Time-Dependent Superfluid Band Theory for the Inner Crust of Neutron Stars: Current Status and Future Challenges
This research uses time-dependent band theory to study neutron properties in neutron star inner crusts using periodic potentials. Initial findings showed increased effective mass due to entrainment, but recent calculations suggest a reduction by 30-40%. Extending the theory to superfluid systems reveals anti-entrainment effects caused by counter flows. Future work plans include finite temperature and magnetic field extensions.