The Complex-Time Segal-Bargmann Transform
arXiv:1610.00090
Abstract
We introduce a new form of the Segal--Bargmann transform for a Lie group of compact type. We show that the heat kernel has a space-time analytic continuation to a holomorphic function \[ (ρ_{\mathbb{C}}(τ,z))_{\mathrm{Re}\,τ>0,z\in K_{\mathbb{C}}} \] where is the complexification of . The new transform is defined by the integral \[ (B_τf)(z)=\int_{K}ρ_{\mathbb{C}}(τ,zk^{-1})f(k)\,dk,\quad z\in K_{\mathbb{C}}. \] If and (the disk of radius centered at ), this integral defines a holomorphic function on for each . We construct a heat kernel density on such that, for all as above, is an isometric isomorphism from onto the space of holomorphic functions in . When , the transform coincides with the one introduced by the second author for compact groups and extended by the first author to groups of compact type. When , the transform coincides with the one introduced by the first two authors.
32 pages