Riemann Zeta Function
The Riemann zeta function is an extremely important special function of mathematics and physics that arises in definite integration and is
intimately related with very deep results surrounding the prime
number theorem. While many of the properties of this function have been investigated,
there remain important fundamental conjectures (most notably the Riemann
hypothesis) that remain unproved to this day. The Riemann zeta function is denoted
and is plotted above (using two
different scales) along the real axis.
![]() |
In general,
is defined over the complex plane
for one complex variable, which is conventionally denoted
(instead of the
usual
) in deference to the notation used by
Riemann in his 1859 paper that founded the study of this function (Riemann 1859).
is implemented in the Wolfram
Language as Zeta[s].
The plot above shows the "ridges" of
for
and
. The
fact that the ridges appear to decrease monotonically for
is not a coincidence since it turns out that monotonic decrease implies the Riemann
hypothesis (Zvengrowski and Saidak 2003; Borwein and Bailey 2003, pp. 95-96).
On the real line with
, the Riemann
zeta function can be defined by the integral
|
(1)
|
where
is the gamma
function. If
is an integer
, then we have the identity
|
(2)
| |||
|
(3)
| |||
|
(4)
|
so
|
(5)
|
To evaluate
, let
so that
and plug in the above identity to obtain
|
(6)
| |||
|
(7)
| |||
|
(8)
|
Integrating the final expression in (8) gives
, which
cancels the factor
and gives
the most common form of the Riemann zeta function,
|
(9)
|
which is sometimes known as a p-series.
The Riemann zeta function can also be defined in terms of multiple integrals by
![]() |
(10)
|
and as a Mellin transform by
|
(11)
|
for
, where
is the fractional part (Balazard and Saias 2000).
It appears in the unit square integral
|
(12)
|
valid for
(Guillera and Sondow 2005).
For
a nonnegative integer, this formula is
due to Hadjicostas (2002), and the special cases
and
are due to Beukers
(1979).
Note that the zeta function
has a singularity
at
, where it reduces to the divergent
harmonic series.
The Riemann zeta function satisfies the reflection functional equation
|
(13)
|
(Hardy 1999, p. 14; Krantz 1999, p. 160), a similar form of which was conjectured by Euler for real
(Euler, read in 1749, published in 1768;
Ayoub 1974; Havil 2003, p. 193). A symmetrical form of this functional equation
is given by
|
(14)
|
(Ayoub 1974), which was proved by Riemann for all complex
(Riemann 1859).
As defined above, the zeta function
with
a complex
number is defined for
. However,
has a unique analytic
continuation to the entire complex plane, excluding
the point
, which corresponds to a simple
pole with complex residue 1 (Krantz 1999,
p. 160). In particular, as
,
obeys
|
(15)
|
where
is the Euler-Mascheroni
constant (Whittaker and Watson 1990, p. 271).
To perform the analytic continuation for
, write
|
(16)
| |||
|
(17)
| |||
|
(18)
|
so rewriting in terms of
immediately
gives
|
(19)
|
Therefore,
|
(20)
|
Here, the sum on the right-hand side is exactly the Dirichlet eta function
(sometimes also called the alternating
zeta function). While this formula defines
for only
the right half-plane
, equation
(◇) can be used to analytically continue it to the rest of the complex
plane. Analytic continuation can also
be performed using Hankel functions. A globally
convergent series for the Riemann zeta function (which provides the analytic
continuation of
to the entire
complex plane except
) is given by
|
(21)
|
(Havil 2003, p. 206), where
is a binomial
coefficient, which was conjectured by Knopp around 1930, proved by Hasse (1930),
and rediscovered by Sondow (1994). This equation is related to renormalization and
random variates (Biane et al. 2001) and can be derived by applying Euler's
series transformation with
to equation
(20).
Hasse (1930) also proved the related globally (but more slowly) convergent series
|
(22)
|
that, unlike (21), can also be extended to a generalization of the Riemann zeta function known as the Hurwitz
zeta function
.
is defined
such that
|
(23)
|
(If the singular term is excluded from the sum definition of
, then
as well.) Expanding
about
gives
|
(24)
|
where
are the so-called Stieltjes
constants.
The Riemann zeta function can also be defined in the complex plane by the contour integral
|
(25)
|
for all
, where the contour
is illustrated above (Havil 2003, pp. 193 and 249-252).
Zeros of
come in (at least) two different
types. So-called "trivial zeros" occur at all negative even integers
,
,
, ..., and "nontrivial
zeros" at certain
|
(26)
|
for
in the "critical
strip"
. The Riemann
hypothesis asserts that the nontrivial Riemann
zeta function zeros of
all have
real part
,
a line called the "critical line." This
is now known to be true for the first
roots.
The plot above shows the real and imaginary parts of
(i.e.,
values of
along the critical
line) as
is varied from 0 to 35 (Derbyshire 2004,
p. 221).
The Riemann zeta function can be split up into
|
(27)
|
where
and
are the
Riemann-Siegel functions.
The Riemann zeta function is related to the Dirichlet lambda function
and Dirichlet eta function
by
|
(28)
|
and
|
(29)
|
(Spanier and Oldham 1987).
It is related to the Liouville function
by
|
(30)
|
(Lehman 1960, Hardy and Wright 1979). Furthermore,
|
(31)
|
where
is the number of distinct
prime factors of
(Hardy and Wright
1979, p. 254).
For
a positive even integer
,
, ...,
|
(32)
|
giving the first few as
|
(33)
| |||
|
(34)
| |||
|
(35)
| |||
|
(36)
|
(OEIS A117972 and A117973). For
,
|
(37)
|
where
is the Glaisher-Kinkelin
constant. Using equation (◇) gives the derivative
|
(38)
|
which can be derived directly from the Wallis formula (Sondow 1994).
can also be
derived directly from the Euler-Maclaurin summation formula (Edwards 2001, pp. 134-135).
In general,
can be expressed analytically
in terms of
,
, the Euler-Mascheroni constant
, and the Stieltjes constants
, with the
first few examples being
|
(39)
| |||
|
(40)
|
Derivatives
can also be given in closed
form, for example,
|
(41)
| |||
|
(42)
|
(OEIS A114875).
The derivative of the Riemann zeta function for
is defined by
|
(43)
| |||
|
(44)
|
can be given in closed form
as
|
(45)
| |||
|
(46)
|
(OEIS A073002), where
is the Glaisher-Kinkelin
constant (given in series form by Glaisher 1894).
The series for
about
is
|
(47)
|
where
are Stieltjes
constants.
In 1739, Euler found the rational coefficients
in
in terms of the Bernoulli numbers. Which, when
combined with the 1882 proof by Lindemann that
is transcendental,
effectively proves that
is transcendental.
The study of
is significantly more difficult.
Apéry (1979) finally proved
to be irrational, but no similar results are known for
other odd
. As a result of
Apéry's important discovery,
is sometimes
called Apéry's constant. Rivoal (2000)
and Ball and Rivoal (2001) proved that there are infinitely many integers
such that
is irrational, and subsequently that at
least one of
,
, ...,
is irrational
(Rivoal 2001). This result was subsequently tightened by Zudilin (2001), who showed
that at least one of
,
,
, or
is irrational.
A number of interesting sums for
, with
a positive integer,
can be written in terms of binomial coefficients as the binomial
sums
![]() |
(48)
| ||
![]() |
(49)
| ||
![]() |
(50)
|
(Guy 1994, p. 257; Bailey et al. 2007, p. 70). Apéry arrived at his result with the aid of the
sum formula
above. A relation of the form
![]() |
(51)
|
has been searched for with
a rational
or algebraic number, but if
is a root
of a polynomial of degree 25 or less, then the Euclidean
norm of the coefficients must be larger than
,
and if
if algebraic of degree 25 or less,
then the norm of coefficients must exceed
(Bailey et al. 2007, pp. 70-71, updating Bailey and Plouffe). Therefore,
no such sums for
are known for
.
The identity
|
(52)
| |||
|
(53)
| |||
![]() |
(54)
| ||
|
(55)
|
for
is complex number not equal to a nonzero
integer gives an Apéry-like formula for even positive
(Bailey et al.
2006, pp. 72-77).
The Riemann zeta function
may be
computed analytically for even
using either contour integration or Parseval's
theorem with the appropriate Fourier series.
An unexpected and important formula involving a product over the primes
was first discovered by Euler in 1737,
|
(56)
| |||
|
(57)
| |||
|
(58)
| |||
|
(59)
| |||
|
(60)
|
Here, each subsequent multiplication by the
th prime
leaves only terms that are powers
of
. Therefore,
|
(61)
|
which is known as the Euler product formula (Hardy 1999, p. 18; Krantz 1999, p. 159), and called "the golden key" by Derbyshire (2004, pp. 104-106). The formula can also be written
![]() |
(62)
|
where
and
are the primes
congruent to 1 and 3 modulo 4, respectively.
For even
,
|
(63)
|
where
is a Bernoulli
number (Mathews and Walker 1970, pp. 50-53; Havil 2003, p. 194). Another
intimate connection with the Bernoulli numbers
is provided by
|
(64)
|
for
, which can be written
|
(65)
|
for
. (In both cases, only the even
cases are of interest since
trivially
for odd
.) Rewriting (65),
|
(66)
|
for
, 3, ... (Havil 2003, p. 194),
where
is a Bernoulli
number, the first few values of which are
, 1/120,
, 1/240, ... (OEIS A001067
and A006953).
Although no analytic form for
is known
for odd
,
|
(67)
|
where
is a harmonic
number (Stark 1974). In addition,
can be expressed
as the sum limit
|
(68)
|
for
, 5, ... (Apostol 1973, given incorrectly
in Stark 1974).
For
the Möbius
function,
|
(69)
|
(Havil 2003, p. 209).
The values of
for small positive integer values
of
are
|
(70)
| |||
|
(71)
| |||
|
(72)
| |||
|
(73)
| |||
|
(74)
| |||
|
(75)
| |||
|
(76)
| |||
|
(77)
| |||
|
(78)
| |||
|
(79)
|
Euler gave
to
for even
(Wells 1986, p. 54),
and Stieltjes (1993) determined the values of
, ...,
to 30 digits of accuracy in 1887. The denominators
of
for
, 2, ... are
6, 90, 945, 9450, 93555, 638512875, ... (OEIS A002432).
The numbers of decimal digits in the denominators of
for
, 1, ... are 1, 5, 133, 2277, 32660, 426486, 5264705,
... (OEIS A114474).
An integral for positive even integers is given by
|
(80)
|
and integrals for positive odd integers are given by
|
(81)
| |||
|
(82)
| |||
|
(83)
| |||
|
(84)
|
where
is an Euler
polynomial and
is a Bernoulli
polynomial (Cvijović and Klinowski 2002; J. Crepps, pers. comm., Apr.
2002).
The value of
can be computed by performing
the inner sum in equation (◇) with
,
|
(85)
|
to obtain
|
(86)
|
where
is the Kronecker
delta.
Similarly, the value of
can be
computed by performing the inner sum in equation (◇) with
,
|
(87)
|
which gives
|
(88)
| |||
|
(89)
| |||
|
(90)
|
This value is related to a deep result in renormalization theory (Elizalde et al. 1994, 1995, Bloch 1996, Lepowski 1999).
It is apparently not known if the value
|
(91)
|
(OEIS A059750) can be expressed in terms of known mathematical constants. This constant appears, for example, in Knuth's series.
Rapidly converging series for
for
odd were first discovered by Ramanujan (Zucker
1979, 1984, Berndt 1988, Bailey et al. 1997, Cohen 2000). For
and
,
|
(92)
|
where
is again a Bernoulli
number and
is a binomial
coefficient. The values of the left-hand sums (divided by
) in (92)
for
, 7, 11, ... are 7/180, 19/56700, 1453/425675250,
13687/390769879500, 7708537/21438612514068750, ... (OEIS A057866
and A057867). For
and
, the corresponding formula is slightly
messier,
![]() |
(93)
|
(Cohen 2000).
Defining
|
(94)
|
the first few values can then be written
|
(95)
| |||
|
(96)
| |||
|
(97)
| |||
|
(98)
| |||
|
(99)
| |||
|
(100)
| |||
|
(101)
| |||
|
(102)
| |||
|
(103)
| |||
|
(104)
|
(Plouffe 1998).
Another set of related formulas are
|
(105)
| |||
|
(106)
| |||
![]() |
(107)
| ||
|
(108)
| |||
![]() |
(109)
|
(Plouffe 2006).
Multiterm sums for odd
include
![]() |
(110)
| ||
![]() |
(111)
| ||
![]() |
(112)
| ||
![]() |
(113)
|
(Borwein and Bradley 1996, 1997; Bailey et al. 2007, p. 71), where
is a generalized harmonic
number.
G. Huvent (2002) found the beautiful formula
|
(114)
|
A number of sum identities involving
include
|
(115)
| |||
|
(116)
| |||
|
(117)
| |||
|
(118)
|
Sums involving integers multiples of the argument include
|
(119)
| |||
|
(120)
| |||
|
(121)
|
where
is a harmonic
number.
Two surprising sums involving
are given
by
|
(122)
| |||
|
(123)
|
where
is the Euler-Mascheroni
constant (Havil 2003, pp. 109 and 111-112). Equation (122)
can be generalized to
|
(124)
|
(T. Drane, pers. comm., Jul. 7, 2006) for
.
Other unexpected sums are
|
(125)
|
(Tyler and Chernhoff 1985; Boros and Moll 2004, p. 248) and
|
(126)
|
(125) is a special case of
![]() |
(127)
|
where
is a Hurwitz
zeta function (Danese 1967; Boros and Moll 2004, p. 248).
Considering the sum
|
(128)
|
then
|
(129)
|
where
is the natural
logarithm of 2, which is a particular case of
|
(130)
|
where
is the digamma
function and
is the Euler-Mascheroni
constant, which can be derived from
|
(131)
|
(B. Cloitre, pers. comm., Dec. 11, 2005; cf. Borwein et al. 2000, eqn. 27).
A generalization of a result of Ramanujan (who gave the
case) is given
by
|
(132)
|
where
is a binomial
coefficient (B. Cloitre, pers. comm., Sep. 20, 2005).
An additional set of sums over
is given
by
|
(133)
| |||
|
(134)
| |||
|
(135)
| |||
|
(136)
| |||
|
(137)
| |||
|
(138)
| |||
|
(139)
| |||
|
(140)
| |||
|
(141)
| |||
|
(142)
| |||
|
(143)
|
(OEIS A093720, A076813, and A093721), where
is a modified
Bessel function of the first kind,
is a regularized hypergeometric function.
These sums have no known closed-form expression.
The inverse of the Riemann zeta function
, plotted
above, is the asymptotic density of
th-powerfree numbers
(i.e., squarefree numbers, cubefree
numbers, etc.). The following table gives the number
of
th-powerfree numbers
for several values of
.
| 2 | 0.607927 | 7 | 61 | 608 | 6083 | 60794 | 607926 |
| 3 | 0.831907 | 9 | 85 | 833 | 8319 | 83190 | 831910 |
| 4 | 0.923938 | 10 | 93 | 925 | 9240 | 92395 | 923939 |
| 5 | 0.964387 | 10 | 97 | 965 | 9645 | 96440 | 964388 |
| 6 | 0.982953 | 10 | 99 | 984 | 9831 | 98297 | 982954 |














![5/2sum_(k=1)^(infty)((-1)^(k+1))/(k^(11)(2k; k))+(25)/2sum_(k=1)^(infty)((-1)^(k+1)H_(k-1)^((4)))/(k^7(2k; k))-(75)/4sum_(k=1)^(infty)((-1)^(k+1)H_(k-1)^((8)))/(k^3(2k; k))+(125)/4sum_(k=1)^(infty)((-1)^(k+1)[H_(k-1)^((4))]^2)/(k^3(2k; k))](/images/equations/RiemannZetaFunction/Inline378.gif)

Riemann hypothesis




