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Signatures of Majorana dark matter with t-channel mediators

Three main strategies are being pursued to search for non-gravitational dark matter signals: direct detection, indirect detection and collider searches. Interestingly, experiments have reached sensitivities in these three search strategies which may allow detection in the near future. In order to ta...

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Detalles Bibliográficos
Autores principales: Garny, Mathias, Ibarra, Alejandro, Vogl, Stefan
Lenguaje:eng
Publicado: 2015
Materias:
Acceso en línea:https://dx.doi.org/10.1142/S0218271815300190
http://cds.cern.ch/record/1999386
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author Garny, Mathias
Ibarra, Alejandro
Vogl, Stefan
author_facet Garny, Mathias
Ibarra, Alejandro
Vogl, Stefan
author_sort Garny, Mathias
collection CERN
description Three main strategies are being pursued to search for non-gravitational dark matter signals: direct detection, indirect detection and collider searches. Interestingly, experiments have reached sensitivities in these three search strategies which may allow detection in the near future. In order to take full benefit of the wealth of experimental data, and in order to confirm a possible dark matter signal, it is necessary to specify the nature of the dark matter particle and of the mediator to the Standard Model. In this paper, we focus on a simplified model where the dark matter particle is a Majorana fermion that couples to a light Standard Model fermion via a Yukawa coupling with a scalar mediator. We review the observational signatures of this model and we discuss the complementarity among the various search strategies, with emphasis in the well motivated scenario where the dark matter particles are produced in the early Universe via thermal freeze-out.
id cern-1999386
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2015
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spelling cern-19993862021-05-03T20:02:30Zdoi:10.1142/S0218271815300190http://cds.cern.ch/record/1999386engGarny, MathiasIbarra, AlejandroVogl, StefanSignatures of Majorana dark matter with t-channel mediatorsParticle Physics - PhenomenologyThree main strategies are being pursued to search for non-gravitational dark matter signals: direct detection, indirect detection and collider searches. Interestingly, experiments have reached sensitivities in these three search strategies which may allow detection in the near future. In order to take full benefit of the wealth of experimental data, and in order to confirm a possible dark matter signal, it is necessary to specify the nature of the dark matter particle and of the mediator to the Standard Model. In this paper, we focus on a simplified model where the dark matter particle is a Majorana fermion that couples to a light Standard Model fermion via a Yukawa coupling with a scalar mediator. We review the observational signatures of this model and we discuss the complementarity among the various search strategies, with emphasis in the well motivated scenario where the dark matter particles are produced in the early Universe via thermal freeze-out.Three main strategies are being pursued to search for non-gravitational dark matter signals: direct detection, indirect detection and collider searches. Interestingly, experiments have reached sensitivities in these three search strategies which may allow detection in the near future. In order to take full benefit of the wealth of experimental data, and in order to confirm a possible dark matter signal, it is necessary to specify the nature of the dark matter particle and of the mediator to the Standard Model. In this paper, we focus on a simplified model where the dark matter particle is a Majorana fermion that couples to a light Standard Model fermion via a Yukawa coupling with a scalar mediator. We review the observational signatures of this model and we discuss the complementarity among the various search strategies, with emphasis in the well motivated scenario where the dark matter particles are produced in the early Universe via thermal freeze-out.Three main strategies are being pursued to search for nongravitational dark matter signals: direct detection, indirect detection and collider searches. Interestingly, experiments have reached sensitivities in these three search strategies which may allow detection in the near future. In order to take full benefit of the wealth of experimental data, and in order to confirm a possible dark matter signal, it is necessary to specify the nature of the dark matter particle and of the mediator to the Standard Model. In this paper, we focus on a simplified model where the dark matter particle is a Majorana fermion that couples to a light Standard Model fermion via a Yukawa coupling with a scalar mediator. We review the observational signatures of this model and we discuss the complementarity among the various search strategies, with emphasis in the well motivated scenario where the dark matter particles are produced in the early universe via thermal freeze-out.CERN-PH-TH-2015-036TUM-HEP-985-15arXiv:1503.01500CERN-PH-TH-2015-036TUM-HEP 985-15oai:cds.cern.ch:19993862015-03-04
spellingShingle Particle Physics - Phenomenology
Garny, Mathias
Ibarra, Alejandro
Vogl, Stefan
Signatures of Majorana dark matter with t-channel mediators
title Signatures of Majorana dark matter with t-channel mediators
title_full Signatures of Majorana dark matter with t-channel mediators
title_fullStr Signatures of Majorana dark matter with t-channel mediators
title_full_unstemmed Signatures of Majorana dark matter with t-channel mediators
title_short Signatures of Majorana dark matter with t-channel mediators
title_sort signatures of majorana dark matter with t-channel mediators
topic Particle Physics - Phenomenology
url https://dx.doi.org/10.1142/S0218271815300190
http://cds.cern.ch/record/1999386
work_keys_str_mv AT garnymathias signaturesofmajoranadarkmatterwithtchannelmediators
AT ibarraalejandro signaturesofmajoranadarkmatterwithtchannelmediators
AT voglstefan signaturesofmajoranadarkmatterwithtchannelmediators