Results 1 to 10 of about 29,791 (204)

Precise estimate of charged Wino decay rate [PDF]

open access: yesJournal of High Energy Physics, 2023
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]

open access: yesJournal of High Energy Physics, 2018
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]

open access: yesJournal of High Energy Physics, 2018
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]

open access: yesJournal of High Energy Physics, 2019
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]

open access: yesJournal of High Energy Physics, 2018
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]

open access: yesJournal of High Energy Physics, 2017
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]

open access: yesJournal of High Energy Physics, 2021
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]

open access: yesPhysics Letters B, 2020
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]

open access: yesPhysics Letters B, 2021
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]

open access: yesEuropean Physical Journal C: Particles and Fields, 2019
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

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