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).
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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:
.
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).