Handing-Off the Outcome of Binary Neutron Star Mergers for Accurate and Long-Term Post-Merger Simulations
ORAL
Abstract
We present the HandOff, a set of computational tools that enables the transition of a general relativistic magnetohydrodynamic (GRMHD) simulation between two numerical codes, IllinoisGRMHD and Harm3d. While the first code evolves the equations of full dynamical General Relativity, making use of a Cartesian grid with adaptive-mesh refinement, the second code specializes in modeling black hole accretion disks in static spacetimes over long timescales, making use of general coordinate systems with spherical topology. The HandOff is particularly interesting for transitioning the outcomes of binary neutron star mergers (BNS) to a grid better suited to the geometry and requirements of the post-merger. 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.
*NASA TCAN grant No. 80NSSC18K1488
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Publication:Recently submitted to PRD and arXiv.
Presenters
Federico G Lopez Armengol
Rochester Institute of Technology
Authors
Federico G Lopez Armengol
Rochester Institute of Technology
Zachariah B Etienne
University of Idaho
Scott C Noble
NASA Goddard Space Flight Center
Bernard J Kelly
University of Maryland, Baltimore County
Leonardo Werneck
University of Idaho
Brendan Drachler
Rochester Institute of Technology
Manuela Campanelli
Rochester Institute of Technology
Federico Cipolletta
Rochester Institute of Technology
Yosef Zlochower
Rochester Institute of Technology
Ariadna Berthier
Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA), 1800 Sherman Ave., Evanston, IL 60201, USA
UCSC
Lorenzo Enoggi
Center for Computational Relativity and Gravitation,Rochester Institute of Technology, Rochester, New York 14623, USA