2014
DOI: 10.1140/epjc/s10052-014-2947-7
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The extent of the stop coannihilation strip

Abstract: Many supersymmetric models such as the constrained minimal supersymmetric extension of the Standard Model (CMSSM) feature a strip in parameter space where the lightest neutralino is identified as the lightest supersymmetric particle, the lighter stop squark is the next-to-lightest supersymmetric particle (NLSP), and the relic cold dark matter density is brought into the range allowed by astrophysics and cosmology by coannihilation with the lighter stop squark NLSP. We calculate the stop coannihilation stri… Show more

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Cited by 73 publications
(110 citation statements)
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References 113 publications
(82 reference statements)
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“…Alternatively, there might be one or more heavier supersymmetric particles that are nearly degenerate with the LSP, χ, and would have coannihilated with it in the early Universe [37]. There are several examples of possible coannihilating sparticles, including the lighter stau, or possibly some other slepton [38][39][40][41][42][43][44][45], the lighter stop squark [46][47][48][49][50][51][52][53][54][55][56], the lighter chargino [55,[57][58][59][60] and the gluino [56,[61][62][63][64][65][66][67][68][69][70][71][72].…”
Section: Introductionmentioning
confidence: 99%
“…Alternatively, there might be one or more heavier supersymmetric particles that are nearly degenerate with the LSP, χ, and would have coannihilated with it in the early Universe [37]. There are several examples of possible coannihilating sparticles, including the lighter stau, or possibly some other slepton [38][39][40][41][42][43][44][45], the lighter stop squark [46][47][48][49][50][51][52][53][54][55][56], the lighter chargino [55,[57][58][59][60] and the gluino [56,[61][62][63][64][65][66][67][68][69][70][71][72].…”
Section: Introductionmentioning
confidence: 99%
“…Their importance to Ωχ0 1 h 2 has been discussed in Refs. [11,18]. Our corrections to the given channels enter the total cross section σ ann in the Boltzmann equation (1.3).…”
Section: Introductionmentioning
confidence: 99%
“…They are able to lead to the correct relic density of dark matter through co-annihilation of the neutralino with the light stop [140][141][142][143][144], and they also enable electroweak baryogenesis (EWBG) sufficiently strong to explain the matter-antimatter asymmetry present in the universe today. Electroweak baryogenesis refers to any mechanism that produces an asymmetry in the density of baryons during the electroweak phase transition.…”
Section: Overviewmentioning
confidence: 99%