Zobrazeno 1 - 10
of 32
pro vyhledávání: '"Hasan Serce"'
Publikováno v:
Physics Letters B, Vol 820, Iss , Pp 136480- (2021)
The recent measurement of the muon anomalous magnetic moment aμ≡(g−2)μ/2 by the Fermilab Muon g−2 experiment sharpens an earlier discrepancy between theory and the BNL E821 experiment. We examine the predicted Δaμ≡aμ(exp)−aμ(th) in th
Externí odkaz:
https://doaj.org/article/daa458e155fc4786a65c80dc43c5536a
Publikováno v:
European Physical Journal C: Particles and Fields, Vol 79, Iss 11, Pp 1-16 (2019)
Abstract The value of the Higgs boson mass plus the lack of signal at LHC13 has led to a naturalness crisis for supersymmetric models. In contrast, rather general considerations of the string theory landscape imply a mild statistical draw towards lar
Externí odkaz:
https://doaj.org/article/ce0bcf98082b4776a9e719778a6ca9b5
Publikováno v:
Journal of High Energy Physics, Vol 2019, Iss 4, Pp 1-23 (2019)
Abstract The string theory landscape of vacua solutions provides physicists with some understanding as to the magnitude of the cosmological constant. Similar reasoning can be applied to the magnitude of the soft SUSY breaking terms in supersymmetric
Externí odkaz:
https://doaj.org/article/6e244d4db27b47daadba836577219e11
Publikováno v:
Journal of High Energy Physics, Vol 2018, Iss 3, Pp 1-32 (2018)
Abstract Predictions for the scale of SUSY breaking from the string landscape go back at least a decade to the work of Denef and Douglas on the statistics of flux vacua. The assumption that an assortment of SUSY breaking F and D terms are present in
Externí odkaz:
https://doaj.org/article/ddfa7c16c11f4be4be623562b73a5578
Autor:
Howard Baer, Vernon Barger, James S. Gainer, Peisi Huang, Michael Savoy, Hasan Serce, Xerxes Tata
Publikováno v:
Physics Letters B, Vol 774, Iss C, Pp 451-455 (2017)
Weak scale supersymmetry (SUSY) remains a compelling extension of the Standard Model because it stabilizes the quantum corrections to the Higgs and W,Z boson masses. In natural SUSY models these corrections are, by definition, never much larger than
Externí odkaz:
https://doaj.org/article/d97676c242f347e2881f9a55c170f1ce
Publikováno v:
Journal of High Energy Physics, Vol 2017, Iss 6, Pp 1-34 (2017)
Abstract The methodology of the heterotic mini-landscape attempts to zero in on phenomenologically viable corners of the string landscape where the effective low energy theory is the Minimal Supersymmetric Standard Model with localized grand unificat
Externí odkaz:
https://doaj.org/article/72a1e6afa625451cb8b3844561addd77
Publikováno v:
Physics Letters B, Vol 758, Iss C, Pp 113-117 (2016)
In supersymmetric models where the superpotential μ term is generated with μ≪msoft (e.g. from radiative Peccei–Quinn symmetry breaking or compactified string models with sequestration and stabilized moduli), and where the string landscape 1. fa
Externí odkaz:
https://doaj.org/article/a2a9942ba8834646bdc5c4d06cb5c6d5
Publikováno v:
Symmetry, Vol 7, Iss 2, Pp 788-814 (2015)
By insisting on naturalness in both the electroweak and quantum chromodynamics (QCD) sectors of the minimal supersymmetric standard model (MSSM), the portrait for dark matter production is seriously modified from the usual weakly interacting massive
Externí odkaz:
https://doaj.org/article/1df97a7c146a4f6ca7abce4c2ce67126
Publikováno v:
Physical Review Research, Vol 1, Iss 3, p 033022 (2019)
Right-handed neutrinos in supersymmetric models can act as the source of lepton flavor violation (LFV). We present experimental implications of lepton flavor-violating processes within a supersymmetric type-I seesaw framework in the three-extra-param
Externí odkaz:
https://doaj.org/article/fae96a21a50448b6b0e6c762d0ef7fa6
Publikováno v:
Physical Review
Perturbative supersymmetry breaking on the landscape of string vacua is expected to favor large soft terms as a power-law or log distribution, but tempered by an anthropic veto of inappropriate vacua or vacua leading to too large a value for the deri
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::532c7b31b52649cb3c3823e2ea188055
https://doi.org/10.1103/physrevd.104.115025
https://doi.org/10.1103/physrevd.104.115025