Microphysical Aspects of Binary Neutron Star Mergers

Michail Chabanov, Alejandro Cruz-Osorio, Christian Ecker (), Claudio Meringolo, Carlo Musolino, Luciano Rezzolla, Samuel Tootle and Konrad Topolski
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Michail Chabanov: Goethe Universität, Institut für Theoretische Physik
Alejandro Cruz-Osorio: Goethe Universität, Institut für Theoretische Physik
Christian Ecker: Goethe Universität, Institut für Theoretische Physik
Claudio Meringolo: Universit‘a della Calabria, Dipartimento di Fisica
Carlo Musolino: Goethe Universität, Institut für Theoretische Physik
Luciano Rezzolla: Goethe Universität, Institut für Theoretische Physik
Samuel Tootle: Goethe Universität, Institut für Theoretische Physik
Konrad Topolski: Goethe Universität, Institut für Theoretische Physik

A chapter in High Performance Computing in Science and Engineering '22, 2024, pp 19-34 from Springer

Abstract: Abstract Neutron stars and their mergers challenge our fundamental understanding of dense matter and strong gravity. We present three projects that cover different aspects of these systems, namely the formation of quark matter in neutron star mergers, the determination of the limiting mass to prompt black hole formation and the dynamics of charged particles that occur in magnetised plasmas such as formed around black holes in these events. We also give a brief introduction to the numerical techniques used to model these scenarios and summarise their performance on the HAWK supercomputer system.

Date: 2024
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DOI: 10.1007/978-3-031-46870-4_2

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