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Microphysical Aspects of Binary Neutron Star Mergers

In: High Performance Computing in Science and Engineering '22

Author

Listed:
  • 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
    Frankfurt Institute for Advanced Studies
    Trinity College, School of Mathematics)

  • Samuel Tootle

    (Goethe Universität, Institut für Theoretische Physik)

  • Konrad Topolski

    (Goethe Universität, Institut für Theoretische Physik)

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.

Suggested Citation

  • Michail Chabanov & Alejandro Cruz-Osorio & Christian Ecker & Claudio Meringolo & Carlo Musolino & Luciano Rezzolla & Samuel Tootle & Konrad Topolski, 2024. "Microphysical Aspects of Binary Neutron Star Mergers," Springer Books, in: Wolfgang E. Nagel & Dietmar H. Kröner & Michael M. Resch (ed.), High Performance Computing in Science and Engineering '22, pages 19-34, Springer.
    • Handle: RePEc:spr:sprchp:978-3-031-46870-4_2
    DOI: 10.1007/978-3-031-46870-4_2
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