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.
Energy Emission from a Neutron Star
2 Pith papers cite this work, alongside 541 external citations. Polarity classification is still indexing.
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Middle-aged PWNe exhibit diverse reverberation-phase evolution but converge to Sedov-like states; 2D instabilities increase apparent size by up to 50% without changing global dynamics, supporting 1D model robustness.
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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.