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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Strong magnetic fields in compact stars induce Landau quantization and magnetic-moment couplings that change the equation of state and allow additional degrees of freedom such as hyperons, Delta resonances, and quark matter.
A review of parity-doublet models in effective field theory that accommodate a chirally invariant mass m0 to describe baryons across vacuum, nuclear, and astrophysical densities.
citing papers explorer
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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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Dense Matter and Compact Stars in Strong Magnetic Fields
Strong magnetic fields in compact stars induce Landau quantization and magnetic-moment couplings that change the equation of state and allow additional degrees of freedom such as hyperons, Delta resonances, and quark matter.
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Chiral, parity-doublet, effective-Lagrangian mean-field theories for nuclear and astrophysical phenomenology
A review of parity-doublet models in effective field theory that accommodate a chirally invariant mass m0 to describe baryons across vacuum, nuclear, and astrophysical densities.