Bibliografi : hlm. 367-377 No Inv.: 141166/PSM/Perp/14/1c
Perpustakaan hanya memiliki jil.23
No Inv.: 108450/PSM/Perp/06/1c
No Inv.: 333-334/Pb/Perp/92/2c~117187/P/Perp/09/1c
No Inv.: 3495/P/Perp/97/1c
This thesis presents a systematic study of the orbital evolution, gravitational wave radiation, and merger remnant of the black hole–neutron 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 ze…