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Large Lepton Number of the Universe and The Fate of Topological Defects
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We show that the monopole problem in Grand Unified Theories as well as the domain wall problem may be easily solved if the lepton number asymmetry in the Universe is large enough.
Forward citations
Cited by 2 Pith papers
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Loss of the scaling attractor in self-gravitating domain wall networks
Coupling domain wall networks to dynamical expansion shows the scaling attractor is lost, leading to wall-dominated frustration.
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Neutrinophilic $\mathbf{\Lambda}$CDM Extension for EMPRESS, DESI and Hubble Tension
A combined fit of EMPRESS, DESI BAO, and CMB data prefers a neutrino asymmetry xi_nu = 0.056 +/- 0.017 and extra radiation delta_Neff = 0.41 +/- 0.16 in a neutrinophilic LambdaCDM model.
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