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QCD, 20 years later : Aachen, June 9-13, 1992
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ISBN: 9810210868 981021085X 9789810210861 9789810210854 Year: 1993 Publisher: Singapore : World Scientific,

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5th workshop on perspectives in nuclear physics at intermediate energies, ICTP, Trieste, Italy, May 6-10, 1991
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ISBN: 9810207816 Year: 1992 Publisher: Singapore ; London ; Hong Kong World Scientific

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Intersections of particle and nuclear physics : 7th conference CIPANP2000, Quebec City, Canada, 22-28 May 2000
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ISSN: 0094243X ISBN: 1563969785 9781563969782 Year: 2000 Volume: 549 Publisher: New York, NY : AIP - American Institute of Physics,

Proceedings of the Sixth Workshop on Non-Perturbative QCD
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ISBN: 1281929964 9786611929961 9812778357 9789812778352 9810247486 9789810247485 0817631275 9780817631277 Year: 2002 Volume: 8 Publisher: River Edge, NJ World Scientific

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This volume is devoted to different facets of QCD, stressing non-perturbative, analytic and lattice formulations, scattering solutions and approximations, and the understanding of recent RHIC experiments. It discusses ideas of the fifth dimension, originating in brane theory, as well as possible experimental tests and predictions of those ideas.

Proceedings of the UCLA Workshop : observable standard model physics at the SSC : Monte Carlo stimulation and detector capabilities, 15-24 January 1986
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ISBN: 9971501252 9789971501259 Year: 1986 Publisher: Singapore World Scientific


Dissertation
The black hole-neutron star binary merger in full general relativity
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ISBN: 4431547339 4431542000 4431542019 1299198007 Year: 2013 Publisher: Tokyo ; London : Springer,

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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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