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Jetlike structures in low-mass binary neutron star merger remnants
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Crustal Magnetic Fields Do Not Lead to Large Magnetic-field Amplifications in Binary Neutron Star Mergers
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Collapse of Rotating Massive Stars Leading to Black Hole Formation and Energetic Supernovae
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Constraints on the merging binary neutron star mass distribution and equation of state based on the incidence of jets in the population
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Local energy density functional for superfluid Fermi gases from effective field theory
Turbulent magnetic-field amplification in the first 10 milliseconds after a binary neutron star merger: Comparing high-resolution and large-eddy simulations
Philipp Mösta, David Radice, Roland Haas, Erik Schnetter and Sebastiano Bernuzzi The Astrophysical Journal Letters 901(2) L37 (2020) https://doi.org/10.3847/2041-8213/abb6ef
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Constraints on gamma-ray burst inner engines in a Blandford–Znajek framework
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When Did the Remnant of GW170817 Collapse to a Black Hole?
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Resistive and Multi-fluid RMHD on Graphics Processing Units
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Electrical resistivity and Hall effect in binary neutron star mergers
Broadband Radio Polarimetry of Fornax A. I. Depolarized Patches Generated by Advected Thermal Material from NGC 1316
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Magnetorotational instability in neutron star mergers: impact of neutrinos
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Binary neutron star mergers: a review of Einstein’s richest laboratory
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Minimally implicit Runge-Kutta methods for Resistive Relativistic MHD
Dynamical mass ejection from binary neutron star mergers
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PRODUCING MAGNETAR MAGNETIC FIELDS IN THE MERGER OF BINARY NEUTRON STARS
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