PIRSA:13110046 Scientific Series Particle Physics

DOI10.48660/13110046

Series: Particle Physics

(2013). Baryogenesis from WIMPs. Perimeter Institute. https://pirsa.org/13110046

Baryogenesis from WIMPs. Perimeter Institute, Nov. 12, 2013, https://pirsa.org/13110046 

@misc{ pirsa_PIRSA:13110046,
  doi = {10.48660/13110046},
  url = {https://pirsa.org/13110046},
  author = {},
  keywords = {Particle Physics},
  language = {en},
  title = {Baryogenesis from WIMPs},
  publisher = {Perimeter Institute},
  year = {2013},
  month = {nov},
  note = {PIRSA:13110046 see, \url{https://pirsa.org}}
}

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 meta-stable WIMP after its thermal freezeout at or below the weak scale. A minimal model and its embedding in R-parity violating (RPV) natural SUSY are studied as examples. The new mechanism saves RPV SUSY from the potential crisis of washing out primordial baryon asymmetry. We also consider the embedding of this idea in RPV split SUSY, where the mechanism works within the minimal model, and independently motivates the mini-split scale. Phenomenological implications for the LHC and precision tests are discussed.

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