ebook img

The $r$-Bell numbers PDF

0.14 MB·
Save to my drive
Quick download
Download
Most books are stored in the elastic cloud where traffic is expensive. For this reason, we have a limit on daily download.

Preview The $r$-Bell numbers

The r-Bell numbers Istva´n Mezo˝1 Department of Applied Mathematics and Probability Theory, Faculty of 0 Informatics, University of Debrecen, Hungary 1 0 2 n Abstract a J 8 ThenotionofgeneralizedBellnumbershasappearedinseveralworksbutthereisno systematic treatise on this topic. In this paper we fill this gap. We discuss the most ] O important combinatorial, algebraic and analytic properties of these numbers which C generalize the similar properties of the Bell numbers. Most of these results seem to . be new. It turns out that in a paper of Whitehead these numbers appeared in a h very different context. In addition, we introduce the so-called r-Bell polynomials. t a m [ Key words: Bell numbers, r-Bell numbers, Stirling numbers, r-Stirling numbers 1991 MSC: 11B73 2 v 7 1 4 4 . 9 1 Introduction 0 9 0 : The B Bell number [11] counts the partitions of a set with n elements. Since v n i n , for a fixed n and k, enumerates the number of partitions of a set with X k r nn eolements consisting k disjoint, nonempty sets, we get immediately that Bn a can be given by the sum n n B = . (1) n k ( ) k=0 X The numbers n are called Stirling numbers of the second kind. The n-th k Bell polynomianl ios n n B (x) = xk. n k ( ) k=0 X Email address: [email protected](Istva´n Mez˝o). URL: http://www.inf.unideb.hu/valseg/dolgozok/mezoistvan/mezoistvan.html (Istva´n Mez˝o). 1 Presentaddress:UniversityofDebrecen,H-4010,Debrecen,P.O.Box12,Hungary Preprint submitted to Elsevier 8 January 2010 These numbers and polynomials have many interesting properties and appear in several combinatorial identities. A comprehensive paper is [11]. There is a more general version of Stirling numbers, the so-called r-Stirling numbers. The number n , for fixed n ≥ k ≥ r, enumerates the partitions k r of a set of n elements nintoo k nonempty, disjoint subsets such that the first r elements are in distinct subsets. A systematic treatment on the r-Stirling numbersisgivenin[4],andadifferent approachisdescribedin[6,7].According to (1), it seems to be natural to define the numbers n n+r B = . (2) n,r (k +r) k=0 r X (It is obvious that B = B , because n = n by the definitions.) n n,0 k k 0 n o n o The very first question is on the meaning of the r-Bell numbers. By (2), B n,r is the number of the partitions of a set with n+r element such that the first r elements are in distinct subsets in each partition. The name of r-Stirling numbers suggests the name for the numbers B : we n,r call them as r-Bell numbers, and the name of the polynomials n n+r B (x) = xk n,r (k +r) k=0 r X will be r-Bell polynomials. Thus B = B (1). n,r n,r As far as we know, this paper is the first one fully devoted to the r-Bell num- bers, although Carlitz [6,7] defined these numbers and proved some identities for them. His original notation was B = B(n,r). n,r 2 Example and tables The following example illuminates again the meaning of the r-Bell numbers. By definition, 4 4 4 B = + + . 2,2 (2) (3) (4) 2 2 2 4 counts the partitions of 4 element into 2 subsets such that the first 2 2 2 neleoment are in distinct subsets: {1,3,4},{2} ; {1},{2,3,4} ; {1,3},{2,4} ; {1,4},{2,3}. 2 4 belongs to the partitions 3 2 n o {1},{2},{3,4} ; {1,3},{2},{4} ; {1,4},{2},{3} ; {1},{2,3},{4} ; {1},{2,4},{3}. Finally, 4 equals to the number of partitions of 4 elements into 4 subsets 4 2 (and trivniaolly, the first two elements are in distinct subsets again): {1},{2},{3},{4}. That is, 4 4 4 B = + + = 4+5+1 = 10 2,2 (2) (3) (4) 2 2 2 is really the number of all partitions of the set {1,2,3,4} such that the first two element are in distinct subsets. The first r-Bell numbers n = 0 n = 1 n = 2 n = 3 n = 4 n = 5 n = 6 r = 0 1 1 2 5 15 52 203 r = 1 1 2 5 15 52 203 877 r = 2 1 3 10 37 151 674 3263 r = 3 1 4 17 77 372 1915 10481 r = 4 1 5 26 141 799 4736 29371 r = 5 1 6 37 235 1540 10427 73013 r = 6 1 7 50 365 2727 20878 163967 The first r-Bell polynomials B (x)=1 0,r B (x)=x+r 1,r B (x)=x2 +(2r+1)x+r2 2,r B (x)=x3 +(3r+3)x2 +(3r2 +3r+1)x+r3 3,r B (x)=x4 +(4r+6)x3 +(6r2 +12r+7)x2 + 4,r (4r3 +6r2 +4r +1)x+r4 3 3 Generating functions We start to derive the properties of r-Bell numbers. First of all, the generating functions are determined. Theorem 3.1 The exponential generating function for the r-Bell polynomials is ∞ zn B (x) = ex(ez−1)+rz. n,r n! n=0 X Proof. Broder [4] gave the double generating function of r-Stirling numbers ∞ n n+r zn xk = ex(ez−1)+rz. (k +r) ! n! n=0 k=0 X X Althoughhedidnotusetheinnersuminthepastofhispaper,theyareexactly 2 our polynomials. We note that this identity is remarked in [6, eq. (3.19)] Corollary 3.2 The r-Bell polynomials can be expressed by the usual Bell ones. n n Bn,r(x) = rk Bn−k(x). k ! k=0 X Proof. In the following steps we use the well known identity for ordinary Bell polynomials: n n Bn(x+y) = Bk(x)Bn−k(y). k ! k=0 X Then the exponential generating function of the r-Bell polynomials can be transformed as ∞ x x zn B + = e(x2+x2)(ez−1)+rz n,r 2 2 n! n=0 (cid:18) (cid:19) X ∞ zn ∞ x zn ∞ x zn = rn B B n n n=0 n!!" n=0 (cid:18)2(cid:19) n!! n=0 (cid:18)2(cid:19) n!!# X X X ∞ zn ∞ x x zn = rn B + n n=0 n!! n=0 (cid:18)2 2(cid:19) n!! X X ∞ n n zn = rk Bn−k(x) , k! ! n! n=0 k=0 X X 2 by the Cauchy product. Comparing the coefficients, the Corollary follows. We remark that the non-polynomial version was proven by Carlitz [6, eq. (3.18)]. 4 In order to determine the ordinary generating function we need some other notions. The falling factorial of a given real number x is denoted and defined by xn = x(x−1)(x−2)···(x−n+1), (n = 1,2,...) (3) and (x)0 = 1, while the rising factorial (a.k.a. Pochhammer symbol) is (x) ≡ xn = x(x+1)(x+2)···(x+n−1) (n = 1,2,...) (4) n with (x) = 1. It is obvious that (1) = n!. Fitting our notations to the theory 0 n of hypergeometric functions introduced immediately, we apply the notation (x) instead of xn. The next transformation formula holds n xn = (−1)n(−x) . (5) n Thehypergeometricfunction(orhypergeometric series) isdefinedbytheseries F a1, a2, ..., ap t = ∞ (a1)k(a2)k···(ap)k tk. p q b1, b2, ..., bq (cid:12)(cid:12)(cid:12)  kX=0 (b1)k(b2)k···(bq)k k!  (cid:12)   (cid:12)  (cid:12) The ordinary generating function ca(cid:12)n be given with this function. Theorem 3.3 The r-Bell polynomials have the generating function ∞ rz−1 −1 1 B (x)zn = F z x . n,r rz −1 ex 1 1 rz+z−1 (cid:12)(cid:12)  nX=0 z (cid:12)  (cid:12)   (cid:12)  (cid:12) (cid:12) Proof. It is known [4] that for the Stirling numbers ∞ n zm zn = (m ≥ r ≥ 0). (m) (1−rz)(1−(r +1)z)···(1−mz) n=0 r X This can be rewritten as ∞ n+r zm zn = . n=m(m+r)r (1−rz)(1−(r +1)z)···(1−(m+r)z) X We transform the denominator using the falling factorial: (1−rz)(1−(r +1)z)···(1−(m+r)z) m+r+1 (1−z)(1−2z)···(1−(m+r)z) zm+1 1 z = = . (1−z)(1−2z)···(1−(r −1)z) (cid:16)1(cid:17)r z Hence (cid:16) (cid:17) ∞ k +r 1 1 r 1 zk = . (m+r) z z 1 m+r+1 k=m r (cid:18) (cid:19) X z (cid:16) (cid:17) 5 Rule (5) and the definitions (3)-(4) give that 1 m+r+1 1 = (−1)m+r+1 − z z (cid:18) (cid:19) (cid:18) (cid:19)m+r+1 1 1 = (−1)m+r+1 − − +r+1 . z z (cid:18) (cid:19)r+1(cid:18) (cid:19)m Consequently, r ∞ n+r 1 1 (−1)m+r+1 zn = z . nX=m(m+r)r z −(cid:16)z1(cid:17)r+1 rz+zz−1 m (cid:16) (cid:17) (cid:16) (cid:17) Since r 1 z z = (−1)r , −(cid:16)1(cid:17) rz −1 z r+1 (cid:16) (cid:17) we get that ∞ n+r −1 (−1)m zn = . nX=m(m+r)r rz −1 rz+zz−1 m Let us multiplication with xm and take a su(cid:16)mmatio(cid:17)n for m over the non- negative integers, ∞ −1 ∞ (−x)m −1 1 B (x)zn = = F −x . n,r rz −1 rz+z−1 rz −1 1 1 rz+z−1 (cid:12)(cid:12)  nX=0 mX=0 z m z (cid:12)  (cid:12)  (cid:16) (cid:17)  (cid:12)  (cid:12) Finally, we apply Kummer’s formula [1, p. 505.] (cid:12) a b−a e−x F x = F −x 1 1 (cid:12)  1 1 (cid:12)  b (cid:12) b (cid:12) (cid:12) (cid:12)  (cid:12)   (cid:12)   (cid:12)   (cid:12)  (cid:12) (cid:12) with b = rz+z−1 and a = rz−1. (cid:12) 2 (cid:12) z z 4 Basic recurrences In an earlier paper of the author [18], the polynomials B (x) were introduced n,r because of a very different reason. These functions were used to study the properties of the r-Stirling numbers and some necessary properties of them were proven in that paper. We repeat those results without proof. Theorem 4.1 We have the next recursive identities: 6 d Bn,r(x)=x dxBn−1,r(x)+Bn−1,r(x) +rBn−1,r(x), ! d exxrBn,r(x)=xdx (exxrBn−1,r(x)). Moreover, all roots of B (x) are real and negative. n,r A straightforward corollary that for a fixed r the constant term of the n-th polynomial is rn: B (0) = rn n,r and that the derivative of an r-Bell polynomial is determined by the relation ∂ B (x) rB (x) B (x) = n+1,r − n,r −B (x). n,r n,r ∂x x x The identity n+r n+r n−1+r = −(r −1) (k +r)r (k +r)r−1 ( k +r )r−1 was proven in [4] and implies the recursive relation Bn,r(x) = Bn,r−1(x)−(r −1)Bn−1,r−1(x). Finally, we cite Carlitz’s identities [6, eq. (3.22-3.23)]: m m+r B = B , (6) n+m,r (j +r) n,r+j j=0 r X m m+r B = (−1)m−j B . n,r+m "j +r# n+j,r j=0 r X Here n is an r-Stirling number of the first kind (see [4,6,7]). m r h i 5 Dobinski’s formula The Bell numbers are involved in Dobinski’s nice formula [9,13,14,19]: 1 ∞ kn B = . n e k! k=0 X Our goal is to generalize this identity to our case. 7 Theorem 5.1 (Dobinski’s formula) The r-Bell polynomials satisfy the i- dentity 1 ∞ (k +r)n B (x) = xk. n,r ex k! k=0 X Consequently, the r-Bell numbers are generated by 1 ∞ (k +r)n B = . n,r e k! k=0 X Proof. The r-Stirling numbers for a fixed n (and r) have the ’horizontal’ gen- erating function [4] n n+r (x+r)n = xk, (k +r) k=0 r X whence, for an arbitrary integer m, (m+r)n m n+r 1 = . m! (k +r) (m−k)! k=0 r X In the next step we multiply both sides with xm and sum from m = 0 to ∞. Then ∞ (m+r)n ∞ m n+r xm n n+r xm = = ex xk . m! (k +r) (m−k)! (k +r) ! m=0 m=0k=0 r k=0 r X X X X 2 We can determine some interesting sum with the aid of r-Bell numbers. For example, we know from the second paragraph that B = 10, so 2,2 1 ∞ (k +2)2 = 10. e k! k=0 X 6 An integral representation In 1885, Cesa`ro [8] found an amazing integral representation of the Bell num- bers (see also [3,5]): B = 2n! Im πeeeiθ sin(nθ)dθ. n πe Z0 It is not hard to deduce the ’r-Bell version’. Theorem 6.1 The r-Bell numbers have the integral representation as B = 2n! Im πeeeiθereiθ sin(nθ)dθ. n,r πe Z0 8 Proof. In [6] we find that n+r k k k! = (−1)k−j (j +r)n. (7) (k +r) j! r j=0 X In [5] the next equality appears: π πjn Im ejeiθ sin(nθ)dθ = . (8) 2 n! Z0 Unifying the equations (7)-(8), we get that π 1 n+r 1 k k π = (−1)k−j Im e(j+r)eiθ sin(nθ)dθ 2 n!(k +r)r k! j=0 j! Z0 X = 1 Im π k (−1)k−j k eeiθ j ereiθ sin(nθ)dθ k! Z0 jX=0 j!(cid:16) (cid:17)  π eeiθ −1 k  =Im ereiθ sin(nθ)dθ, (cid:16) k! (cid:17) Z0 whence ∞ n+r 2n! π ∞ eeiθ −1 k = Im ereiθ sin(nθ)dθ, k=0(k +r)r π Z0 k=0 (cid:16) k! (cid:17)  X X     2 and the result follows. Remark 6.2 The imaginary part of the above integral can be calculated with a bit of effort. The result is 2n! π B = eecosθcossinθ+rcosθ· n,r πe Z0 · cos(ecosθsinsinθ)sin(rsinθ)+sin(ecosθsinsinθ)cos(rsinθ) sin(nθ)dθ. h i Without the r-Bellnumbers in background, the evaluation of this integral seems to be impossible... Citing the general version of Dobinski’sformula we find the compellingidentity ∞ (k +r)n = 2n! Im πeeeiθereiθ sin(nθ)dθ. k! π k=0 Z0 X 9 7 Hankel transformation and log-convexity Since ∞ tn et B (x) = ex(et−1)+(r+1)t, n,r n! n=0 X Cauchy’s product immediately implies the next Theorem 7.1 The r-Bell polynomials satisfy the relations n n B (x)= B (x), n,r+1 k k,r ! k=0 X n n B (x)= (−1)n−kB (x). n,r k k,r+1 ! k=0 X Aninteresting corollaryisconnected withthenotionof Hankel transform. The H Hankel matrix [15] of an integer sequence (a ) is n a a a a ··· 0 1 2 3   a a a a ··· 1 2 3 4 H =  ,   a a a a ···  2 3 4 5   ... ... ... ... ...       while the Hankel matrix of order n, denoted by h , is the upper-left submatrix n of H of size n × n. The Hankel transform of the sequence (a ) is again a n sequence formed by the determinants of the matrices h . n A notable result of Aigner and Lenard [2,16] is that the Hankel transform of the sequence of Bell numbers is (1!,1!2!,1!2!3!,...), that is, for any fixed n, B B B ··· B 0 1 2 n (cid:12) (cid:12) (cid:12)B B B ··· B (cid:12) n (cid:12) 1 2 3 n+1(cid:12) (cid:12) . . . . (cid:12) = i! (cid:12) . . . . (cid:12) (cid:12) . . . . (cid:12) i=0 (cid:12) (cid:12) Y (cid:12) (cid:12) (cid:12)B B B ··· B (cid:12) (cid:12) n n+1 n+2 2n (cid:12) (cid:12) (cid:12) (cid:12) (cid:12) (cid:12) (cid:12) (cid:12) (cid:12) We can determine the Hankel transform of r-Bell numbers easily. To reach this aim, we recall an other notion. If (a ) is a sequence, then its binomial n 10

See more

The list of books you might like

Most books are stored in the elastic cloud where traffic is expensive. For this reason, we have a limit on daily download.