New York Journal of Mathematics New York J. Math. 10 (2004) 69–81. Error inequalities for a corrected interpolating polynomial Nenad Ujević Abstract. A corrected interpolating polynomial is derived. Error inequalities of Ostrowski type for the corrected interpolating polynomial are established. Some similar inequalities are also obtained. Contents 1. Introduction 2. Corrected interpolating polynomial 3. Error inequalities References 69 70 76 80 1. Introduction Many error inequalities in polynomial interpolation can be found in [2] and [12]. These error bounds for interpolating polynomials are usually expressed by means of the norms ·p , 1 ≤ p ≤ ∞. Some new error inequalities in polynomial interpolation can be found in [16]. In this paper we derive error inequalities for a corrected interpolating polynomial. Similar inequalities are obtained in numerical integration. For example see [3]–[11], [14] and [15]. In some of the mentioned papers we can find estimations for errors of quadrature formulas which are expressed by means of the differences Γk − γk , S − γk , Γk − S, where Γk , γk are real numbers such that γk ≤ f (k) (t) ≤ Γk , t ∈ [a, b] (k is a positive integer while [a, b] is an interval of integration) and S = f (k−1) (b) − f (k−1) (a) /(b−a). It is shown that the estimations expressed in such a way can be much better than estimations expressed by means of the norms f (k) p , 1 ≤ p ≤ ∞. Furthermore, it is well-known that corrected quadrature formulas have better estimations of errors than corresponding original formulas. As we know there is a close relationship between interpolation polynomials and quadrature rules. Thus, it is a natural try to establish similar error inequalities in Received November 5, 2003. Mathematics Subject Classification. 26D10, 41A80, 65D05. Key words and phrases. corrected interpolating polynomial, representation of remainder, Ostrowski type inequalities. ISSN 1076-9803/04 69 70 Nenad Ujević polynomial interpolation. The usual procedure is to find an interpolating formula and then we write a corresponding quadrature formula. Here we reverse the procedure. We have some results for quadrature formulas and we derive corresponding results for interpolating polynomials. We first establish general error inequalities, expressed by means of f (k) − Pm , where Pm is any polynomial of degree m and then we obtain inequalities of the above mentioned types. For that purpose we derive a representation of remainder in corrected interpolating polynomial. This is done in Section 2. In the same section we give a relationship between the corrected interpolating polynomial and a corresponding quadrature rule. In Section 3 we obtain the error inequalities. Finally, we emphasize that the usual error inequalities in polynomial interpolation (for the Lagrange interpolating polynomial Ln (x)) are given by means of the (n+1)th derivative while in this paper we can find these error inequalities expressed by means of the kth derivative for k = 1, 2, . . . , n. 2. Corrected interpolating polynomial Let π = {a = x0 < x1 < · · · < xn = b} be a given subdivision of the interval [a, b] and let f : [a, b] → R be a given function. The Lagrange interpolation polynomial is given by Ln (x) = (2.1) n pni (x)f (xi ), i=0 where (2.2) pni (x) = (x − x0 ) · · · (x − xi−1 )(x − xi+1 ) · · · (x − xn ) , (xi − x0 ) · · · (xi − xi−1 )(xi − xi+1 ) · · · (xi − xn ) for i = 0, 1, . . . , n. We have the Cauchy relations ([12, pp. 160-161]), n (2.3) pni (x) = 1 i=0 and (2.4) n pni (x)(x − xi )j = 0, j = 1, 2, . . . , n. i=0 Let π = {x0 = a < x1 < · · · < xn = b} be a given uniform subdivision of the interval [a, b], i.e., xi = x0 + ih, h = (b − a)/n, i = 0, 1, 2, . . . , n. Then the Lagrange interpolating polynomial is given by Ln (x) = Ln (x0 + th) n t(t = (−1) n − 1) · · · (t − n) i n f (xi ) , (−1) n! i t−i i=0 where t ∈ / {0, 1, 2, . . . , n}, 0 < t < n. As we know the divided difference of the first order of the function f is given by f [x0 ; x1 ] = f (x1 ) − f (x0 ) . x1 − x0 Error inequalities 71 The divided difference of order n is defined via the divided differences of order n − 1 by the recurrence formula f [x1 ; x2 ; . . . ; xn ] − f [x0 ; x1 ; . . . ; xn−1 ] f [x0 ; x1 ; . . . ; xn ] = . xn − x1 The following lemma is valid ([2, p. 86]): Lemma 2.1. The nth-order divided difference satisfies the relation n f (xi ) . f [x0 ; x1 ; . . . ; xn ] = (x − x ) · · · (x − x i 0 i i−1 )(xi − xi+1 ) · · · (xi − xn ) i=0 The interpolating polynomial can be written in the Newton form as Ln (x) = f (x0 ) + n−1 (x − x0 ) · · · (x − xi )f [x0 ; . . . ; xi+1 ] i=0 = f (x0 ) + n−1 ωi (x)f [x0 ; . . . ; xi+1 ] , i=0 where ωi (x) = (x − x0 )(x − x1 ) · · · (x − xi ), (2.5) for i = 0, 1, 2, . . . , n. We also recall some properties of Euler polynomials. The Euler polynomials are defined by the relation ∞ tk 2ext = , |t| < π, E (x) k et + 1 k! k=0 such that 1 E0 (x) = 1, E1 (x) = x − , E2 (x) = x2 − x, . . . 2 (2.6) We have Ek (x) = kEk−1 (x) or (2.7) 1 (2.8) 0 and Ek (x)dx = Ek+1 (x) , k = 1, 2, . . . , k+1 En (t)Em (t)dt = (−1)n 4(2m+n+2 − 1) (2.9) 0 1 En (t)dt = m!n! Bm+n+2 (m + n + 2)! En+1 (1) − En+1 (0) , n = 1, 2, . . . . n+1 We also have (2.10) Ek (0) = −Ek (1) = −2 2k+1 − 1 Bk+1 , k+1 where Bk are Bernoulli numbers such that 1 1 E1 (0) = − , E2 (0) = 0, E3 (0) = , E4 (0) = 0, . . . 2 4 or generally E2n (0) = 0. Further properties of Euler polynomials can be found in [1]. 72 Nenad Ujević Lemma 2.2. Let Pm (t) be any polynomial of degree ≤ m and let π be a given subdivision of the interval [a, b]. Then x n t − xi k dt = 0, pni (x)(x − xi ) Pm (t)Ek x − xi xi i=0 for 0 ≤ k + m ≤ n − 1 and x ∈ [a, b], where Ek (t) are Euler polynomials. Proof. Let x be a real number. Then we have m Pm (t) = cj (x − t)j , j=0 for some coefficients cj = cj (x), j = 0, 1, . . . , m. (This is a consequence of the Taylor formula.) Thus, x x m t − xi t − xi j dt = dt. Pm (t)Ek cj (x − t) Ek x − xi x − xi xi xi j=0 We now calculate x x−xi t − xi u j j dt = du (x − t) Ek (x − xi − u) Ek x − xi x − xi xi 0 j x−xi u u = (x − xi )j 1− du Ek x − xi x − xi 0 1 j+1 = (x − xi ) (1 − v)j Ek (v)dv. 0 Integrating by parts and using the property (2.7), we obtain 1 1 1 j Ek+1 (0) + (1 − v)j Ek (v)dv = − (1 − v)j−1 Ek+1 (v)dv. k+1 k+1 0 0 In a similar way we get 1 1 j−1 1 (1 − v)j−1 Ek+1 (v)dv = − (1 − v)j−2 Ek+2 (v)dv. Ek+2 (0) + k+2 k+2 0 0 Hence, we have 1 1 j Ek+1 (0) − Ek+2 (0) (1 − v)j Ek (v)dv = − k+1 (k + 1)(k + 2) 0 1 j(j − 1) (1 − v)j−2 Ek+2 (v)dv. + (k + 1)(k + 2) 0 Continuing in this way we get 1 j−1 k!j! k!j!Ek+j+1 (0) , (1 − v)j Ek (v)dv = − Ek+l+1 (0) − 2 (k + l + 1)!(j − l)! (k + j + 1)! 0 l=0 for j ≥ 1, since k+1 (0) − 2Ek+1 . Thus, 1 0 Ek+j (v)dv = −2 x xi (x − t)j Ek Ek+j+1 (0) k+j+1 . t − xi x − xi For j = 0, 1 (1 0 dt = (x − xi )j+1 Dkj , − v)0 Ek (v)dv = 73 Error inequalities where Dkj ⎧ 2Ek+1 (0) ⎪ , j=0 ⎨− k+1 j−1 = k!j!Ek+j+1 (0) k!j! ⎪ ⎩− (k+l+1)!(j−l)! Ek+l+1 (0) − 2 (k+j+1)! , 1 ≤ j ≤ m. l=0 It follows that x xi Pm (t)Ek t − xi x − xi dt = m cj Dkj (x − xi )j+1 . j=0 Finally, we get n k pni (x)(x − xi ) i=0 = m j=0 cj Dkj n x xi Pm (t)Ek t − xi x − xi dt pni (x)(x − xi )k+j+1 = 0, i=0 for 0 ≤ k + m ≤ n − 1, since (2.4) holds. Theorem 2.1. Under the assumptions of Lemma 2.2 suppose that f ∈ C k+1 (a, b). Then (2.11) f (x) = Ln (x) + ωn (x) k (−1)j Ej (0) j=1 j! gj [x0 ; x1 ; . . . ; xn ] + Rk,m (x), where (2.12) Rk,m (x) = x n t − xi (−1)k dt f (k+1) (t) − Pm (t) Ek pni (x)(x − xi )k k! i=0 x − xi xi and gj (t) = (x − t)j−1 f (j) (t), Proof. We have Rk,m (x) = j = 1, 2, . . . , k. x n t − xi (−1)k dt pni (x)(x − xi )k f (k+1) (t)Ek k! i=0 x − xi xi x n t − xi (−1)k k dt. pni (x)(x − xi ) Pm (t)Ek − k! i=0 x − xi xi From the above relation and Lemma 2.2 it follows that x n t − xi (−1)k k (k+1) Rk,m (x) = Rk (x) = dt. pni (x)(x − xi ) f (t)Ek k! i=0 x − xi xi 74 Nenad Ujević Integrating by parts, we obtain x t − xi (−1)k k (k+1) (x − xi ) dt f (t)Ek k! x − xi xi (−1)k = (x − xi )k Ek (1)f (k) (x) − Ek (0)f (k) (xi ) k! x t − xi (−1)k−1 k−1 (k) dt, f (t)Ek−1 + (x − xi ) (k − 1)! x − xi xi since (2.7) holds. In a similar way we get x (−1)k−1 t − xi k−1 (k) (x − xi ) dt f (t)Ek−1 (k − 1)! x − xi xi (−1)k−1 = (x − xi )k−1 Ek−1 (1)f (k−1) (x) − Ek−1 (0)f (k−1) (xi ) (k − 1)! x t − xi (−1)k−2 (x − xi )k−2 dt. f (k−1) (t)Ek−2 + (k − 2)! x − xi xi Continuing in this way we get x t − xi (−1)k k (k+1) (x − xi ) dt f (t)Ek k! x − xi xi k x (−1)j = f (t)dt (x − xi )j Ej (1)f (j) (x) − Ej (0)f (j) (xi ) + j! x i j=1 = k (−1)j j=1 j! (x − xi )j Ej (1)f (j) (x) − Ej (0)f (j) (xi ) + f (x) − f (xi ). Then we have Rk (x) = n pni (x) [f (x) − f (xi )] i=0 + n i=0 pni (x) k (−1)j j! j=1 = f (x) − Ln (x) + k n (−1)j j! j=1 = f (x) − Ln (x) − (x − xi )j Ej (1)f (j) (x) − Ej (0)f (j) (xi ) k j=1 pni (x)(x − xi )j Ej (1)f (j) (x) − Ej (0)f (j) (xi ) i=0 n (−1)j Ej (0) pni (x)(x − xi )j f (j) (xi ), j! i=0 since (2.3) holds and n i=0 pni (x)(x − xi )j Ej (1)f (j) (x) = 0, Error inequalities 75 for 1 ≤ j ≤ n. We have n pni (x)(x − xi )j f (j) (xi ) i=0 n = ωn (x) i=0 (x − xi )j−1 f (j) (xi ) (xi − x0 ) · · · (xi − xi−1 )(xi − xi+1 ) · · · (xi − xn ) and gj [x0 ; x1 ; . . . ; xn ] = n i=0 (x − xi )j−1 f (j) (xi ) , (xi − x0 ) · · · (xi − xi−1 )(xi − xi+1 ) · · · (xi − xn ) by Lemma 2.1, so that Rk (x) = f (x) − Ln (x) − ωn (x) k (−1)j j=1 j! Ej (0)gj [x0 ; x1 ; . . . ; xn ] . This completes the proof. Remark 2.1. Since E2j (0) = 0, j = 1, 2, . . . , we can write f (x) = Ln (x) − ωn (x) k−1 [ 2 ] j=0 E2j+1 (0) g2j+1 [x0 ; x1 ; . . . ; xn ] + Rk,m (x). (2j + 1)! Example 2.1. If we choose n = 1 in (2.11) then we get x − x0 x − x1 f (x0 ) + f (x1 ) f (x) = x0 − x1 x1 − x0 1 f (x1 ) − f (x0 ) + (x − x0 )(x − x1 ) + R. 2 x1 − x0 Thus, x1 f (x0 ) + f (x1 ) f (x)dx = (x1 − x0 ) 2 x0 x1 (x1 − x0 )2 [f (x1 ) − f (x0 )] + − Rdx, 12 x0 since x1 x − x1 dx = x0 − x1 x0 1 2 x1 x0 x1 x0 x − x0 dx = x1 − x0 , x1 − x0 (x − x0 )(x − x1 ) (x1 − x0 )2 dx = − . x1 − x0 12 We see that the above quadrature formula is the well-known corrected trapezoidal rule. Remark 2.2. If we generalize the above example then we find that the following conclusions are valid: If we integrate (2.11) from x0 to xn then we get a corrected Newton-Cotes formula. (Of course, we suppose that the partition π is uniform.) It is well-known that the corrected formulas have better estimations of errors than corresponding original quadrature formulas. 76 Nenad Ujević 3. Error inequalities We now introduce the notations (3.1) Ck (x) = n i=0 (3.2) Fk (x) = n i=0 (3.3) Dk (x) = n i=0 k |x − xi | , |xi − x0 | · · · |xi − xi−1 | |xi − xi+1 | · · · |xi − xn | k (Ski − γk+1 ) |x − xi | , |xi − x0 | · · · |xi − xi−1 | |xi − xi+1 | · · · |xi − xn | k (Γk+1 − Ski ) |x − xi | , |xi − x0 | · · · |xi − xi−1 | |xi − xi+1 | · · · |xi − xn | where Ski = f (k) (x) − f (k) (xi ) /(x − xi ), i = 0, 1, . . . , n and γk+1 , Γk+1 are real numbers such that γk+1 ≤ f (k+1 (t) ≤ Γk+1 , t ∈ [a, b], k = 0, 1, . . . , n − 1. We also define the constant |B2k+2 | 2k+2 δk = (3.4) 2 − 1. (2k + 2)! Let g ∈ C(a, b). As we know among all algebraic polynomials of degree ≤ m there ∗ exists the only polynomial Pm (t) having the property that ∗ g − Pm ∞ ≤ g − Pm ∞ , where Pm ∈ Πm is an arbitrary polynomial of degree ≤ m. We define (3.5) ∗ Gm (g) = g − Pm = inf Pm ∈Πm g − Pm ∞ . Theorem 3.1. Under the assumptions of Theorem 2.1 we have k j (−1) Ej (0) f (x) − Ln (x) − ωn (x) g [x ; x ; . . . ; x ] j 0 1 n j! j=1 ≤ 2δk Gm (f (k+1) )Ck (x) |ωn (x)| , where Ck (·), δk and Gm (·) are defined by (3.1), (3.4) and (3.5), respectively. Proof. We have x 2 2 x t − xi t − xi dt ≤ |x − xi | Ek Ek dt x − x x − x i i xi xi 1 2 = (x − xi )2 (Ek (u)) du 0 (k!)2 =4 (22k+2 − 1)(x − xi )2 |B2k+2 | , (2k + 2)! since (2.8) holds. Error inequalities 77 ∗ ∗ Let Pm (t) = Pm (t), where Pm (t) is defined by (3.5) for the function g(t) = (t). Then we have f x n (−1)k t − xi k (k+1) ∗ dt f pni (x)(x − xi ) (t) − Pm (t) Ek |Rk,m (x)| = k! x − x i xi i=0 n x (k+1) 1 t − xi ∗ ≤ dt f pni (x)(x − xi )k (t) − Pm (t) Ek k! i=0 x − x i xi (k+1) ∗ f − Pm ∞ 2k! |B2k+2 | ≤ 22k+2 − 1Ck (x) |ωn (x)| k! (2k + 2)! Gm (f (k+1) ) |B2k+2 | 2k+2 =2 2 − 1Ck (x) |ωn (x)| (2k + 2)! (k+1) and Rk,m (x) = f (x) − Ln (x) − ωn (x) k (−1)j j=1 j! Ej (0)gj [x0 ; x1 ; . . . ; xn ] . This completes the proof. Remark 3.1. The above estimate has only theoretical importance, since it is difficult to find the polynomial P ∗ . In fact, we can find P ∗ only for some special cases of functions. However, we can use the estimate to obtain some practical estimations — see Theorem 3.2. Theorem 3.2. Let the assumptions of Theorem 2.1 hold. If γk+1 , Γk+1 are real numbers such that γk+1 ≤ f (k+1) (t) ≤ Γk+1 , t ∈ [a, b], k = 0, 1, . . . , n − 1, then k j (−1) E (0) j f (x) − Ln (x) − ωn (x) gj [x0 ; x1 ; . . . ; xn ] j! j=1 ≤ δk [Γk+1 − γk+1 ] Ck (x) |ωn (x)| , where ωn , δk and Ck (·) are defined by (2.5), (3.4) and (3.1), respectively. We also have k j (−1) Bj f (x) − Ln (x) − ωn (x) g [x ; x ; . . . ; x ] j 0 1 n ≤ 2δk |ωn (x)| Fk (x) j! j=1 and k j (−1) B j f (x) − Ln (x) − ωn (x) gj [x0 ; x1 ; . . . ; xn ] ≤ 2δk |ωn (x)| Dk (x), j! j=1 where Fk (·) and Dk (·) are defined by (3.2) and (3.3), respectively. 78 Nenad Ujević Proof. We set Pm (t) = (Γk+1 + γk+1 )/2 in (2.12). Then we have k j (−1) f (x) − Ln (x) − ωn (x) Ej (0)gj [x0 ; x1 ; . . . ; xn ] j! j=1 = |Rk,m (x)| x n t − xi 1 Γk+1 + γk+1 k (k+1) dt . pni (x)(x − xi ) f ≤ − Ek k! i=0 2 x − xi xi ∞ We also have (k+1) Γk+1 + γk+1 ≤ Γk+1 − γk+1 f − 2 2 ∞ and x xi Ek t − xi x − xi 2k! dt ≤ 22k+2 − 1 |x − xi | |B2k+2 |. (2k + 2)! From the above three relations we get k j (−1) f (x) − Ln (x) − ωn (x) Ej (0)gj [x0 ; x1 ; . . . ; xn ] j! j=1 n Γk+1 − γk+1 2k+2 k+1 ≤ 2 − 1 |B2k+2 | |pni (x)| |x − xi | (2k + 2)! i=0 Γk+1 − γk+1 2k+2 = 2 − 1 |B2k+2 |Ck (x) |ωn (x)| . (2k + 2)! The first inequality is proved. We now set Pm (t) = γk+1 in (2.12). Then we have k j (−1) f (x) − Ln (x) − ωn (x) (0)g [x ; x ; . . . ; x ] E j j 0 1 n j! j=1 = |Rk,m (x)| ≤ n x (k+1) 1 t − xi dt . f pni (x)(x − xi )k (t) − γk+1 Ek k! i=0 x − xi xi We also have x (k+1) f (t) − γk+1 dt = f (k) (x) − f (k) (xi ) − γk+1 (x − xi ) xi = (Ski − γk+1 ) |x − xi | . Error inequalities Thus, 79 k j (−1) f (x) − Ln (x) − ωn (x) (0)g [x ; x ; . . . ; x ] E j j 0 1 n j! j=1 n 2k! |B2k+2 | 2k+2 1 k+1 ≤ |pni (x)| |x − xi | (Ski − γk+1 ) 2 −1 k! i=0 (2k + 2)! |ωn (x)| 2k+2 2 − 1 |B2k+2 |Fk (x). = 2 (2k + 2)! The second inequality is proved. The third inequality holds by a similar proof. Lemma 3.1. Let π = {x0 = a < x1 < · · · < xn = b} be a given uniform subdivision of the interval [a, b], i.e., xi = x0 + ih, h = (b − a)/n, i = 0, 1, 2, . . . , n. If x ∈ (xj−1 , xj ), for some j ∈ {1, 2, . . . , n}, then |ωn (x)| ≤ j!(n − j + 1)!hn+1 , (3.6) Ck (x) ≤ (3.7) 2n n! k 1 [n + 1 + |n − 2j + 1|] hk−n , 2 and Ck (x) |ωn (x)| ≤ αjnk (3.8) where αjnk = (3.9) n − j + 1 2n (b − a)k+1 n , n j k 1 (n + 1 + |2j − n − 1|) . 2n Proof. For i < j we have |x − xi | ≤ (j − i)h and for i ≥ j we have |x − xi | ≤ (i − j + 1)h such that |(x − x0 ) · · · (x − xj−1 )(x − xj ) · · · (x − xn )| ≤ j!hj (n − j + 1)!hn−j+1 = j!(n − j + 1)!hn+1 . We have Ck (x) ≤ j−1 n (j − i)k hk (i − j + 1)k hk + i!(n − i)!hn i=j i!(n − i)!hn i=0 j−1 n (n − j + 1)k hk j k hk + i!(n − i)!hn i=j i!(n − i)!hn i=0 n 1 k n k−n k ≤h max j , (n − j + 1) n! i=0 i k 2n 1 [n + 1 + |n − 2j + 1|] hk−n , = n! 2 ≤ 80 Nenad Ujević since 1 (n + 1 + |2j − n − 1|) 2 such that it is not difficult to show that (3.7) holds. Finally, from the above relations we find that (3.8) holds, too. max [j, n − j + 1] = Remark 3.2. Note that αjnk ≤ 1 and αjnk = 1 if and only if j = 1 or j = n. If we choose x ∈ [xj , xj+1 ], j = 0, 1, . . . , n − 1, then we get the factor (j + 1)/n instead of the factor (n − j + 1)/n in (3.8). Theorem 3.3. Under the assumptions of Lemma 3.1 and Theorem 3.2 we have k j (−1) Ej (0) f (x) − Ln (x) − ωn (x) g [x ; x ; . . . ; x ] j 0 1 n j! j=1 ≤ [Γk+1 − γk+1 ] δk αjnk n − j + 1 2n (b − a)k+1 n . n j Proof. The proof follows immediately from Theorem 3.2 and Lemma 3.1. References [1] M. Abramowitz and I. A. 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