Cosmological phase transition: Difference between revisions

Revision as of 23:26, 25 January 2025

Revision as of 23:36, 25 January 2025

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Just as for the strong force, latticeLattice studies of the electroweak model have found the transition to be a smooth crossover, taking place at {{nobr| 159.5 ± 1.5 [[GeV]].}}<ref name=donofrio-rummukainen>

{{cite journal

|last1 = d'Onofrio |first1 = Michela

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|bibcode=2013JCAP...01..012C

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</ref> The [[electroweak baryogenesis]] model may explain the [[baryon asymmetry]] in the universe, the observation that the amount of matter vastly exceeds the amount of matter.<ref name=Manzudar-2019/>

</ref>

==Beyond the Standard Model==