 Z 2 Z 2 1 = + + 2πi σ−iT 1 Ω−iT 1 Ω+iT 2 = I1 + I2 + I3 , say. Now, if we fix T 1 and T 2 and let Ω → ∞, then we see that I2 → 0, ∞ P −µ s for g(s) is the sum-function of bn n , where bn = am+n , µn = λm+n −ω, 1 π with µ1 > 0, and hence g(s) = o(1) as s → ∞ in the angle |ams| ≤ − δ. 2 Thus σ+iT Z 1 ∞+iT Z 2 Z 2 ∞−iT 1 1 g(s) ds = − 2πi s 2πi σ−iT 1 σ−iT 1 σ+iT 2 if the two integrals on the right converge. Now if h(s) ≡ g(s)e(λm+1 −ω)s = am+1 + am+2 e−(λm+2 −λm+1 )s + · · · then by lemma 2, we have |h(s)| < εT 2 86 for s = σ + iT 2 , σ ≥ σ0 + ε, T 2 ≥ T 0 . Therefore for the second integral on the right we have Z 2 Z∞ ∞+iT εT 2 g(s) ds < q e−µ1 ξ di < ε/µ1 s 2 2 σ +T σ+iT 2 2 σ µ1 > 0. This proves not only that the integral converges for a finite T 2 , but also that as T 2 → ∞, the second integral tends to zero. Similarly for the first integral on the right. 2. (Contd). Elementary theory of Dirichlet series 81 N.B. An estimate for g(s) alone (instead of h(s)) will not work! Remarks. More generally we have for σ > σ0 and σ > σ∗ X′ an e−λn s∗ λn ≤ω for X an e−λn S ∗ σ+i∞ Z f (s) ω(s−s∗ ) e ds, s − s∗ σ−i∞ X λn (s−s∗ ) ·e = an e−λn s = f (s), 1 = 2πi ∗ and writing s′ = s − s∗ and bn = an e−λn s , we have f (s) ≡ f (s′ ) = P ′ bn e−λn s . We shall now give an alternative proof of Person’s formula without using the order of f (s) as s → ∞ [14, Lec. 4] Aliter. If f (s) = ∞ P 1 an e−λn s has σ0 , ∞ as its abscissa of convergence, and if a > 0, a > σ0 , then for ω , λn , we have 1 an = 2πi <ω X λn a+i∞ Z f (s) eωs ds s a−i∞ Proof. Define 87 fm (s) = m X an e−λn s 1 and rm (s) = ∞ X m+1 an .e−λn s = f (s) − fm (s) Then (A) 1 2πi a+iT Z a−iT 1 eωs ds = f (s) s 2πi a+iT Z a−iT 1 eωs ds + fm (s) s 2πi a+iT Z rm (s) eωs ds s a−iT Here the integral on the left exists since f (s) is regular on σ = a > σ0 . By Lemma 1, as applied to the first integral on the right hand side, we 10. The Zeta Function of Riemann (Contd) 82 get (B) 1 lim T →∞ 2πi a+iT Z a−iT a+iT Z X 1 eωs eωs ds − an = lim ds f (s) rm (s) T →∞ 2πi s s λ <ω n a−iT the limits existing. Since λn → ∞, we can choose m0 such that for all m ≥ m0 we have λm > ω. For all such m the last relation holds. P ′ ′ Now write bn = an e−λn σ , φ(x) = e−x(s−σ ) , so that an e−λn s = P P bn φ(λ). Write B(x) = bn . n≤x Then applying the Lemma of the 9th lecture, we get N X m+1 −λn s an e N m X X = − 1 1 ′ = (s − σ ) ZλN ′ B(x)e−x(s−σ ) dx λm ′ ′ + B(λN )e−λN (s−σ ) − B(m)e−λm (s−σ ) ′ = {B(λN ) − B(λm )}e−λN (s−σ ) ZλN ′ + (s − σ′ ) {B(x) − B(λm )}e−x(s−σ ) dx. λm 88 Now choose σ′ > 0 and a > σ′ > σ0 . [If σo ≥ 0 the second condition implies the first; if σ0 < 0, then since a > 0, choose 0 < σ′ < a]. Then B(x) tends to a limit as x → ∞, so that B(x) = o(1) for all x; ′ ′ while |e−x(s−σ ) | = e−x(σ−σ ) → 0 as x → ∞ for σ > σ′ . Hence, letting N → ∞, we get ′ rm (s) = (s − σ ) Z∞ λm ′ {B(x) − B(λm )}e−x(s−σ ) dx, 2. (Contd). Elementary theory of Dirichlet series or |rm (s)| ≤ c Now consider 1 2πi Z 83 |s − σ′ | −λm (σ−σ′ ) e σ − σ′ rm (s) eωs ds s L+CR where L + CR is the contour indicated in the diagram. rm (s) is regular in this contour, and the integral is therefore zero. 89 Hence Z Z =− L CR On CR , however, s = σ′ + reiθ and σ ≥ a, so that r |rm (s)| ≤ c · · e−λm r cos θ a − σ′ ′ |eωs | = eω(σ +r cos θ) , |s| ≥ r. Hence Zπ/2 Z ωs ′ cr e 1 rm (s) e(ω−λm )r cos θ dθ ds ≤ eωσ 2πi ′) s 2π(a − σ −π/2 CR = ′ cr eωσ π(a − σ′ ) Zπ/2 e(ω−λm )r sin θ dθ 0 10. The Zeta Function of Riemann (Contd) 84 2θ for 0 ≤ θ ≤ π/2; hence π a+iT Zπ/2 Z ′ ωs 2 e creωσ 1 e π (ω−λm )rθ dθ ds ≤ rm (s) 2πi ′ s π(a − σ ) a−iT 0 However, sin θ ≥ ′ creωσ ≤ , 2(a − σ′ )(λm − ω)r for all T . Hence a+iT Z ωs c1 e ds ≤ lim rm (s) T →∞ s (λm − ω) a−iT (C) 90 for all m ≥ mo . Now reverting to relation (A), we get a+iT a+iT Z Z ωs ωs 1 e 1 e (D) lim f (s) ds − fm (s) ds T →∞ 2πi s 2πi s a−iT a−iT a+iT Z ωs 1 e ds rm (s) = lim T →∞ 2πi s a−iT for every m. However, 1 lim T →∞ 2πi a+iT Z a−iT fm (s) X eωs ds = an s λ <ω independently of m. Hence1 1 We use the fact that if lim | f (T ) − g(T )| = α T →∞ and lim g(T ) = β, then T →∞ lim | f (T ) − β| ≤ α T →∞ n 2. (Contd). Elementary theory of Dirichlet series 85 a+iT Z ωs X 1 e lim ds − an ≤ left hand side in (D) f (s) T →∞ 2πi s λn <ω a−iT c1 for m > mo . ≤ λm − ω Letting m → ∞ we get the result. Remarks. (i) If ω = λn the last term in the sum 1 multiplied by . 2 91 P an has to be λn <ω (ii) If a < 0, (and a > σ0 ) then in the contour-integration the residue at the origin has to be taken, and this will contribute a term - f (0). In the proof, the relation between |s| and r has to be modified. Lecture 11 The Zeta Function of Riemann (Contd) 3 Analytic continuation of ζ(s). First method [16, p.18] 92 We have, for σ > 0, Γ(s) = Z∞ x s−1 e−x dx. 0 Writing nx for x, and summing over n, we get ∞ X Γ(s) n=1 ns ∞ = ∞ Z X n=1n=0 Z∞ X ∞ −nx = e x s−1 dx, if σ > 1. 0 since x s−1 e−nx dx n=1 ∞ Z∞ ∞ Z∞ ∞ X X X Γ(σ) s−1 −nx σ−1 −nx < ∞, x e dx ≤ x e dx = σ n n=1 n=1 n=1 0 87 11. The Zeta Function of Riemann (Contd) 88 if σ > 1. Hence ∞ X Γ(s) n=1 ns = Z∞ 0 e−x s−1 x dx = 1 − e−x Z∞ 0 x s−1 dx ex − 1 or Γ(s)ζ(s) = Z∞ 0 x s−1 dx, σ > 1 ex − 1 In order to continue ζ(s) analytically all over the s-plane, consider the complex integral Z s−1 z dz I(s) = e−1 C 93 where C is a contour consisting of the real axis from +∞ to ρ, 0 < ρ < 2π, the circle |z| = ρ; and the real axis from ρ to ∞. I(s), if convergent, is independent of ρ, by Cauchy′ s theorem. Now, on the circle |z| = ρ, we have |z s−1 | = |e(s−1) log z | = |e{(σ−1)+it}{log |z|+i arg z} | = e(σ−1) log |z|−t arg z = |z|σ−1 e2π|t| , while |ez − 1| > A|z|; Hence, for fixed s, Z 2πρ · ρσ−1 2π|t| | |≤ ·e → 0 as ρ → 0, if σ > 1. Aρ |z|=ρ Thus, on letting ρ → 0, we get, if σ > 1, I(s) = − Z∞ 0 x s−1 dx + ex − 1 Z∞ 0 (xe2πi ) s−1 dx ex − 1 3. Analytic continuation of ζ(s). First method 89 = −Γ(s)ζ(s) + e2πis Γ(s)ζ(s) = Γ(s)ζ(s)(e2πs − 1). Using the result Γ(s)Γ(1 − s) = π sin πs we get 94 e2πis −1 ζ(s) · 2πi. πis Γ(1 − s) e − e−πis ζ(s) = · 2πi · eπis , Γ(1 − s) I(s) = or e−iπs Γ(1 − s) ζ(s) = 2πi Z C z s−1 dz , σ > 1. ez − 1 The integral on the right is uniformly convergent in any finite region of the s-plane (by obvious majorization of the integrand), and so defines an entire function. Hence the above formula, proved first for σ > 1, defines ζ(s), as a meromorphic function, all over the s-plane. This only possible poles are the poles of Γ(1 − s), namely s = 1, 2, 3, . . .. We know that ζ(s) is regular for s = 2, 3, . . . (As a matter of fact, I(s) vanishes at these points). Hence the only possible pole is at s = 1. Hence Z dz I(1) = = 2πi, z e −1 C while 1 + ··· s−1 Hence the residue of ζ(s) at s = 1 is 1. We see in passing, since Γ(1 − s) = − that 1 1 1 z z3 = − + B − B + ··· 1 2 ez − 1 z 2 2! 4! 1 ζ(0) = − , ζ(−2m) = 0, ζ(1 − 2m) = 2 (−1)m Bm 2m , m = 1, 2, 3, . . . 95 11. The Zeta Function of Riemann (Contd) 90 4 Functional Equation (First method) [16, p.18] Consider the integral Z taken along Cn as in the diagram. z s−1 dz ez − 1 Between C and Cn , the integrand has poles at ±2iπ, . . . , ±2niπ. The residue at π 2mπi is (2mπe 2 i ) s−1 while the residue at −2mπi is (2mπe3/2πi ) s−1 ; taken together they amount to h πi i πi (2mπ)eπi(s−1) e 2 (s − 1) + e− 2 (s−1) π = (2mπ) s−1 eπi(s−1) 2 cos (s − 1) 2 π s−1 πis = −2(2mπ) e sin s 2 4. Functional Equation (First method) 96 Hence I(s) = 91 n sin πs πis X z s−1 dz + 4πi e (2mπ) s−1 ez − 1 2 m=1 Z Cn by the theorem of residues. Now let σ < 0, and n → ∞. Then, on Cn , |z s−1 | = O(|z|σ−1 ) = O(nσ−1 ), and 1 = O(1), ez − 1 for |ez − 1|2 = |e x+iy − 1|2 = |e x (cos y + i sin y) − 1|2 = e2x − 2e x cos y + 1, which, on the vertical lines, is ≥ (e x − 1)2 and, on the horizontal lines, = (e x + 1)2 . (since cos y = −1 there). Also the length of the square-path is O(n). Hence the integral round the square → 0 as n → ∞. Hence πis sin πs I(s) = 4πie πis = 4πie 2 ∞ X (2mπ) s−1 m=1 πs · (2π) s−1 ζ(1 − s), if σ < 0. sin 2 or 97 ζ(s)Γ(s)(e2πis − 1) = (4πi)(2π) s−1 eπis sin = 2πieπis πs ζ(1 − s) 2 ζ(s) Γ(1 − s) Thus ζ(s) = Γ(1 − s)ζ(1 − s)2 s π s−1 sin πs , 2 11. The Zeta Function of Riemann (Contd) 92 for σ < 0, and hence, by analytic continuation, for all values of s (each side is regular except for poles!). This is the functional equation. Since √ x x + 1! π Γ Γ = x−1 Γ(x), 2 2 2 we get, on writing x = 1 − s, ! 1−s s √ −s 2 Γ Γ 1− = πΓ(1 − s); 2 2 also Γ Hence s s π Γ 1− = 2 2 sin πs 2 Γ(1 − s) = 2−s Γ Thus ! πs 1 − s s −1 √ π{sin }−1 Γ 2 2 2 π−s/2 Γ(s/2)ζ(s) = π− 98 (1−s) 2 Γ ! 1−s ζ(1 − s) 2 If 1 s(s − 1)π−s/2 Γ(s/2)ζ(s) 2 1 ≡ s(s − 1)η(s), 2 ξ(s) ≡ then η(s) = η(1 − s) and ξ(s) = ξ(1 − s). If ≡ (z) = ξ( 12 + iz), then ≡ (z) ≡ (−z). 5 Functional Equation (Second Method) [16, p.13] Consider the lemma given in Lecture 9, and write λn = n, an = 1, φ(x) = x−s in it. We then get X n≤x −s n =s ZX 1 [X] [x] dx + s , if X ≥ 1. X x s+1 5. Functional Equation (Second Method) s s −s = − s − 1 (s − 1)X s−1 ZX 93 1 X − [X] x − [x] dx + s−1 − s+1 Xs x X 1 Since 1 = 1/X σ−1 , and X − [X] ≤ 1/X σ , X s−1 Xs we deduce, on making X → ∞, s ζ(s) = −s s−1 Z∞ x − [x] dx, if σ > 1 x s+1 1 or ζ(s) = s Z∞ [x] − x + 1 2 x s+1 dx + 1 1 1 + , if σ > 1 s−1 2 1 5.1 Since [x] − x + is bounded, the integral on the right hand side 99 2 converges for σ > 0, and uniformly in any finite region to the right of σ = 0. Hence it represents an analytic function of s regular for σ > 0, and so provides the continuation of ζ(s) up to σ = 0, and s = 1 is clearly a simple pole with residue 1. For 0 < σ < 1, we have, however, Z1 [x] − x dx = − x s+1 0 x−s dx = 0 and s = 2 Z∞ 1 Hence Z1 dx 1 = s+1 2 x 1 , s−1 11. The Zeta Function of Riemann (Contd) 94 5.2 ζ(s) = s Z∞ [x] − x dx, x s+1 0<σ<1 0 We have seen that (5.1) gives the analytic continuation up to σ = 0. By refining the argument dealing with the integral on the right-hand side of (5.1) we can get the continuation all over the s-plane. For, if 1 f (x) ≡ [x] − x + , 2 f1 (x) ≡ Zx f (y)dy, 1 then f1 (x) is also bounded, since n+1 R f (y)dy = 0 for any integer n. n 100 Hence Zx2 x1 x2 Zx2 f1 (x) f (x) f1 (x) dx = s+1 + (s + 1) dx s+1 x x x s+2 x1 x1 → 0, as x1 → ∞, x2 → ∞, if σ > −1. Hence the integral in (5.1) converges for σ > −1. Further s Z1 [x] − x + x s+1 1 2 dx = 0 ζ(s) = s Z∞ 1 1 + , for σ < 0; s−1 2 [x] − x + 1 2 x s+1 dx, −1 < σ < 0 0 Now the function [x] − x + 1 2 has the Fourier expansion ∞ X sin 2nπx n=1 nπ (5.3) 5. Functional Equation (Second Method) 95 if x is not an integer. The series is boundedly convergent. If we substitute it in (5.3), we get ∞ sX1 ζ(s) = π n=1 n s = π ∞ X n=1 Z∞ sin 2nπx dx x s+1 0 (2nπ) s n Z∞ sin y dy y s+1 0 s sπ ζ(s) = (2π) s {−Γ(1 − s)} sin ζ(1 − s), π 2 5.4 If termwise integration is permitted, for −1 < σ < 0. The right 101 hand side is, however, analytic for all values of s such that σ < 0. Hence (5.4) provides the analytic continuation (not only for −1 < σ < 0) all over the s-plane. The term-wise integration preceding (5.4) is certainly justified over any finite range since the concerned series is boundedly convergent. We have therefore only to prove that ∞ Z ∞ X 1 sin 2nπx dx = 0, −1 < σ < 0 lim X→∞ n x s+1 n=1 X Now Z∞ X " #∞ Z∞ cos 2nπx s+1 sin 2nπx 2nπx dx = − dx − s+1 s+1 2nπ x 2nπx x s+2 X X ∞ ! Z 1 dx 1 =O + O n nX σ+1 xσ+2 X ! 1 =O nX σ+1 11. The Zeta Function of Riemann (Contd) 96 and hence ∞ Z ∞ X 1 sin 2nπx dx = 0, if − 1 < σ < 0 lim X→∞ n x s+1 n=1 X This completes the analytic continuation and the proof of the Functional equation by the second method. As a consequence of (5.1), we get ( lim ζ(s) − s→1 ) Z∞ [x] − x + 12 1 1 dx + = 2 s−1 2 x 1 = lim n→∞ Zn [x] − x dx + 1 x2 1 m+1 Z n−1 X dx − log n + 1 = lim m 2 n→∞ x m=1 m n−1 X 1 = lim + 1 − log n n→∞ m+1 m=1 =γ 102 Hence, near s = 1, we have ζ(s) = 1 + γ + O(|s − 1|) s−1 Lecture 12 The Zeta Function of Riemann (Contd) 6 Some estimates for ζ(s) [11, p.27] 103 In any fixed half-plane σ ≥ 1 + ε > 1, we know that ζ(s) is bounded, since |ζ(s)| ≤ ζ(σ) ≤ ζ(1 + ε). We shall now use the formulae of §5 to estimate |ζ(s)| for large t, where s = σ + it. Theorem. |ζ(s)| < A log t, |ζ(s)| < A(δ)t1−δ , σ ≥ 1, σ ≥ δ, t ≥ 2. t ≥ 1, if 0 < δ < 1. Proof. From (5.1) we get s ζ(s) = −s s−1 Z∞ x − [x] dx, x s+1 1 97 σ>0 12. The Zeta Function of Riemann (Contd) 98 Also from §5 of the 11th Lecture, ZX X 1 [X] [x] dx + s , if X ≥ 1, s , 1 =s s s+1 n X x n≤X 1 If σ > 0, t ≥ 1, X ≥ 1, we get ∞ Z X 1 x − [x] 1 X − [X] = −s ζ(s) − dx + + s s+1 s−1 n Xs x (s − 1)X n≤X X Hence Z∞ X 1 1 dx 1 + σ−1 + σ + |s| |ζ(s)| < σ n X tX xσ+1 n≤X X X 1 1 t 1 1 + + 1 + , since |s| < σ + t. < + nσ txσ−1 X σ σ Xσ n≤X 104 If σ ≥ 1, |ζ(s)| < X1 n≤X n + 1 1 1+t + + t X X ≤ (log X + 1) + 3 + t , since t ≥ 1, X Taking X = t, we get the first result. If σ ≥ η, where 0 < η < 1, ! X 1 1 1 1 + 2+ |ζ(s)| < + nη tX η−1 η xη n≤X < Z[X] 3t dx X 1−η + + xη t ηX η 0 ≤ 3t X 1−η + X 1−η + 1−η ηX η X ≥ 1. 7. Functional Equation (Third Method) 99 Taking X = t, we deduce |ζ(s)| < t 1−η ! 3 1 +1+ , 1−η η σ ≥ η, t ≥ 1. 7 Functional Equation (Third Method) [16, p.21] The third method is based on the ‘theta-relation’ ! 1 1 ϑ(x) = √ ϑ , x x where ϑ(x) = ∞ X 2 e−πn x , Re x > 0 n=−∞ This relation can be proved directly, or obtained as a special case of 105 ‘Poisson’s formula’. We shall here give a proof of that formula [2, p.37] Let f (x) be continuous in (−∞, ∞). Let φ(α) = Z∞ 2πiαx f (x)e dx ≡ lim T →∞ −∞ ZT f (x)e2πiαx dx, −T if the integral exists. Then, for α and pro-positive integers, we have 1 p+ 2 Z −p− 12 1 Z2 p 2πiαx X 2πiαx e dx. f (x + k) f (x)e dx = − 12 −p If we assume that lim p→∞ p X −p f (x + k) = g(x) (7.1) 12. The Zeta Function of Riemann (Contd) 100 uniformly in − 12 ≤ x ≤ 21 , then g(x) is continuous, and on letting p → ∞ in (7.1), we get 1 Z2 φ(α) = g(x)e2πiαx dx. − 21 Thus φ(α) is the Fourier coefficient of the continuous periodic function g(x). Hence, by Fejer’s theorem, X g(o) = φ(α) (C,1) If we assume, however, that −∞ Hence lim p→∞ 106 ∞ P or φ(α) < ∞, then p X f (k) = lim ∞ X f (k) = p→∞ −p ∞ X p X P (C,1) φ(α) = ∞ P φ(α) −∞ φ(α) −p (7.2) φ(α) −∞ −∞ This is Poisson’s formula. We may summarize our result as follows. Poisson’s Formula. If (i) f (x) is continuous in (−∞, ∞), (ii) ∞ P −∞ (iii) ∞ P f (x + k) converges uniformly in − 21 ≤ x < 1 2 and φ(α) converges, −∞ then ∞ X −∞ f (k) = ∞ X φ(α) −∞ Remarks . This result can be improved by a relaxation of the hypotheses. 7. Functional Equation (Third Method) 101 2 The Theta Relation. If we take f (x) = e−πx t , t > 0, in the above discussion, we obtain the required relation. However, we have to show that for this function the conditions of Poisson’s formula are satisfied. This is easily done. f (x) is obviously continuous in (−∞, ∞). Secondly 2 e−π(x+k) t ≤ e|k|t for |k| ≥ k0 (t) This proves the uniform convergence of ∞ X 2 e−π(x+k) t , k=−∞ t > 0. − 1 1 ≤x< 2 2 Thirdly we show that, for t > 0 φ(α) ≡ Z∞ 2 πt+2παyi e−y −∞ For φ(α) = e− πα2 t Z∞ −∞ dy = 1 t1/2 2 /t e−πα 107 α 2 e−πt y − i dy, and t If α ≷ 0, we consider the contour integral Z 2 e−πts ds, s = σ + iτ C taken over C as indicated. Then on the vertical lines, we have 12. The Zeta Function of Riemann (Contd) 102 2 2 −τ2 ) e−πt Re(±σ+τi) = e−πt(σ 2 −πt(σ2 − α2 ) ≤e t Letting σ → ∞, we thus see that the integrals along the vertical lines vanish. Hence we have, for all real α, Z∞ −πtσ2 e dσ = −∞ Z∞ α 2 e−πt(σ− t i) dσ −∞ Thus −πα2 /t φ(α) = e Z∞ e−πtσ dσ 1 √ t Z∞ −∞ −πα2 /t =e = 2 e−πα /t √ t 2 2 e−πu du −∞ 2 √ π Z∞ 2 −ν2 e e−πα /t 1 dv = √ t π 0 = 108 2 e−πα /t √ t Z∞ 1 e−z z− 2 dz 0 1 1 √ Γ( ) = π 2 2 e−πα /t √ t Hence we have the desired relation: ∞ X −∞ −πk2 t e ∞ 1 X −πk2 /t =√ e , for t > 0, t −∞ (7.3) or, writing ψ(t) = ∞ X 2 e−πk t , we get 1 ! ) ( 1 1 2ψ(t) + 1 = √ 2ψ +1 t t Remark. (7.3) holds for t complex, with Re(t) > 0. (7.4) 7. Functional Equation (Third Method) 103 Functional Equation (Third method). We have, for σ > 0, Γ s = 2 Z∞ e−x x s/2−1 dx. 0 If σ > 0, n > 0, we then have on writing πn2 x for x, Γ s 2 = Z∞ s 2 e−πn x (πn2 x) 2 −1 πn2 dx 0 =π s/2 s n Z∞ e−πn 2 dx x s/2−1 dx 0 or Z∞ 1 π s/2 = n s Γ(s/2) 2 e−πn x x s/2−1 dx. 0 Now if σ > 1, we have 109 ∞ ∞ Z ∞ X 2 π s/2 X 1 = ζ(s) = e−πn x x s/2−1 dx s n Γ(s/2) n=1 1 0 = π s/2 Γ(s/2) Z∞ X ∞ s/2−1 −πn2 x x dx e 0 1 the inversion being justified by absolute convergence. Hence, for σ > 1, we have Z∞ π s/2 ζ(s) = ψ(x)x s/2−1 dx. Γ(s/2) 0 Using (7.4) we rewrite this as −s/2 π Γ(s/2)ζ(s) = Z1 0 x s/2−1 ψ(x)dx + Z∞ 1 ψ(x)x s/2−1 dx 12. The Zeta Function of Riemann (Contd) 104 = Z1 x s/2−1 0 = = 110 ( ! ) Z∞ 1 1 1 1 √ ψ + √ − dx + ψ(x)x s/2−1 dx 2 x 2 x x 1 1 1 − + s−1 s 1 + s(s − 1) Z1 0 Z∞ 1 x s/2−3/2 ψ Z∞ ! 1 dx + x 1 1 x−s/2− 2 + x s/2−1 ψ(x)dx, (7.5) for σ > 1. Now the integral on the right converges uniformly in a ≤ s ≤ b, for if x ≥ 1, we have −s/2−1/2 x + x s/2−1 ≤ xb/2−1 + x−a/2−1/2 while ψ(x) < ∞ X e−πnx = 1 1 , −1 eπx and hence the integral on the right hand side of (7.5) is an entire function. Hence (7.5) provides the analytic continuation to the left of σ = 1. It also yields the functional equation directly. We have also deduced that π−s/2 Γ(s/2)ζ(s) − 1 s(s − 1) is an entire function; so is π s/2 {Γ(s/2)}−1 . Hence ζ(s) − 1 π s/2 1 π s/2 · = ζ(s) − · s(s − 1) Γ(s/2) s − 1 2Γ(s/2 + 1) is an entire function. But entire function. π1/2 1 = 1. Hence ζ(s) − is an 2Γ(1/2 + 1) s−1 Lecture 13 The Zeta Function of Riemann (Contd) 8 The zeros of ζ(s) 111 In the 11th Lecture, (p.98) we defined ξ(s) ≡ 1 1 s(s − 1)π−s/2 Γ(s/2)ζ(s) ≡ s(s − 1)η(s). 2 2 The following theorem about ξ(s) is a consequence of the results which we have already proved. Theorem 1. [11, p.45] (i) ξ(s) is an entire function, and ξ(s) = ξ(1 − s); (ii) ξ(s) is real on t = 0 and σ = 12 ; (iii) ξ(0) = ξ(1) = 12 . Proof. That ξ(s) = ξ(1 − s) is immediate from the functional equation of ζ(s) (cf. p.97, Lecture 11) Clearly ξ(s) is regular for σ > 0, and since ξ(s) = ξ(1 − s) it is also regular for σ < 1, and hence it is entire. 105 13. The Zeta Function of Riemann (Contd) 106 This proves (i) ξ(s) is obviously real for real s. Hence by a general theorem it takes conjugate values at conjugate points. Thus ξ( 21 + ti) and ξ( 12 − ti) are conjugate; they are equal by the functional equation. So they are real. This proves (ii). To prove (iii) we observe that −s/2 ξ(s) = π Γ s 2 + 1 · (s − 1)ζ(s), so that 1 ξ(1) = π−1/2 Γ(3/2) · 1 = , 2 and by the functional equation, ξ(0) = 21 . 112 We shall next examine the location of the zeros of ξ(s) and of ζ(s). Theorem 2. [11, p.48] (i) The zeros of ξ(s) (if any !) are all situated in the strip 0 ≤ σ ≤ 1, and lie symmetrical about the lines t = 0 and σ = 21 (ii) The zeros of ζ(s) are identical (in position and order of multiplicity) with those of ξ(s), except that ζ(s) has a simple zero at each of the points s = −2, −4. − 6, . . . (iii) ξ(s) has no zeros on the real axis. Proof. (i) ξ(s) = (s − 1)π−s/2 Γ s 2 + 1 ζ(s) ≡ h(s)ζ(s), say. Now ζ(s) , 0; for σ > 1; (Euler Product!) also h(s) , 0, for σ > 1; hence ξ(s) , 0, for σ > 1; hence ξ(s) , 0, for σ < 0; since ξ(s) = ξ(1 − s). 8. The zeros of ζ(s) 107 The zeros, if any, are symmetrical about the real axis since ξ(σ ± ti) are conjugates, and about the point s = 21 , since ξ(s) = ξ(1 − s); they are therefore also symmetrical about the line σ = 12 . (ii) The zeros of ζ(s) differ from those of ξ(s) only in so far as h(s) has zeros or poles. The only zero of h(s) is at s = 1. But this is not a zero of ξ(s) since ξ(1) = 12 , nor of ζ(s) for it is a pole of the latter. The poles of h(s) are simple ones at s = −2, −4, −6, . . .. Since these are points at which ξ(s) is regular and not zero, they must be simple zeros 113 of ζ(s). We have already seen this by a different argument on p.95. (iii) Since ξ(s) , 0 for σ < 0 and σ > 1, it is enough, in view of (ii), to show that ζ(σ) , 0, for 0 < σ < 1. Now (1 − 21−s )ζ(s) = (1 − 2−s ) + (3−s − 4−s ) + · · · , for σ > 0. To prove this we first notice that the relation is obvious for σ > 1, and secondly each side is regular for σ > 0; the left side is obviously regular for σ > 0 (in fact it is entire); and, as for the right side, we have Z2n 1 dx 1 s = − (2n − 1) s (2n) s s+1 x 2n−1 13. The Zeta Function of Riemann (Contd) 108 ≤ |s| ∆ < σ+1 (2n − 1) (2n − 1)δ+1 if σ > δ and |s| < ∆ for any fixed δ and ∆ But, if 0 < σ < 1, the above relation gives (1 − 21−σ )ζ(σ) > 0, or ζ(σ) < 0. This establishes (iii). 114 Remarks . The strip 0 ≤ σ ≤ 1 is called the ‘critical strip’; the line σ = 12 the ‘critical line’; the zeros at −2, −4, −6, . . . are the ‘trivial zeros’ of ζ(s). We still have to show that ξ(s) actually has zeros, i.e. ζ(s) has ‘non-trivial’ zeros. This is done by an appeal to the theory of entire functions gives in the first few lectures. Theorem 3. [11, p.56] If M(r) ≡ max |ξ(s)|, then |s|=r 1 log M(r) ∼ r log r, as r → ∞ 2 Proof. For σ ≥ 2, we have |ζ(s)| ≤ ζ(2), and for σ ≥ 12 , |t| ≥ 1, we have |ζ(s)| < c1 |t|1/2 , so that 1 |ζ(s)| < c2 |s|1/2 , for σ ≥ , |s| > 3. 2 Applying Stirlingl’s formula to Γ(s/2), we get, for 1 σ ≥ , |s| = r > 3, 2 1 1 |ξ(s)| < e| 2 s log 2 s|+c3 |s| 1 < e 2 r log r+c4 r , 8. The zeros of ζ(s) 109 s since log = log |s| − log 2 + i arg s, | arg s| < 2 ξ(s) = ξ(1 − s), we infer that π 2. From the equation 1 |ξ(s)| < e 2 |1−s| log |1−s|+c4 |1−s| 1 < e 2 r log r+c5 r for σ ≤ 12 , |s| = r > 4. Combining the results we get 1 M(r) < e 2 r log r+c6 r , r > 4. On the other hand, if r > 2, 115 ! 1 1 r e 2 r log r−c7 r 2 1 M(r) ≥ ξ(r) > 1.π− 2 r Γ Thus we have, for r > 4, 1 1 r log r − C7 r < log M(r) < r log r + c6 r, 2 2 and hence the result. Theorem 4. [11, p.57] (i) ξ(s) has an infinity of zeros; (ii) If they are denoted by ‘ρ’, then verges for α ≤ 1; P |ρ|−α converges for α > 1, di- ( ! ) s s/ρ 1− e , ρ (iii) b0 +b1 s ξ(s) = e πρ where b0 , b1 are constants; ! P 1 1 ξ′ (s) = b1 + + (iv) ξ(s) s−ρ ρ ! P 1 ′ s ζ ′ (s) 1 1 1Γ (v) =b− − +1 + + , ζ(s) s−1 2 Γ 2 ρ ρ s−ρ 13. The Zeta Function of Riemann (Contd) 110 where b = b1 + 21 log 2π. Proof. ξ(0) = 12 , 0, and we apply the theory of entire functions as developed in the earlier lectures. By Theorem 3, ξ(s) is of order 1, and the relation log M(r) = O(r) does not hold. Hence ρ1 = 1, ξ(s) has P 1 diverges (by a previous theorem). This an infinity of zeros and |ρ| proves (i), (ii) and (iii). (iv) follows by logarithmic differentiation. (v) is obtained from ξ(s) = (s − 1)π−s/2 Γ( 2s + 1)ζ(s). We shall now show that ζ(s) has no zeros on the line σ = 1. Theorem 5. [11, p.28] ζ(1 + it) , 0. 116 First Proof. 2(1 + cos θt)2 = 3 + 4 cos θ + cos 2θ ≥ 0 for real θ. Since XX 1 log ζ(s) = , for σ > 1, mpms m p we have log |ζ(s)| = Re = ∞ X ∞ X cn n−σ−ti n=2 cn n−σ cos(t log n), n=2 1/m if n is the mth power of a prime where cn = 0 otherwise. Hence log ζ 3 (σ) · ζ(σ + ti)ζ(σ + 2ti) X = cn n−σ 3 + 4 cos(t log n) + cos(2t log n) ≥ 0, because cn ≥ 0 and we have the trigonometric identity above. Thus 4 1 3 ζ(σ + ti) |ζ(σ + 2ti)| ≥ , {(σ − 1)ζ(σ)} σ−1 σ−1 8. The zeros of ζ(s) 111 if σ > 1. Now suppose 1 + ti(t ≷ 0) were a zero of ζ(s); then, on letting σ → 1 + 0, we see that the left hand side in the above inequality would tend to a finite limit, viz. |ζ ′ (1 + ti)|4 |ζ(1 + 2ti)|, while the right hand side 117 tends to ∞. Hence ζ(1 + it) , 0. Second Proof. [11, p.89] We know from the 8th Lecture (1.12) that if α is real, and α , 0, then f (s) ≡ ∞ ζ 2 (s)ζ(s − αi)ζ(s + αi) X |σαi (n)|2 = ,σ > 1 s ζ(2s) n n=1 (8.1) Let σ0 be the abscissa of convergence of the series on the right hand side. Then σ0 ≤ 1. The sum-function of the series is then regular in the half-plane σ > σ0 , and hence, by analytic continuation, (8.1) can be upheld for σ > σ0 . And since the coefficients of the series are positive, the point s = σ0 is a singularity of f (s). Now, if 1 + αi is a zero of ζ(s), then so is (1 − αi), and these two zeros cancel the double pole of ξ2 (s) at s = 1. Hence f (s) is regular on the real axis, as far to the left as s = −1, where ζ(2s) = 0. Hence σ0 = −1. This is, however, impossible since (8.1) gives ! 1 ≥ |σαi (1)|2 = 1, f 2 while f ( 21 ) = 0. Thus ζ(1 + αi) , 0. Remarks. (i) We shall show later on that this fact (ζ(1 + it) , 0) is equivalent to the Prime Number Theorem. (ii) If ρ = β + γi is a zero of ξ(s), then we have seen that 0 ≤ β ≤ 1, and since ζ(1 + it) , 0, we actually have 0 ≤ β < 1, and by symmetry about the line σ = 21 , we have 0 < β < 1. Lecture 14 The Zeta Function of Riemann (Contd) 9 Riemann-Von Magoldt Formula [11, p.68] Let N(T ) denote the number of zeros (necessarily finite) of ζ(s) in 0 ≤ 118 σ ≤ 1, 0 ≤ t ≤ T . Then, by what we have proved, N(T ) is the number of zeros ρ = β + iγ of ζ(s), or of ξ(s), for which 0 < γ ≤ T Theorem 1. N(T ) = T T T log − + O(log T ) as T → ∞. 2n 2π 2π Proof. Suppose first that T is not equal to any γ. Also let T > 3. Consider the rectangle R as indicated. ξ(s) has 2N(T ) zeros inside it, and none on the boundary. Hence, by the principle of the argument, 2N(T ) = 1 [arg ξ(s)]R , 2π where [arg ξ(s)]R denotes the increase in arg ξ(s), as s describes the boundary of R. 113 14. The Zeta Function of Riemann (Contd) 114 Now 1 [arg ξ(s)]R = [arg s(s − 1)]R + [arg η(s)]R , 2 where η(s) = π−s/2 Γ(s/2)ζ(s). Here 1 [arg s(s − 1)]R = 4π, 2 119 and η(s) has the properties: η(s) = η(1 − s), and η(σ ± ti) are conjugates. Hence [arg η(s)]R = 4[arg η(s)]ABC Hence πN(T ) = π + arg[π−s/2 ] + [arg Γ(s/2)]ABC + [arg ζ(s)]ABC (9.1) Now t T = − log π. [arg π−s/2 ]ABC = − log π 2 2 ABC (9.2) Next, since Γ(z+α) = (z+α− 12 ) log z−z+ 12 log 2π+O(|z|−1 ) as |z| → ∞, in any angle | arg z| ≤ π − ε < π, we have 9. Riemann-Von Magoldt Formula 115 !# " 1 = im log Γ(s/2) ABC arg Γ 2 ABC ! 1 1 = im log Γ + iT − im log Γ(1) 4 2 ( ! ! ) 1 1 1 1 1 −1 = im − + iT log iT − iT + log 2π + O(T ) 4 2 2 2 2 ! 1 1 T 1 = T log T − π − + O T −1 , as T → ∞ (9.3) 2 2 8 2 Using (9.2) and (9.3) in (9.1), we get T T T 7 1 1 N(T ) = log − + + [arg ζ(s)]ABC + 0 2π 2π 2π 8 π T ! (9.4) Consider the broken line ABC exclusive of the end-points A and C. If m is the number of distinct points s′ on ABC at which Re ζ(s) = 0, then [arg ζ(s)]ABC ≤ (m + 1)π, (9.5) since arg ζ(s) cannot vary by more than π (since Re ζ does not change 120 sign here) on any one of the m + 1 segments into which ABC is divided by the point s′ Now no point s′ can be on AB, for ∞ Z ∞ X 1 1 du 1 Re ζ(2 + iT ) ≥ 1 − > 1 − − = 2 2 2 4 n 2 u 2 (9.6) 2 Thus m is the number of distinct points σ of 12 < σ < 2 at which Re ζ(σ + iT ) = 0, i.e. the number of distinct zeros of 1 g(s) = {ζ(s + iT ) + ζ(s − iT )} 2 on the real axis for which 12 < σ < 2, because g(σ) = Re ζ(σ + iT ) for real σ, since ζ(σ ± iT ) are conjugate. 14. The Zeta Function of Riemann (Contd) 116 Now since g(s) is regular except for s = 1 ± iT , m must be finite, and we can get an upper bound for m by using a theorem proved earlier. 3 7 Consider the two circles: |s − 2| ≤ , |s − 2| ≤ . Since T > 3, g(s) 4 2 is regular in the larger circle. At all points s of this circle, we have 1 σ≥ , 4 1 < |t ± T | < 2 + T. Hence, by an appeal to the other of ζ(s) obtained in the 12th Lecture (with δ = 14 ), we get 1 |g(s)| < c1 (|t + T |3/4 + |t − T |3/4 ) 2 < c1 (T + 2)3/4 , on the larger circle. At the centre, we have g(2) = Re ζ(2 + iT ) > 121 1 by (9.6) 4 Hence, by using the theorem (given in the Appendix), we get !m c1 (T + 2)3/4 7 < T, for T > T 0 ≥ 3. < 1 6 4 Thus m < c2 log T, for T > T 0 . Substituting this into (9.5) and (9.4) we get N(T ) − T log T + T ≤ c log T, 3 2π 2π 2π T > T0, provided that T , γ for any ‘γ’. The last restriction may be removed by first taking T ′ larger than T and distinct from the γ′ s and then letting T ′ → T + 0. Remarks . The above theorem was stated by Riemann but proved by Von Mangoldt in 1894. The proof given here is due to Backlund (1914). 9. Riemann-Von Magoldt Formula 117 Corollary 1. If h > 0 (fixed), then N(T + h) − N(T ) = O(log T ), as T → ∞ Proof. If we write f (t) = t t t log − , 2π 2π 2π we get f (t + h) − f (t) = h f ′ (t + θh), 0 < θ < 1, where f ′ (t) = t 1 log . Now use the Theorem. 2π 2π Corollary 2. ! X 1 X 1 log T 2 ′ =O = O(log T ); S ∃ S ≡ γ T γ2 γ>T 0≤γ≤T (summed over all zeros ρ whose imaginary parts γ satisfy the given conditions). Let 122 X1 , m < γ ≤ m + 1, and sm = γ X 1 , m < γ ≤ m + 1. s′m = γ2 Then S ≤ [T ] X sm , m=0 ′ S ≤ ∞ X s′m m=[T ] If m ≥ 1, the number of terms in sm (or s′m ) is N(m + 1) − N(m) = νm , say. By Corollary 1, νm = O(log m) as m → ∞; and sm ≤ νm , m sm ≤ νm m2 14. The Zeta Function of Riemann (Contd) 118 Hence, as T → ∞, [T ] X log m = O(log2 T ) S = O(1) + O m 2 ∞ ! X log m log T ′ = O S = O T m2 [T ] Corollary 3. If the zeros ‘ρ’ for which γ > 0 are arranged as a sequence ρn = βn + iγn , so that γn+1 ≥ γn , then |ρn | ∼ γn ∼ 2πn , as n → ∞ log n Proof. Since N(γn − 1) < n ≤ N(γn + 1), and 2πN(γn ± 1) ∼ (γn ± 1) log(γn ± 1) ∼ γn log γn , 123 we have first 2πn ∼ γn log γn whence log n ∼ log γn , and 2πn 2πn ∼ log γn log n γn ≤ |ρn | < γn + 1. γn ∼ And Remarks. (i) The main theorem proves incidentally the existence of an infinity of complex zeros of ζ(s), without the use of the theory of entire functions. (ii) We see from corollary 3 that X 1 |ρ|(log |ρ|)α converges for α > 2 and diverges for α ≤ 2. 9. Riemann-Von Magoldt Formula 119 (iii) Corollary 1 may be obtained directly by applying the theorem (on the number of zeros) to ζ(s) and to two circles with centre at c + iT and passing through 12 + (T + 2h)i, 12 + (T + h)i respectively, where c = c(h) is sufficiently large, and using the symmetry about σ = 1/2 (iv) If N0 (T ) denotes the number of complex zeros of ζ(s) with real part 21 and imaginary part between 0 and T , then Hardy and Littlewood proved that N0 (T ) > cT in comparison with N(T ) ∼ 1 T log A. Selberg has shown, however, that N0 (T ) > cT log T . 2π Appendix Theorem. Let f (z) be regular in |z − z0 | ≤ R and have n zeros (at least) 124 in |z − z0 | ≤ r < R. Then, if f (z0 ) , 0. R n M , ≤ r | f (z0 )| where M = max | f (z)| |z−z0 |=R Proof. Multiple zeros are counted according to multiplicity. Suppose z0 = 0 (for otherwise put z = z0 + z′ ). Let a1 , . . . an be the zeros of f (z) in |z| ≤ r. Then n Y R(z − aν ) f (z) = ϕ(z) R2 − λ̄ν z ν=1 where aν , aν are conjugates and ϕ is regular in |z| ≤ R. On |z| = R, each factor has modulus 1; hence |ϕ(z)| = | f (z)| ≤ M on |z| = R Since ϕ is regular in |z| ≤ R, we have |ϕ(0)| ≤ M Hence result. | f (0)| = |ϕ(0)| n n |aν | Q ≤ M Rr and f (0) , 0, hence the ν=1 R 120 14. The Zeta Function of Riemann (Contd) Theorem. If f is analytic inside and on C and N is the number of zero inside C, then Z ′ 1 f (z) dz = N 2πi f (z) C = ∆c log{ f (z)} so that N= 1 ∆c arg f (z). 2π Lecture 15 The Zeta Function of Riemann (Contd) 10 Hardy’s Theorem [16, p.214] We have proved that ζ(s) has an infinity of complex zeros in o < σ < 1. 125 Riemann conjectured that all these zeros lie on the line σ = 21 . Though this conjecture is yet to be proved, Hardy showed in 1914 that an infinity of these zeros do lie on the ‘critical’ line. We shall prove this result. In obtaining the functional equation by the third method, we have used the formula: Z∞ s 1 −s/2 π Γ(s/2)ζ(s) = + ψ(x)(x 2 −1 + x−s/2−1/2 )dx, s(s − 1) 1 where ψ(x) = x= 1 2 ∞ P e−n 2 πx , x > 0. Multiplying by n=1 1 s(s − 1), and writing 2 + it, we get ! ! ! Z∞ 1 1 1 1 2 −3/4 ζ + it =≡ (t) = − t + ψ(x)x cos t log x dx 2 2 4 2 1 It is a question of showing that ≡ (t), which is an even, entire function of t, real for real t, has an infinity of real zeros. 121 15. The Zeta Function of Riemann (Contd) 122 Writing x = e4u , we get 1 1 ≡ (t) = − 4 t2 + 2 4 ! Z∞ ψ(04u )eu cos(2ut)du. 0 If we write ψ(u) = ψ(e4u )eu , 126 we obtain 1 = − (t2 + 1) ≡ 2 2 t Z∞ φ(u) cos ut du 0 We wish now to get rid of the factor + 1) and the additive constant 12 so as to obtain ≡ (t/2) as a cosine transform of φ. This we can achieve by two integrations (by parts). However, to get rid of the extra term arising out of partial integration we need to know φ′ (0). We shall show that φ′ (0) = − 21 . For, by the functional equation of the theta-function, !# " 1 1 1 + 2ψ(x) = √ 1 + 2ψ x x (t2 or 1 + 2ψ(e4u ) = e−2u [1 + 2ψ(e−4u )] or eu + 2eu ψ(e4u ) = e−u + 2e−u ψ(e−4u ) or so that eu + 2φ(u) = e−u + 2φ(−u) d u e + 2φ(u) u=0 = 0 du i.e. 1 φ′ (0) = − . 2 We also know that ψ(x) = O(e−πx ) as x → ∞. Hence t 2 Z∞ 0 1 φ(u) cos ut du = − 2 Z∞ 0 φ′′ (u) cos ut du 10. Hardy’s Theorem 127 123 Hence ≡ (t/2) = Z∞ [φ′′ (u) − φ(u)] cos ut du (10.1) 0 By actual computation it may be verified that φ′′ (t) − φ(t) = 4[6e5t ψ′ (e4t ) + 4e9t ψ′′ (e4t )] Again if we write 1 1 φ(u) = eu ψ(e4u ) + eu = φ(u) + eu 2 2 1 u 4u = e ϑ(e ), 2 then by the theta relation, we have Φ(u) = Φ(−u), and Φ′′ (u) − Φ(u) = φ′′ (u) − φ(u) Let us now write (10.1) in the form ≡ (t) = 2 Z∞ f (u) cos ut du Z∞ ≡ (t) cos ut dt, 0 We wish to deduce that 1 f (u) = π (10.2) 0 by Fourier’s integral theorem. We need to establish this result. Fourier Inversion Formula.[5, p.10] If f (x) is absolutely integrable in (−∞, ∞), then Z∞ φ(α) ≡ f (x)eiαx dx −∞ 15. The Zeta Function of Riemann (Contd) 124 exists for every real α, −∞ < α < ∞, is continuous and bounded in (−∞, ∞). We wish to find out when 1 f (x) = 2π Z∞ φ(α)e−iαx dα −∞ 128 for a given x. The conditions will bear on the behaviour of f in a neighbourhood of x. If 1 S R (x) = 2πi ZR e−iαx φ(α)dα −R = = 1 π 2 π Z∞ −∞ Z∞ sin Rt f (x + t) dt t sin Rt f (x + t) + f (x − t) dt, t 2 0 and g x (t) = then 1 f (x + t) + f (x − t) − f (x), 2 Z∞ sin Rt g x (t) dt t 0 ε Z Z∞ 2 = + = I1 + I2 , say, π 2 S R (x) − f (x) = π 0 ǫ for a fixed ǫ > 0. g x (t) I2 → 0 as R → ∞, by the Riemann-Lebesgue Lemma. So, if t is absolutely integrable in (0, ε), then I1 → 0 as ε → 0. Hence we have the 10. Hardy’s Theorem 125 Theorem . [5, p.10] If lim S R (x) = f (x). g x (t) is absolutely integrable in (0, ε), then t R→∞ If, in particular, f is absolutely integrable in (−∞, ∞) and differen- 129 tiable in (−∞, ∞) then lim S R (x) = f (x) for every x in (−∞, ∞). It R→∞ should be noted that sufficient conditions for the validity of the theorem are: (i) f (x) is of bounded variation in a neighbourhood of x, and (ii) f (x) is absolutely integrable in (−∞, ∞). Then lim S R (x) = R→∞ 1 2 [ f (x + 0) + f (x − 0)]. We now return to (10.2) which is an immediate deduction from the formula for ≡ (t), on using Fourier’s inversion formula. π Now we know that ≡ (t) = ξ( 12 + it) = O(tε1 e− 4 t ); and ≡ (t) is an entire function of t. Hence we are justified in obtaining, by differentiation of (10.2), Z∞ (−1)n (2n) ≡ (t)t2n cos ut dt. f (u) = π 0 Since ψ(x) is regular for Re x > 0, f (u) is regular for −π/4 < Im u < (Note that x = e2u ). Let π 4 f (iu) = c0 + c1 u2 + c2 u4 + · · · Then 1 (−1)n f (2n) (0) = cn = (2n)! (2n)!π Z∞ ≡ (t)t2n dt 0 If ≡ (t) had only a finite number of zeros, then ≡ (t) would be of constant sign for t > T . Let ≡ (t) > 0 for t > T . Then cn > 0 for n > 2n0 , since Z∞ 0 ≡ (t)t 2n dt > T +2 Z ≡ (t)t 2n dt − T +1 > (T + 1) ZT | ≡ (t)|t2n dt 0 2n T +2 Z T +1 ≡ (t)dt − T 2n ZT 0 | ≡ (t)| dt 15. The Zeta Function of Riemann (Contd) 126 > 0 for n > 2n0 , say. 130 Hence f (n) (iu) increases steadily with u for n > 2n0 . However we πi along shall se that f (u), and all its derivatives, tend to zero as u → 4 the imaginary axis. We know that ! 1 1 1 1 −1/2 ψ(x) = x ψ + x− 2 − x 2 2 Further ψ(i + δ) = ∞ X e−n n=1 ∞ X =2 1 i.e. 1 2 2 (i+δ)π e−(2n) = 2 πδ ∞ X − (−1)n e−n n=1 ∞ X e−n 2 πδ 2 πδ 1 = 2ψ(4δ) − ψ(δ) ! ! 1 1 1 1 1 =√ ψ − ψ − δ δ 2 δ 4δ ! ! 1 1 1 1 1 + ψ(i + δ) = √ ψ −√ ψ 2 δ 4δ δ δ + ψ(x) → 0 as δ → 0, and so do its derivatives (by a similar πi argument). Hence 12 + ψ(u) → 0 as u → along the imaginary axis, 4 πi and so do its derivatives. Thus f (u) and all its derivatives → 0 as u − . 4 Thus Lecture 16 The Zeta Function of Riemann (Contd) Hamburger’s Theorem.[13] 131 We have seen that the functional equation of the Gamma function, together with its logarithmic convexity, determine the Gamma function ‘essentially’ uniquely (i.e. up to a constant). A corresponding result can be proved for a the zeta function. G(s) , where G(s) is an entire function of finite P(s) order and P(s) is a polynomial, and let Theorem 1. Let f (s) = f (s) = ∞ X an n=1 ns , the series on the right converging absolutely for σ > 1. Let ! s 1 s − (1−s) −s/2 π = g(1 − s)Γ − π 2 f (s)Γ 2 2 2 where g(1 − s) = ∞ X bn , n1−s n=1 127 (1.1) (1.2) (1.3) 16. The Zeta Function of Riemann (Contd) 128 The series on the right converging absolutely for σ < −α < 0. Then f (s) = a1 ζ(s)(= g(s)). For the proof we need to evaluate two integrals: −y e 1 = 2πi 1+∞i Z y−s Γ(s)ds, y>0 (1) 1−∞i Z∞ 2 −a2 x− bx e √ π −2ab dx √ = e , a x a > 0, b ≥ 0. (2) 0 132 The first formula is a classic example of Mellin’s inversion formula which can be obtained as an instance of Fourier’s inversion formula discussed in the last lecture. We have seen that if f (x) ∈ L1 (−∞, ∞), then its Fourier transform φ(α) is defined in −∞ < α < ∞, and if in a neighbourhood of x0 , f (x) is differentiable, then 1 f (x0 ) = 2π Z∞ −ix0 α e F (s) = f (y)eiαy dy. −∞ −∞ If we define dα Z∞ Z∞ f (x)x s−1 dx, (3) 0 for s = c + it, c > 0, where f (x)xc−1 ∈ L1 (0, ∞), so that the integral on the right exists absolutely, we can look upon this as a Fourier transform by a change of variable: x → ey , for F (c + it) = Z∞ f (ey )eyc eit y dy −∞ Hence, provided that f (ey )eyc satisfies a suitable ‘local’ condition, such as differentiability in the neighbourhood of a point, we can invert this 16. The Zeta Function of Riemann (Contd) 129 relation and obtain 1 f (e ) · e = 2π y yc or f (ey ) = = or f (x) = 1 2π Z∞ F (c + it)e−iyt dt −∞ Z∞ 133 F (c + it)e−(c+it)y dt −∞ c+i∞ Z 1 2πi 1 2πi F (s)e−ys ds c−i∞ c+i∞ Z F (s)x−s ds, c > 0. (4) c−i∞ Relations (3) and (4) give the Mellin inversion formulae. Since R∞ Γ(s) = e−x x s−1 dx, Re s > 0, we get (1) as in immediate application. 0 We know that, for k > 0 ZA e−(k−iα)x dx = 0 so that 2 Z∞ 1 1 − e−kA eiαA k − iα e−kx cos αxdx = 0 2.k k 2 + α2 and by Fourier’s inversion formula, Z∞ cos αx πe−kx dα = , 2k k 2 + α2 k>0 0 On the other hand, we have for k ≥ 0 Z∞ 2 2 Γ(1) = e−(x +k )y dy, x2 + k 2 0 (5) 16. The Zeta Function of Riemann (Contd) 130 134 so that Z∞ 0 √ Z∞ 2 π cos αx − 12 −(k2 y+ α4y ) dx = dy e y 2 x2 + k 2 0 π = e−|α|k , from (5). 2k Setting k2 = a2 , α2 = 4b2 , we get Z∞ √ π −2ab dx √ = e ,a > 0 b ≥ 0 a x 2 −a2 x− bx e 0 which proves formula (2). Proof of Theorem 1. For any x > 0, we have by (1.1) and (1.2), (Here f (s) = O(1)) 1 S1 ≡ 2πi 2+i∞ Z f (s)Γ (s) (−s/2) −s/2 π ·x ds 2 2−i∞ 2+i∞ Z ∞ X an = Γ(s/2)(πn2 x)−s/2 ds 2πi n=1 2−i∞ =2 ∞ X an e−πn 2x n=1 We have, however, by (1.2), S 1 = S 2 , where 1 S2 = 2πi 2+i∞ Z 2−i∞ 135 ! 1 − s −(1−s) −s/2 ds. π 2 x g(1 − s)Γ 2 Now we wish to move the line of integration here from σ = 2 to σ = −1 − α. By the hypothesis on the ‘order’ of f (s) and (1.2), it follows that there exist two numbers T > 0, γ > 0, such that for |t| ≥ T and −1 − α ≤ 16. The Zeta Function of Riemann (Contd) 131 γ σ ≤ 2, the function g(1 − s) is regular and O(e|t| ). By (1.3), we see that g(1 − s) = O(1) on σ = −1 − α; and, since f (s) = O(1) on σ = 2, while Γ(s/2) = O(|t|3/2 ), on σ = 2, Γ( 1−s ) 2 it follows that g(1 − s) = O(|t|3/2 ) on σ = 2. Hence, by the principle of Phragmen-Lindelöf, we observe that g(1 − s) = O(|t|3/2 ) for |t| ≥ T , −α − 1 ≤ σ ≤ 2. Taking a suitable rectangle, and applying Cauchy’s theorem, we get 1 S2 = 2πi −α−1+i∞ Z −α−1−i∞ ! m X 1 − s − (1−s) −s/2 2 x ds + Rν π g(1 − s)Γ 2 v=1 where Rν is the residue of the integrand at the pole sν lying in the region −α − 1 < σ < 2. The integrand, however, equals 136 16. The Zeta Function of Riemann (Contd) 132 f (s)Γ s 2 π−s/2 x−s/2 The residue of this at a pole sν of order qν is −sν (ν) (ν) qν −1 log x + · · · + A log x + A x 2 A(ν) qν −1 1 0 Hence m X Rν = ν=1 m X x−sν /2 Qν (log x) = Q(x), say, where ν=1 Qν is a polynomial Here Re sν ≤ 2 − θ, θ > 0. (i.e. we are using the absolute convergence P of an n−s only for σ > 2 − θ). Hence ∞ 1 X bn S2 = √ x n=1 2πi ∞ 2 X bn =√ x n=1 2πi −α−1+i∞ Z Γ(1 − s) πn2 2 x −α−1−i∞ α 2 +1+i∞ Z α 2 +1−i∞ πn2 Γ(s) x !−s !− (1−s) 2 ds + Q(x) ds + Q(x) ∞ 2 2 X =√ bn e−πn /x + Q(x) x n=1 137 Hence (since S 1 = S 2 ) we have 2 ∞ X an e−πn 1 2x ∞ 2 2 X bn e−πn /x + Q(x) =√ x n=1 2 Multiplying this by e−πt x , t > 0, and integrating over (0, ∞) w.r.t. x, we get Z∞ ∞ ∞ X X 2 bn −2πnt an e + Q(x)e−πt x dx =2 2 2 + n2 ) t π(t n=1 n=1 0 16. The Zeta Function of Riemann (Contd) 133 by (2). The last integral is convergent. Since Re sν ≤ 2 − θ, ν = 1, 2, . . . m, θ each term of Q(x) is O(x−1+ 4 ) as x → 0. Now Z∞ 0 −πt2 x Q(x)e 1 dx = 2 t Z∞ 0 Q x t2 e−πx dx = m X t sν −2 Hν (log t), 1 where Hν is a polynomial, = H(t), say. Hence ! ∞ ∞ X X 1 1 an − πtH(t) = 2π + bn e−2πnt t + ni t − ni n=1 n=1 The series on the left hand side is uniformly convergent in any finite region of the t-plane which excludes t = ±ki, k = 1, 2, . . . ; It is a meromorphic function with poles of the first order at t = ±ki. H(t) is regular and single-valued in the t-plane with the negative real 138 axis deleted and t , 0. The right hand side is a periodic function of t with period i for Re t > 0. Hence, by analytical continuation, so is the function on the left. Hence the residues at ki, (k + 1)i are equal. So ak = ak+1 Lecture 17 The Zeta Function of Riemann (Contd) 12 The Prime Number Theorem [11, pp.1-18] The number of primes is infinite. For consider any finite set of primes; 139 let P denote their product, and let Q = P + 1. Then (P, Q) = 1, since any common prime factor would divide Q − P, which would be impossible if (P, Q) , 1. But Q > 1, and so divisible by some prime. Hence there exists at least one prime distinct from those occurring in P. If there were only a finite number of primes, by taking P to be their product we would arrive at a contradiction. Actually we get a little more by this argument: if pn is the nth prime, the integer Qn = p1 . . . pn + 1 is divisible by some pm with m > n, so that pn+1 ≤ pm ≤ Qn n from which we get, by induction, pn < 22 . For if this inequality was true for n = 1, 2, . . . N, then N pN+1 ≤ p1 . . . pN + 1 < 22+4+···+2 + 1 < 22 and the inequality is known to be true for n = 1. 135 N+1 , 17. The Zeta Function of Riemann (Contd) 136 The fact that the number of primes is infinite is equivalent to the P statement that π(x) = 1 → ∞ as x → ∞. Actually far more is true; p≤x x n . Again the relation pn < 22 is far log x weaker than the asymptotic formula: pn ∼ n log n, which is know to be x (The Prime Number Theorem!). equivalent to the formula: π(x) ∼ log x We shall prove the Prime Number Theorem, and show that it is equivalent to the non-vanishing of the zeta function on the line σ = 1. We shall state a few preliminary results on primes. !−1 P1 1 Theorem 1. The series and the product π 1 − are divergent. p p !−1 Q P 1 1 , P(x) = , x > 2. 1− Proof. Let S (x) = p p≤x p≤x p Then, for 0 < u < 1, we shall show that π(x) ∼ 140 Hence 1 1 − um+1 > = 1 + u + · · · + um 1−u 1−u P(x) ≥ Y (1 + p−1 + · · · + p−m ), p≤x P1 summed n over a certain set of positive integers n, and if m is so chosen that 2m+1 > x, this set will certainly include all integers from 1 to [x]. Hence where m is any positive integer. The product on the right is P(x) > [x] X 1 1 141 n > we have du > log x. u 1 Since − log(1 − u) − u < [x]+1 Z 1 2 2u 1−u log P(x) − S (x) < X p≤x , for 0 < u < 1, − p−2 2(1 − p−1 ) (1) 12. The Prime Number Theorem 137 < ∞ X n=2 1 1 = 2n(n − 1) 2 Hence, by (1), 1 S (x) > log log x − . 2 (1) and (2) prove the theorem. (2) The Chebyschev Functions. Let X X log p, ψ(x) = log p, x > 0. ϑ(x) = p≤x pm ≤x Grouping together terms of ψ(x) for which m has the same value, we get ψ(x) = ϑ(x) + ϑ(x1/2 ) + ϑ(x1/3 ) + · · · , (3) this series having only a finite number of non-zero terms, since ϑ(x) = 0 if x < 2. Grouping together terms for which ‘p’ has the same value (≤ x), we obtain X " log x # log p, (4) ψ(x) = log p p≤x since the number of values of m associated with a given p is equal to the of positive integers m satisfying m log p ≤ x, and this is 142 # " number log x log p Theorem 2. The functions π(x) , x/ log x ϑ(x) , x ψ(x) x have the same limits of indetermination as x → ∞. Proof. Let the upper limits (may be ∞) be L1 , L2 , L3 and the lower limits be l1 , l2 , l3 , respectively. Then by (3) and (4), X log x log p = π(x) log x. ϑ(x) ≤ ψ(x) ≤ log p p≤x 17. The Zeta Function of Riemann (Contd) 138 Hence L2 ≤ L3 ≤ L1 . (5) On the other hand, if 0 < α < 1, x > 1, then X log p ≥ {π(x) − π(xα )} log xα ϑ(x) ≥ xα <p≤x and π(xα ) < xα , so that ϑ(x) π(x) log x log x ≥α − 1−α x x x 143 ! log x Keep α fixed, and let x → ∞; then 1−α → 0 x Hence L2 ≥ αL1 , i.e. L2 ≥ L1 , as α → 1 − 0. This combined with (5) gives L2 = L3 = L1 , and similarly for the l’s. π(x) ϑ(x) ψ(x) or or tends to a limit, then so do all, x/ log x x x and the limits are equal. log p, if n is a +ve power of a prime p Remarks. If ∧(n) = 0, otherwise, then X X ψ(x) = log p = ∧(n), and Corollary . If − ζ ′ (s) ζ(s) pm ≤x ∞ X = 1 Also ζ ′ (s) =s − ζ(s) n≤x ∧(n) , σ > 1 [p.69] ns Z∞ 1 ψ(x) dx, σ > 1. x s+1 12. The Prime Number Theorem 139 The Wiener-Ikehara theorem. [3, 4] Let A(u) be a non-negative nondecreasing function defined for 0 ≤ u < ∞. Let f (s) ≡ Z∞ A(u)e−us du, s = σ + iτ, 0 converge for σ > 1, and be analytic for σ ≥ 1 except at s = 1, where it 144 has a simple pole with residue 1. Then e−u A(u) → 1 as u → ∞ Proof. If σ > 1, 1 = s−1 Z∞ e−(s−1)u du 0 Therefore 1 = g(s) ≡ f (s) − s−1 ≡ Z∞ Z∞ {A(u) − eu }e−us du 0 {B(u) − 1}e−(s−1)u du, 0 where B(u) ≡ A(u)e−u Take s = 1 + ε + iτ. Then g(1 + ε + iτ) ≡ gε (τ) = Z∞ {B(u) − 1}e−εu · e−iτu du 0 Now g(s) is analytic for σ ≥ 1; therefore gε (t) → g(1 + it) as ε → 0. uniformly in any finite interval −2λ ≤ t ≤ 2λ. 17. The Zeta Function of Riemann (Contd) 140 We should like to form the Fourier transform of gε (τ), but since we do not know that it is bounded on the whole line, we shall introduce a smoothing kernel. Thus 1 2 Z2λ −2λ ! |τ| iyτ e dτ gε (τ) 1 − 2λ Z2λ 1 = 2 iyτ e −2λ 145 ! Z∞ |τ| dτ {B(u) − 1}e−εu−iτu du. 1− 2λ 0 For a fixed y, a finite τ-interval, and an infinite u-interval we wish to change the order of integration. This is permitted if Z∞ {B(u) − 1}e−εu · e−iτu du 0 converges uniformly in −2λ ≤ τ ≤ 2λ. This is so, because it is equal to Z∞ −εu −iτu B(u)e e du − 0 Z∞ e−εu e−ετu du. 0 For a fixed ε > 0, the second converges absolutely and uniformly in τ. In the first we have B(u) · e−(ε/2)u = A(u) · e−(1+ε/2)u → 0 as u → ∞ Hence B(u) = O(e(ε/2)u ), which implies the first integral converges uniformly and absolutely. Thus 1 2 Z2λ −2λ iyτ e ! |τ| gε (τ)dτ 1− 2λ ∞ ! Z2λ Z |τ| 1 i(y−u)τ = {B(u) − 1}e−εu du e dτ 1− 2 2λ 0 −2λ 12. The Prime Number Theorem = Z∞ [B(u) − 1]e−εu 0 141 sin2 λ(y − u) du λ(y − u)2 Now consider the limit as ε → 0. The left hand side tends to ! Z2λ 1 |τ| iyτ g(1 + iτ)dτ e 1− 2 2λ −2λ since g is analytic, or rather, since gε (τ) → g(1 + iτ) uniformly. On the right side, we have Z∞ 2 Z∞ 2 sin λ(y − u) −εu sin λ(y − u) du → du. e 2 λ(y − u) λ(y − u)2 0 0 Hence lim ε→0 Z∞ 0 e−εu B(u) sin2 λ(y − u) du = λ(y − u)2 Z∞ 0 sin2 λ(y − u) du + λ(y − u)2 Z2λ iyt e −2λ ! |t| g(1 + it) dt 1− 2λ The integrand of the left hand side increases monotonically as ε → 0; it is positive. Hence by the monotone-convergence theorem, Z∞ 0 sin2 λ(y − u) B(u) du = λ(y − u)2 Z∞ 0 sin2 λ(y − u) du λ(y − u)2 + Z2λ −2λ iyt e ! |t| 1− g(1 + it) dt 2λ Now let y → ∞; then the second term on the right-hand side tends to zero by the Riemann-Lebesgue lemma, while the first term is lim Zλy y→∞ −∞ sin2 ν dv = v2 Z∞ −∞ sin2 v dv = π v2 146 17. The Zeta Function of Riemann (Contd) 142 147 Hence Zλy v sin2 v B y− lim dv = π for every λ. y→∞ λ v2 To prove that −∞ lim B(u) = 1. u→∞ Second Part. (i) limB(u) ≤ 1. For a fixed ‘a’ such that 0 < a < λy, we have lim y→∞ Za v sin2 v dv ≤ π B y− λ v2 −a By definition B(u) = A(u)e−u , where A(u) ↑, so that v d a v ≤ ey− λ B y − ey− λ B y − λ λ or v a (v−a)/λ B y− ≥e B y− . λ λ Hence Za a (v−a)/λ sin2 v B y− lim e dv ≤ π y→∞ λ v2 or Za −a e −2a λ −a or −2a/λ e a sin2 v limB y − dv ≤ π λ v2 Za −a 148 sin2 v lim B(y) · dv ≤ π v2 y→∞ Now let a → ∞, λ → ∞ in such a way that Then π lim B(y) ≤ π y→∞ a → 0. λ 12. The Prime Number Theorem 143 (ii) lim B(u) ≥ 1. u→∞ Z−a Za Zλy Zλy v sin2 v dv = + + B y− λ v2 −∞ −∞ −a (⊛) a We know that |B(u)| ≤ c, so that −a Zλy Z∞ 2 Z Za 2 sin v sin v ≤ c dv + dv + v2 v2 −∞ −∞ −a a We know that |B(u)| ≤ c, so that −a Z∞ 2 Zλy Za Z 2 sin v sin v dv + dv + ≤ c v2 v2 −∞ −∞ a −a As before we get a v ey+a/λ B y + ≥ ey−v/λ B y − λ λ or a 2a/λ v a a+v B y− ≤ B y+ e λ ≤ B y+ e λ λ λ Therefore Za −a Za a 2a/λ sin2 v v sin2 v dv ≤ dv B y+ e B y− λ v2 λ v2 −a Za a sin2 v 2a/λ ≤e B y+ dv λ v2 −a Hence taking the lim in (⊛) we get, since lim Zλy y→∞ −∞ = lim = π y→∞ 149 17. The Zeta Function of Riemann (Contd) 144 and lim(c + ψ(y)) ≤ c + limψ(y), that −a ∞ Za Z Z 2 sin v π ≤ c + 2 dv + lim v −∞ −a a a 2a/λ e ≤ {· · · } + limB y + λ ≤ {· · · } + e2a/λ Za limB(y) −a Za −a sin2 v dv v2 sin2 v dv v2 a Let a → ∞, λ → ∞ in such a way that → 0. λ Then π ≤ πlimB(y) Thus lim B(u) = lim A(u)e−u = 1. u→∞ 150 u→∞ Proof of the Prime Number Theorem. We have seen [p.143] that −ζ ′ (s) = sζ(s) Z∞ ψ(x) dx, x s+1 = Z∞ e−st ψ(et )dt, σ>1 1 σ > 1. 0 Since ζ(s) is analytic for σ ≥ 1 except for s = 1, where it has a simple pole with residue 1, and has no zeros for σ ≥ 1, and ψ(et ) ≥ 0 and non-decreasing, we can appeal to the Wiener-Ikehara theorem with ζ ′ (s) f (s) = − , and obtain sζ(s) ψ(et ) ∼ et as t → ∞ 13. Prime Number Theorem and the zeros of ζ(s) 145 ψ(x) ∼ x. or 13 Prime Number Theorem and the zeros of ζ(s) We have seen that the Prime Number Theorem follows from the Wiener- 151 Ikehara Theorem if we assume that ζ(1+it) , 0. On the other hand, if we assume the Prime Number Theorem, it is easy to deduce that ζ(1 + it) , 0. If X X ψ(x) = log p = ∧(n), pm ≤x n≤x then, for σ > 1, we have Z∞ ζ ′ (s) 1 ψ(x) − x dx = − − ≡ φ(s), say. s+1 sζ(s) 1 − s x 1 Now φ(s) is regular for σ > 0 except (possibly) for simple poles at the zeros of ζ(s). Now, if ψ(x) = x + O(x), [which is a consequence of the p.n. theorem], then, given ε > 0, |ψ(x) − x| < εx, for x ≥ x0 (ε) > 1. Hence, for σ > 1, |φ(s)| < Zx0 |ψ(x) − x| dx + x2 Z∞ x0 1 ε ε dx < K + xσ σ−1 where K = K(x0 ) = K(ε). Thus |(σ − 1)φ(σ + it)| < K(σ − 1) + ε < 2ε, for 1 < σ < σ0 (ε, K) = σ0 (ε). Hence, for any fixed t, (σ − 1)φ(σ + it) → 0 as σ → 1 + 0. This shows that 1 + it cannot be a zero of ζ(s), for in that case (σ − 1)φ(σ + it) would tend to a limit different from zero, namely the residue of φ(s) at the simple pole 1 + it. 17. The Zeta Function of Riemann (Contd) 146 14 Prime Number Theorem and the magnitude of pn 152 It is easy to see that the p.n. theorem is equivalent to the result: pn ∼ n log n. For if τ(x) log x →1 (1) x then log π(x) + log log x − log x → 0, hence log π(x) →1 log x (2) Now (1) and (2) give π(x) · log π(x) →1 x Taking x = pn , we get pn ∼ n log n, since π(pn ) = n. Conversely, if n is defined by : pn ≤ x < pn+1 , then pn ∼ n log n implies pn+1 ∼ (n + 1) log(n + 1) ∼ n log n, as x → ∞. Hence or x ∼ n log n x ∼ y log y, y = π(x) = n. Hence log x ∼ log y, as above, so that y ∼ x/ log x Bibliography [1] L.Bieberbach: Lehrbuch der Funktionentheorie I & II, Chelsea, 153 1945 [2] S.Bochner: Vorlesungen über Fouriersche Integrale, Leipzig, 1932 [3] S.Bochner: Notes on Fourier Analysis, Princeton, 1936-37 [4] S.Bochner: Math. Zeit. 37(1933), pp.1-9 [5] S.Bochner & K.Chandrasekharan: Fourier Transforms, Princeton, 1949 [6] A.P.Calderon & A.Zygmund: Contributions to Fourier Analysis, Princeton, 1950, pp. 166-188 [7] C.Caratheodory: Funktionentheorie, I & II, Basel, 1950 [8] K.Chandrasekharan: J.Indian Math. Soc. 5(1941), pp. 128-132 [9] K.Chandrasekharan & S.Minakshisundaram: Bombay, 1952 Typical Means, [10] G.H.Hardy & M.Riesz: The General Theory of Dirichlet Series, Cambridge, 1915 [11] A.E.Ingham: The Distribution of Prime Numbers, Cambridge, 1932 [12] J.E.Littlewood: The Theory of Functions, Oxford, 1945 147 148 BIBLIOGRAPHY [13] C.L.Siegel: Math. Annalen, 86 (1922), pp.276-9 [14] C.L.Siegel: Lectures on Analytic Number Theory, New York, 1945 [15] E.C.Titchmarsh: The Theory of Functions, Oxford, 1932 [16] E.C.Titchmarsh: The Theory of the Riemann Zeta-Funcation, Oxford, 1951 [17] W.Thron: Introduction to the Theory of Functions of a Complex Variable, Wiley, 1953