Microscopic quantum mechanics of the p=ρ universe

T. Banks, W. Fischler, and L. Mannelli
Phys. Rev. D 71, 123514 – Published 9 June 2005

Abstract

We present a complete quantum mechanical description of a flat Friedmann-Robertson-Walker universe with equation of state p=ρ. We find a detailed correspondence with our heuristic picture of such a universe as a dense black hole fluid. Features of the geometry are derived from purely quantum input.

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  • Received 13 December 2004

DOI:https://doi.org/10.1103/PhysRevD.71.123514

©2005 American Physical Society

Authors & Affiliations

T. Banks*

  • Department of Physics and Astronomy-NHETC, Rutgers University, Piscataway, New Jersey 08540, USA
  • and Department of Physics, SCIPP, University of California, Santa Cruz, California 95064, USA

W. Fischler

  • Department of Physics, University of Texas, Austin, Texas 78712, USA

L. Mannelli

  • Department of Physics, SCIPP, University of California, Santa Cruz, California 95064, USA

  • *Electronic address: banks@scipp.ucsc.edu
  • Electronic address: fischler@utexas.edu
  • Electronic address: lorenzo@scipp.ucsc.edu

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Issue

Vol. 71, Iss. 12 — 15 June 2005

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