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The Resource The Black Hole-Neutron Star Binary Merger in Full General Relativity : Dependence on Neutron Star Equations of State, by Koutarou Kyutoku, (electronic resource)

The Black Hole-Neutron Star Binary Merger in Full General Relativity : Dependence on Neutron Star Equations of State, by Koutarou Kyutoku, (electronic resource)

Label
The Black Hole-Neutron Star Binary Merger in Full General Relativity : Dependence on Neutron Star Equations of State
Title
The Black Hole-Neutron Star Binary Merger in Full General Relativity
Title remainder
Dependence on Neutron Star Equations of State
Statement of responsibility
by Koutarou Kyutoku
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Subject
Language
eng
Summary
This thesis presents a systematic study of the orbital evolution, gravitational wave radiation, and merger remnant of the black hole{u2013}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
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0
Literary form
non fiction
Series statement
Springer Theses, Recognizing Outstanding Ph.D. Research,
The Black Hole-Neutron Star Binary Merger in Full General Relativity : Dependence on Neutron Star Equations of State, by Koutarou Kyutoku, (electronic resource)
Label
The Black Hole-Neutron Star Binary Merger in Full General Relativity : Dependence on Neutron Star Equations of State, by Koutarou Kyutoku, (electronic resource)
Link
http://libproxy.rpi.edu/login?url=http://dx.doi.org/10.1007/978-4-431-54201-8
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Antecedent source
mixed
Carrier category
online resource
Carrier category code
cr
Carrier MARC source
rdacarrier
Color
not applicable
Content category
text
Content type code
txt
Content type MARC source
rdacontent
Contents
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
http://library.link/vocab/cover_art
https://contentcafe2.btol.com/ContentCafe/Jacket.aspx?Return=1&Type=S&Value=9784431542018&userID=ebsco-test&password=ebsco-test
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unknown
http://library.link/vocab/discovery_link
{'f': 'http://opac.lib.rpi.edu/record=b3388095'}
Extent
XIII, 178 p. 46 illus. in color.
File format
multiple file formats
Form of item
electronic
Isbn
9784431542018
Level of compression
uncompressed
Media category
computer
Media MARC source
rdamedia
Media type code
c
Other physical details
online resource.
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absent
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access
Specific material designation
remote

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