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New constraints on neutralino dark matter in the supersymmetric standard model
We investigate the prospects for neutralino dark matter within the Supersymmetric Standard Model (SSM) including the constraints from universal soft supersymmetry breaking and radiative breaking of the electroweak symmetry. The latter is enforced by using the one-loop Higgs effective potential which...
Autores principales: | , , , , |
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Lenguaje: | eng |
Publicado: |
1993
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1103/PhysRevD.47.2461 http://cds.cern.ch/record/239232 |
_version_ | 1780884832110247936 |
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author | Kelley, S. Lopez, Jorge L. Nanopoulos, Dimitri V. Pois, H. Yuan, Ka-jia |
author_facet | Kelley, S. Lopez, Jorge L. Nanopoulos, Dimitri V. Pois, H. Yuan, Ka-jia |
author_sort | Kelley, S. |
collection | CERN |
description | We investigate the prospects for neutralino dark matter within the Supersymmetric Standard Model (SSM) including the constraints from universal soft supersymmetry breaking and radiative breaking of the electroweak symmetry. The latter is enforced by using the one-loop Higgs effective potential which automatically gives the one-loop corrected Higgs boson masses. We perform an exhaustive search of the allowed five-dimensional parameter space and find that the neutralino relic abundance $\Omega_\chi h^2_0$ depends most strongly on the ratio $\xi_0\equiv m_0/m_{1/2}$. For $\xi_0\gg1$ the relic abundance is almost always much too large, whereas for $\xi_0\ll1$ the opposite occurs. For $\xi_0\sim1$ there are wide ranges of the remaining parameters for which $\Omega_\chi\sim1$. We also determine that $m_{\tilde q}\gsim250\GeV$ and $m_{\tilde l}\gsim100\GeV$ are necessary in order to possibly achieve $\Omega_\chi\sim1$. These lower bounds are much weaker than the corresponding ones derived previously when radiative breaking was {\it not} enforced. |
id | cern-239232 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 1993 |
record_format | invenio |
spelling | cern-2392322023-03-14T18:53:14Zdoi:10.1103/PhysRevD.47.2461http://cds.cern.ch/record/239232engKelley, S.Lopez, Jorge L.Nanopoulos, Dimitri V.Pois, H.Yuan, Ka-jiaNew constraints on neutralino dark matter in the supersymmetric standard modelParticle Physics - TheoryWe investigate the prospects for neutralino dark matter within the Supersymmetric Standard Model (SSM) including the constraints from universal soft supersymmetry breaking and radiative breaking of the electroweak symmetry. The latter is enforced by using the one-loop Higgs effective potential which automatically gives the one-loop corrected Higgs boson masses. We perform an exhaustive search of the allowed five-dimensional parameter space and find that the neutralino relic abundance $\Omega_\chi h^2_0$ depends most strongly on the ratio $\xi_0\equiv m_0/m_{1/2}$. For $\xi_0\gg1$ the relic abundance is almost always much too large, whereas for $\xi_0\ll1$ the opposite occurs. For $\xi_0\sim1$ there are wide ranges of the remaining parameters for which $\Omega_\chi\sim1$. We also determine that $m_{\tilde q}\gsim250\GeV$ and $m_{\tilde l}\gsim100\GeV$ are necessary in order to possibly achieve $\Omega_\chi\sim1$. These lower bounds are much weaker than the corresponding ones derived previously when radiative breaking was {\it not} enforced.We investigate the prospects for neutralino dark matter within the Supersymmetric Standard Model (SSM) including the constraints from universal soft supersymmetry breaking and radiative breaking of the electroweak symmetry. The latter is enforced by using the one-loop Higgs effective potential which automatically gives the one-loop corrected Higgs boson masses. We perform an exhaustive search of the allowed five-dimensional parameter space and find that the neutralino relic abundance $\Omega_\chi h^2_0$ depends most strongly on the ratio $\xi_0\equiv m_0/m_{1/2}$. For $\xi_0\gg1$ the relic abundance is almost always much too large, whereas for $\xi_0\ll1$ the opposite occurs. For $\xi_0\sim1$ there are wide ranges of the remaining parameters for which $\Omega_\chi\sim1$. We also determine that $m_{\tilde q}\gsim250\GeV$ and $m_{\tilde l}\gsim100\GeV$ are necessary in order to possibly achieve $\Omega_\chi\sim1$. These lower bounds are much weaker than the corresponding ones derived previously when radiative breaking was {\it not} enforced.hep-ph/9207253CERN-TH-6584-92CTP-TAMU-56-92ACT-16-92UAHEP-9212ACT-1992-16CERN-TH-6584-92CTP-TAMU-92-56UA-HEP-92-12oai:cds.cern.ch:2392321993 |
spellingShingle | Particle Physics - Theory Kelley, S. Lopez, Jorge L. Nanopoulos, Dimitri V. Pois, H. Yuan, Ka-jia New constraints on neutralino dark matter in the supersymmetric standard model |
title | New constraints on neutralino dark matter in the supersymmetric standard model |
title_full | New constraints on neutralino dark matter in the supersymmetric standard model |
title_fullStr | New constraints on neutralino dark matter in the supersymmetric standard model |
title_full_unstemmed | New constraints on neutralino dark matter in the supersymmetric standard model |
title_short | New constraints on neutralino dark matter in the supersymmetric standard model |
title_sort | new constraints on neutralino dark matter in the supersymmetric standard model |
topic | Particle Physics - Theory |
url | https://dx.doi.org/10.1103/PhysRevD.47.2461 http://cds.cern.ch/record/239232 |
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