Authors:
- Derives relations between the gravitational wave cutoff frequency and neutron star compactness
- Clarifies formation of massive accretion disks for short-hard gamma ray bursts
- Nominated as an outstanding Ph.D thesis by Kyoto University’s Physics Department in 2012.
Part of the book series: Springer Theses (Springer Theses)
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Table of contents (8 chapters)
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Front Matter
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Back Matter
About this book
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.
Keywords
- Adaptive Mesh Refinement
- Black Hole-neutron Star Binary
- Compact Binary Coalescence
- Gravitational Waves from Compact Binaries
- Neutron Star Equation of State
- Numerical Relativity for Non-vacuum Spacetimes
- Piecewise Polytropic Equations of State
- Short-hard Gamma-ray Bursts
- Supranuclear Density Matter
- The Tidal Disruption of Neutron Stars
Authors and Affiliations
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KEK, Cosmophysics Group, Institute of Particle and Nuclear Studie, Ibaraki, Japan
Koutarou Kyutoku
About the author
Cosmophysics Group, Theory Center, IPNS (Institute of Particle and Nuclear Studies), KEK (High Energy Accelerator Research Organization)
kyutoku@post.kek.jp
Bibliographic Information
Book Title: The Black Hole-Neutron Star Binary Merger in Full General Relativity
Book Subtitle: Dependence on Neutron Star Equations of State
Authors: Koutarou Kyutoku
Series Title: Springer Theses
DOI: https://doi.org/10.1007/978-4-431-54201-8
Publisher: Springer Tokyo
eBook Packages: Physics and Astronomy, Physics and Astronomy (R0)
Copyright Information: Springer Japan 2013
Hardcover ISBN: 978-4-431-54200-1Published: 11 January 2013
Softcover ISBN: 978-4-431-54733-4Published: 25 June 2015
eBook ISBN: 978-4-431-54201-8Published: 11 January 2013
Series ISSN: 2190-5053
Series E-ISSN: 2190-5061
Edition Number: 1
Number of Pages: XIII, 178
Topics: Astronomy, Astrophysics and Cosmology, Mathematical Applications in the Physical Sciences, Numerical and Computational Physics, Simulation