Impact of Sommerfeld effect and bound state formation in simplified t-channel dark matter models

被引:10
|
作者
Becker, Mathias [1 ]
Copello, Emanuele [1 ]
Harz, Julia [1 ]
Mohan, Kirtimaan A. [2 ]
Sengupta, Dipan [3 ,4 ]
机构
[1] Tech Univ Munich, Phys Dept T70, James Franck Str 1, D-85748 Garching, Germany
[2] Michigan State Univ, Dept Phys & Astron, 567 Wilson Rd, E Lansing, MI 48824 USA
[3] Univ Calif San Diego, Dept Phys & Astron, 9500 Gilman Dr, San Diego, CA 92103 USA
[4] Univ Adelaide, ARC Ctr Excellence Dark Matter Particle Phys, Dept Phys, Adelaide, SA 5005, Australia
基金
美国国家科学基金会;
关键词
Dark Matter at Colliders; Particle Nature of Dark Matter; Early Universe Particle Physics; Cosmology of Theories BSM; RELIC DENSITY;
D O I
10.1007/JHEP08(2022)145
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
The existence of a dark matter model with a rich dark sector could be the reason why WIMP dark matter has evaded its detection so far. For instance, colored co-annihilation naturally leads to the prediction of heavier dark matter masses. Importantly, in such a scenario the Sommerfeld effect and bound state formation must be considered in order to accurately predict the relic abundance. Based on the example of the currently widely studied t-channel simplified model with a colored mediator, we demonstrate the importance of considering these non-perturbative effects for correctly inferring the viable model parameters. We emphasize that a flat correction factor on the relic abundance is not sufficient in this context. Moreover, we find that parameter space thought to be excluded by direct detection experiments and LHC searches remains still viable. Additionally, we illustrate that long-lived particle searches and bound-state searches at the LHC can play a crucial role in probing such a model. We demonstrate how future direct detection experiments will be able to close almost all of the remaining window for freeze-out production, making it a highly testable scenario.
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页数:54
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