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| DOI | 10.1103/PHYSREVD.99.115003 | ||||
| Año | 2019 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
In this work we present a simple extension of the Standard Model that contains, as the only new physics component, a massive spin-one matter field in the adjoint representation of SU(2)(L). In order to be consistent with perturbative unitarity, the vector field must be odd under a Z(2), symmetry. Radiative corrections make the neutral component of the triplet (V-0) slightly lighter than the charged ones. We show that V-0 can be the dark matter particle while satisfying all current bounds if it has a mass between 2.8 and 3.8 TeV. We present the current limit on the model parameter space from highly complementary experimental constraints, including dark matter relic density measurement, dark matter direct and indirect detection searches, LHC data on Higgs couplings to photons and LHC data on disappearing track searches. We also show that the two-dimensional parameter space can be fully covered by disappearing track searches at a future 100 TeV hadron collider, which will probe, in particular, the whole mass range relevant for dark matter, thus giving an opportunity to discover or exclude the model.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | Belyaev, A. | Hombre |
Univ Southampton - Reino Unido
University of Southampton - Reino Unido |
| 2 | Cacciapaglia, Giacomo | Hombre |
UNIV LYON 1 - Francia
Université Claude Bernard Lyon 1 - Francia |
| 3 | Mckay, James | Hombre |
Imperial Coll London - Reino Unido
Imperial College London - Reino Unido |
| 4 | Marin, Dixon | Hombre |
Universidad Técnica Federico Santa María - Chile
|
| 5 | ZERWEKH-ARROYO, ALFONSO RAUL | Hombre |
Universidad Técnica Federico Santa María - Chile
|
| Fuente |
|---|
| FONDECYT |
| FAPESP |
| CONICYT (Chile) |
| Fondo Nacional de Desarrollo Científico y Tecnológico |
| Fundação de Amparo à Pesquisa do Estado de São Paulo |
| Comisión Nacional de Investigación Científica y Tecnológica |
| Comisión Nacional de Investigación CientÃfica y Tecnológica |
| Fundação de Amparo à Pesquisa do Estado de São Paulo |
| STFC |
| Science and Technology Facilities Council |
| Consejo Nacional de Innovacion, Ciencia y Tecnologia |
| Royal Society |
| Fondo Nacional de Desarrollo Científico, Tecnológico y de Innovación Tecnológica |
| Agence Nationale de la Recherche |
| Leverhulme Trust |
| Horizon 2020 |
| Fondo Nacional de Desarrollo CientÃfico, Tecnológico y de Innovación Tecnológica |
| NExT Institute |
| Horizon 2020 Framework Programme |
| European Union Horizon 2020 |
| Royal Society Leverhulme Trust |
| University of Salford Manchester |
| Labex-LIO (Lyon Institute of Origins) |
| Soton-FAPESP grant |
| Imperial College London Presidents PhD Scholarship |
| Royal Society International Exchange Grant |
| FRAMA (Federation de Recherche "Andre Marie Ampere") |
| Royal Society Leverhulme Trust Senior Research Fellowship |
| InvisiblesPlus RISE from the European Union Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie |
| USM internal project USM PIIC program |
| Imperial College London |
| InvisiblesPlus RISE |
| NExT Institute and Royal Society International Exchange |
| Labex-LIO |
| Fédération de Recherche |
| FRAMA |
| Imperial College London Presidents |
| Agradecimiento |
|---|
| The authors thank P. Schwaller and J. Zurita for useful discussions and email exchanges on clarifications of the results in Ref. [62]. We would also like to thank A. Pukhov, P. Scott and I. Shapiro for valuable discussions. This work was partially financed by Fondecyt Grants No. 1120346 and No. 1160423, USM internal project USM PIIC program, Conicyt (Chile) Grants No. ACT-1406 and No. PIA/Basal FB0821. G. C. acknowledges partial support from the Labex-LIO (Lyon Institute of Origins) under Grant No. ANR-10-LABX-66 (Agence Nationale de la Recherche) and FRAMA (FR3127, Federation de Recherche "Andre Marie Ampere"). A. Z. is very thankful to the developers of MAXIMA [64] and the package Dirac2 [65]. These software packages were used in parts of this work. A. B. acknowledges partial support from the STFC Grant No. ST/L000296/1, Royal Society Leverhulme Trust Senior Research Fellowship LT140094, and Soton-FAPESP grant. A. B. also thanks the NExT Institute and Royal Society International Exchange Grant No. IE150682, partial support from the InvisiblesPlus RISE from the European Union Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie Grant Agreement No. 690575. J. M. was funded by the Imperial College London Presidents PhD Scholarship. T. T. and P. M. would like to thank FAPESP for support through Grant No. 2013/01907-0. T. T. would like also to thank FAPESP for support through Grant No. 2016/15897-4. |
| The authors thank P. Schwaller and J. Zurita for useful discussions and email exchanges on clarifications of the results in Ref. . We would also like to thank A. Pukhov, P. Scott and I. Shapiro for valuable discussions. This work was partially financed by Fondecyt Grants No. 1120346 and No. 1160423, USM internal project USM PIIC program, Conicyt (Chile) Grants No. ACT-1406 and No. PIA/Basal FB0821. G. C. acknowledges partial support from the Labex-LIO (Lyon Institute of Origins) under Grant No. ANR-10-LABX-66 (Agence Nationale de la Recherche) and FRAMA (FR3127, Fédération de Recherche “André Marie Ampère”). A. Z. is very thankful to the developers of MAXIMA and the package Dirac2 . These software packages were used in parts of this work. A. B. acknowledges partial support from the STFC Grant No. ST/L000296/1, Royal Society Leverhulme Trust Senior Research Fellowship LT140094, and Soton-FAPESP grant. A. B. also thanks the NExT Institute and Royal Society International Exchange Grant No. IE150682, partial support from the InvisiblesPlus RISE from the European Union Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie Grant Agreement No. 690575. J. M. was funded by the Imperial College London Presidents PhD Scholarship. T. T. and P. M. would like to thank FAPESP for support through Grant No. 2013/01907-0. T. T. would like also to thank FAPESP for support through Grant No. 2016/15897-4. |