Baryogenesis for weakly interacting massive particles

Yanou Cui and Raman Sundrum
Phys. Rev. D 87, 116013 – Published 26 June 2013

Abstract

We propose a robust, unified framework, in which the similar baryon and dark matter cosmic abundances both arise from the physics of weakly interacting massive particles (WIMPs), with the rough quantitative success of the so-called “WIMP miracle.” In particular the baryon asymmetry arises from the decay of a metastable WIMP after its thermal freeze-out at or below the weak scale. A minimal model and its embedding in R-parity violating supersymmetry are studied as examples. The new mechanism saves R-parity violating supersymmetry from the potential crisis of washing out primordial baryon asymmetry. Phenomenological implications for the LHC and precision tests are discussed.

  • Figure
  • Received 29 January 2013

DOI:https://doi.org/10.1103/PhysRevD.87.116013

© 2013 American Physical Society

Authors & Affiliations

Yanou Cui and Raman Sundrum

  • Department of Physics, Maryland Center for Fundamental Physics, University of Maryland, College Park, Maryland 20742, USA

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Issue

Vol. 87, Iss. 11 — 1 June 2013

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