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The B−L Phase Transition - Implications for Cosmology and Neutrinos (Paperback, Softcover reprint of the original 1st ed. 2014)
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The B−L Phase Transition - Implications for Cosmology and Neutrinos (Paperback, Softcover reprint of the original 1st ed. 2014)
Series: Springer Theses
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Several of the very foundations of the cosmological standard model
— the baryon asymmetry of the universe, dark matter, and the
origin of the hot big bang itself — still call for an explanation
from the perspective of fundamental physics. This
work advocates one intriguing possibility for a consistent
cosmology that fills in the theoretical gaps while being fully in
accordance with the observational data. At very high energies, the
universe might have been in a false vacuum state that preserved
B-L, the difference between the baryon number B and the lepton
number L as a local symmetry. In this state, the universe
experienced a stage of hybrid inflation that only ended when the
false vacuum became unstable and decayed, in the course of a
waterfall transition, into a phase with spontaneously broken B-L
symmetry. This B-L Phase Transition was accompanied by tachyonic
preheating that transferred almost the entire energy of the false
vacuum into a gas of B-L Higgs bosons, which in turn decayed into
heavy Majorana neutrinos. Eventually, these neutrinos decayed into
massless radiation, thereby producing the entropy of the hot big
bang, generating the baryon asymmetry of the universe via the
leptogenesis mechanism and setting the stage for the production of
dark matter. Next to a variety of conceptual novelties and
phenomenological predictions, the main achievement of the thesis is
hence the fascinating notion that the leading role in the first act
of our universe might have actually been played by neutrinos.
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