Comprehensive exploration of t-channel simplified models of dark matter

被引:5
|
作者
Arina, Chiara [1 ]
Fuks, Benjamin [2 ,3 ]
Heisig, Jan [4 ,5 ]
Kraemer, Michael [4 ]
Mantani, Luca [6 ]
Panizzi, Luca [7 ,8 ,9 ]
机构
[1] Catholic Univ Louvain, Ctr Cosmol Particle Phys & Phenomenol CP3, B-1348 Louvain La Neuve, Belgium
[2] Sorbonne Univ, Lab Phys Theor & Hautes Energies LPTHE, UMR 7589, 4 Pl Jussieu, F-75252 Paris 05, France
[3] CNRS, 4 Pl Jussieu, F-75252 Paris 05, France
[4] Rhein Westfal TH Aachen, Inst Theoret Particle Phys & Cosmol, D-52056 Aachen, Germany
[5] Univ Virginia, Dept Phys, Charlottesville, VA 22904 USA
[6] Univ Cambridge, DAMTP, Wilberforce Rd, Cambridge CB3 0WA, England
[7] Univ Calabria, Dipartimento Fis, I-87036 Cosenza, Italy
[8] INFN Cosenza, I-87036 Cosenza, Cosenza, Italy
[9] Univ Southampton, Sch Phys & Astron, Southampton SO17 1BJ, England
关键词
SEARCH;
D O I
10.1103/PhysRevD.108.115007
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We analyze six classes of t-channel dark matter simplified models in which the Standard Model field content is extended by a colored 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. In large parts of the parameter space these strong bounds are driven by same -sign mediator pair production, a channel so far not considered in the experimental analyses embedding t-channel dark matter model interpretations.
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页数:20
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