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Minimal spin-one isotriplet dark matter
Indexado
WoS WOS:000470863000004
Scopus SCOPUS_ID:85068522303
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


Abstract



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.

Revista



Revista ISSN
Physical Review D 2470-0010

Métricas Externas



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Disciplinas de Investigación



WOS
Astronomy & Astrophysics
Physics, Particles & Fields
Scopus
Physics And Astronomy (Miscellaneous)
SciELO
Sin Disciplinas

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Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional



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Autores - Afiliación



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

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Financiamiento



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 Científica 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 Científico, 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

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Agradecimientos



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.

Muestra la fuente de financiamiento declarada en la publicación.