Showing 101 - 120 results of 168 for search 'relic particle abundance', query time: 1.38s Refine Results
  1. 101
    by J.A. Casas, D.G. Cerdeño, J.M. Moreno, J. Quilis
    Published 2017-05-01
    ... allow to reproduce the correct DM relic abundance while avoiding the bounds from direct and indirect...
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    Article
  2. 102
    ... coannihilation channels are highly relevant for a determination of the correct relic abundance. Firstly, we...
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  3. 103
    by Luiz, Vivian Ventura Ferreira.
    Published 2017
    ... is one of the open questions of cosmology and particle physics. Several observations, at di erent...
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  4. 104
    by Mamiya Kawaguchi, Shinya Matsuzaki, Akio Tomiya
    Published 2021-02-01
    ... and the cosmological evolution of QCD axion including the estimate of the relic abundance as a dark matter candidate....
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    Article
  5. 105
    by Pyungwon Ko, Toshinori Matsui, Yi-Lei Tang
    Published 2020-10-01
    ... to induce a significant reannihilation process, reducing the dark matter relic abundance. Most...
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    Article
  6. 106
    by Xuewen Liu, Ligong Bian, Xue-Qian Li, Jing Shu
    Published 2016-08-01
    ... processes τ→μγ and Higgs decay gained at LHC. Within the same parameter spaces, the DM relic abundance...
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    Article
  7. 107
    by Chuan-Hung Chen, Cheng-Wei Chiang, Takaaki Nomura
    Published 2015-07-01
    ... relic abundance and satisfying the current direct search bounds. We extend the Higgs triplet model...
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    Article
  8. 108
    ... dark matter are not large enough to generate its relic abundance within the observed limit. We include...
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    Article
  9. 109
    by Manuel Drees, Fazlollah Hajkarim
    Published 2018-12-01
    ... neutralino, as the best-known supersymmetric (SUSY) WIMP, obtains the required relic abundance. Many...
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    Article
  10. 110
    ... sector in the early Universe. We compute the DM relic abundance as a function of the model parameters...
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    Article
  11. 111
    by Miguel G. Folgado, Andrea Donini, Nuria Rius
    Published 2020-04-01
    ..., or one of each), finding that it is possible to obtain the observed relic abundance via thermal freeze...
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    Article
  12. 112
    by Mateusz Duch, Bohdan Grzadkowski, Da Huang
    Published 2020-03-01
    ... mediator. In this model, the DM relic abundance is dominated by the fermionic DM particle which...
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    Article
  13. 113
    ... non-universality, we find that higgsino can be the lightest SUSY particle and its thermal relic...
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    Article
  14. 114
    by Takeshi Fukuyama, Nobuchika Okada, Hieu Minh Tran
    Published 2017-04-01
    ..., the observed SM-like Higgs boson mass of around 125 GeV and the relic abundance of the neutralino dark matter...
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    Article
  15. 115
    ... of the observed relic abundance if the dark matter particles solely originate from thermal production....
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    Article
  16. 116
    ... that the impact of these new effects on the thermal relic abundance is significant enough to make it worthwhile...
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    Article
  17. 117
    by Jae Hyeok Chang, Rouven Essig, Annika Reinert
    Published 2021-03-01
    ... relic abundance from freeze-in are excluded below a few tens of keV, depending on the value of the dark...
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    Article
  18. 118
    by Rizzo, T.G, Wojcik, G.N
    Published 2022
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    Article
  19. 119
    by Julia Harz, Kalliopi Petraki
    Published 2019-04-01
    ... force between TeV-scale particles, that can impact considerably their annihilation due to the Sommerfeld...
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    Article
  20. 120
    by Aleksandr Azatov, Miguel Vanvlasselaer, Wen Yin
    Published 2021-03-01
    ...) relic abundance during the First Order Phase Transition (FOPT) in the early universe. We show...
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    Article