NMSSM explanation for excesses in the search for neutralinos and charginos and a 95 GeV Higgs Boson
NMSSM explanation for excesses in the search for neutralinos and charginos and a 95 GeV Higgs Boson
The observed excesses in the search for neutralinos and charginos by ATLAS and CMS can be fitted simultaneously in the minimal supersymmetric standard model (MSSM) assuming a light higgsino mass, of magnitude less than about 250 GeV, and a compressed higgsino dominated neutralino and chargino spectrum, with 5−10% mass splittings. However, light higgsinos as dark matter would have far too large direct detection cross sections. We consider the next-to-MSSM (NMSSM) with an additional singlino-like lightest supersymmetric particle (LSP) a few GeV below the next-to-lightest supersymmetric particle (NLSP). Sparticles prefer to decay first into the NLSP and remnants from the final decay into the LSP are too soft to contribute to the observed signals. Co-annihilation in the higgsino-sector can generate a relic density in the WMAP/Planck window. The singlino-like LSP has automatically a direct detection cross section below present and future sensitivities: a direct detection signal in the near future would exclude this scenario. The singlet-like Higgs scalar of the NMSSM can have a mass around 95 GeV and signal cross sections in the bb¯ channel at LEP and in the γγ channel at the LHC compatible with the respective observations.
hep-ph
Ellwanger, Ulrich
13d3bd7e-8699-4502-be9f-e6327b4aab22
Hugonie, Cyril
7dfcb431-4486-4299-8fb0-32adabd4234a
King, Stephen F.
f8c616b7-0336-4046-a943-700af83a1538
Moretti, Stefano
b57cf0f0-4bc3-4e02-96e3-071255366614
Ellwanger, Ulrich
13d3bd7e-8699-4502-be9f-e6327b4aab22
Hugonie, Cyril
7dfcb431-4486-4299-8fb0-32adabd4234a
King, Stephen F.
f8c616b7-0336-4046-a943-700af83a1538
Moretti, Stefano
b57cf0f0-4bc3-4e02-96e3-071255366614
[Unknown type: UNSPECIFIED]
Abstract
The observed excesses in the search for neutralinos and charginos by ATLAS and CMS can be fitted simultaneously in the minimal supersymmetric standard model (MSSM) assuming a light higgsino mass, of magnitude less than about 250 GeV, and a compressed higgsino dominated neutralino and chargino spectrum, with 5−10% mass splittings. However, light higgsinos as dark matter would have far too large direct detection cross sections. We consider the next-to-MSSM (NMSSM) with an additional singlino-like lightest supersymmetric particle (LSP) a few GeV below the next-to-lightest supersymmetric particle (NLSP). Sparticles prefer to decay first into the NLSP and remnants from the final decay into the LSP are too soft to contribute to the observed signals. Co-annihilation in the higgsino-sector can generate a relic density in the WMAP/Planck window. The singlino-like LSP has automatically a direct detection cross section below present and future sensitivities: a direct detection signal in the near future would exclude this scenario. The singlet-like Higgs scalar of the NMSSM can have a mass around 95 GeV and signal cross sections in the bb¯ channel at LEP and in the γγ channel at the LHC compatible with the respective observations.
Text
2404.19338v1
- Author's Original
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Accepted/In Press date: 30 April 2024
Additional Information:
17 pages, 9 Figures, 4 Tables
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hep-ph
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Local EPrints ID: 490031
URI: http://eprints.soton.ac.uk/id/eprint/490031
PURE UUID: 2559a043-50f3-4a27-882c-dbec00fe3e98
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Date deposited: 14 May 2024 16:30
Last modified: 15 May 2024 01:38
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Author:
Ulrich Ellwanger
Author:
Cyril Hugonie
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