activity
20182026
most citedTwo first-order phase transitions in hybrid compact stars: higher-order multiplet stars, reaction modes and intermediate conversion speeds

27 citations · 82 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.HE2026

Magnetar magnetothermal evolution with Landau-quantized electrons: enhanced Joule heating due to free electron diamagnetism and the magnetar heating problem

Peter B. Rau

Magnetars are systematically more luminous than other neutron stars. Previous studies suggest that supporting such high luminosities requires a heat source beyond standard Ohmic di…

astro-ph.HE2024

Numerical simulation of electron magnetohydrodynamics with Landau-quantized electrons in magnetar crusts

Peter B. Rau, Ira Wasserman

In magnetar crusts, magnetic fields are sufficiently strong to confine electrons into a small to moderate number of quantized Landau levels. This can have a dramatic effect on the…

astro-ph.HE2024★ 5 cited

Josephson currents in neutron stars

Armen Sedrakian, Peter B. Rau

We demonstrate that the interface between -wave and -wave paired superfluids in neutron stars induces a neutron supercurrent, a charge-neutral analog of the Josephson junctio…

astro-ph.HE2022★ 27 cited

Two first-order phase transitions in hybrid compact stars: higher-order multiplet stars, reaction modes and intermediate conversion speeds

Peter B. Rau, Armen Sedrakian

We study compact stars with hybrid equations of state consisting of a nuclear outer region and two nested quark phases, each separated from the lower density phase by a strong firs…

astro-ph.HE2022★ 3 cited

Magnetohydrodynamic stability of magnetars in the ultrastrong field regime II: The crust

Peter B. Rau, Ira Wasserman

We study the stability of Hall MHD with strong magnetic fields in which Landau quantization of electrons is important. We find that the strong-field Hall modes can be destabilized…

gr-qc2021★ 3 cited

Unstable modes of hypermassive compact stars driven by viscosity and gravitational radiation

Peter B. Rau, Armen Sedrakian

We study the oscillations modes of differential rotating remnants of binary neutron star inspirals by modeling them as incompressible Riemann ellipsoids parametrized by the ratio $…

astro-ph.HE2021★ 6 cited

Magnetohydrodynamic stability of magnetars in the ultrastrong field regime I: The core

Peter B. Rau, Ira Wasserman

We study magnetohydrodynamic stability of neutron star core matter composed of neutrons, protons and leptons threaded by a magnetar-strength magnetic field -- G,…

gr-qc2020★ 2 cited

Oscillations of hypermassive compact stars with gravitational radiation and viscosity

Peter B. Rau, Armen Sedrakian

Binary neutron star mergers, such as the multimessenger GW170817 event, may produce hypermassive compact objects which are supported against collapse by the internal circulation of…

astro-ph.HE2020★ 25 cited

Relativistic finite temperature multifluid hydrodynamics in a neutron star from a variational principle

Peter B. Rau, Ira Wasserman

We develop a relativistic multifluid dynamics appropriate for describing neutron star cores at finite temperatures based on Carter's convective variational procedure. The model inc…

astro-ph.HE2018★ 11 cited

Compressional modes in two-superfluid neutron stars with leptonic buoyancy

P. B. Rau, I. Wasserman

We investigate the compressional modes of cold neutron stars with cores consisting of superfluid neutrons, superconducting protons and normal fluid electrons and muons, and crusts…