The Black Hole-Neutron Star Binary Merger in Full General Relativity: Dependence on Neutron Star Equations of State
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| Format: | Electronic eBook |
|---|---|
| Language: | English |
| Published: |
Tokyo
Springer Japan
2013
|
| Series: | Springer Theses, Recognizing Outstanding Ph.D. Research
|
| Subjects: | |
| Online Access: | TUM01 UBT01 Volltext Inhaltsverzeichnis Abstract |
| Item Description: | 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. 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. |
| Physical Description: | 1 Online-Ressource |
| ISBN: | 9784431542018 |
| DOI: | 10.1007/978-4-431-54201-8 |
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| 245 | 1 | 0 | |a The Black Hole-Neutron Star Binary Merger in Full General Relativity |b Dependence on Neutron Star Equations of State |c by Koutarou Kyutoku |
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| 500 | |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. | ||
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Record in the Search Index
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| adam_text | THE BLACK HOLE-NEUTRON STAR BINARY MERGER IN FULL GENERAL RELATIVITY
/ KYUTOKU, KOUTAROU
: 2013
TABLE OF CONTENTS / INHALTSVERZEICHNIS
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
DIESES SCHRIFTSTUECK WURDE MASCHINELL ERZEUGT.
THE BLACK HOLE-NEUTRON STAR BINARY MERGER IN FULL GENERAL RELATIVITY
/ KYUTOKU, KOUTAROU
: 2013
ABSTRACT / INHALTSTEXT
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
DIESES SCHRIFTSTUECK WURDE MASCHINELL ERZEUGT.
|
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| isbn | 9784431542018 |
| language | English |
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| spelling | The Black Hole-Neutron Star Binary Merger in Full General Relativity Dependence on Neutron Star Equations of State by Koutarou Kyutoku Tokyo Springer Japan 2013 1 Online-Ressource txt rdacontent c rdamedia cr rdacarrier Springer Theses, Recognizing Outstanding Ph.D. Research 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. 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. Physics Astronomy Astronomy, Astrophysics and Cosmology Mathematical Applications in the Physical Sciences Numerical and Computational Physics Kyutoku, Koutarou Sonstige oth https://doi.org/10.1007/978-4-431-54201-8 Verlag Volltext Springer Fremddatenuebernahme application/pdf http://bvbr.bib-bvb.de:8991/F?func=service&doc_library=BVB01&local_base=BVB01&doc_number=025731167&sequence=000001&line_number=0001&func_code=DB_RECORDS&service_type=MEDIA Inhaltsverzeichnis Springer Fremddatenuebernahme application/pdf http://bvbr.bib-bvb.de:8991/F?func=service&doc_library=BVB01&local_base=BVB01&doc_number=025731167&sequence=000003&line_number=0002&func_code=DB_RECORDS&service_type=MEDIA Abstract |
| spellingShingle | The Black Hole-Neutron Star Binary Merger in Full General Relativity Dependence on Neutron Star Equations of State Physics Astronomy Astronomy, Astrophysics and Cosmology Mathematical Applications in the Physical Sciences Numerical and Computational Physics |
| title | The Black Hole-Neutron Star Binary Merger in Full General Relativity Dependence on Neutron Star Equations of State |
| title_auth | The Black Hole-Neutron Star Binary Merger in Full General Relativity Dependence on Neutron Star Equations of State |
| title_exact_search | The Black Hole-Neutron Star Binary Merger in Full General Relativity Dependence on Neutron Star Equations of State |
| title_full | The Black Hole-Neutron Star Binary Merger in Full General Relativity Dependence on Neutron Star Equations of State by Koutarou Kyutoku |
| title_fullStr | The Black Hole-Neutron Star Binary Merger in Full General Relativity Dependence on Neutron Star Equations of State by Koutarou Kyutoku |
| title_full_unstemmed | The Black Hole-Neutron Star Binary Merger in Full General Relativity Dependence on Neutron Star Equations of State by Koutarou Kyutoku |
| title_short | The Black Hole-Neutron Star Binary Merger in Full General Relativity |
| title_sort | the black hole neutron star binary merger in full general relativity dependence on neutron star equations of state |
| title_sub | Dependence on Neutron Star Equations of State |
| topic | Physics Astronomy Astronomy, Astrophysics and Cosmology Mathematical Applications in the Physical Sciences Numerical and Computational Physics |
| topic_facet | Physics Astronomy Astronomy, Astrophysics and Cosmology Mathematical Applications in the Physical Sciences Numerical and Computational Physics |
| url | https://doi.org/10.1007/978-4-431-54201-8 http://bvbr.bib-bvb.de:8991/F?func=service&doc_library=BVB01&local_base=BVB01&doc_number=025731167&sequence=000001&line_number=0001&func_code=DB_RECORDS&service_type=MEDIA http://bvbr.bib-bvb.de:8991/F?func=service&doc_library=BVB01&local_base=BVB01&doc_number=025731167&sequence=000003&line_number=0002&func_code=DB_RECORDS&service_type=MEDIA |
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