Precise estimate of charged Wino decay rate [PDF]
The Wino is an SU(2) L triplet Majorana fermion and a well-motivated dark matter candidate. The mass difference between the charged and the neutral Winos is small thanks to the SU(2) L symmetry. The small mass difference makes the charged Wino metastable,
Masahiro Ibe +3 more
doaj +4 more sources
Zero-range effective field theory for resonant wino dark matter. Part III. Annihilation effects [PDF]
Near a critical value of the wino mass where there is a zero-energy S-wave resonance at the neutral-wino-pair threshold, low-energy winos can be described by a zero-range effective field theory (ZREFT) in which the winos interact nonperturbatively ...
Eric Braaten, Evan Johnson, Hong Zhang
doaj +4 more sources
Zero-range effective field theory for resonant wino dark matter. Part II. Coulomb resummation [PDF]
Near a critical value of the wino mass where there is a zero-energy S-wave resonance at the neutral-wino-pair threshold, low-energy winos can be described by a zero-range effective field theory (ZREFT) in which the winos interact nonperturbatively ...
Eric Braaten, Evan Johnson, Hong Zhang
doaj +4 more sources
R-parity violating decays of Wino chargino and wino neutralino LSPs and NLSPs at the LHC [PDF]
The R-parity violating decays of both Wino chargino and Wino neutralino LSPs are analyzed within the context of the B − L MSSM “heterotic standard model”.
Sebastian Dumitru +2 more
doaj +6 more sources
Closing in on the Wino LSP via trilepton searches at the LHC [PDF]
The neutralino dark matter (DM) predicted by the Minimal Supersymmetric Standard Model (MSSM) has been probed in several search modes at the Large Hadron Collider (LHC), one of the leading ones among which is the trilepton plus missing transverse ...
W. Abdallah +3 more
doaj +4 more sources
How light a higgsino or a wino dark matter can become in a compressed scenario of MSSM [PDF]
Higgsinos and Wino have strong motivations for being Dark Matter (DM) candidates in supersymmetry, but their annihilation cross sections are quite large.
Manimala Chakraborti +2 more
doaj +4 more sources
Sommerfeld-corrected relic abundance of wino dark matter with NLO electroweak potentials [PDF]
Extending previous work, we calculate the electroweak potentials for all co-annihilation channels of wino dark matter at the one-loop order and obtain the wino relic abundance including the Sommerfeld effect at the next-to-leading order (NLO).
Martin Beneke, Robert Szafron, Kai Urban
doaj +2 more sources
Wino potential and Sommerfeld effect at NLO [PDF]
We calculate the SU(2)×U(1) electroweak static potential between a fermionic triplet in the broken phase of the Standard Model in the one-loop order (NLO).
Martin Beneke, Robert Szafron, Kai Urban
doaj +2 more sources
Wino-Higgsino dark matter in MSSM from the g − 2 anomaly [PDF]
In this letter, we show that the wino-Higgsino dark matter (DM) is detectable in near future DM direct detection experiments for almost all consistent parameter space in the spontaneously broken supergravity (SUGRA) if the muon g−2 anomaly is explained ...
Sho Iwamoto +2 more
doaj +2 more sources
Discovery reach for wino and higgsino dark matter with a disappearing track signature at a 100 TeV pp collider [PDF]
Within the theory of supersymmetry, the lightest neutralino is a dark matter candidate and is often assumed to be the lightest supersymmetric particle (LSP) as well.
Masahiko Saito +3 more
doaj +3 more sources

