The null energy condition and instability

Roman V. Buniy, Stephen D. H. Hsu, and Brian M. Murray
Phys. Rev. D 74, 063518 – Published 21 September 2006

Abstract

We extend previous work showing that violation of the null energy condition implies instability in a broad class of models, including gauge theories with scalar and fermionic matter as well as any perfect fluid. Simple examples are given to illustrate these results. The role of causality in our results is discussed. Finally, we extend the fluid results to more general systems in thermal equilibrium. When applied to the dark energy, our results imply that w=p/ρ is unlikely to be less than 1.

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  • Received 16 June 2006

DOI:https://doi.org/10.1103/PhysRevD.74.063518

©2006 American Physical Society

Authors & Affiliations

Roman V. Buniy*, Stephen D. H. Hsu, and Brian M. Murray

  • Institute of Theoretical Science, University of Oregon, Eugene, Oregon 97403-5203, USA

  • *Electronic address: roman@uoregon.edu
  • Electronic address: hsu@duende.uoregon.edu
  • Electronic address: bmurray1@uoregon.edu

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Issue

Vol. 74, Iss. 6 — 15 September 2006

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