Results 11 to 20 of about 2,327 (186)
Precision photon spectra for wino annihilation [PDF]
Journal of High Energy Physics, 2019 We provide precise predictions for the hard photon spectrum resulting from neutral SU(2) W triplet (wino) dark matter annihilation. Our calculation is performed utilizing an effective field theory expansion around the endpoint region where the photon ...
Matthew Baumgart +8 more
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Zero-range effective field theory for resonant wino dark matter. Part I. Framework
Journal of High Energy Physics, 2017 The most dramatic “Sommerfeld enhancements” of neutral-wino-pair annihilation occur when the wino mass is near a critical value where there is a zero-energy S-wave resonance at the neutral-wino-pair threshold.
Eric Braaten, Evan Johnson, Hong Zhang
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Sommerfeld-corrected relic abundance of wino dark matter with NLO electroweak potentials
Journal 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
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R-parity violating decays of Wino chargino and wino neutralino LSPs and NLSPs at the LHC [PDF]
Journal 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
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Zero-range effective field theory for resonant wino dark matter. Part II. Coulomb resummation
Journal 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
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Smallest halos in thermal wino dark matter [PDF]
Physical Review D, 2019 (Mini) split supersymmetry explains the observed Higgs mass and evades stringent constraints, while keeping good features of TeV-scale supersymmetry other than the little hierarchy problem. Such scenarios naturally predict thermal wino dark matter whose mass is around $3 \, {\rm TeV}$.
Shin’ichiro Ando +3 more
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Wino w wybranych epigramatach greckich [PDF]
Język. Religia. Tożsamość, 2023 Poetry and wine not only permeate throughout Greek culture but also emerge as inseparable motifs. The Dionysian gift has accompanied the creators of poetic works since as early as the 7th century BC.
Magadalena Jaworska
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European 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
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Taking aim at the wino-Higgsino plane with the LHC [PDF]
Physical Review DIn this work we explore multiple search strategies for Higgsinos and mixed Higgsino-wino states in the minimal supersymmetric Standard Model (MSSM) and project the results onto the (μ,M2) plane. Assuming associated production of Higgsino-like pairs with a W/Z boson, we develop a search in a channel characterized by a hadronically tagged vector boson ...
Linda M. Carpenter +3 more
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Closing in on the Wino LSP via trilepton searches at the LHC
Journal 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
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