Handing off the outcome of binary neutron star mergers for accurate and long-term post-merger simulations

TL;DR

This paper introduces the Handoff tools that transfer data from neutron star merger simulations to specialized black hole accretion codes, enabling accurate long-term post-merger evolution in more suitable coordinate systems.

Contribution

The paper presents the Handoff methodology for seamless data transfer between GRMHD codes, improving long-term post-merger simulation accuracy and efficiency.

Findings

Handoff enables smooth transition of GRMHD data between codes.

Long-term evolution of BNS mergers is feasible with the new approach.

Future integration of advanced physics into BNS simulations planned.

Abstract

We perform binary neutron star (BNS) merger simulations in full dynamical general relativity with IllinoisGRMHD, on a Cartesian grid with adaptive-mesh refinement. After the remnant black hole has become nearly stationary, the evolution of the surrounding accretion disk on Cartesian grids over long timescales (1s) is suboptimal, as Cartesian coordinates over-resolve the angular coordinates at large distances, and the accreting plasma flows obliquely across coordinate lines dissipating angular momentum artificially from the disk. To address this, we present the Handoff, a set of computational tools that enables the transfer of general relativistic magnetohydrodynamic (GRMHD) and spacetime data from IllinoisGRMHD to HARM3D, a GRMHD code that specializes in modeling black hole accretion disks in static spacetimes over long timescales, making use of general coordinate systems with spherical topology. We demonstrate that the Handoff allows for a smooth and reliable transition of GRMHD fields and spacetime data, enabling us to efficiently and reliably evolve BNS dynamics well beyond merger. We also discuss future plans, which involve incorporating advanced equations of state and neutrino physics into BNS simulations using the \handoff approach.