Exploring neutralino dark matter resonance annihilation via bA,bH -> b mu^+ mu^- at the LHC
Howard Baer, Alexander Belyaev, Chung Kao, Patrik Svantesson

TL;DR
This paper investigates the potential of the LHC to measure the Higgs boson width and related parameters through the process pp→bφ→bμ+μ−, focusing on the A-resonance in neutralino dark matter models, using simulations to evaluate signal and background.
Contribution
It introduces a method to measure the Higgs width at the LHC via the bμ+μ− channel, providing a new approach to probe neutralino dark matter resonance.
Findings
Higgs width can be measured with 8-17% accuracy for m_A=400-600 GeV.
The process offers a unique way to directly measure the Higgs width at the LHC.
Potential to test the relation 2m_{χ̃_1^0} ≈ m_A through dilepton mass edges.
Abstract
One of the main channels which allows for a large rate of neutralino dark matter annihilation in the early Universe is via the pseudoscalar Higgs A-resonance. In this case, the measured dark matter abundance can be obtained in the minimal supergravity (mSUGRA) model when tan(beta)\sim 50 and 2m_{\tz_1}\sim m_A. We investigate the reaction pp\to b\phi\to b\mu^+\mu^- +X (where \phi =A or H) at the CERN LHC where requiring the tag of a single b-jet allows for amplification of the signal-to-background ratio. The rare but observable Higgs decay to muon pairs allows for a precise measurement of the Higgs boson mass and decay width. We evaluate signal and background using CalcHEP, with muon energy smearing according to the CMS detector. We find that the Higgs width (\Gamma_A) can typically be determined with the accuracy up to \sim 8% (\sim 17%) for m_A\sim 400 (600) GeV assuming 10^3 fb^{-1}…
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