The Complex-Time Segal-Bargmann Transform
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 where is the complexification of . The new transform is defined by the integral 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.
Cite
@article{arxiv.1610.00090,
title = {The Complex-Time Segal-Bargmann Transform},
author = {Bruce Driver and Brian Hall and Todd Kemp},
journal= {arXiv preprint arXiv:1610.00090},
year = {2019}
}
Comments
32 pages