Outline Introduction Crash Course in Number Theory Zeta Function Roots of the Zeta Function Prime Number Theorem Riemann Hy Zeta Function and Riemann Hypothesis Ivan G. Avramidi Department of Mathematics New Mexico Tech October 25, 2013 Outline Introduction Crash Course in Number Theory Zeta Function Roots of the Zeta Function Prime Number Theorem Riemann Hy 1 Introduction 2 Crash Course in Number Theory 3 Zeta Function 4 Roots of the Zeta Function 5 Prime Number Theorem 6 Riemann Hypothesis 7 Randomness in Prime Numbers 8 Random Hermitian Matrices 9 Free Riemann Gas Outline Introduction Crash Course in Number Theory Zeta Function Roots of the Zeta Function Prime Number Theorem Riemann Hy History of Prime Numbers 1 Euclid (300 BC) 2 Fermat (1640) 3 Euler (1737) 4 Dirichlet (1837) 5 Gauss (1849) 6 Chebyshev (1848) 7 Riemann (1859) 8 Dr X (2020)? Outline Introduction Crash Course in Number Theory Zeta Function Roots of the Zeta Function Prime Number Theorem Riemann Hy Millenium Prize Problem B. Riemann, “On the number of primes less that a given magnitude” (1859), 8 pages One of twenty-three most important mathematical problems composed by David Hilbert in 1900. One of the seven Millennium Prize Problems of the Clay Mathematics Institute (1 Million Dollar prize!) composed in 2000. Outline Introduction Crash Course in Number Theory Zeta Function Roots of the Zeta Function Prime Number Theorem Riemann Hy Evidence for the Riemann Hypothesis Strong numerical evidence. Riemann hypothesis holds for over 108 zeros at heights up to 1020 . The exceptions to the Riemann hypothesis, if they exist, must be rare. More than 40% of the nontrivial zeros are simple and satisfy the Riemann hypothesis. Profoundly deep relation to such diverse areas of mathematics as: analytic number theory, fractal geometry, noncommutative geometry, random matrix theory, chaotic dynamical systems (classical and quantum), quantum theory, solid state physics, quasi-crystals, etc Outline Introduction Crash Course in Number Theory Zeta Function Roots of the Zeta Function Prime Number Theorem Riemann Hy Prime Numbers A positive integer d divides a positive integer n, denoted by d |n, if there is an integer k such that n = kd. A positive integer d is the greatest common divisor of positive integers a and b, denoted by d = (a , b ) if it is a common divisor of a and b and is divisible by any other common divisor. Two positive integers a and b are relatively prime if (a , b ) = 1. A positive integer p > 1 is prime if it is divisible only by 1 and p. Outline Introduction Crash Course in Number Theory Zeta Function Roots of the Zeta Function Prime Number Theorem Riemann Hy Notation Summation over all positive divisors of n is denoted by X f (d ) d |n Summation over all positive integers relatively prime to n is denoted by X f (k ) ( k ,n ) Summation over all primes is denoted by X f (p ) p Summation over all powers of primes is denoted by X pk f (n) Outline Introduction Crash Course in Number Theory Zeta Function Roots of the Zeta Function Prime Number Theorem Riemann Hy Fundamental Theorem of Arithmetic The primes form an increasing sequence (pj )∞ j =1 p1 < p2 < p3 < · · · The study of this sequence as j → ∞ is central problem of number theory. Unique Factorization Theorem. Every positive integer n > 1 can be identified with a sequence of non-negative integers (nj )∞ , nj ≥ 0, containing only finitely many non-zero terms j =1 such that n= ∞ Y j =1 n pj j Outline Introduction Crash Course in Number Theory Zeta Function Roots of the Zeta Function Prime Number Theorem Riemann Hy Examples If all nj = 0, then n = 1 If only one nj is nonzero and nj = 1, then n = pj is a prime If only one nj is non-zero and nj = k > 1, then n = pjk is a power of prime If all non-zero nj are equal to 1, then n is the product of distinct primes Outline Introduction Crash Course in Number Theory Zeta Function Roots of the Zeta Function Prime Number Theorem Riemann Hy Arithmetic Functions Arithmetic function is a real valued function f : Z+ → R defined on the set of positive integers that expresses some arithmetical property of integers. All arithmetic functions can be extended to functions of positive real numbers, f : R → R as step functions by f (x ) = f ([x ]) if x is not an integer and equal to the average of the left and right values at the jumps. Outline Introduction Crash Course in Number Theory Zeta Function Roots of the Zeta Function Prime Number Theorem Riemann Hy Examples of Arithmetic Functions The unit function e (1) = 1, and e (n ) = 0 for n > 1 Function ω(n) is defined as the number of distinct prime divisors of n. Möbius function µ(1) = 1, and µ(n) = (−1)ω(n) if all primes divisors of n > 1 are distinct and zero otherwise. The Von Mangoldt function Λ(n) = log p if n = p k for some prime p with some k ≥ 1 and zero otherwise. Outline Introduction Crash Course in Number Theory Zeta Function Roots of the Zeta Function Prime Number Theorem Riemann Hy Dirichlet Convolution The Dirichlet convolution h = f ∗ g of two arithmetic functions, f , g, is defined by h (n) = X f (d )g d |n n d The convolution inverse of an arithmetic function f is an arithmetic function g such that its convolution with f is equal to the unit function, f ∗g =e, that is, X d |n f (d )g n d = e (n) In particular, g (1) = 1/f (1). So, if f (1) = 0, then it does not exist. Outline Introduction Crash Course in Number Theory Zeta Function Roots of the Zeta Function Prime Number Theorem Riemann Hy Möbius Inversion Fundamental Property of the Möbius Function The Möbius function is the convolution inverse of the constant function 1, that is, µ ∗ 1 = e or X µ(d ) = e (n) d |n It allows us to invert relations between arithmetic functions n X X F (n ) = f (d ) iff f (n) = µ(d )F d d |n d |n One can also show that g (x ) = ∞ X n=1 f (nx ) iff f (x ) = ∞ X n =1 µ(n)g (nx ) Outline Introduction Crash Course in Number Theory Zeta Function Roots of the Zeta Function Prime Number Theorem Riemann Hy Summatory Functions Given an arithmetic function f one defines a function of a real variable x ≥ 0, X Mf ( x ) = f (n), n ≤x One is interested in the asymptotic behavior as x → ∞ Outline Introduction Crash Course in Number Theory Zeta Function Roots of the Zeta Function Prime Number Theorem Riemann Hy Examples The Mertens function M (x ) = X µ(n) n ≤x The prime counting function π(x ) = X 1. p ≤x The weighted prime counting function Π(x ) = X 1 p k ≤x k = X Λ(n) . log n n ≤x The Chebyshev function ψ(x ) = X p k ≤x log p = X n ≤x Λ(n) . Outline Introduction Crash Course in Number Theory Zeta Function Roots of the Zeta Function Prime Number Theorem Riemann Hy Dirichlet Series The asymptotics of a summatory function Mf of an arithmetic function f as x → ∞ are described by the analytical properties of the function of a complex variable s = σ + it, Df (s ) = ∞ X f (n ) ns n=1 , σ>c called the Dirichlet Series of f . The Dirichlet series Df (s ) and the summatory function Mf (x ) are related by the Mellin transform ∞ Z dx x −s −1 Mf (x ), Df (s ) = s 0 1 Mf (x ) = 2πi Z c +i ∞ c −i ∞ ds s x Df (s ) s Outline Introduction Crash Course in Number Theory Zeta Function Roots of the Zeta Function Prime Number Theorem Riemann Hy Dirichlet Series of a Convolution The Dirichlet series of a Dirichlet convolution h = f ∗ g is equal to the product of Dirichlet series, Dh (s ) = Df (s )Dg (s ) The Dirichlet series of a convolution inverse g of a function f is equal to the reciprocal of the Dirichlet series of f , that is, Reciprocal of Dirichlet Series 1 = Dg (s ) Df (s ) iff f ∗g =e Outline Introduction Crash Course in Number Theory Zeta Function Roots of the Zeta Function Prime Number Theorem Riemann Hy Euler Product An arithmetic function f is called multiplicative if f (1) = 1 and for any relatively prime integers a and b f (ab ) = f (a )f (b ). The Dirichlet series of a multiplicative function f can be represented as the product over primes Euler product ∞ Y X f (p k ) 1 + Df (s ) = ks p p k =1 Outline Introduction Crash Course in Number Theory Zeta Function Roots of the Zeta Function Prime Number Theorem Riemann Hy Zeta Function Riemann zeta function ζ(s ) = D1 (s ) = ∞ X 1 n=1 ns , s = σ + it , σ>1 By the convolution inverse one can immediately obtain ∞ X µ(n) 1 = Dµ (s ) = , ns ζ(s ) n=1 σ>1 The Euler product for the zeta function has the form !−1 ∞ Y X 1 Y 1 ζ(s ) = 1− s , 1 + = p p ks p k =1 p σ>1 Outline Introduction Crash Course in Number Theory Zeta Function Roots of the Zeta Function Prime Number Theorem Riemann Hy Zeta Function This means that log ζ(s ) = ∞ X X 1 1 k =1 p k p ks ∞ X Λ(n) 1 = , log n ns n =1 And, therefore, ∞ X ζ 0 (s ) Λ(n) − = DΛ (s ) = , ns ζ(s ) n =1 σ>1 σ>1 Outline Introduction Crash Course in Number Theory Zeta Function Roots of the Zeta Function Prime Number Theorem Riemann Hy Integral Representations of Zeta Function Zeta function is the Mellin transform of the integer part function [x ] ζ(s ) = s ∞ Z σ>1 dx x −s −1 [x ], 1 It can be written in the form ζ(s ) = s s−1 ∞ Z dx x −s −1 {x }, −s σ>0 1 where {x } = x − [x ] is the fractional part of x, which reveals a simple pole at s = 1. Zeta function is directly related to the prime counting functions log ζ(s ) = s ∞ Z Z dx x 1 −s −1 Π(x ) = s ∞ dx 1 π(x ) , x (x s − 1) σ>1 Outline Introduction Crash Course in Number Theory Zeta Function Roots of the Zeta Function Prime Number Theorem Riemann Hy Integral Representations of Zeta Function More importantly Mellin Transform of Mertens Function 1 =s ζ(s ) ∞ Z σ>1 dx x −s −1 M (x ), 1 It is easy to show that 1 ζ(s ) = Γ(s ) ∞ Z dx x s −1 0 1 ex −1 , σ>1 Analytic Continuation of Zeta Function 1 ζ(s ) = Γ(1 − s ) 2πi Z C dz (−z )s , z ez − 1 where C is the contour that goes from +∞ + i ε to +∞ − i ε around the origin in the counterclockwise direction. Outline Introduction Crash Course in Number Theory Zeta Function Roots of the Zeta Function Prime Number Theorem Riemann Hy Heat Kernel Representation of Zeta Function The heat trace on the circle S 1 is given by θ(t ) = Tr exp(−tD 2 ) = ∞ X e −n 2 πt =1+2 n=−∞ ∞ X e −n n =1 Fundamental Duality (Possion Summation Formula) 1 1 θ(t ) = √ θ t t ! It is easy to show ζ(s ) = 1 πs /2 2Γ s 2 ∞ Z 0 dt s /2 t [θ(t ) − 1] , t σ>1 2 πt Outline Introduction Crash Course in Number Theory Zeta Function Roots of the Zeta Function Prime Number Theorem Riemann Hy Functional Equation for Zeta Function By using the duality one can get ) ( Z πs /2 1 ∞ dt s /2 1 (1−s )/2 [θ(t ) − 1] t +t ζ(s ) = + Γ 2s s (s − 1) 2 1 t which provides an analytic continuation for any s and reveals a pole at s = 1. This immediately leads to Functional Equation ξ(s ) = ξ(1 − s ) where 1 s ξ(s ) = s (s − 1)π−s /2 Γ ζ(s ) 2 2 Outline Introduction Crash Course in Number Theory Zeta Function Roots of the Zeta Function Prime Number Theorem Riemann Hy Roots of the Zeta Function Zeta function is a meromorphic function with a simple pole at s = 1. It has some trivial zeros at the negative even integer points, that is, ζ(−2n) = 0 , n = 1, 2, . . . . All non-trivial roots coincide with the roots of the entire function ξ . Outline Introduction Crash Course in Number Theory Zeta Function Roots of the Zeta Function Prime Number Theorem Riemann Hy Non-Trivial Roots of the Zeta Function There are no roots for σ > 1. A complex number 1 − ρ is a root if and only if ρ is a root. The roots are located symmetrically with respect to the critical line 1 σ= . 2 There are no non-trivial roots for σ < 0. All roots are located in the critical strip 0 ≤ σ ≤ 1. If ρ is a root then ρ̄ is also a root. The roots are located symmetrically with respect to the real axis. Outline Introduction Crash Course in Number Theory Zeta Function Roots of the Zeta Function Prime Number Theorem Riemann Hy Non-Trivial Roots of the Zeta Function There are infinitely many roots on the critical line. The number of zeros (with s = σ + it) in the rectangle 0 ≤ σ ≤ 1, 0<t <T as T → ∞ is N (T ) = T T 7 1 T log − + + O ( log T ) 2π 2π 2π 8 There holds X 1 < ∞, |ρ|2 ρ X 1 →∞ |ρ| ρ There holds ψ(x ) = x − X xρ ρ 1 1 − log 2π − log 1 − 2 ρ 2 x ! Outline Introduction Crash Course in Number Theory Zeta Function Roots of the Zeta Function Prime Number Theorem Riemann Hy Prime Number Theorem Equivalent formulations of Prime Number Theorem: As x → ∞ π(x ) ∼ Li(x ), where Li(x ) = >x 0 dt log t ψ(x ) ∼ x , π(x ) ∼ or x log x is the integral logarithm or lim x →∞ X1 ρ ρ x ρ−1 = 0 There are no roots of zeta function on the line σ = 1. Outline Introduction Crash Course in Number Theory Zeta Function Roots of the Zeta Function Prime Number Theorem Riemann Hy Riemann Hypothesis The equivalent formulations of the Riemann hypothesis Riemann Hypothesis All non-trivial roots of the zeta function are located on the critical line. There are no non-trivial roots for σ , 1/2. π(x ) = Li(x ) + O (x 1/2 log x ) For any ε > 0 For any ε > 0 π(x ) = Li(x ) + O x 1/2+ε ψ(x ) = x + O x 1/2+ε Outline Introduction Crash Course in Number Theory Zeta Function Roots of the Zeta Function Prime Number Theorem Riemann Hy Riemann Hypothesis For any ε > 0 X1 ρ The series ρ x ρ = O x 1/2+ε ∞ X µ(n) n =1 ns converges for σ > 1/2. For any ε > 0 the Mertens function M (x ) grows less rapidly than x 1/2+ε , that is, for any ε > 0 M (x ) = O x 1/2+ε For large n that is equal to the product of distinct primes the probablity of even and odd number of distinct primes are equal. Outline Introduction Crash Course in Number Theory Zeta Function Roots of the Zeta Function Prime Number Theorem Riemann Hy Hilbert-Polya Conjecture Hilbert-Polya Conjecture There is a unbounded self-adjoint operator H such that the spectrum of the operator 1 + iH 2 coincides with the zeros of the Riemann zeta function Hints: the dynamics is chaotic, that is, unstable and bounded, the dynamics is time-irreversible, periodic orbits have periods independent of energy, dynamics is quasi-one-dimensional. Outline Introduction Crash Course in Number Theory Zeta Function Roots of the Zeta Function Prime Number Theorem Riemann Hy Randomness in Prime Numbers Suppose an unbiased coin is flipped a large number of times. Then the probability of getting exactly H heads in N trials is given by the binomial distribution ! N 1 B (N , H ) = H 2N de Moivre-Laplace Theorem As N → ∞ the binomial distribution approaches the√normal distribution with mean N /2 and standard deviation N /2, r B (N , H ) ∼ F (N , H ) = 2 2 N exp − H− πN N 2 !2 Outline Introduction Crash Course in Number Theory Zeta Function Roots of the Zeta Function Prime Number Theorem Riemann Hy Randomness in Prime Numbers The probability that the number of heads deviates from the expected value N2 by KN 1/2+ε as N → ∞ is equal ! N P H − < KN 1/2+ε ∼ 2 √ 2 = √ π Z 2 Nε N /2+ ZKN 1/2+ε dH F (N , H ) N /2−KN 1/2+ε 2 dx e −x → 1 0 The probability that the number of heads deviates from the number of tails by 2KN 1/2+ε as N → ∞ P |H − T | < 2KN 1/2+ε → 1 Outline Introduction Crash Course in Number Theory Zeta Function Roots of the Zeta Function Prime Number Theorem Riemann Hy Randomness in Prime Numbers With probability 1 the number of heads minus the number of tails grows less rapidly than N 1/2+ε . Let n be a large integer such that it is product of distinct primes, so that, µ(n) , 0. If the number of factors is odd then µ(n) = −1 and if the number of factors is even then µ(n) = 1. Then the evaluation of the Mertens function M (x ) is like flipping a coin for each integer n ≤ x which is a product of distinct primes and subtracting the number of tails from the number of heads. If the values of µ(n) are independent, that is, with equal probability a large square-free integer has either an odd number of factors or an even number of factors, then for any given ε > 0 as x → ∞ with probability 1, M (x ) < O x 1/2+ε . This is equivalent to Riemann hypothesis. Outline Introduction Crash Course in Number Theory Zeta Function Roots of the Zeta Function Prime Number Theorem Riemann Hy Random Hermitian Matrices There are conjectures that relate the statistical behavior of the nontrivial zeros of the Riemann zeta function to the distribution of the eigenvalues of large N × N random Hermitian matrices M with the probability measure ( N P (M ) = CN exp − tr M 2 2 ) Such a system is called the Gaussian Unitary Ensemble. The zeros of the zeta function ρk = 1 + itk 2 are distributed like the eigenvalues of the eigenvalues of random Hermitian matrices. Outline Introduction Crash Course in Number Theory Zeta Function Roots of the Zeta Function Prime Number Theorem Riemann Hy Free Riemann Gas The free Riemann gas is a quantum theory of identical non-interacting particles. The particles can be in infinitely many different states labeled by primes p The particles can be either bosonic or fermionic Bosonic particles can be in the same state Fermionic particles cannot be in the same state (Pauli Exclusion Principle) Every state of a system can be described by a positive integer n= Y p kp p In such a state there k1 particles in state p1 , k2 particles in state p2 , etc. Outline Introduction Crash Course in Number Theory Zeta Function Roots of the Zeta Function Prime Number Theorem Riemann Hy Free Riemann Gas States of bosonic particles are described by any integer States of fermionic particles are described only by integers which are product of distinct primes, that is, kp are equal to 0 or 1. The states of fermionic particles can be even or odd depending on the number of particles, that is, the parity of the fermionic state is equal to the Möbius function µ(n) Outline Introduction Crash Course in Number Theory Zeta Function Roots of the Zeta Function Prime Number Theorem Riemann Hy Free Riemann Gas The energy of a particle in the state p is log p. The energy of the state |ni is E (n) = X kp log p = log p Y p kp = log n p The partition function of the bosonic system is Z (β) = Tr exp(−βH ) = ∞ X exp [−βE (n)] = ζ(β) , n =1 where β = 1/T is the inverse temperature. The partition function of the fermionic system is Z (β) = Str exp(−βH ) = ∞ X n =1 µ(n) exp [−βE (n)] = 1 ζ(β)