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Sneutrino NLSP Scenarios in the NUHM with Gravitino Dark Matter
We analyze scenarios in which some flavour of sneutrino is the next-to-lightest supersymmetric particle (NLSP), assuming that the gravitino is the lightest supersymmetric particle (LSP) and provides the cold dark matter. Such scenarios do not arise in the constrained supersymmetric extension of the...
Autores principales: | , , |
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Lenguaje: | eng |
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2008
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Acceso en línea: | https://dx.doi.org/10.1088/1126-6708/2008/10/005 http://cds.cern.ch/record/1116996 |
_version_ | 1780914433867907072 |
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author | Ellis, John R. Olive, Keith A. Santoso, Yudi |
author_facet | Ellis, John R. Olive, Keith A. Santoso, Yudi |
author_sort | Ellis, John R. |
collection | CERN |
description | We analyze scenarios in which some flavour of sneutrino is the next-to-lightest supersymmetric particle (NLSP), assuming that the gravitino is the lightest supersymmetric particle (LSP) and provides the cold dark matter. Such scenarios do not arise in the constrained supersymmetric extension of the Standard Model (CMSSM) with universal gaugino and scalar masses input at the GUT scale. However, models with non-universal Higgs masses (NUHM) do allow scenarios with a sneutrino NLSP, which are quite generic. We illustrate how such scenarios may arise, analyze the possible metastable sneutrino lifetime, and explore the theoretical, phenomenological, experimental and cosmological constraints on such scenarios. We also discuss the collider signatures of such scenarios, how they may be distinguished from neutralino LSP scenarios, and how different flavours of sneutrino NLSP may be distinguished. |
id | cern-1116996 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2008 |
record_format | invenio |
spelling | cern-11169962023-03-14T16:47:25Zdoi:10.1088/1126-6708/2008/10/005http://cds.cern.ch/record/1116996engEllis, John R.Olive, Keith A.Santoso, YudiSneutrino NLSP Scenarios in the NUHM with Gravitino Dark MatterParticle Physics - PhenomenologyWe analyze scenarios in which some flavour of sneutrino is the next-to-lightest supersymmetric particle (NLSP), assuming that the gravitino is the lightest supersymmetric particle (LSP) and provides the cold dark matter. Such scenarios do not arise in the constrained supersymmetric extension of the Standard Model (CMSSM) with universal gaugino and scalar masses input at the GUT scale. However, models with non-universal Higgs masses (NUHM) do allow scenarios with a sneutrino NLSP, which are quite generic. We illustrate how such scenarios may arise, analyze the possible metastable sneutrino lifetime, and explore the theoretical, phenomenological, experimental and cosmological constraints on such scenarios. We also discuss the collider signatures of such scenarios, how they may be distinguished from neutralino LSP scenarios, and how different flavours of sneutrino NLSP may be distinguished.We analyze scenarios in which some flavour of sneutrino is the next-to-lightest supersymmetric particle (NLSP), assuming that the gravitino is the lightest supersymmetric particle (LSP) and provides the cold dark matter. Such scenarios do not arise in the constrained supersymmetric extension of the Standard Model (CMSSM) with universal gaugino and scalar masses input at the GUT scale. However, models with non-universal Higgs masses (NUHM) do allow scenarios with a sneutrino NLSP, which are quite generic. We illustrate how such scenarios may arise, analyze the possible metastable sneutrino lifetime, and explore the theoretical, phenomenological, experimental and cosmological constraints on such scenarios. We also discuss the collider signatures of such scenarios, how they may be distinguished from neutralino LSP scenarios, and how different flavours of sneutrino NLSP may be distinguished.arXiv:0807.3736CERN-PH-TH-2008-159UMN-TH-2708-08FTPI-MINN-08-28IPPP-08-53DCPT-08-106CERN-PH-TH-2008-159DCPT-08-106FTPI-MINN-08-28IPPP-08-53UMN-TH-2708-08oai:cds.cern.ch:11169962008-07-24 |
spellingShingle | Particle Physics - Phenomenology Ellis, John R. Olive, Keith A. Santoso, Yudi Sneutrino NLSP Scenarios in the NUHM with Gravitino Dark Matter |
title | Sneutrino NLSP Scenarios in the NUHM with Gravitino Dark Matter |
title_full | Sneutrino NLSP Scenarios in the NUHM with Gravitino Dark Matter |
title_fullStr | Sneutrino NLSP Scenarios in the NUHM with Gravitino Dark Matter |
title_full_unstemmed | Sneutrino NLSP Scenarios in the NUHM with Gravitino Dark Matter |
title_short | Sneutrino NLSP Scenarios in the NUHM with Gravitino Dark Matter |
title_sort | sneutrino nlsp scenarios in the nuhm with gravitino dark matter |
topic | Particle Physics - Phenomenology |
url | https://dx.doi.org/10.1088/1126-6708/2008/10/005 http://cds.cern.ch/record/1116996 |
work_keys_str_mv | AT ellisjohnr sneutrinonlspscenariosinthenuhmwithgravitinodarkmatter AT olivekeitha sneutrinonlspscenariosinthenuhmwithgravitinodarkmatter AT santosoyudi sneutrinonlspscenariosinthenuhmwithgravitinodarkmatter |