Definition

For a VV of a FF and a nontrivial additive ψ\psi, the local gamma factor is

γ(s,V,ψ)=ε(s,V,ψ)L(1s,V)L(s,V),\gamma(s,V,\psi)= \varepsilon(s,V,\psi) \frac{L(1-s,V^\vee)}{L(s,V)},

where ε(s,V,ψ)\varepsilon(s,V,\psi) is the and VV^\vee is the . This convention places the functional equation around s=12s=\tfrac12; shifts occur when an L-function is normalized differently.

Analytic characterization

In Tate's thesis the factor is characterized by the local functional equation for . Higher-rank Rankin–Selberg integrals and the Langlands–Shahidi method similarly compare a zeta integral with its dual and produce a gamma factor.

Gamma factors are especially useful because local converse theorems can recognize a representation from families of twisted gamma factors. Under , the analytic factors agree with the corresponding Artin factors on the Weil–Deligne side.

Convention warning

Some authors write the quotient of L-factors in the reciprocal order or use ψ1\psi^{-1} on the dual side. A bare symbol γ(s,)\gamma(s,\cdots) is therefore not portable without its functional equation.

References
  1. John Tate, “Fourier analysis in number fields and Hecke's zeta-functions,” in Algebraic Number Theory, Academic Press, 1967, 305–347.
  2. Hervé Jacquet, Ilya Piatetski-Shapiro, and Joseph Shalika, “Rankin–Selberg convolutions,” American Journal of Mathematics 105 (1983), 367–464. JSTOR.