String Perturbation Theory on the Schwinger-Keldysh Time Contour
High Energy Physics - Theory
2021-01-04 v3 Cosmology and Nongalactic Astrophysics
Other Condensed Matter
General Relativity and Quantum Cosmology
High Energy Physics - Phenomenology
Abstract
We perform the large- expansion in the Schwinger-Keldysh formulation of non-equilibrium quantum systems with matrix degrees of freedom, and study universal features of the anticipated dual string theory. We find a rich refinement of the topological genus expansion: In the original formulation, the future time instant where the forward and backward branches of the Schwinger-Keldysh time contour meet is associated with its own worldsheet genus expansion. After the Keldysh rotation, the worldsheets decompose into a classical and quantum part.
Keywords
Cite
@article{arxiv.2009.03940,
title = {String Perturbation Theory on the Schwinger-Keldysh Time Contour},
author = {Petr Horava and Christopher J. Mogni},
journal= {arXiv preprint arXiv:2009.03940},
year = {2021}
}
Comments
5 pages, a few figures; v2: references added; v3: references updated, small clarifying comments added. Final version accepted in Phys. Rev. Lett