Spence's function

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Short description: Special case of the polylogarithm


The dilogarithm along the real axis

In mathematics, Spence's function, or dilogarithm, denoted as Li2(z), is a particular case of the polylogarithm. Two related special functions are referred to as Spence's function, the dilogarithm itself:

Li2(z)=−∫0zln⁡(1−u)udu, z∈ℂ

and its reflection. For |z| < 1, an infinite series also applies (the integral definition constitutes its analytical extension to the complex plane):

Li2(z)=∑k=1∞zkk2.

Alternatively, the dilogarithm function is sometimes defined as

∫1vln⁡t1−tdt=Li2(1−v).

In hyperbolic geometry the dilogarithm can be used to compute the volume of an ideal simplex. Specifically, a simplex whose vertices have cross ratio z has hyperbolic volume

D(z)=Im⁡Li2(z)+arg⁡(1−z)log⁡|z|.

The function D(z) is sometimes called the Bloch-Wigner function.[1] Lobachevsky's function and Clausen's function are closely related functions.

William Spence, after whom the function was named by early writers in the field, was a Scottish mathematician working in the early nineteenth century.[2] He was at school with John Galt,[3] who later wrote a biographical essay on Spence.

Analytic structure

Using the former definition above, the dilogarithm function is analytic everywhere on the complex plane except at z=1, where it has a logarithmic branch point. The standard choice of branch cut is along the positive real axis (1,∞). However, the function is continuous at the branch point and takes on the value Li2(1)=π2/6.

Identities

Li2(z)+Li2(−z)=12Li2(z2).[4]
Li2(1−z)+Li2(1−1z)=−(ln⁡z)22.[5]
Li2(z)+Li2(1−z)=π26−ln⁡z⋅ln⁡(1−z).[4]
Li2(−z)−Li2(1−z)+12Li2(1−z2)=−π212−ln⁡z⋅ln⁡(z+1).[5]
Li2(z)+Li2(1z)=−π26−(ln⁡(−z))22.[4]

Particular value identities

Li2(13)−16Li2(19)=π218−(ln⁡3)26.[5]
Li2(−13)−13Li2(19)=−π218+(ln⁡3)26.[5]
Li2(−12)+16Li2(19)=−π218+ln⁡2⋅ln⁡3−(ln⁡2)22−(ln⁡3)23.[5]
Li2(14)+13Li2(19)=π218+2ln⁡2⋅ln⁡3−2(ln⁡2)2−23(ln⁡3)2. [5]
Li2(−18)+Li2(19)=−12(ln⁡98)2.[5]
36Li2(12)−36Li2(14)−12Li2(18)+6Li2(164)=π2.

Special values

Li2(−1)=−π212.
Li2(0)=0.
Li2(12)=π212−(ln⁡2)22.
Li2(1)=ζ(2)=π26, where ζ(s) is the Riemann zeta function.
Li2(2)=π24−iπln⁡2.
Li2(−5−12)=−π215+12(ln⁡5+12)2=−π215+12arcsch22.
Li2(−5+12)=−π210−ln25+12=−π210−arcsch22.
Li2(3−52)=π215−ln25+12=π215−arcsch22.
Li2(5−12)=π210−ln25+12=π210−arcsch22.

In particle physics

Spence's Function is commonly encountered in particle physics while calculating radiative corrections. In this context, the function is often defined with an absolute value inside the logarithm:

Φ⁡(x)=−∫0xln⁡|1−u|udu={Li2(x),x≤1;π23−12(ln⁡x)2−Li2(1x),x>1.

Notes

References

Further reading

  • Bloch, Spencer J. (2000). Higher regulators, algebraic K-theory, and zeta functions of elliptic curves. CRM Monograph Series. 11. Providence, RI: American Mathematical Society. ISBN 0-8218-2114-8.