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We perform general relativistic, magnetohydrodynamic (GRMHD) simulations of binary neutron stars in quasi-circular orbit that merge and undergo delayed or prompt collapse to a black hole (BH).
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2021
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A. Perego, F. K. Thielemann, and G. Cescutti, “r-Process Nucleosynthesis from Compact Binary Mergers,” in Handbook of Gravitational Wave Astronomy. Edited by C. Bambi (2021) p. 1
2021
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2021
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