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Research article

Simplifying coefficients in differential equations associated with higher order Bernoulli numbers of the second kind

  • Received: 21 December 2018 Accepted: 14 February 2019 Published: 19 February 2019
  • MSC : Primary 34A05; Secondary 11A25, 11B68, 11B73, 11B83

  • In the paper, by virtue of the Faà di Bruno formula, some properties of the Bell polynomials of the second kind, and an inversion formula for the Stirling numbers of the first and second kinds, the authors establish meaningfully and significantly two identities which simplify coefficients in a family of ordinary differential equations associated with higher order Bernoulli numbers of the second kind.

    Citation: Feng Qi, Da-Wei Niu, Bai-Ni Guo. Simplifying coefficients in differential equations associated with higher order Bernoulli numbers of the second kind[J]. AIMS Mathematics, 2019, 4(2): 170-175. doi: 10.3934/math.2019.2.170

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  • In the paper, by virtue of the Faà di Bruno formula, some properties of the Bell polynomials of the second kind, and an inversion formula for the Stirling numbers of the first and second kinds, the authors establish meaningfully and significantly two identities which simplify coefficients in a family of ordinary differential equations associated with higher order Bernoulli numbers of the second kind.


    In [2,Theorem 1], it was inductively and recursively established that the family of differential equations

    (1)n(r)nF(t)=[ln(1+t)]nni=1ai(n)(1+t)iF(i)(t),nN (1)

    has a solution

    F(t)=F(t,r)=[1ln(1+t)]r,rN, (2)

    where a1(n)=1 and

    ai(n)=niki1=0niki1ki2=0niki1k2k1=0i=2k1,2in. (3)

    Let

    (x)n=n1=0(x+)={x(x+1)(x+2)(x+n1),n11,n=0

    and

    xn=n1=0(x)={x(x1)(x2)(xn+1),n11,n=0

    be the rising and falling factorials of xR for n{0}N. Let b(r)n for rN, generated by

    [tln(1+t)]r=n=0b(r)ntnn!,

    stand for the Bernoulli numbers of the second kind with order r. Theorem 2 in [2] reads that, if n=0,1,2, and N=1,2,3,, then

    1. for 0n<N+r,

    (1)N(r)Nb(r+N)n=min{N1,n}i=0n=max{i,nr+1}(Nii)nrNinaNi(N)b(r)n;

    2. for nN+r,

    (1)N(r)Nb(r+N)n=(min{n,N1}i=0n=max{i,nr+1}+N1i=0nNr+i=i)(Nii)nrNinaNi(N)b(r)n.

    It is not difficult to see that the expression (3) of the quantity ai(n) is too complicated to be computed by hand and computer software. Can one find a simple, meaningful, and significant expression for the quantity ai(n) in (3)?

    For answering the above question and proving our main results, we need the following lemmas.

    Lemma 1. ([1,p. 134,Theorem A] and [1,p. 139,Theorem C]) For nk0, the Bell polynomials of the second kind, or say, partial Bell polynomials, denoted by Bn,k(x1,x2,,xnk+1), are defined by

    Bn,k(x1,x2,,xnk+1)=1ink+1,i{0}Nnk+1i=1ii=n,nk+1i=1i=kn!nk+1i=1i!nk+1i=1(xii!)i.

    The Faà di Bruno formula can be described in terms of the Bell polynomials of the second kind Bn,k by

    dndtnfh(t)=nk=0f(k)(h(t))Bn,k(h(t),h (4)

    Lemma 2. [1,p. 135] For n\ge k\ge0 , we have

    \begin{equation} \text{B}_{n,k}\bigl(abx_1,ab^2x_2,\dotsc,ab^{n-k+1}x_{n-k+1}\bigr) = a^kb^n \text{B}_{n,k}(x_1,x_2,\dotsc,x_{n-k+1}) \end{equation} (5)

    and

    \begin{equation} \text{B}_{n,k}(0!,1!,2!,\dotsc,(n-k)!) = (-1)^{n-k}s(n,k), \end{equation} (6)

    where a and b are any complex numbers and s(n, k) for n\ge k\ge0 , which can be generated by

    \begin{equation*} \frac{[\ln(1+x)]^k}{k!} = \sum\limits_{n = k}^\infty s(n,k)\frac{x^n}{n!},\quad |x| \lt 1, \end{equation*}

    stand for the Stirling numbers of the first kind.

    Lemma 3. [26,p. 171,Theorem 12.1] If b_\alpha and a_k are a collection of constants independent of n , then

    \begin{equation*} a_n = \sum\limits_{\alpha = 0}^{n}S(n,\alpha)b_\alpha \quad if \;and \;only\; if \quad b_n = \sum\limits_{k = 0}^{n}s(n,k)a_k, \end{equation*}

    where S(n, k) for n\ge k\ge0 , which can be generated by

    \begin{equation*} \frac{(e^x-1)^k}{k!} = \sum\limits_{n = k}^\infty S(n,k)\frac{x^n}{n!}, \end{equation*}

    stand for the Stirling numbers of the second kind.

    Now we are in a position to answer the above question and to state and prove our main results.

    Theorem 1. For n\ge0 and r\in\mathbb{R} , the function F(t) = F(t, r) defined by (2) satisfies

    \begin{equation} F^{(n)}(t) = \biggl(\frac{1}{1+t}\biggr)^{n} \Biggl[\sum\limits_{k = 0}^{n}s(n,k)\frac{\langle-r\rangle_k}{[\ln(1+t)]^k}\Biggr]F(t) \quad and \quad \sum\limits_{k = 0}^{n}S(n,k)(1+t)^kF^{(k)}(t) = \frac{\langle-r\rangle_n}{[\ln(1+t)]^n}F(t). \end{equation} (7)

    Proof. Let u = u(t) = \ln(1+t) and r\in\mathbb{R} . Then, by virtue of the Faà di Bruno formula (4) and the identities (5) and (6) in sequence,

    \begin{align*} F^{(n)}(t)& = \sum\limits_{k = 0}^{n}\bigl(u^{-r}\bigr)^{(k)} \text{B}_{n,k}\biggl(\frac{0!}{1+t}, -\frac{1!}{(1+t)^2},\dotsc,(-1)^{n-k}\frac{(n-k)!}{(1+t)^{n-k+1}}\biggr)\\ & = \sum\limits_{k = 0}^{n}\frac{\langle-r\rangle_k}{u^{r+k}} \biggl(\frac{1}{1+t}\biggr)^{n} (-1)^{n+k} \text{B}_{n,k}(0!,1!,\dotsc,(n-k)!)\\ & = \sum\limits_{k = 0}^{n}\frac{\langle-r\rangle_k}{[\ln(1+t)]^{r+k}} \biggl(\frac{1}{1+t}\biggr)^{n} (-1)^{n+k} (-1)^{n-k}s(n,k) \end{align*}

    for n\ge0 . Thus, the first identity in (7) is proved.

    Applying Lemma 3 to the first equality in (7) leads to

    \begin{equation*} \frac{\langle-r\rangle_n}{[\ln(1+t)]^n}F(t) = \sum\limits_{k = 0}^{n}S(n,k)(1+t)^kF^{(k)}(t) \end{equation*}

    which can be rewritten as the second equality in (7). The required proof is complete.

    Corollary 1. Comparing (1) with two equalities in (7) reveals that

    \begin{equation} a_i(n) = S(n,i), \quad n\ge i\ge0. \end{equation} (8)

    This implies that the second identity in (7) is more meaningful, more significant, more computable than (1).

    In this section, we give several remarks and some explanation about our main results.

    Remark 1. Theorem 1 extends the range of r from \mathbb{N} to \mathbb{R} .

    Remark 2. By virtue of the expression (8), all the above mentioned results in the paper [2] can be reformulated simpler, more meaningfully, and more significantly. For the sake of saving the space and shortening the length of this paper, we do not rewrite them in details here.

    Remark 3. Currently we can see that the method used in this paper is simpler, shorter, nicer, more meaningful, and more significant than the inductive and recursive method used in [2] and closely related references therein.

    Remark 4. In the papers [5,8,24,25], there are some new results about the Bernoulli numbers of the second kind.

    Remark 5. In the papers [3,4,6,7,9,10,11,12,13,14,15,16,17,18,20,21,22,23,25,27], there are similar ideas, methods, techniques, and purposes to this paper.

    Remark 6. This paper is a slightly revised version of the preprint [19].

    The authors are thankful to Professors Dmitry V. Dolgy (Far Eastern State University, Russia) and Taekyun Kim (Kwangwoon University, South Korea) for their supplying an electronic version of the paper [2] through e-mail on 3 August 2017. The authors are grateful to anonymous referees for their careful corrections to and valuable comments on the original version of this paper.

    The authors declare no conflict of interest.



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