JETP Letters

, Volume 105, Issue 2, pp 74–77

Dark matter from dark energy in q-theory

Astrophysics and Cosmology

DOI: 10.1134/S0021364017020011

Cite this article as:
Klinkhamer, F.R. & Volovik, G.E. Jetp Lett. (2017) 105: 74. doi:10.1134/S0021364017020011

Abstract

A constant (spacetime-independent) q-field may play a crucial role for the cancellation of Planck-scale contributions to the gravitating vacuum energy density. We now show that a small spacetime-dependent perturbation of the equilibrium q-field behaves gravitationally as a pressureless perfect fluid. This makes the fluctuating part of the q-field a candidate for the inferred dark-matter component of the present universe. For a Planck-scale oscillation frequency of the q-field perturbation, the implication would be that direct searches for dark-matter particles would remain unsuccessful in the foreseeable future.

Copyright information

© Pleiades Publishing, Inc. 2017

Authors and Affiliations

  1. 1.Institute for Theoretical PhysicsKarlsruhe Institute of Technology (KIT)KarlsruheGermany
  2. 2.Low Temperature LaboratoryAalto UniversityAaltoFinland
  3. 3.Landau Institute for Theoretical PhysicsRussian Academy of SciencesMoscowRussia

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