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| DOI | 10.1007/JHEP03(2022)034 | ||||
| Año | 2022 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
Building up on previous work we propose a Dark Matter (DM) model with gauged matter parity and dynamical gauge coupling unification, driven by the same physics responsible for scotogenic neutrino mass generation. Our construction is based on the extended gauge group SU(3)(c) circle times SU(3)(L) circle times U(1)(X) circle times U(1)(N), whose spontaneous breaking leaves a residual conserved matter parity, M-P, stabilizing the DM particle candidates of the model. The key role is played by Majorana SU(3) (L)-octet leptons, allowing the successful gauge coupling unification and a one-loop scotogenic neutrino mass generation. Theoretical consistency allows for a plethora of new particles at the less than or similar to O(10) TeV scale, hence accessible to future collider and low-energy experiments.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | CARCAMO-HERNANDEZ, ANTONIO ENRIQUE | Hombre |
Universidad Técnica Federico Santa María - Chile
Centro Científico Tecnológico de Valparaíso - Chile Instituto Milenio de Física Subatómica en la Frontera de Altas Energías - Chile |
| 2 | Hati, Chandan | Hombre |
TECH UNIV MUNICH - Alemania
Fakultät für Physik, Technische Universität München - Alemania Technische Universität München - Alemania |
| 3 | Kovalenko, S. | Hombre |
Centro Científico Tecnológico de Valparaíso - Chile
Instituto Milenio de Física Subatómica en la Frontera de Altas Energías - Chile Universidad Nacional Andrés Bello - Chile |
| 4 | Conley, R. | Hombre |
Univ Valencia - España
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| 5 | Vaquera-Araujo, C. A. | Hombre |
UNIV GUANAJUATO - México
CONSEJO NACL CIENCIA & TECHNOL - México Dual CP Inst High Energy Phys - México Universidad de Guanajuato - México Consejo Nacional de Ciencia y Tecnologia Mexico - México Universidad de Colima - México Consejo Nacional de Humanidades, Ciencias y Tecnologías - México |
| Fuente |
|---|
| Milenio |
| DFG |
| Generalitat Valenciana |
| AEI |
| Mexican Cátedras CONACYT |
| ANID PIA/APOYO |
| ANID-Chile FONDECYT |
| Agradecimiento |
|---|
| Work supported by the Spanish grants PID2020-113775GB-I00 (AEI/10.13039/501100011033) and PROMETEO/2018/165 (Generalitat Valenciana). A.E.C.H and S.K. are supported by ANID-Chile FONDECYT 1210378 and ANID-Chile FONDECYT 1190845 as well as by ANID PIA/APOYO AFB180002 and Milenio-ANIDICN2019_044. C.H. acknowledges support from the DFG Emmy Noether Grant No. HA 8555/1-1. CAV-A is supported by the Mexican Catedras CONACYT project 749 and SNI 58928. The relic abundance and direct detection constraints were calculated using the MicroOmegas package [43] at GuaCAL (Guanajuato Computational Astroparticle Lab). |