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024 7 $a10.1007/978-4-431-54201-8
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100   $a20130131d2013      uy         0
101 0 $aeng
135   $aur|n|---|||||
181   $ctxt
182   $cc
183   $acr
200 14$aThe black hole-neutron star binary merger in full general relativity /$fKoutarou Kyutoku
205   $a1st ed. 2013.
210   $aTokyo ;$aLondon $cSpringer$d2013
215   $a1 online resource (185 p.)
225  0$aSpringer theses
300   $aDescription based upon print version of record.
311   $a4-431-54733-9 
311   $a4-431-54200-0 
320   $aIncludes bibliographical references.
327   $aEquations of State of Neutron Star Matter -- Computing Initial Conditions -- Methods of Simulations -- Diagnostics for Numerical Simulations -- The Merger of Nonspinning Black Hole-Neutron Star Binaries -- The Merger of Spinning Black Hole-Neutron Star Binaries.
330   $aThis thesis presents a systematic study of the orbital evolution, gravitational wave radiation, and merger remnant of the black hole?neutron star binary merger in full general relativity for the first time. Numerical-relativity simulations are performed using an adaptive mesh refinement code, SimulAtor for Compact objects in Relativistic Astrophysics (SACRA), which adopts a wide variety of zero-temperature equations of state for the neutron star matter.   Gravitational waves provide us with quantitative information on the neutron star compactness and equation of state via the cutoff frequency in the spectra, if tidal disruption of the neutron star occurs before the binary merges. The cutoff frequency will be observed by next-generation laser interferometric ground-based gravitational wave detectors, such as Advanced LIGO, Advanced VIRGO, and KAGRA.   The author has also determined that the mass of remnant disks are sufficient for the remnant black hole accretion disk to become a progenitor of short-hard gamma ray bursts accompanied by tidal disruptions and suggests that overspinning black holes may not be formed after the merger of even an extremely spinning black hole and an irrotational neutron star.
410  0$aSpringer Theses, Recognizing Outstanding Ph.D. Research,$x2190-5053
606   $aGeneral relativity (Physics)
606   $aBlack holes (Astronomy)
606   $aNeutron stars
606   $aGravitational waves
615  0$aGeneral relativity (Physics)
615  0$aBlack holes (Astronomy)
615  0$aNeutron stars.
615  0$aGravitational waves.
676   $a530.11
700   $aKyutoku$b Koutarou$0862395
801  0$bMiAaPQ
801  1$bMiAaPQ
801  2$bMiAaPQ
906   $aBOOK
912   $a9910437975303321
996   $aThe Black Hole-Neutron Star Binary Merger in Full General Relativity$91924983
997   $aUNINA