1994
DOI: 10.1103/physrevd.49.3881
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Hypercharge and the cosmological baryon asymmetry

Abstract: Stringent bounds on baryon and lepton number violating interactions have been derived from the requirement that such interactions, together with electroweak instantons, do not destroy a cosmological baryon asymmetry produced at an extremely high temperature in the big bang. While these bounds apply in specific models, we find that they are generically evaded. In particular, the only requirement for a theory to avoid these bounds is that it contain charged particles which, during a certain cosmological epoch, c… Show more

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Cited by 23 publications
(22 citation statements)
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“…Finally, we discuss the flavor structure of several nucleon decay modes. We observe surprising enhancement of the decays in charged lepton modes [28), as opposed to more conventional SU(5) considerations.…”
Section: Introductionmentioning
confidence: 81%
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“…Finally, we discuss the flavor structure of several nucleon decay modes. We observe surprising enhancement of the decays in charged lepton modes [28), as opposed to more conventional SU(5) considerations.…”
Section: Introductionmentioning
confidence: 81%
“…Several solutions exist, such as the popular weak scale baryogenesis [22] in which there is no need for a primordial baryon asymmetry. In section 3, a different possibility is explained [23]. It is shown that the primordial baryon symmetry, in the presence of flavor changing interactions, can be saved by simply adding a new charged partide with its own asymmetry.…”
Section: Introductionmentioning
confidence: 99%
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“…-✓ --COBRA 116 Cd (and 130 Te) 5 We note here that if lepton number is violated not by two units but by three or more, there will be no neutrinoless double beta decay, but rather processes with L 3, 4, D = ¼ One explicit example is 'neutrinoless quadruple beta decay' presented in [22].…”
Section: Camentioning
confidence: 88%
“…But detailed calculations [11] belied this hope by revealing that e R enter chemical equilibrium, at T < ∼ 10T eV , well before the sphalerons have dropped out of thermal equilibrium. Antaramian et al [12] also discuss survival of baryon asymmetry but without any models.…”
Section: Footnotesmentioning
confidence: 99%