The Black Hole-Neutron Star Binary Merger in Full General Relativity Dependence on Neutron Star Equations of State /

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, SimulA...

Πλήρης περιγραφή

Λεπτομέρειες βιβλιογραφικής εγγραφής
Κύριος συγγραφέας: Kyutoku, Koutarou (Συγγραφέας)
Συγγραφή απο Οργανισμό/Αρχή: SpringerLink (Online service)
Μορφή: Ηλεκτρονική πηγή Ηλ. βιβλίο
Γλώσσα:English
Έκδοση: Tokyo : Springer Japan : Imprint: Springer, 2013.
Σειρά:Springer Theses, Recognizing Outstanding Ph.D. Research,
Θέματα:
Διαθέσιμο Online:Full Text via HEAL-Link
LEADER 03333nam a22005295i 4500
001 978-4-431-54201-8
003 DE-He213
005 20151030061333.0
007 cr nn 008mamaa
008 130125s2013 ja | s |||| 0|eng d
020 |a 9784431542018  |9 978-4-431-54201-8 
024 7 |a 10.1007/978-4-431-54201-8  |2 doi 
040 |d GrThAP 
050 4 |a QB1-991 
050 4 |a QB460-466 
050 4 |a QB980-991 
072 7 |a PGC  |2 bicssc 
072 7 |a SCI004000  |2 bisacsh 
072 7 |a SCI005000  |2 bisacsh 
082 0 4 |a 520  |2 23 
100 1 |a Kyutoku, Koutarou.  |e author. 
245 1 4 |a The Black Hole-Neutron Star Binary Merger in Full General Relativity  |h [electronic resource] :  |b Dependence on Neutron Star Equations of State /  |c by Koutarou Kyutoku. 
264 1 |a Tokyo :  |b Springer Japan :  |b Imprint: Springer,  |c 2013. 
300 |a XIII, 178 p.  |b online resource. 
336 |a text  |b txt  |2 rdacontent 
337 |a computer  |b c  |2 rdamedia 
338 |a online resource  |b cr  |2 rdacarrier 
347 |a text file  |b PDF  |2 rda 
490 1 |a Springer Theses, Recognizing Outstanding Ph.D. Research,  |x 2190-5053 
505 0 |a Equations 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. 
520 |a 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 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. 
650 0 |a Physics. 
650 0 |a Mathematical physics. 
650 0 |a Astronomy. 
650 0 |a Astrophysics. 
650 0 |a Cosmology. 
650 1 4 |a Physics. 
650 2 4 |a Astronomy, Astrophysics and Cosmology. 
650 2 4 |a Mathematical Applications in the Physical Sciences. 
650 2 4 |a Numerical and Computational Physics. 
710 2 |a SpringerLink (Online service) 
773 0 |t Springer eBooks 
776 0 8 |i Printed edition:  |z 9784431542001 
830 0 |a Springer Theses, Recognizing Outstanding Ph.D. Research,  |x 2190-5053 
856 4 0 |u http://dx.doi.org/10.1007/978-4-431-54201-8  |z Full Text via HEAL-Link 
912 |a ZDB-2-PHA 
950 |a Physics and Astronomy (Springer-11651)