No-Go Theorem for k-Essence Dark Energy

Camille Bonvin, Chiara Caprini, and Ruth Durrer
Phys. Rev. Lett. 97, 081303 – Published 25 August 2006

Abstract

We demonstrate that if k-essence can solve the coincidence problem and play the role of dark energy in the Universe, the fluctuations of the field have to propagate superluminally at some stage. We argue that this implies that successful k-essence models violate causality. It is not possible to define a time ordered succession of events in a Lorentz invariant way. Therefore, k-essence cannot arise as a low energy effective field theory of a causal, consistent high energy theory.

  • Figure
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  • Received 23 June 2006

DOI:https://doi.org/10.1103/PhysRevLett.97.081303

©2006 American Physical Society

Authors & Affiliations

Camille Bonvin*, Chiara Caprini, and Ruth Durrer

  • Département de Physique Théorique, Université de Genève, 24 quai Ernest Ansermet, CH-1211 Genève 4, Switzerland

  • *Electronic address: camille.bonvin@physics.unige.ch
  • Electronic address: chiara.caprini@physics.unige.ch
  • Electronic address: ruth.durrer@physics.unige.ch

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Issue

Vol. 97, Iss. 8 — 25 August 2006

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