Comprehensive exploration of t -channel simplified models of dark matter
We analyse six classes of t-channel dark matter simplified models in which the Standard Model field content is extended by a coloured mediator and a dark matter state. The two new states are enforced to be odd under a new parity, while all Standard Model fields are taken even so that dark matter sta...
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Veröffentlicht in: | Physical review. D 2023-12, Vol.108 (11), Article 115007 |
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Format: | Artikel |
Sprache: | eng |
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Zusammenfassung: | We analyse six classes of t-channel dark matter simplified models in which the Standard Model field content is extended by a coloured mediator and a dark matter state. The two new states are enforced to be odd under a new parity, while all Standard Model fields are taken even so that dark matter stability is guaranteed. We study several possibilities for the spin of the new particles and the self-conjugate property of the dark matter, and we focus on model configurations in which the dark matter couples to the right-handed up quark for simplicity. We investigate how the parameter spaces of the six models can be constrained by current and future cosmological, astrophysical and collider searches, and we highlight the strong complementary between those probes. Our results demonstrate that scenarios featuring a complex (non self-conjugate) dark matter field are excluded by cosmology and astrophysics alone, the only possibility to avoid these bounds being to invoke very weak couplings and mechanisms such as conversion-driven freeze-out. For models with self-conjugate dark matter, mediator and dark matter masses are pushed deep into the TeV regime, with the lower limits on the mediator mass reaching 3 to 4 TeV and those on the dark matter mass 1 to 2 TeV. Those bounds are much stronger than those obtained in previous studies of t-channel dark matter models, due in particular to overlooked contributions to LHC signal modelling that we incorporate in this work for the first time. |
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ISSN: | 2470-0010 2470-0029 |
DOI: | 10.1103/PhysRevD.108.115007 |