Search for sharp and smooth spectral signatures of μν SSM gravitino dark matter with Fermi-LAT
- Autores
- Gomez Vargas, German Arturo; López-Fogliani, Daniel E.; Muñoz, Carlos; Perez, Andres Daniel; Ruiz De Austri, Roberto
- Año de publicación
- 2017
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- The μνSSM solves the μ problem of supersymmetric models and reproduces neutrino data, simply using couplings with right-handed neutrinos ν's. Given that these couplings break explicitly R parity, the gravitino is a natural candidate for decaying dark matter in the μνSSM. In this work we carry out a complete analysis of the detection of μνSSM gravitino dark matter through γ-ray observations. In addition to the two-body decay producing a sharp line, we include in the analysis the three-body decays producing a smooth spectral signature. We perform first a deep exploration of the low-energy parameter space of the μνSSM taking into account that neutrino data must be reproduced. Then, we compare the γ-ray fluxes predicted by the model with Fermi-LAT observations. In particular, with the 95% CL upper limits on the total diffuse extragalactic γ-ray background using 50 months of data, together with the upper limits on line emission from an updated analysis using 69.9 months of data. For standard values of bino and wino masses, gravitinos with masses larger than about 4 GeV, or lifetimes smaller than about 1028 s, produce too large fluxes and are excluded as dark matter candidates. However, when limiting scenarios with large and close values of the gaugino masses are considered, the constraints turn out to be less stringent, excluding masses larger than 17 GeV and lifetimes smaller than 4 × 1025 s.
Fil: Gomez Vargas, German Arturo. Universidad Católica de Chile; Chile. Pontificia Universidad Católica de Chile; Chile. Istituto Nazionale Di Fisica Nucleare; Italia
Fil: López-Fogliani, Daniel E.. Universidad de Buenos Aires; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; Argentina
Fil: Muñoz, Carlos. Universidad Autónoma de Madrid; España
Fil: Perez, Andres Daniel. Universidad de Buenos Aires; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; Argentina
Fil: Ruiz De Austri, Roberto. Instituto de Física Corpuscular (csic-uv); España - Materia
-
DARK MATTER EXPERIMENTS
DARK MATTER THEORY
GAMMA RAY EXPERIMENTS - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/52151
Ver los metadatos del registro completo
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Search for sharp and smooth spectral signatures of μν SSM gravitino dark matter with Fermi-LATGomez Vargas, German ArturoLópez-Fogliani, Daniel E.Muñoz, CarlosPerez, Andres DanielRuiz De Austri, RobertoDARK MATTER EXPERIMENTSDARK MATTER THEORYGAMMA RAY EXPERIMENTShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The μνSSM solves the μ problem of supersymmetric models and reproduces neutrino data, simply using couplings with right-handed neutrinos ν's. Given that these couplings break explicitly R parity, the gravitino is a natural candidate for decaying dark matter in the μνSSM. In this work we carry out a complete analysis of the detection of μνSSM gravitino dark matter through γ-ray observations. In addition to the two-body decay producing a sharp line, we include in the analysis the three-body decays producing a smooth spectral signature. We perform first a deep exploration of the low-energy parameter space of the μνSSM taking into account that neutrino data must be reproduced. Then, we compare the γ-ray fluxes predicted by the model with Fermi-LAT observations. In particular, with the 95% CL upper limits on the total diffuse extragalactic γ-ray background using 50 months of data, together with the upper limits on line emission from an updated analysis using 69.9 months of data. For standard values of bino and wino masses, gravitinos with masses larger than about 4 GeV, or lifetimes smaller than about 1028 s, produce too large fluxes and are excluded as dark matter candidates. However, when limiting scenarios with large and close values of the gaugino masses are considered, the constraints turn out to be less stringent, excluding masses larger than 17 GeV and lifetimes smaller than 4 × 1025 s.Fil: Gomez Vargas, German Arturo. Universidad Católica de Chile; Chile. Pontificia Universidad Católica de Chile; Chile. Istituto Nazionale Di Fisica Nucleare; ItaliaFil: López-Fogliani, Daniel E.. Universidad de Buenos Aires; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; ArgentinaFil: Muñoz, Carlos. Universidad Autónoma de Madrid; EspañaFil: Perez, Andres Daniel. Universidad de Buenos Aires; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; ArgentinaFil: Ruiz De Austri, Roberto. Instituto de Física Corpuscular (csic-uv); EspañaIOP Publishing2017-03info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/52151Gomez Vargas, German Arturo; López-Fogliani, Daniel E.; Muñoz, Carlos; Perez, Andres Daniel; Ruiz De Austri, Roberto; Search for sharp and smooth spectral signatures of μν SSM gravitino dark matter with Fermi-LAT; IOP Publishing; Journal of Cosmology and Astroparticle Physics; 2017; 3; 3-2017; 1-241475-7516CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1608.08640info:eu-repo/semantics/altIdentifier/doi/10.1088/1475-7516/2017/03/047info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:19:40Zoai:ri.conicet.gov.ar:11336/52151instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 10:19:41.195CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Search for sharp and smooth spectral signatures of μν SSM gravitino dark matter with Fermi-LAT |
title |
Search for sharp and smooth spectral signatures of μν SSM gravitino dark matter with Fermi-LAT |
spellingShingle |
Search for sharp and smooth spectral signatures of μν SSM gravitino dark matter with Fermi-LAT Gomez Vargas, German Arturo DARK MATTER EXPERIMENTS DARK MATTER THEORY GAMMA RAY EXPERIMENTS |
title_short |
Search for sharp and smooth spectral signatures of μν SSM gravitino dark matter with Fermi-LAT |
title_full |
Search for sharp and smooth spectral signatures of μν SSM gravitino dark matter with Fermi-LAT |
title_fullStr |
Search for sharp and smooth spectral signatures of μν SSM gravitino dark matter with Fermi-LAT |
title_full_unstemmed |
Search for sharp and smooth spectral signatures of μν SSM gravitino dark matter with Fermi-LAT |
title_sort |
Search for sharp and smooth spectral signatures of μν SSM gravitino dark matter with Fermi-LAT |
dc.creator.none.fl_str_mv |
Gomez Vargas, German Arturo López-Fogliani, Daniel E. Muñoz, Carlos Perez, Andres Daniel Ruiz De Austri, Roberto |
author |
Gomez Vargas, German Arturo |
author_facet |
Gomez Vargas, German Arturo López-Fogliani, Daniel E. Muñoz, Carlos Perez, Andres Daniel Ruiz De Austri, Roberto |
author_role |
author |
author2 |
López-Fogliani, Daniel E. Muñoz, Carlos Perez, Andres Daniel Ruiz De Austri, Roberto |
author2_role |
author author author author |
dc.subject.none.fl_str_mv |
DARK MATTER EXPERIMENTS DARK MATTER THEORY GAMMA RAY EXPERIMENTS |
topic |
DARK MATTER EXPERIMENTS DARK MATTER THEORY GAMMA RAY EXPERIMENTS |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
The μνSSM solves the μ problem of supersymmetric models and reproduces neutrino data, simply using couplings with right-handed neutrinos ν's. Given that these couplings break explicitly R parity, the gravitino is a natural candidate for decaying dark matter in the μνSSM. In this work we carry out a complete analysis of the detection of μνSSM gravitino dark matter through γ-ray observations. In addition to the two-body decay producing a sharp line, we include in the analysis the three-body decays producing a smooth spectral signature. We perform first a deep exploration of the low-energy parameter space of the μνSSM taking into account that neutrino data must be reproduced. Then, we compare the γ-ray fluxes predicted by the model with Fermi-LAT observations. In particular, with the 95% CL upper limits on the total diffuse extragalactic γ-ray background using 50 months of data, together with the upper limits on line emission from an updated analysis using 69.9 months of data. For standard values of bino and wino masses, gravitinos with masses larger than about 4 GeV, or lifetimes smaller than about 1028 s, produce too large fluxes and are excluded as dark matter candidates. However, when limiting scenarios with large and close values of the gaugino masses are considered, the constraints turn out to be less stringent, excluding masses larger than 17 GeV and lifetimes smaller than 4 × 1025 s. Fil: Gomez Vargas, German Arturo. Universidad Católica de Chile; Chile. Pontificia Universidad Católica de Chile; Chile. Istituto Nazionale Di Fisica Nucleare; Italia Fil: López-Fogliani, Daniel E.. Universidad de Buenos Aires; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; Argentina Fil: Muñoz, Carlos. Universidad Autónoma de Madrid; España Fil: Perez, Andres Daniel. Universidad de Buenos Aires; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; Argentina Fil: Ruiz De Austri, Roberto. Instituto de Física Corpuscular (csic-uv); España |
description |
The μνSSM solves the μ problem of supersymmetric models and reproduces neutrino data, simply using couplings with right-handed neutrinos ν's. Given that these couplings break explicitly R parity, the gravitino is a natural candidate for decaying dark matter in the μνSSM. In this work we carry out a complete analysis of the detection of μνSSM gravitino dark matter through γ-ray observations. In addition to the two-body decay producing a sharp line, we include in the analysis the three-body decays producing a smooth spectral signature. We perform first a deep exploration of the low-energy parameter space of the μνSSM taking into account that neutrino data must be reproduced. Then, we compare the γ-ray fluxes predicted by the model with Fermi-LAT observations. In particular, with the 95% CL upper limits on the total diffuse extragalactic γ-ray background using 50 months of data, together with the upper limits on line emission from an updated analysis using 69.9 months of data. For standard values of bino and wino masses, gravitinos with masses larger than about 4 GeV, or lifetimes smaller than about 1028 s, produce too large fluxes and are excluded as dark matter candidates. However, when limiting scenarios with large and close values of the gaugino masses are considered, the constraints turn out to be less stringent, excluding masses larger than 17 GeV and lifetimes smaller than 4 × 1025 s. |
publishDate |
2017 |
dc.date.none.fl_str_mv |
2017-03 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
format |
article |
status_str |
publishedVersion |
dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/52151 Gomez Vargas, German Arturo; López-Fogliani, Daniel E.; Muñoz, Carlos; Perez, Andres Daniel; Ruiz De Austri, Roberto; Search for sharp and smooth spectral signatures of μν SSM gravitino dark matter with Fermi-LAT; IOP Publishing; Journal of Cosmology and Astroparticle Physics; 2017; 3; 3-2017; 1-24 1475-7516 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/52151 |
identifier_str_mv |
Gomez Vargas, German Arturo; López-Fogliani, Daniel E.; Muñoz, Carlos; Perez, Andres Daniel; Ruiz De Austri, Roberto; Search for sharp and smooth spectral signatures of μν SSM gravitino dark matter with Fermi-LAT; IOP Publishing; Journal of Cosmology and Astroparticle Physics; 2017; 3; 3-2017; 1-24 1475-7516 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1608.08640 info:eu-repo/semantics/altIdentifier/doi/10.1088/1475-7516/2017/03/047 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
dc.format.none.fl_str_mv |
application/pdf application/pdf |
dc.publisher.none.fl_str_mv |
IOP Publishing |
publisher.none.fl_str_mv |
IOP Publishing |
dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
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CONICET Digital (CONICET) |
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CONICET Digital (CONICET) |
instname_str |
Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.name.fl_str_mv |
CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.mail.fl_str_mv |
dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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13.070432 |