A complex scalar singlet could provide a pseudo-scalar dark matter candidate, whose stability is guaranteed by a discrete symmetry: dark CP. The scalar singlet is also charged under a global U(1) symmetry, which is broken both explicitly and spontaneously. We analyze the phenomenology of different models with just one explicit symmetry breaking term and we also consider the case with more than one symmetry breaking term. Finally, we discuss the possibility that the explicit symmetry breaking term is much smaller than the symmetry breaking scale, leading to a pseudo-Nambu-Goldstone boson as a DM candidate.
Conference proceeding
Dark matter from a complex scalar singlet and the role of dark CP
Journal of physics. Conference series, v 2156(1), 12031
01 Dec 2021
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- Title
- Dark matter from a complex scalar singlet and the role of dark CP
- Creators
- Carlos Faubel - Drexel University, Civil, Architectural, and Environmental EngineeringLeonardo Coito - Universitat de ValènciaJuan Herrero-García - Universitat de ValènciaArcadi Santamaria - Universitat de València
- Publication Details
- Journal of physics. Conference series, v 2156(1), 12031
- Series
- Journal of Physics Conference Series
- Publisher
- Institute of Physics (IOP)
- Number of pages
- 5
- Grant note
- "Generalitat Valenciana": FPA2017-84543-P "Generalitat Valenciana" under the "ACIF" fellowship program: PROMETEO/2019/087, PID2020-113334GB-I00/AEI/10.13039/501100011033
This article is based on the talk given at TAUP 2021. The original work [13] was done in collaboration with Leonardo Coito, Juan Herrero-Garcia and Arcadi Santamaria. Work partially supported by the FEDER/MCIyU-AEI grant FPA2017-84543-P, the "Generalitat Valenciana" under grant PROMETEO/2019/087 and by the AEI-MICINN under grant PID2020-113334GB-I00/AEI/10.13039/501100011033. CF is also supported by the "Generalitat Valenciana" under the "ACIF" fellowship program.
- Resource Type
- Conference proceeding
- Language
- English
- Academic Unit
- Civil, Architectural, and Environmental Engineering
- Web of Science ID
- WOS:001432940800031
- Other Identifier
- 991022199650704721