Transport Properties of the MRI in Differentially Rotating Neutron Stars
Harshraj Bandyopadhyay, Peter Hammond, David Radice
astro-ph.HE, gr-qc
Submitted: 2026-07-27
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
- Origin of the heavy elements in binary neutron-star mergers from a gravitational wave event
- Kilonovae
- Simulation of merging binary neutron stars in full general relativity: $\Gamma=2$ case
- On the Maximum Mass of Differentially Rotating Neutron Stars
- Theory of Core-Collapse Supernovae
- Evolution of magnetized, differentially rotating neutron stars: Simulations in full general relativity
- Efficient magnetic-field amplification due to the Kelvin-Helmholtz instability in binary neutron star mergers
- Global simulations of strongly magnetized remnant massive neutron stars formed in binary neutron star mergers
- A large-scale magnetic field produced by a solar-like dynamo in binary neutron star mergers
- A magnetar formation in binary neutron star merger
- Flares, jets and quasi-periodic outbursts from neutron star merger remnants
- On the impact of neutrinos on the launching of relativistic jets from "magnetars" produced in neutron-star mergers
- Enhanced Angular Momentum Transport in Accretion Disks
- The Magnetorotational Instability in Core Collapse Supernova Explosions
- Semi-global simulations of the magneto-rotational instability in core collapse supernovae
- A global model of the magnetorotational instability in protoneutron stars
- Magnetar formation through a convective dynamo in protoneutron stars
- Viscosity and Rotation in Core-Collapse Supernovae
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