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...
Uloženo v:
| Hlavní autor: | |
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| Médium: | Livre numérique |
| Jazyk: | Anglais |
| Vydáno: |
Tokyo :
Springer Japan
[20..].
Cham : Springer Nature |
| Vydání: | 1st ed. 2013. |
| Edice: | Springer Theses, Recognizing Outstanding Ph.D. Research
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| On-line přístup: | Accès sur la plateforme de l'éditeur Accès sur la plateforme Istex Accès Université d'Orléans Accès INSA CVL |
| Poznámka: |
Archives Springer e-books (Licence nationale) Archives Springer e-books (Licence nationale) |
| Autres localisations: | Voir dans le Sudoc |
| Edition sous un autre format: | • The black hole-neutron star binary merger in full general relativity, dependence on neutron star equations of state, Koutarou Kyutoku, Tokyo, Springer, 2013, 1 vol. (XIII-178 p.), Springer theses, 978-4-431-54200-1 • The Black Hole-Neutron Star Binary Merger in Full General Relativity, Texte imprimé, 9784431542025 • The Black Hole-Neutron Star Binary Merger in Full General Relativity, Texte imprimé, 9784431547334 • The black hole-neutron star binary merger in full general relativity, dependence on neutron star equations of state, Koutarou Kyutoku, Tokyo, Springer, 2013, 1 vol. (XIII-178 p.), Springer theses, 978-4-431-54200-1 |
| Shrnutí: | 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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| Popis jednotky: | Archives Springer e-books (Licence nationale) Archives Springer e-books (Licence nationale) |
| ISBN: | 9784431542018 |
| ISSN: | 2190-5061 |
| Přístup: | Accès en ligne pour les établissements français bénéficiaires des licences nationales Accès soumis à abonnement pour tout autre établissement Conditions particulières de réutilisation pour les bénéficiaires des licences nationales. https://www.licencesnationales.fr/springer-nature-ebooks-contrat-licence-ln-2017 |