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STUDIES OF POST-MERGER BLACK HOLES, NEUTRON STARS AND DISKS: STABILITY AND ELECTROMAGNETIC SIGNALS
Dissertation

STUDIES OF POST-MERGER BLACK HOLES, NEUTRON STARS AND DISKS: STABILITY AND ELECTROMAGNETIC SIGNALS

Nishad Muhammed
Doctor of Philosophy (PhD), Washington State University
2026
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Abstract

Binary neutron star (BNS) mergers undergoing prompt collapse and black hole neutron star (BHNS) mergers in which the neutron star is tidally disrupted before the plunge produce black hole-accretion disk systems. On the other hand, BNS mergers that undergo delayed collapse produce hypermassive neutron stars (HMNS) as an intermediate remnant before collapsing into black holes. The post-merger systems are important for gravitational wave emissions, electromagnetic counterparts and heavy element formation. We study the stability of these post-merger HMNS systems. We validate the turning point criterion for differentially rotating realistic post-merger-like stars. We find that the conformal flatness approximation for highly differentially rotating toroidal star simulations is not a reliable approximation. We also analyze the energy deposition from neutrino pair annihilation for both general relativity (GR) and beyond GR theories for post-merger black holes. We find the energies can be sufficient for certain low-energy short gamma-ray bursts. Finally, we investigate the advantage and importance of different neutrino treatments in the post-merger phase. We find that an energy-dependent two moment closure scheme is important to consider for analysis of r-process yields, ejecta composition and kilonovae signals. We also show that inelastic neutrino-electron scattering in simulations of hypermassive neutron stars is important for simulations of hypermassive neutron stars, particularly for disk properties and neutrino luminosities.

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