English

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-NN 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