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2012

Direct Detection of Dynamical Dark Matter

Dienes, Keith R., Kumar, Jason, Thomas, Brooks

Understand

Dynamical dark matter (DDM) is an alternative framework for dark-matter physics in which the dark-matter candidate is an ensemble of constituent fields with differing masses, lifetimes, and cosmological abundances.

In this framework, it is the balancing of these quantities against each other across the ensemble as a whole which ensures phenomenological viability.
In this paper, we examine the prospects for the direct detection of a DDM ensemble.
In particular, we study the constraints imposed by current limits from direct-detection experiments on the parameter space of DDM models, and we assess the prospects for detecting such an ensemble and distinguishing it from traditional dark-matter candidates on the basis of data from the next generation of direct-detection experiments.

Built on

K. R. Dienes and B. Thomas, Phys. Rev. D 86
Original
1923
Earlier work this paper cites.
M. W. Goodman and E. Witten, Phys. Rev. D 31
1985
Earlier work this paper cites.
R. H. Helm, Phys. Rev. 104
1991
Earlier work this paper cites.
J. D. Lewin and P. F. Smith, Astropart. Phys. 6
1996
Earlier work this paper cites.
T. Han and R. Hempfling, Phys. Lett. B415
1998
Earlier work this paper cites.
D. Tucker-Smith and N. Weiner, Phys. Rev. D 64
2005
Earlier work this paper cites.
E. Aprile et al
2006
Earlier work this paper cites.
M. C. Smith et al
2007
Earlier work this paper cites.
For example, see: T. Hur, H. S. Lee and S. Nasri, Phys. Rev. D 77
Original
2009
Earlier work this paper cites.
S. Profumo, K. Sigurdson and L. Ubaldi, JCAP 0912
Original
2009
Earlier work this paper cites.