corner
corner

Phys. Rev. D 79, 103504 (2009) [7 pages]

Dark radiation as a signature of dark energy

Download: PDF (232 kB) Buy this article Export: BibTeX or EndNote (RIS)

Sourish Dutta1,*, Stephen D. H. Hsu2,†, David Reeb2,‡, and Robert J. Scherrer1,§
1Department of Physics and Astronomy, Vanderbilt University, Nashville, Tennessee 37235, USA
2Institute of Theoretical Science, University of Oregon, Eugene, Oregon 97403-5203, USA

Received 7 March 2009; published 6 May 2009

We propose a simple dark energy model with the following properties: the model predicts a late-time dark radiation component that is not ruled out by current observational data, but which produces a distinctive time-dependent equation of state w(z) for z<3. The dark energy field can be coupled strongly enough to standard model particles to be detected in colliders, and the model requires only modest additional particle content and little or no fine-tuning other than a new energy scale of order milli-electron volts.

© 2009 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.79.103504
DOI:
10.1103/PhysRevD.79.103504
PACS:
95.36.+x, 98.80.Cq

*sourish.d@gmail.com

hsu@uoregon.edu

dreeb@uoregon.edu

§robert.scherrer@vanderbilt.edu