Electroweak phase transition in a vector dark matter scenario
Fuente:
arXiv
Guardado en:
| Autores principales: | , , , , |
|---|---|
| Formato: | Preprint |
| Publicado: |
2024
|
| Materias: | |
| Acceso en línea: | |
| Etiquetas: |
Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
|
| _version_ | 1866913525137408000 |
|---|---|
| author | Benincasa, Nico Rose, Luigi Delle Panizzi, Luca Razzaq, Maimoona Urzetta, Savio |
| author_facet | Benincasa, Nico Rose, Luigi Delle Panizzi, Luca Razzaq, Maimoona Urzetta, Savio |
| contents | This study explores the parameter space of a minimal extension of the Standard Model with a non-abelian $SU(2)$ group, in which the gauge bosons are stable and acquire mass through a mechanism of spontaneous symmetry breaking involving a new scalar doublet which interacts with the Higgs boson through a quartic coupling. The exploration aims to assess whether it is possible to obtain a first-order phase transition while ensuring that the gauge bosons are viable dark matter candidates. Theoretical, astrophysical and collider bounds are considered. The results are then tested against the sensitivity of future experiments for the detection of gravitational wave signals. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2410_00501 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Electroweak phase transition in a vector dark matter scenario Benincasa, Nico Rose, Luigi Delle Panizzi, Luca Razzaq, Maimoona Urzetta, Savio High Energy Physics - Phenomenology This study explores the parameter space of a minimal extension of the Standard Model with a non-abelian $SU(2)$ group, in which the gauge bosons are stable and acquire mass through a mechanism of spontaneous symmetry breaking involving a new scalar doublet which interacts with the Higgs boson through a quartic coupling. The exploration aims to assess whether it is possible to obtain a first-order phase transition while ensuring that the gauge bosons are viable dark matter candidates. Theoretical, astrophysical and collider bounds are considered. The results are then tested against the sensitivity of future experiments for the detection of gravitational wave signals. |
| title | Electroweak phase transition in a vector dark matter scenario |
| topic | High Energy Physics - Phenomenology |
| url | https://arxiv.org/abs/2410.00501 |