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A running spectral index in supersymmetric dark-matter models with quasistable charged particles

Profumo, Stefano and Sigurdson, Kris and Ullio, Piero and Kamionkowski, Marc (2005) A running spectral index in supersymmetric dark-matter models with quasistable charged particles. Physical Review D, 71 (2). Art. No. 023518. ISSN 2470-0010. doi:10.1103/PhysRevD.71.023518.

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We show that charged particles decaying in the early Universe can induce a scale-dependent or running spectral index in the small-scale linear and nonlinear matter power spectrum and discuss examples of this effect in minimal supersymmetric models in which the lightest neutralino is a viable cold-dark-matter candidate. We find configurations in which the neutralino relic density is set by coannihilations with a long-lived stau and the late decay of staus partially suppresses the linear matter power spectrum. Nonlinear evolution on small scales then causes the modified linear power spectrum to evolve to a nonlinear power spectrum similar to (but different in detail) models parametrized by a constant running alphas = dns/dlnk by redshifts of 2 to 4. Thus, Lyman-alpha forest observations, which probe the matter power spectrum at these redshifts, might not discriminate between the two effects. However, a measurement of the angular power spectrum of primordial 21-cm radiation from redshift z[approximate]30–200 might distinguish between this charged-decay model and a primordial running spectral index. The direct production of a long-lived charged particle at future colliders is a dramatic prediction of this model.

Item Type:Article
Related URLs:
URLURL TypeDescription
Profumo, Stefano0000-0002-9159-7556
Sigurdson, Kris0000-0002-6729-0765
Kamionkowski, Marc0000-0001-7018-2055
Additional Information:© 2005 The American Physical Society (Received 29 October 2004; published 20 January 2005) We thank R. R. Caldwell and U. Seljak for useful discussions. S. P. acknowledges fruitful help and elucidations from Y. Mambrini about the SDECAY package. K. S. acknowledges the support of the Canadian NSERC. This work was supported in part by NASA NAG5-9821 and DoE DE-FG03-92-ER40701.
Funding AgencyGrant Number
Natural Sciences and Engineering Research Council of Canada (NSERC)UNSPECIFIED
Department of Energy (DOE)DE-FG03-92-ER40701
Subject Keywords:dark matter; supersymmetric field theory; unified field theories; gravitational red shift; cosmology; sparticles
Issue or Number:2
Record Number:CaltechAUTHORS:PROprd05
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Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:2346
Deposited By: Archive Administrator
Deposited On:28 Mar 2006
Last Modified:08 Nov 2021 19:47

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