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Invisible decays of the supersymmetric Higgs and dark matter
We discuss effects of the light sparticles on decays of the lightest Higgs in a supersymmetric model with nonuniversal gaugino masses at the high scale, focusing on the `invisible' decays into neutralinos. These can impact significanlty the discovery possibilities of the lightest Higgs at the L...
Autores principales: | , , |
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Lenguaje: | eng |
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2002
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Acceso en línea: | http://cds.cern.ch/record/565490 |
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author | Boudjema, F. Belanger, G. Godbole, R.M. |
author_facet | Boudjema, F. Belanger, G. Godbole, R.M. |
author_sort | Boudjema, F. |
collection | CERN |
description | We discuss effects of the light sparticles on decays of the lightest Higgs in a supersymmetric model with nonuniversal gaugino masses at the high scale, focusing on the `invisible' decays into neutralinos. These can impact significanlty the discovery possibilities of the lightest Higgs at the LHC. We show that due to these decays, there exist regions of the $M_2-\mu$ space where the B.R. $(h \to \gamma \gamma)$ becomes dangerously low even after imposing the LEP constraints on the sparticle masses, implying a possible preclusion of its discovery in the $\gamma \gamma$ channel. We find that there exist regions in the parameter space with acceptable relic density and where the ratio ${B.R. (h \to \gamma \gamma)_{SUSY} \over B.R. (h \to \gamma \gamma)_{SM}}$ falls below 0.6, implying loss of signal in the $\gamma \gamma$ channel. These regions correspond to $\tilde \chi_1^+, \tilde \chi_2^0$ masses which should be accessible already at the Tevatron. Further we find that considerations of relic density put lower limit on the U(1) gaugino mass parameter $M_1$ independently of $\mu, \tan \beta$ and $m_0$. |
id | cern-565490 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2002 |
record_format | invenio |
spelling | cern-5654902023-03-20T14:28:18Zhttp://cds.cern.ch/record/565490engBoudjema, F.Belanger, G.Godbole, R.M.Invisible decays of the supersymmetric Higgs and dark matterParticle Physics - PhenomenologyWe discuss effects of the light sparticles on decays of the lightest Higgs in a supersymmetric model with nonuniversal gaugino masses at the high scale, focusing on the `invisible' decays into neutralinos. These can impact significanlty the discovery possibilities of the lightest Higgs at the LHC. We show that due to these decays, there exist regions of the $M_2-\mu$ space where the B.R. $(h \to \gamma \gamma)$ becomes dangerously low even after imposing the LEP constraints on the sparticle masses, implying a possible preclusion of its discovery in the $\gamma \gamma$ channel. We find that there exist regions in the parameter space with acceptable relic density and where the ratio ${B.R. (h \to \gamma \gamma)_{SUSY} \over B.R. (h \to \gamma \gamma)_{SM}}$ falls below 0.6, implying loss of signal in the $\gamma \gamma$ channel. These regions correspond to $\tilde \chi_1^+, \tilde \chi_2^0$ masses which should be accessible already at the Tevatron. Further we find that considerations of relic density put lower limit on the U(1) gaugino mass parameter $M_1$ independently of $\mu, \tan \beta$ and $m_0$.We discuss effects of the light sparticles on decays of the lightest Higgs in a supersymmetric model with nonuniversal gaugino masses at the high scale, focusing on the `invisible' decays into neutralinos. These can impact significanlty the discovery possibilities of the lightest Higgs at the LHC. We show that due to these decays, there exist regions of the $M_2-\mu$ space where the B.R. $(h \to \gamma \gamma)$ becomes dangerously low even after imposing the LEP constraints on the sparticle masses, implying a possible preclusion of its discovery in the $\gamma \gamma$ channel. We find that there exist regions in the parameter space with acceptable relic density and where the ratio ${B.R. (h \to \gamma \gamma)_{SUSY} \over B.R. (h \to \gamma \gamma)_{SM}}$ falls below 0.6, implying loss of signal in the $\gamma \gamma$ channel. These regions correspond to $\tilde \chi_1^+, \tilde \chi_2^0$ masses which should be accessible already at the Tevatron. Further we find that considerations of relic density put lower limit on the U(1) gaugino mass parameter $M_1$ independently of $\mu, \tan \beta$ and $m_0$.hep-ph/0206311CERN-TH-2002-141LAPTH-CONF-919CERN-TH-2002-141LAPP-TH-CONF-919oai:cds.cern.ch:5654902002-06-28 |
spellingShingle | Particle Physics - Phenomenology Boudjema, F. Belanger, G. Godbole, R.M. Invisible decays of the supersymmetric Higgs and dark matter |
title | Invisible decays of the supersymmetric Higgs and dark matter |
title_full | Invisible decays of the supersymmetric Higgs and dark matter |
title_fullStr | Invisible decays of the supersymmetric Higgs and dark matter |
title_full_unstemmed | Invisible decays of the supersymmetric Higgs and dark matter |
title_short | Invisible decays of the supersymmetric Higgs and dark matter |
title_sort | invisible decays of the supersymmetric higgs and dark matter |
topic | Particle Physics - Phenomenology |
url | http://cds.cern.ch/record/565490 |
work_keys_str_mv | AT boudjemaf invisibledecaysofthesupersymmetrichiggsanddarkmatter AT belangerg invisibledecaysofthesupersymmetrichiggsanddarkmatter AT godbolerm invisibledecaysofthesupersymmetrichiggsanddarkmatter |