2017
DOI: 10.1103/physrevd.96.055018
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Not-so-well-tempered neutralino

Abstract: Light electroweakinos, the neutral and charged fermionic supersymmetric partners of the Standard Model SU(2) × U(1) gauge bosons and of the two SU(2) Higgs doublets, are an important target for searches for new physics with the Large Hadron Collider (LHC). However, if the lightest neutralino is the dark matter, constraints from direct dark matter detection experiments rule out large swaths of the parameter space accessible to the LHC, including in large part the so-called "well-tempered" neutralinos. We focus … Show more

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Cited by 31 publications
(24 citation statements)
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“…Such mass spectra and couplings are also expected in scenarios with neutralino dark matter compatible with indirect and direct detection constraints, see e.g. discussions in[56][57][58] 5. Depending on the exact SUSY spectrum, sizable electroweak corrections could appear for these calculations, see Ref [61,62]…”
mentioning
confidence: 69%
“…Such mass spectra and couplings are also expected in scenarios with neutralino dark matter compatible with indirect and direct detection constraints, see e.g. discussions in[56][57][58] 5. Depending on the exact SUSY spectrum, sizable electroweak corrections could appear for these calculations, see Ref [61,62]…”
mentioning
confidence: 69%
“…Therefore, in our study, we will focus on the bino-like dark matter, which can give the observed relic density by mixing with higgsino/wino, resonantly annihilating through Z/Higgs bosons or coannihilating with other light sparticles. The first two mechanisms have been tightly constrained by current XENON1T and LHC experiments [40][41][42], while the coannihilation with light sparticles can still be consistent with current data [43].…”
Section: Neutralino Dark Matter and Muon G − 2 In The Mssmmentioning
confidence: 82%
“…Previous studies have investigated the combined impacts of various DM and collider constraints on the electroweakino sector, in the limit that other sparticles are decoupled [54][55][56][57][58][59][60][61][62][63][64][65][66][67][68]. Here, we carry out a more detailed, model-independent study, performing a global fit of the EWMSSM using only collider constraints from LEP, ATLAS and CMS arising either from direct searches for electroweakinos, or SM particle decays into them.…”
Section: Introductionmentioning
confidence: 99%