Cosmic abundances of SIMP dark matter
Journal of High Energy Physics, ISSN: 1029-8479, Vol: 2017, Issue: 4
2017
- 56Citations
- 7Captures
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Example: if you select the 1-year option for an article published in 2019 and a metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019. If you select the 3-year option for the same article published in 2019 and the metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019, 2018 and 2017.
Citation Benchmarking is provided by Scopus and SciVal and is different from the metrics context provided by PlumX Metrics.
Article Description
Thermal production of light dark matter with sub-GeV scale mass can be attributed to 3 → 2 self-annihilation processes. We consider the thermal average for annihilation cross sections of dark matter at 3 → 2 and general higher-order interactions. A correct thermal average for initial dark matter particles is important, in particular, for annihilation cross sections with overall velocity dependence and/or resonance poles. We apply our general results to benchmark models for SIMP dark matter and discuss the effects of the resonance pole in determining the relic density.
Bibliographic Details
http://www.scopus.com/inward/record.url?partnerID=HzOxMe3b&scp=85018433515&origin=inward; http://dx.doi.org/10.1007/jhep04(2017)154; http://link.springer.com/10.1007/JHEP04(2017)154; http://link.springer.com/content/pdf/10.1007/JHEP04(2017)154.pdf; http://dx.doi.org/10.1007/jhep04%282017%29154; https://dx.doi.org/10.1007/jhep04%282017%29154; https://link.springer.com/article/10.1007/JHEP04(2017)154
Springer Nature
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