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General-relativistic radiation magnetohydrodynamics simulations of binary neutron star mergers: The influence of spin on the multimessenger picture

Anna Neuweiler ¹, Henrique Gieg ¹, Henrik Rose ¹, Hauke Koehn ¹, Ivan Markin ¹, Federico Schianchi^2,1, Liam Brodie ³, Alexander Haber^3,4, Vsevolod Nedora ^1,5 et al.

Mattia Bulla ^6,7,8 and Tim Dietrich^1,5

¹Institut für Physik und Astronomie, Universität Potsdam, Haus 28, Karl-Liebknecht-Strasse 24/25, 14476, Potsdam, Germany
²Departament de Física & IAC3, Universitat de les Illes Balears, Palma de Mallorca, Baleares E-07122, Spain
³Department of Physics, Washington University in St. Louis, St. Louis, Missouri 63130, USA
⁴Mathematical Sciences and STAG Research Centre, University of Southampton, Southampton SO17 1BJ, United Kingdom
⁵Max Planck Institute for Gravitational Physics (Albert Einstein Institute), Am Mühlenberg 1, Potsdam 14476, Germany
⁶Department of Physics and Earth Science, University of Ferrara, via Saragat 1, I-44122 Ferrara, Italy
⁷INFN, Sezione di Ferrara, via Saragat 1, I-44122 Ferrara, Italy
⁸INAF, Osservatorio Astronomico d’Abruzzo, via Mentore Maggini snc, 64100 Teramo, Italy

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Articles Citing

General-relativistic radiation magnetohydrodynamics simulations of binary neutron star mergers: The influence of spin on the multimessenger picture

Thermalization of neutrinos in a neutron star merger simulation

Consistent treatment of muons in binary neutron star mergers

Binary neutron star merger simulations with neutrino transport using gr-athena++

Magnetic eruption and nucleosynthesis in GRνMHD simulations of spinning neutron star mergers

Black hole-neutron star binaries with high spins and large mass asymmetries. III. Properties of the ejected material and its electromagnetic signatures

General-relativistic radiation magnetohydrodynamics simulations of binary neutron star mergers: The influence of spin on the multimessenger picture

Thermal and magnetic effects on bulk viscosity in binary neutron star mergers

Nucleosynthesis in the fast ejecta of a neutron star merger

56Ni Production in Long-lived Binary Neutron Star Merger Remnants

Spinning Down Neutron-star Merger Remnants with the Tayler–Spruit Dynamo: Global Simulations Reveal the Formation of Massive Disks and Neutron-rich Ejecta

The Initial Spin Matters: The Impact of Rapid Rotation on Magnetic-field Amplification at Merger

Do Accretion Disks Get Bent Out of Shape? Investigating the Origin of Rapid Fluctuations in the Tails of Long Thermonuclear X-Ray Bursts

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