Baryon washout, electroweak phase transition, and perturbation theory
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Publication:467323
DOI10.1007/JHEP07(2011)029zbMath1298.81491arXiv1101.4665OpenAlexW2038874801MaRDI QIDQ467323
Michael J. Ramsey-Musolf, Hiren H. Patel
Publication date: 3 November 2014
Published in: Journal of High Energy Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1101.4665
Unified quantum theories (81V22) Nuclear physics (81V35) Perturbative methods of renormalization applied to problems in quantum field theory (81T15) Finite-dimensional groups and algebras motivated by physics and their representations (81R05) Thermal quantum field theory (81T28)
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Cites Work
- Unnamed Item
- MSSM baryogenesis and electric dipole moments: An update on the phenomenology
- The sphaleron rate in SU(\(N\)) gauge theory
- The baryogenesis window in the MSSM
- Electroweak phase transitions in the secluded U(1)'-extended MSSM
- Brownian motion in a field of force and the diffusion model of chemical reactions
- The end point of the first-order phase transition of the SU(2) gauge-Higgs model on a four-dimensional isotropic lattice
- Where does the hot electroweak phase transition end?
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