The Black Hole-Neutron Star Binary Merger in Full General Relativity III durch Hessen bis Kastel geführt
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The Black Hole-Neutron Star Binary Merger in Full General Relativity III durch Hessen bis Kastel geführtThis thesis presents a systematic study of the orbital evolution, gravitational wave radiation, and merger remnant of the black holeneutron star binary merger in full general relativity for the first time. Numerical relativity simulations are performed using an adaptive mesh refinement code, SimulAtor for Compact objects in Relativistic Astrophysics (SACRA), which adopts a wide variety of zero temperature equations of state for the neutron star
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