Cargando…

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...

Descripción completa

Detalles Bibliográficos
Autores principales: Boudjema, F., Belanger, G., Godbole, R.M.
Lenguaje:eng
Publicado: 2002
Materias:
Acceso en línea:http://cds.cern.ch/record/565490
_version_ 1780899149699350528
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