The routine model with bulk viscosity best reproduces the Crab pulsar's magnetic inclination angle, spin period, and derivative, while electromagnetic torque and accretion suppress inclination growth and most other effects are negligible.
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The chapter summarizes established nuclear many-body theory formalisms for calculating low-energy neutrino cross sections in nuclear matter and their implications for astrophysics.
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Evolution of Crab Pulsar: Magnetic Inclination Angle and Spin
The routine model with bulk viscosity best reproduces the Crab pulsar's magnetic inclination angle, spin period, and derivative, while electromagnetic torque and accretion suppress inclination growth and most other effects are negligible.
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Neutrino Cross Sections: Low Energy
The chapter summarizes established nuclear many-body theory formalisms for calculating low-energy neutrino cross sections in nuclear matter and their implications for astrophysics.