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Magnetic field configurations in binary neutron star mergers. II. Inspiral, merger and ejecta

William Cook ¹, Eduardo M. Gutiérrez ^2,3, Sebastiano Bernuzzi ¹, David Radice ^2,3,4, Boris Daszuta ¹, Jacob Fields ^2,3, Peter Hammond ^2,3,5, Harshraj Bandyopadhyay ³, and Maximilian Jacobi ¹

¹Theoretisch-Physikalisches Institut, Friedrich-Schiller-Universität Jena, 07743, Jena, Germany
²Institute for Gravitation and the Cosmos, The Pennsylvania State University, University Park, Pennsylvania, 16802, USA
³Department of Physics, The Pennsylvania State University, University Park, Pennsylvania, 16802, USA
⁴Department of Astronomy and Astrophysics, The Pennsylvania State University, University Park, Pennsylvania, 16802, USA
⁵Department of Physics and Astronomy, University of New Hampshire, Durham, New Hampshire 03824, USA

Magnetic field configurations in binary neutron star mergers. I. Postmerger remnant and disk

Eduardo M. Gutiérrez, William Cook, David Radice, Sebastiano Bernuzzi, Jacob Fields, Peter Hammond, Boris Daszuta, Harshraj Bandyopadhyay, and Maximilian Jacobi

Phys. Rev. D 114 063049 (2026)

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Physical Review D

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Magnetic field configurations in binary neutron star mergers. II. Inspiral, merger and ejecta

Magnetic field configurations in binary neutron star mergers. I. Postmerger remnant and disk

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