Cosmological phase transitions and their properties in the NMSSM
From MaRDI portal
Publication:1754833
DOI10.1007/JHEP01(2015)144zbMath1388.83928arXiv1407.4134MaRDI QIDQ1754833
Jonathan Kozaczuk, Stefano Profumo, Laurel Stephenson Haskins, Carroll L. Wainwright
Publication date: 31 May 2018
Published in: Journal of High Energy Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1407.4134
supersymmetric standard modelcosmology of theories beyond the SMbeyond standard modelthermal field theory
Related Items (7)
Gravitational wave signatures from an extended inert doublet dark matter model ⋮ Generating non-topological solitons via thermal corrections: Higgs balls ⋮ Detection of early-universe gravitational-wave signatures and fundamental physics ⋮ Combining thermal resummation and gauge invariance for electroweak phase transition ⋮ Electroweak baryogenesis in the \( {\mathbb{Z}}_3 \)-invariant NMSSM ⋮ Cosmological backgrounds of gravitational waves ⋮ Gravitational waves from first-order phase transitions: towards model separation by bubble nucleation rate
Uses Software
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