Extends thermal field theory to fermions with angular momentum and shows neutrino production in rotating neutron stars grows indefinitely with angular velocity near the inverse system size.
Field theory at finite tempera- ture and phase transitions
2 Pith papers cite this work. Polarity classification is still indexing.
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hep-ph 2representative citing papers
Supercooled phase transitions from radiative symmetry breaking can be described, at leading and next-to-leading order, by formulas depending only on three or four parameters (χ0, β̄, g, and g̃ at NLO).
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Fermion Thermal Field Theory for a Rotating Plasma (with Applications to Neutron Stars)
Extends thermal field theory to fermions with angular momentum and shows neutrino production in rotating neutron stars grows indefinitely with angular velocity near the inverse system size.
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Supercooled Phase Transitions with Radiative Symmetry Breaking
Supercooled phase transitions from radiative symmetry breaking can be described, at leading and next-to-leading order, by formulas depending only on three or four parameters (χ0, β̄, g, and g̃ at NLO).