1 Introduction
A finite sequence $\mathbf {k}=(k_1,\ldots ,k_n)$ of positive integers is called an index. The weight, depth and height of the index $\mathbf {k}$ are defined respectively by $k_1{\kern-1.5pt}+\cdots +k_n$ , n and the cardinality $|\{\,j\mid 1\leq j\leq n, k_j\geq 2\}|$ . If $k_1>1$ , the index $\mathbf {k}$ is called admissible. For an admissible index $\mathbf {k}=(k_1,\ldots ,k_n)$ , the multiple zeta value $\zeta (\mathbf {k})$ and the multiple zeta-star value $\zeta ^{\star }(\mathbf {k})$ are defined respectively by
A systematic study of multiple zeta values was carried out by Hoffman [Reference Hoffman2] and Zagier [Reference Zagier, Joseph, Mignot, Murat, Prum and Rentschler10]. More results of multiple zeta values can be found in the book [Reference Zhao11] of Zhao.
We focus on Ohno–Zagier type relations. For nonnegative integers $k,n,s$ , denote by $I_0(k,n,s)$ the set of admissible indices of weight k, depth n and height s. It is easy to see that $I_0(k,n,s)$ is nonempty if and only if $k\geq n+s$ and $n\geq s\geq 1$ . Using the Gaussian hypergeometric function, Ohno and Zagier proved in [Reference Ohno and Zagier7] that
where $\alpha $ and $\beta $ are determined by $\alpha +\beta =u+v$ and $\alpha \beta =w$ . Similar studies were carried out on various generalisations of multiple zeta values. For example, Aoki et al. [Reference Aoki, Kombu and Ohno1] gave a similar formula for the sums of multiple zeta-star values involving the generalised hypergeometric function ${}_3F_2$ :
with $\alpha $ and $\beta $ determined by $\alpha +\beta =u+v$ and $\alpha \beta =uv-w^2$ . Here, for a positive integer m and complex numbers $a_1,\ldots ,a_{m+1},b_1,\ldots ,b_m$ with $b_1,\ldots ,b_m\neq 0,-1,-2,\ldots ,$ the generalised hypergeometric function ${}_{m+1}F_m$ is defined by
with the Pochhammer symbol $(a)_n$ defined by
It is known that this formal power series converges absolutely for $|z|<1$ , and it also converges absolutely for $|z|=1$ if $\Re (\sum b_i-\sum a_i)>0$ . If $m=1$ , we get the Gaussian hypergeometric function.
In [Reference Takeyama9], Takeyama studied the Ohno–Zagier type relation for a level two variant of multiple zeta values, called multiple T-values, introduced by Kaneko and Tsumura [Reference Kaneko, Tsumura, Mishou, Nakamura, Suzuki and Umegaki6]. As a consequence, a weighted sum formula of multiple T-values with fixed weight and depth was given in [Reference Takeyama9]. We consider another level two variant of multiple zeta values, called multiple t-values, introduced by Hoffman in [Reference Hoffman3].
For an admissible index $\mathbf {k}=(k_1,\ldots ,k_n)$ , the multiple t-value $t(\mathbf {k})$ and the multiple t-star value $t^{\star }(\mathbf {k})$ are defined respectively by
It is easy to obtain the following iterated integral representations:
where $({dt}/{t})^{k_i-1}={{dt}/{t}\cdots {dt}/{t}}\ (k_i-1 \mbox { factors})$ , and for one-forms $\omega _i(t)=f_i(t)dt$ , $i=1,2,\ldots ,k$ , we define the iterated integral
We want to study the sum of multiple t-(star) values with fixed weight, depth and height. For nonnegative integers $k,n,s$ , define
Then we obtain Ohno–Zagier type relations which represent the generating functions of $G_0(k,n,s)$ and $G_0^{\star }(k,n,s)$ by the generalised hypergeometric function ${}_3F_2$ .
Theorem 1.1. For formal variables $u,v,w$ ,
where $\alpha $ and $\beta $ are determined by $\alpha +\beta {\kern-1pt}={\kern-1pt}1-\frac{1}{2}u+\frac{1}{2}v$ and $\alpha \beta {\kern-1pt}={\kern-1pt}\tfrac 14(1{\kern-1pt}-{\kern-1pt}u+v- uv+w)$ .
Theorem 1.2. For formal variables $u,v,w$ ,
where $\alpha ^{\star }$ and $\beta ^{\star }$ are determined by $\alpha ^{\star }+\beta ^{\star }=3-\frac{1}{2}u-\frac{1}{2}v$ and $\alpha \beta =\tfrac 14(9-3u-3v+uv-w)$ .
From these theorems and using summation formulae for $\,_3F_2$ , we obtain several corollaries in Section 2. For example, we give a formula for the generating function of sums of multiple t-(star) values of maximal height and a weighted sum formula of sums of multiple t-(star) values with fixed weight and depth. Finally, we prove Theorems 1.1 and 1.2 in Section 3.
2 Applications
2.1 Sums of height one
To save space, we denote a sequence of k repeated n times by $\{k\}^n$ .
Setting $w=0$ in Theorem 1.1,
Hence, we get the following result, which gives the generating function of height one multiple t-values.
Corollary 2.1 [Reference Hoffman3, Theorem 5.1]
We have
Similarly, setting $w=0$ in Theorem 1.2,
Therefore, we obtain the generating function of height one multiple t-star values.
Corollary 2.2. We have
Note that using [Reference Hoffman3, Lemma 5.2], for any integer $m\geq 2$ ,
2.2 Sums of maximal height
Setting $v=0$ in Theorem 1.1, we get the generating function of sums of multiple t-values of maximal height. By the symmetric sum formula [Reference Hoffman3, Theorem 3.2], the sum of multiple t-values with fixed weight, depth and maximal height can be represented by t-values. Here we give a closed formula for the generating function of the sums of maximal height.
Corollary 2.3. For formal variables $u,w$ ,
where x and y are determined by $x+y=u$ and $xy=w$ .
Proof. Setting $v=0$ in Theorem 1.1, we get $\alpha +\beta =1-\frac{1}{2}u$ and $\alpha \beta =\tfrac 14(1-u+w)$ . Let $x=1-2\alpha $ and $y=1-2\beta $ , then $x+y=u$ and $xy=w$ . Using the summation formula [Reference Prudnikov, Brychkov and Marichev8, 7.4.4.28],
With $a=\alpha $ , $b=\beta $ and $c=\tfrac 32$ ,
Using the duplication formula
and the expansion
where $\gamma $ is Euler’s constant,
Since $t(n)=(1-2^{-n})\zeta (n)$ , we find that (see also [Reference Hoffman3, Theorem 3.3])
Now it is easy to finish the proof.
Similarly, we have a formula for the generating function of the sums of multiple t-star values of maximal height.
Corollary 2.4. For formal variables $u,w$ ,
where $x^{\star }$ and $y^{\star }$ are determined by $x^{\star }+y^{\star }=u$ and $x^{\star }y^{\star }=-w$ .
Proof. Setting $v=0$ in Theorem 1.2, we obtain $\alpha ^{\star }+\beta ^{\star }=3-\frac{1}{2}u$ and $\alpha ^{\star }\beta ^{\star }=\tfrac 14 (9-3u-w)$ . Let $x^{\star }=3-2\alpha ^{\star }$ and $y^{\star }=3-2\beta ^{\star }$ , so that $x^{\star }+y^{\star }=u$ and $x^{\star }y^{\star }=-w$ . Using the summation formula (2.2) with $a=\frac{1}{2}(1-u)$ , $b=\tfrac 12$ and $c=\alpha ^{\star }$ ,
Now the result follows from (2.4).
Also, setting $u=0$ in (2.1) and (2.5),
These formulae can also be deduced from the identities [Reference Ihara, Kajikawa, Ohno and Okuda4, Reference Ihara, Kaneko and Zagier5]
in the harmonic shuffle algebra.
2.3 A weighted sum formula
Let $I_0(k,n)$ be the set of admissible indices of weight k and depth n, and define
which are the sums of multiple t-values and multiple t-star values with fixed weight k and depth n, respectively. By setting $w=uv$ and then $v=2u$ or $v=-2u$ in Theorems 1.1 and 1.2, we obtain the following results.
Proposition 2.5. For a formal variable u,
Proof. If $w=uv$ in Theorem 1.1,
Hence, we get the expression for the generating function of sums of multiple t-values with fixed weight and depth:
Setting $v=2u$ ,
Using Dixon’s summation formula [Reference Prudnikov, Brychkov and Marichev8, 7.4.4.21]: for $\Re (a-2b-2c)>-2$ ,
with $a=1$ , $b=\tfrac 12$ and $c=\frac{1}{2}(1+u)$ , we get
Then using (2.3), (2.4), the relation $\zeta (n)=(1-2^{-n})^{-1}t(n)$ and $t(2)={\pi ^2}/{8}$ , we get
Similarly, setting $w=uv$ in Theorem 1.2,
Hence,
Let $v=-2u$ . Then
Now it is easy to finish the proof.
Expanding the right-hand side of (2.6) gives the following weighted sum formula.
Corollary 2.6. For any integer $k\geq 2$ ,
3 Proofs of Theorems 1.1 and 1.2
The proofs of Theorems 1.1 and 1.2 are similar to that of the Ohno–Zagier relation for multiple zeta values in [Reference Ohno and Zagier7].
As in [Reference Hoffman3], for an index $\mathbf {k}=(k_1,\ldots ,k_n)$ , define
Then $\mathcal {L}_{\mathbf {k}}(z)$ and $\mathcal {L}_{\mathbf {k}}^{\star }(z)$ converge absolutely for $|z|<1$ . If $k_1>1$ , $\mathcal {L}_{\mathbf {k}}(1)=t(\mathbf {k})$ and $\mathcal {L}_{\mathbf {k}}^{\star }(1)=t^{\star }(\mathbf {k})$ . From [Reference Hoffman3, Lemma 5.1],
Similarly,
One can also obtain (3.1) and (3.2) from the following iterated integral representations:
3.1 Proof of Theorem 1.1
For nonnegative integers $k,n,s$ , denote by $I(k,n,s)$ the set of indices of weight k, depth n and height s, and define the sums
If the index set is empty, the sum is treated as zero. We also set $G(0,0,0;z)=1$ . Note that if $k\geq n+s$ and $n\geq s\geq 1$ ,
For integers $k,n,s$ , using (3.1), we have the following identities:
-
(1) if $k\geq n+s$ and $n\geq s\geq 1$ ,
(3.3) $$ \begin{align} \frac{d}{dz} & G_0(k,n,s;z) \nonumber\\ & =\frac{1}{z}[G(k-1,n,s-1;z)+G_0(k-1,n,s;z)-G_0(k-1,n,s-1;z)]; \end{align} $$ -
(2) if $k\geq n+s$ , $n\geq s\geq 0$ and $n\geq 2$ ,
(3.4) $$ \begin{align} \frac{d}{dz}[G(k,n,s;z)-G_0(k,n,s;z)]=\frac{z}{1-z^2}G(k-1,n-1,s;z). \end{align} $$
We define the generating functions
Eliminating $\Phi (z)$ , we obtain the differential equation satisfied by $\Phi _0(z)$ .
Proposition 3.1. $\Phi _0=\Phi _0(z)$ satisfies the following differential equation:
We want to find the unique power series solution $\Phi _0(z)=\sum _{n=1}^\infty a_nz^n$ . From (3.5), we see that $a_1={1}/({1-u})$ , $a_2=0$ and
Hence, for any $n\geq 1$ , we have $a_{2n}=0$ and
Since $(\alpha -1)+(\,\beta -1)=-1-\frac{1}{2}u+\frac{1}{2}v$ and $(\alpha -1)(\,\beta -1)=\tfrac 14(1+u-v-uv+w)$ ,
Therefore, we can represent $\Phi _0(z)$ by the generalised hypergeometric function $\,_3F_2$ as displayed in the following theorem.
Theorem 3.2. We have
3.2 Proof of Theorem 1.2
Similarly, for nonnegative integers $k,n,s$ , we define the sums
with $G^{\star }(0,0,0;z)=1$ . Using (3.2), we have the following identities:
-
(1) if $k\geq n+s$ and $n\geq s\geq 1$ ,
(3.6) $$ \begin{align} &\frac{d}{dz} G_0^{\star}(k,n,s;z)\nonumber\\ &\quad =\frac{1}{z}[G^{\star}(k-1,n,s-1;z)+G_0^{\star}(k-1,n,s;z)-G_0^{\star}(k-1,n,s-1;z)]; \end{align} $$ -
(2) if $k\geq n+s$ , $n\geq s\geq 0$ and $n\geq 2$ ,
(3.7) $$ \begin{align} \frac{d}{dz}[G^{\star}(k,n,s;z)-G_0^{\star}(k,n,s;z)]=\frac{1}{z(1-z^2)}G^{\star}(k-1,n-1,s;z). \end{align} $$
We define the generating functions
Then using (3.2), (3.6) and (3.7),
Eliminating $\Phi ^{\star }(z)$ , we get the differential equation satisfied by $\Phi _0^{\star }(z)$ .
Proposition 3.3. $\Phi _0^{\star }=\Phi _0^{\star }(z)$ satisfies the following differential equation:
Assume that $\Phi _0^{\star }(z){\kern-1pt}={\kern-2pt}\sum _{n=1}^\infty{\kern-1pt} a_n^{\star }z^n$ . Using (3.8), we find that $a_1^{\star }{\kern-1pt}={\kern-1pt}{1}/({1{\kern-1pt}-{\kern-1pt}u{\kern-1pt}-{\kern-1pt}v+uv{\kern-1pt}-{\kern-1pt}w})$ , $a_2^{\star }=0$ and
Hence, for any $n\geq 1$ , we have $a_{2n}^{\star }=0$ and
Therefore, we have the following theorem.
Theorem 3.4. We have