Gravitational wave in a filtered vector dark matter model
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arXiv
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| Autores principales: | , , |
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| Formato: | Preprint |
| Publicado: |
2024
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| Acceso en línea: | |
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| _version_ | 1866917715302678528 |
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| author | Hosseini, Mojtaba Ayazi, Seyed Yaser Mohamadnejad, Ahmad |
| author_facet | Hosseini, Mojtaba Ayazi, Seyed Yaser Mohamadnejad, Ahmad |
| contents | We consider a first order phase transition (FOPT) for a Vector Dark Matter (VDM) in the early universe in which its mass may partially arise from such mechanism in the hidden sector. We calculate the ratio of VDM that may enter the bubble for various bubble wall velocities as well as various nucleation temperatures that produce the measured dark matter relic abundance via bubble filtering. In the following, we focus on gravitational wave (GW) signals which produced by FOPT and show that it can be detectable at the DECIGO, TianQin, LISA and Ultimate-DECIGO (UDECIGO) experiments. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2405_10662 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Gravitational wave in a filtered vector dark matter model Hosseini, Mojtaba Ayazi, Seyed Yaser Mohamadnejad, Ahmad High Energy Physics - Phenomenology We consider a first order phase transition (FOPT) for a Vector Dark Matter (VDM) in the early universe in which its mass may partially arise from such mechanism in the hidden sector. We calculate the ratio of VDM that may enter the bubble for various bubble wall velocities as well as various nucleation temperatures that produce the measured dark matter relic abundance via bubble filtering. In the following, we focus on gravitational wave (GW) signals which produced by FOPT and show that it can be detectable at the DECIGO, TianQin, LISA and Ultimate-DECIGO (UDECIGO) experiments. |
| title | Gravitational wave in a filtered vector dark matter model |
| topic | High Energy Physics - Phenomenology |
| url | https://arxiv.org/abs/2405.10662 |