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Particle Physics and Cosmology
Phase transitions
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baryogenesis during electroweak phase transition ?
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Sakharov’s conditions for baryogenesis during electroweak phase transition
baryon number violation interactions ☺ charge conjugation violating interactions ☺ CP – violating interactions ☺ non – equilibrium process ☺
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baryogenesis during electroweak phase transition ?
strongly first order electroweak phase transition can generate baryon asymmetry if CP violation is sufficiently strong no efficient baryogenesis for weak first order phase transition, second order phase transition or crossover presumably too little CP violation in SM ( not definitely settled )
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electroweak phase transition
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order of phase transition
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temperature dependent effective potential
high temperature expansion
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next to leading order in high temperature expansion
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first order cosmological phase transitions
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chaos in the Universe
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relics from cosmological first order phase transitions ?
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electroweak crossover
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critical mass of the Higgs scalar for the onset of crossover
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electroweak “phase transition “ in standard model is crossover !
perhaps strong first order transition in supersymmetric extensions of standard model
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standard model of particle physics and cosmology
no candidate for dark matter no baryon asymmetry no massive neutrinos
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standard model of particle physics and cosmology
prediction : present Universe consists of photons and massless neutrinos
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