The Complex-Time Segal-Bargmann Transform
Bruce Driver, Brian Hall, and Todd Kemp

TL;DR
This paper introduces a new complex-time Segal-Bargmann transform for compact Lie groups, extending heat kernel analyticity and establishing isometric isomorphisms between function spaces with novel holomorphic properties.
Contribution
It defines a new complex-time Segal-Bargmann transform for compact Lie groups, generalizing previous versions and demonstrating its isometric properties with explicit kernel constructions.
Findings
The heat kernel admits a space-time holomorphic extension.
The transform is an isometric isomorphism between L^2 spaces.
Special cases recover known Segal-Bargmann transforms.
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 \[ (\rho_{\mathbb{C}}(\tau,z))_{\mathrm{Re}\,\tau>0,z\in K_{\mathbb{C}}} \] where is the complexification of . The new transform is defined by the integral \[ (B_{\tau}f)(z)=\int_{K}\rho_{\mathbb{C}}(\tau,zk^{-1})f(k)\,dk,\quad z\in K_{\mathbb{C}}. \] 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…
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