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Physical Review D

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Phys. Rev. D (2)

Articles Citing

Numerical simulations of black hole-neutron star mergers with equal and near-equal mass ratios

Ivan Markin ^1,*, Mattia Bulla ^2,3,4, and Tim Dietrich ^1,5

¹University of Potsdam, Institute of Physics and Astronomy, Haus 28, Karl-Liebknecht-Strasse 24/25, 14476, Potsdam, Germany
²Department of Physics and Earth Science, University of Ferrara, via Saragat 1, I-44122 Ferrara, Italy
³INFN, Sezione di Ferrara, via Saragat 1, I-44122 Ferrara, Italy
⁴INAF, Osservatorio Astronomico d’Abruzzo, via Mentore Maggini snc, 64100 Teramo, Italy
⁵Max Planck Institute for Gravitational Physics (Albert Einstein Institute), Am Mühlenberg 1, Potsdam 14476, Germany

^*Contact author: ivan.markin@uni-potsdam.de

Fast gravitational waveform models for quasicircular coalescences of neutron star-black hole binaries

Felip A. Ramis Vidal, Adrian Abac, Marta Colleoni, Tim Dietrich, Pierre Mourier, Alejandra Gonzalez, Ivan Markin, and Anna Puecher

Phys. Rev. D 114 064044 (2026)

Black hole–boson star binaries: Gravitational wave signals and tidal disruption

Gareth Arturo Marks, Seppe J. Staelens, and Ulrich Sperhake

Phys. Rev. D 114 084016 (2026)

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ISSN 2470-0029 (online), 2470-0010 (print).

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