In the particular case of only two parameters we have (with s>1 and n,m integer):
ζ
(
s
,
t
)
=
∑
n
>
m
≥
1
1
n
s
m
t
=
∑
n
=
2
∞
1
n
s
∑
m
=
1
n
−
1
1
m
t
=
∑
n
=
1
∞
1
(
n
+
1
)
s
∑
m
=
1
n
1
m
t
ζ
(
s
,
t
)
=
∑
n
=
1
∞
H
n
,
t
(
n
+
1
)
s
where
H
n
,
t
are the generalized harmonic numbers.
Multiple zeta functions are known to satisfy what is known as MZV duality, the simplest case of which is the famous identity of Euler:
∑
n
=
1
∞
H
n
(
n
+
1
)
2
=
ζ
(
2
,
1
)
=
ζ
(
3
)
=
∑
n
=
1
∞
1
n
3
,
where Hn are the harmonic numbers.
Special values of double zeta functions, with s > 0 and even, t > 1 and odd, but s+t=2N+1 (taking if necessary ζ(0) = 0):
ζ
(
s
,
t
)
=
ζ
(
s
)
ζ
(
t
)
+
1
2
[
(
s
+
t
s
)
−
1
]
ζ
(
s
+
t
)
−
∑
r
=
1
N
−
1
[
(
2
r
s
−
1
)
+
(
2
r
t
−
1
)
]
ζ
(
2
r
+
1
)
ζ
(
s
+
t
−
1
−
2
r
)
Note that if
s
+
t
=
2
p
+
2
we have
p
/
3
irreducibles, i.e. these MZVs cannot be written as function of
ζ
(
a
)
only.
In the particular case of only three parameters we have (with a>1 and n,j,i integer):
ζ
(
a
,
b
,
c
)
=
∑
n
>
j
>
i
≥
1
1
n
a
j
b
i
c
=
∑
n
=
1
∞
1
(
n
+
2
)
a
∑
j
=
1
n
1
(
j
+
1
)
b
∑
i
=
1
j
1
(
i
)
c
=
∑
n
=
1
∞
1
(
n
+
2
)
a
∑
j
=
1
n
H
i
,
c
(
j
+
1
)
b
The above MZVs satisfy the Euler reflection formula:
ζ
(
a
,
b
)
+
ζ
(
b
,
a
)
=
ζ
(
a
)
ζ
(
b
)
−
ζ
(
a
+
b
)
for
a
,
b
>
1
Using the shuffle relations, it is easy to prove that:
ζ
(
a
,
b
,
c
)
+
ζ
(
a
,
c
,
b
)
+
ζ
(
b
,
a
,
c
)
+
ζ
(
b
,
c
,
a
)
+
ζ
(
c
,
a
,
b
)
+
ζ
(
c
,
b
,
a
)
=
ζ
(
a
)
ζ
(
b
)
ζ
(
c
)
+
2
ζ
(
a
+
b
+
c
)
−
ζ
(
a
)
ζ
(
b
+
c
)
−
ζ
(
b
)
ζ
(
a
+
c
)
−
ζ
(
c
)
ζ
(
a
+
b
)
for
a
,
b
,
c
>
1
This function can be seen as a generalization of the reflection formulas.
Let
S
(
i
1
,
i
2
,
⋯
,
i
k
)
=
∑
n
1
≥
n
2
≥
⋯
n
k
≥
1
1
n
1
i
1
n
2
i
2
⋯
n
k
i
k
, and for a partition
Π
=
{
P
1
,
P
2
,
…
,
P
l
}
of the set
{
1
,
2
,
…
,
k
}
, let
c
(
Π
)
=
(
|
P
1
|
−
1
)
!
(
|
P
2
|
−
1
)
!
⋯
(
|
P
l
|
−
1
)
!
. Also, given such a
Π
and a k-tuple
i
=
{
i
1
,
.
.
.
,
i
k
}
of exponents, define
∏
s
=
1
l
ζ
(
∑
j
∈
P
s
i
j
)
.
The relations between the
ζ
and
S
are:
S
(
i
1
,
i
2
)
=
ζ
(
i
1
,
i
2
)
+
ζ
(
i
1
+
i
2
)
and
S
(
i
1
,
i
2
,
i
3
)
=
ζ
(
i
1
,
i
2
,
i
3
)
+
ζ
(
i
1
+
i
2
,
i
3
)
+
ζ
(
i
1
,
i
2
+
i
3
)
+
ζ
(
i
1
+
i
2
+
i
3
)
For any real
i
1
,
⋯
,
i
k
>
1
,
,
∑
σ
∈
∑
k
S
(
i
σ
(
1
)
,
…
,
i
σ
(
k
)
)
=
∑
partitions
Π
of
{
1
,
…
,
k
}
c
(
Π
)
ζ
(
i
,
Π
)
.
Proof. Assume the
i
j
are all distinct. (There is not loss of generality, since we can take limits.) The left-hand side can be written as
∑
σ
∑
n
1
≥
n
2
≥
⋯
≥
n
k
≥
1
1
n
i
1
σ
(
1
)
n
i
2
σ
(
2
)
⋯
n
i
k
σ
(
k
)
. Now thinking on the symmetric
group
∑
k
as acting on k-tuple
n
=
(
1
,
⋯
,
k
)
of positive integers. A given k-tuple
n
=
(
n
1
,
⋯
,
n
k
)
has an isotropy group
∑
k
(
n
)
and an associated partition
Λ
of
(
1
,
2
,
⋯
,
k
)
:
Λ
is the set of equivalence classes of the relation given by
i
∼
j
iff
n
i
=
n
j
, and
∑
k
(
n
)
=
{
σ
∈
∑
k
:
σ
(
i
)
∼
∀
i
}
. Now the term
1
n
i
1
σ
(
1
)
n
i
2
σ
(
2
)
⋯
n
i
k
σ
(
k
)
occurs on the left-hand side of
∑
σ
∈
∑
k
S
(
i
σ
(
1
)
,
…
,
i
σ
(
k
)
)
=
∑
partitions
Π
of
{
1
,
…
,
k
}
c
(
Π
)
ζ
(
i
,
Π
)
exactly
|
∑
k
(
n
)
|
times. It occurs on the right-hand side in those terms corresponding to partitions
Π
that are refinements of
Λ
: letting
⪰
denote refinement,
1
n
i
1
σ
(
1
)
n
i
2
σ
(
2
)
⋯
n
i
k
σ
(
k
)
occurs
∑
Π
⪰
Λ
(
Π
)
times. Thus, the conclusion will follow if
|
∑
k
(
n
)
|
=
∑
Π
⪰
Λ
c
(
Π
)
for any k-tuple
n
=
{
n
1
,
⋯
,
n
k
}
and associated partition
Λ
. To see this, note that
c
(
Π
)
counts the permutations having cycle-type specified by
Π
: since any elements of
∑
k
(
n
)
has a unique cycle-type specified by a partition that refines
Λ
, the result follows.
For
k
=
3
, the theorem says
∑
σ
∈
∑
3
S
(
i
σ
(
1
)
,
i
σ
(
2
)
,
i
σ
(
3
)
)
=
ζ
(
i
1
)
ζ
(
i
2
)
ζ
(
i
3
)
+
ζ
(
i
1
+
i
2
)
ζ
(
i
3
)
+
ζ
(
i
1
)
ζ
(
i
2
+
i
3
)
+
ζ
(
i
1
+
i
3
)
ζ
(
i
2
)
+
2
ζ
(
i
1
+
i
2
+
i
3
)
for
i
1
,
i
2
,
i
3
>
1
. This is the main result of.
Having
ζ
(
i
1
,
i
2
,
⋯
,
i
k
)
=
∑
n
1
>
n
2
>
⋯
n
k
≥
1
1
n
1
i
1
n
2
i
2
⋯
n
k
i
k
. To state the analog of Theorem 1 for the
ζ
′
s
, we require one bit of notation. For a partition
Π
=
{
P
1
,
⋯
,
P
l
}
or
{
1
,
2
⋯
,
k
}
, let
c
~
(
Π
)
=
(
−
1
)
k
−
l
c
(
Π
)
.
For any real
i
1
,
⋯
,
i
k
>
1
,
∑
σ
∈
∑
k
ζ
(
i
σ
(
1
)
,
…
,
i
σ
(
k
)
)
=
∑
partitions
Π
of
{
1
,
…
,
k
}
c
~
(
Π
)
ζ
(
i
,
Π
)
.
Proof. We follow the same line of argument as in the preceding proof. The left-hand side is now
∑
σ
∑
n
1
>
n
2
>
⋯
>
n
k
≥
1
1
n
i
1
σ
(
1
)
n
i
2
σ
(
2
)
⋯
n
i
k
σ
(
k
)
, and a term
1
n
1
i
1
n
2
i
2
⋯
n
k
i
k
occurs on the left-hand since once if all the
n
i
are distinct, and not at all otherwise. Thus, it suffices to show
∑
Π
⪰
Λ
c
~
(
Π
)
=
{
1
,
if
|
Λ
|
=
k
0
,
otherwise
.
(1)
To prove this, note first that the sign of
c
~
(
Π
)
is positive if the permutations of cycle-type
Π
are even, and negative if they are odd: thus, the left-hand side of (1) is the signed sum of the number of even and odd permutations in the isotropy group
∑
k
(
n
)
. But such an isotropy group has equal numbers of even and odd permutations unless it is trivial, i.e. unless the associated partition
Λ
is
{
{
1
}
,
{
2
}
,
⋯
,
{
k
}
}
.
The sum and duality conjectures
We first state the sum conjecture, which is due to C. Moen.
Sum conjecture(Hoffman). For positive integers k and n,
∑
i
1
+
⋯
+
i
k
=
n
,
i
1
>
1
ζ
(
i
1
,
⋯
,
i
k
)
=
ζ
(
n
)
, where the sum is extended over k-tuples
i
1
,
⋯
,
i
k
of positive integers with
i
1
>
1
.
Three remarks concerning this conjecture are in order. First, it implies
∑
i
1
+
⋯
+
i
k
=
n
,
i
1
>
1
S
(
i
1
,
⋯
,
i
k
)
=
(
n
−
1
k
−
1
)
ζ
(
n
)
. Second, in the case
k
=
2
it says that
ζ
(
n
−
1
,
1
)
+
ζ
(
n
−
2
,
2
)
+
⋯
+
ζ
(
2
,
n
−
2
)
=
ζ
(
n
)
, or using the relation between the
ζ
′
s
and
S
′
s
and Theorem 1,
2
S
(
n
−
1
,
1
)
=
(
n
+
1
)
ζ
(
n
)
−
∑
k
=
2
n
−
2
ζ
(
k
)
ζ
(
n
−
k
)
.
This was proved by Euler's paper and has been rediscovered several times, in particular by Williams. Finally, C. Moen has proved the same conjecture for k=3 by lengthy but elementary arguments. For the duality conjecture, we first define an involution
τ
on the set
ℑ
of finite sequences of positive integers whose first element is greater than 1. Let
T
be the set of strictly increasing finite sequences of positive integers, and let
Σ
:
ℑ
→
T
be the function that sends a sequence in
ℑ
to its sequence of partial sums. If
T
n
is the set of sequences in
T
a
u
whose last element is at most
n
, we have two commuting involutions
R
n
and
C
n
on
T
n
defined by
R
n
(
a
1
,
a
2
,
⋯
,
a
l
)
=
(
n
+
1
−
a
l
,
n
+
1
−
a
l
−
1
,
⋯
,
n
+
1
−
a
1
)
and
C
n
(
a
1
,
⋯
,
a
l
)
= complement of
{
a
1
,
⋯
,
a
l
}
in
{
1
,
2
,
⋯
,
n
}
arranged in increasing order. The our definition of
τ
is
τ
(
I
)
=
Σ
−
1
R
n
C
n
Σ
(
I
)
=
Σ
−
1
C
n
R
n
Σ
(
I
)
for
I
=
(
i
1
,
i
2
,
⋯
,
i
k
)
∈
ℑ
with
i
1
+
⋯
+
i
k
=
n
.
For example,
τ
(
3
,
4
,
1
)
=
Σ
−
1
C
8
R
8
(
3
,
7
,
8
)
=
Σ
−
1
(
3
,
4
,
5
,
7
,
8
)
=
(
3
,
1
,
1
,
2
,
1
)
.
We shall say the sequences
(
i
1
,
⋯
,
i
k
)
and
τ
(
i
1
,
⋯
,
i
k
)
are dual to each other, and refer to a sequence fixed by
τ
as self-dual.
Duality conjecture (Hoffman). If
(
h
1
,
⋯
,
h
n
−
k
)
is dual to
(
i
1
,
⋯
,
i
k
)
, then
ζ
(
h
1
,
⋯
,
h
n
−
k
)
=
ζ
(
i
1
,
⋯
,
i
k
)
.
This sum conjecture is also known as Sum Theorem, and it may be expressed as follows: the Riemann zeta value of an integer n ≥ 2 is equal to the sum of all the valid (i.e. with s1 > 1) MZVs of the partitions of length k and weight n, with 1 ≤ k ≤n − 1. In formula:
∑
s
1
>
1
s
1
+
⋯
+
s
k
=
n
ζ
(
s
1
,
…
,
s
k
)
=
ζ
(
n
)
For example with length k = 2 and weight n = 7:
ζ
(
6
,
1
)
+
ζ
(
5
,
2
)
+
ζ
(
4
,
3
)
+
ζ
(
3
,
4
)
+
ζ
(
2
,
5
)
=
ζ
(
7
)
The Euler sum with alternations of sign appears in studies of the non-alternating Euler sum.
∑
n
=
1
∞
H
n
(
b
)
(
−
1
)
(
n
+
1
)
(
n
+
1
)
a
=
ζ
(
a
¯
,
b
)
with
H
n
(
b
)
=
+
1
+
1
2
b
+
1
3
b
+
⋯
are the generalized harmonic numbers.
∑
n
=
1
∞
H
¯
n
(
b
)
(
n
+
1
)
a
=
ζ
(
a
,
b
¯
)
with
H
¯
n
(
b
)
=
−
1
+
1
2
b
−
1
3
b
+
⋯
∑
n
=
1
∞
H
¯
n
(
b
)
(
−
1
)
(
n
+
1
)
(
n
+
1
)
a
=
ζ
(
a
¯
,
b
¯
)
∑
n
=
1
∞
(
−
1
)
n
(
n
+
2
)
a
∑
n
=
1
∞
H
¯
n
(
c
)
(
−
1
)
(
n
+
1
)
(
n
+
1
)
b
=
ζ
(
a
¯
,
b
¯
,
c
¯
)
with
H
¯
n
(
c
)
=
−
1
+
1
2
c
−
1
3
c
+
⋯
∑
n
=
1
∞
(
−
1
)
n
(
n
+
2
)
a
∑
n
=
1
∞
H
n
(
c
)
(
n
+
1
)
b
=
ζ
(
a
¯
,
b
,
c
)
with
H
n
(
c
)
=
+
1
+
1
2
c
+
1
3
c
+
⋯
∑
n
=
1
∞
1
(
n
+
2
)
a
∑
n
=
1
∞
H
n
(
c
)
(
−
1
)
(
n
+
1
)
(
n
+
1
)
b
=
ζ
(
a
,
b
¯
,
c
)
∑
n
=
1
∞
1
(
n
+
2
)
a
∑
n
=
1
∞
H
¯
n
(
c
)
(
n
+
1
)
b
=
ζ
(
a
,
b
,
c
¯
)
As a variant of the Dirichlet eta function we define
ϕ
(
s
)
=
1
−
2
(
s
−
1
)
2
(
s
−
1
)
ζ
(
s
)
with
s
>
1
ϕ
(
1
)
=
−
ln
2
The reflection formula
ζ
(
a
,
b
)
+
ζ
(
b
,
a
)
=
ζ
(
a
)
ζ
(
b
)
−
ζ
(
a
+
b
)
can be generalized as follows:
ζ
(
a
,
b
¯
)
+
ζ
(
b
¯
,
a
)
=
ζ
(
a
)
ϕ
(
b
)
−
ϕ
(
a
+
b
)
ζ
(
a
¯
,
b
)
+
ζ
(
b
,
a
¯
)
=
ζ
(
b
)
ϕ
(
a
)
−
ϕ
(
a
+
b
)
ζ
(
a
¯
,
b
¯
)
+
ζ
(
b
¯
,
a
¯
)
=
ϕ
(
a
)
ϕ
(
b
)
−
ζ
(
a
+
b
)
if
a
=
b
we have
ζ
(
a
¯
,
a
¯
)
=
1
2
[
ϕ
2
(
a
)
−
ζ
(
2
a
)
]
Using the series definition it is easy to prove:
ζ
(
a
,
b
)
+
ζ
(
a
,
b
¯
)
+
ζ
(
a
¯
,
b
)
+
ζ
(
a
¯
,
b
¯
)
=
ζ
(
a
,
b
)
2
(
a
+
b
−
2
)
with
a
>
1
ζ
(
a
,
b
,
c
)
+
ζ
(
a
,
b
,
c
¯
)
+
ζ
(
a
,
b
¯
,
c
)
+
ζ
(
a
¯
,
b
,
c
)
+
ζ
(
a
,
b
¯
,
c
¯
)
+
ζ
(
a
¯
,
b
,
c
¯
)
+
ζ
(
a
¯
,
b
¯
,
c
)
+
ζ
(
a
¯
,
b
¯
,
c
¯
)
=
ζ
(
a
,
b
,
c
)
2
(
a
+
b
+
c
−
3
)
with
a
>
1
A further useful relation is:
ζ
(
a
,
b
)
+
ζ
(
a
¯
,
b
¯
)
=
∑
s
>
0
(
a
+
b
−
s
−
1
)
!
[
Z
a
(
a
+
b
−
s
,
s
)
(
a
−
s
)
!
(
b
−
1
)
!
+
Z
b
(
a
+
b
−
s
,
s
)
(
b
−
s
)
!
(
a
−
1
)
!
]
where
Z
a
(
s
,
t
)
=
ζ
(
s
,
t
)
+
ζ
(
s
¯
,
t
)
−
[
ζ
(
s
,
t
)
+
ζ
(
s
+
t
)
]
2
(
s
−
1
)
and
Z
b
(
s
,
t
)
=
ζ
(
s
,
t
)
2
(
s
−
1
)
Note that
s
must be used for all value
>
1
for whom the argument of the factorials is
⩾
0
For any integer positive :
a
,
b
,
…
,
k
:
∑
n
=
2
∞
ζ
(
n
,
k
)
=
ζ
(
k
+
1
)
or more generally:
∑
n
=
2
∞
ζ
(
n
,
a
,
b
,
…
,
k
)
=
ζ
(
a
+
1
,
b
,
…
,
k
)
∑
n
=
2
∞
ζ
(
n
,
k
¯
)
=
−
ϕ
(
k
+
1
)
∑
n
=
2
∞
ζ
(
n
,
a
¯
,
b
)
=
ζ
(
a
+
1
¯
,
b
)
∑
n
=
2
∞
ζ
(
n
,
a
,
b
¯
)
=
ζ
(
a
+
1
,
b
¯
)
∑
n
=
2
∞
ζ
(
n
,
a
¯
,
b
¯
)
=
ζ
(
a
+
1
¯
,
b
¯
)
lim
k
→
∞
ζ
(
n
,
k
)
=
ζ
(
n
)
−
1
1
−
ζ
(
2
)
+
ζ
(
3
)
−
ζ
(
4
)
+
⋯
=
|
1
2
|
ζ
(
a
,
a
)
=
1
2
[
(
ζ
(
a
)
)
2
−
ζ
(
2
a
)
]
ζ
(
a
,
a
,
a
)
=
1
6
(
ζ
(
a
)
)
3
+
1
3
ζ
(
3
a
)
−
1
2
ζ
(
a
)
ζ
(
2
a
)
The Mordell–Tornheim zeta function, introduced by Matsumoto (2003) who was motivated by the papers Mordell (1958) and Tornheim (1950), is defined by
ζ
M
T
,
r
(
s
1
,
…
,
s
r
;
s
r
+
1
)
=
∑
m
1
,
…
,
m
r
>
0
1
m
1
s
1
⋯
m
r
s
r
(
m
1
+
⋯
+
m
r
)
s
r
+
1
It is a special case of the Shintani zeta function.