Flat space cosmologies in two dimensions: Phase transitions and asymptotic mass domination

Arjun Bagchi, Daniel Grumiller, Jakob Salzer, Sourav Sarkar, and Friedrich Schöller
Phys. Rev. D 90, 084041 – Published 20 October 2014

Abstract

We study flat space cosmologies in two dimensions by taking the flat space limit of the Achúcarro-Ortiz model. We unravel a phase transition between hot flat space and flat space cosmologies, and derive a new dilaton-dependent counterterm required for the consistency of the Euclidean partition function. Our results generalize to asymptotically mass-dominated two-dimensional dilaton gravity models, whose thermodynamical properties we discuss. The novel case of asymptotic mass domination is covered neither by the comprehensive discussion of Grumiller and McNees [J. High Energy Phys. 04 (2007) 074] nor by the more recent generalization to dilaton gravity with confining U(1) charges in Grumiller et al. [Phys. Rev. D 90, 044032 (2014)].

  • Figure
  • Received 28 August 2014

DOI:https://doi.org/10.1103/PhysRevD.90.084041

© 2014 American Physical Society

Authors & Affiliations

Arjun Bagchi1,2,*, Daniel Grumiller2,†, Jakob Salzer2,‡, Sourav Sarkar1,§, and Friedrich Schöller2,¶

  • 1Indian Institute of Science Education and Research, Pune 411008, India
  • 2Institute for Theoretical Physics, Vienna University of Technology, Wiedner Hauptstrasse 8-10/136, A-1040 Vienna, Austria

  • *a.bagchi@iiserpune.ac.in
  • grumil@hep.itp.tuwien.ac.at
  • salzer@hep.itp.tuwien.ac.at
  • §ssarkar@students.iiserpune.ac.in
  • schoeller@hep.itp.tuwien.ac.at

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Issue

Vol. 90, Iss. 8 — 15 October 2014

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