The 125 GeV Higgs in the NMSSM in light of LHC results and astrophysics constraints
Daniel Albornoz Vasquez, Genevieve Belanger, Celine Boehm, Jonathan Da, Silva, Peter Richardson, Chris Wymant

TL;DR
This paper investigates whether the NMSSM model can explain the 125 GeV Higgs signal observed at the LHC, considering astrophysical constraints and potential unique signatures of supersymmetric particles.
Contribution
It demonstrates that the NMSSM can accommodate the Higgs signal while satisfying astrophysical dark matter constraints and proposes new search strategies for supersymmetric signatures.
Findings
NMSSM can explain the Higgs signal within astrophysical constraints
Parameter space configurations compatible with observed Higgs signal
Potential for distinguishing NMSSM Higgs from Standard Model via dedicated searches
Abstract
Recent LHC data suggest an excess in the Higgs decay channels into gamma gamma, W W and Z Z at roughly 125 GeV. The current excess in the diphoton channel is twice that expected from a Standard Model Higgs; whilst this may well change with more statistics, it is interesting to consider the implications should the result persist. Here, we assess whether the NMSSM with a neutralino dark matter candidate could explain this excess when astrophysical constraints (e.g. no overproduction of gamma rays and radio emission in the galaxy, no anomalous excess in the dark matter direct detection experiments and no dark matter overabundance) are imposed on the neutralino. This enables us to disregard unphysical regions of the parameter space even though the Higgs signal is compatible with the observed excess. The result of our analysis is that there are configurations of the parameter space which can…
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Taxonomy
TopicsParticle physics theoretical and experimental studies · Computational Physics and Python Applications · Dark Matter and Cosmic Phenomena
