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| DOI | 10.1140/EPJC/S10052-024-13643-3 | ||||
| Año | 2024 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
In this work, we have studied the vector scotogenic model in the context of the dark matter problem. Due to unitarity considerations, we have focused on the scenario with fermion dark matter, finding out that co-annihilations play a fundamental role in achieving dark matter relic abundance. Moreover, the coannihilation effects allow to separate the parameter space into two regions with different phenomenology. In addition, we have studied the detection prospects of these regions separately, focusing on signatures that can appear in lepton flavor violating decays, indirect and direct searches, and the production of these new particles at collider facilities.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | Areyuna, Paulo C. | - |
Instituto Milenio de Física Subatómica en la Frontera de Altas Energías - Chile
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| 1 | Areyuna, C. Paulo | - |
Millennium Inst Subat Phys - Chile
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| 2 | Zamora-Saa, Jilberto | - |
Instituto Milenio de Física Subatómica en la Frontera de Altas Energías - Chile
Universidad Nacional Andrés Bello - Chile Millennium Inst Subat Phys - Chile |
| 3 | ZERWEKH-ARROYO, ALFONSO RAUL | Hombre |
Instituto Milenio de Física Subatómica en la Frontera de Altas Energías - Chile
Universidad Técnica Federico Santa María - Chile Centro Científico Tecnológico de Valparaíso - Chile Millennium Inst Subat Phys - Chile |
| Fuente |
|---|
| FONDECYT |
| Fondo Nacional de Desarrollo Científico y Tecnológico |
| DGIIP-UTFSM |
| Agencia Nacional de Investigación y Desarrollo |
| ANID - Millennium Program |
| Agradecimiento |
|---|
| This work was funded by ANID - Millennium Program - ICN2019_044. Also, we would like to thank to the DGIIP-UTFSM for funding during the development of this work. AZ was partially supported by Proyecto ANID PIA/APOYO AFB220004 (Chile) and Fondecyt 1230110. Also, JZ was partially supported by Fondecyt 1240216. Finally, PAC is grateful to Toshihiko Ota for insightful discussions related with particle cosmology in the early universe, and to Gonzalo Benitez for a comprehensive guidance on the interpretation of partial wave amplitudes. |
| This work was funded by ANID - Millennium Program - ICN2019_044. Also, we would like to thank to the DGIIP-UTFSM for funding during the development of this work. AZ was partially supported by Proyecto ANID PIA/APOYO AFB220004 (Chile) and Fondecyt 1230110. Also, JZ was partially supported by Fondecyt 1240216. Finally, PAC is grateful to Toshihiko Ota for insightful discussions related with particle cosmology in the early universe, and to Gonzalo Benitez for a comprehensive guidance on the interpretation of partial wave amplitudes. |