The notation
was introduced in Lewin (1981) for a
function discussed in Euler (1768) and called the dilogarithm
in Hill (1828):


Other notations and names for
include
(Kölbig et al. (1970)), Spence function
(’t Hooft and Veltman (1979)), and
(Maximon (2003)).
In the complex plane
has a branch point at
. The
principal branch has a cut along the interval
and agrees with
(25.12.1) when
; see also §4.2(i).
The remainder of the equations in this
subsection apply to principal branches.




When
,
, (25.12.1)
becomes
The cosine series in (25.12.7) has the elementary sum
By (25.12.2)
The right-hand side is called Clausen’s integral.
For graphics see Figures 25.12.1 and 25.12.2, and for further properties see Maximon (2003), Kirillov (1995), Lewin (1981), Nielsen (1909), and Zagier (1989).
For real or complex
and
the polylogarithm
is defined by
For each fixed complex
the series defines an analytic function of
for
. The series also converges when
, provided that
. For other values of
,
is defined
by analytic continuation.
The notation
was used for
in
Truesdell (1945) for a series treated in Jonquière (1889),
hence the alternative name Jonquière’s function. The special case
is the Riemann zeta function:
.
valid when
and
, or
and
. (In the latter case (25.12.11)
becomes (25.5.1)).
Further properties include

and

The Fermi–Dirac and Bose–Einstein integrals are defined by


respectively. Sometimes the factor
is omitted. See
Cloutman (1989) and Gautschi (1993).
In terms of polylogarithms
For a uniform asymptotic approximation for
see
Temme and Olde Daalhuis (1990).