Magnetohydrodynamic stability of magnetars in the ultrastrong field regime I: The core
arXiv:2104.08563 · doi:10.1093/mnras/stab1538
Abstract
We study magnetohydrodynamic stability of neutron star core matter composed of neutrons, protons and leptons threaded by a magnetar-strength magnetic field -- G, where quantum electrodynamical effects and Landau quantization of fermions are important. Stability is determined using the Friedman--Schutz formalism for the canonical energy of fluid perturbations, which we calculate for a magnetizable fluid with . Using this and the Euler--Heisenberg--Fermi--Dirac Lagrangian for a strongly magnetized fluid of Landau-quantized charged fermions, we calculate the local stability criteria for a fluid slab as a stand-in for a segment of a neutron star core, accounting for magnetic and composition gradient buoyancy. The slab is threaded by a field orthogonal to the gravitational field, the Cartesian analogy to a toroidal field. We find that, for sufficiently strong fields G, the magnetized fluid is unstable to a magnetosonic-type instability with growth times of order s. The instability is triggered by sharp changes in the second-order field derivative of the Euler--Heisenberg--Fermi--Dirac Lagrangian which occur where additional Landau levels start being populated. These sharp changes are divergent at zero temperature, but are finite for nonzero temperature, so realistic neutron star core temperatures K K are used. We conjecture that this mechanism could promote the formation of magnetic domains as predicted by Blandford and Hernquist (1982) and Suh and Mathews (2010).
28 pages. Matches published version, including supplemental material
References in corpus (10)
- A NICER View of PSR J0030+0451: Millisecond Pulsar Parameter Estimation
- A bright millisecond-duration radio burst from a Galactic magnetar
- Fast radio bursts as synchrotron maser emission from decelerating relativistic blast waves
- Magnetars: Properties, Origin and Evolution
- A NICER view of PSR J0030+0451: evidence for a global-scale multipolar magnetic field
- Resonant tidal excitation of superfluid neutron stars in coalescing binaries
- Instability of Magnetic Equilibria in Barotropic Stars
- Composition temperature-dependent g-modes in superfluid neutron stars
- Lagrangian perturbation theory for rotating magnetic stars
- Analytical determination of the structure of the outer crust of a cold nonaccreted neutron star: extension to strongly quantizing magnetic fields
Cited by in corpus (6)
- Evidence for an abundant old population of Galactic ultra long period magnetars and implications for fast radio bursts
- Non-Axisymmetric Precession of Magnetars and Fast Radio Bursts
- Magnetar structure in non-linear electrodynamics with mixed poloidal-toroidal fields
- Magnetohydrodynamic stability of magnetars in the ultrastrong field regime II: The crust
- Topology of the Superconducting Heart of Neutron Stars: Effects of Microphysics and Gravitational-Wave Signatures
- Numerical simulation of electron magnetohydrodynamics with Landau-quantized electrons in magnetar crusts