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Elementary particles --- Quantum chromodynamics --- Congresses. --- Quantum chromodynamics - Congresses.
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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.
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Elementary particles --- Mathematical physics --- Particles (Nuclear physics) --- Sum rules (Physics) --- Hadrons --- Gauge fields (Physics) --- Supersymmetry --- Quantum chromodynamics --- Congresses --- Particles (Nuclear physics) - Congresses --- Sum rules (Physics) - Congresses --- Hadrons - Congresses --- Gauge fields (Physics) - Congresses --- Supersymmetry - Congresses --- Quantum chromodynamics - Congresses
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Cosmology --- Dark matter (Astronomy) --- Atomic clocks --- Symmetry (Physics) --- Electroweak interactions --- Particles (Nuclear physics) --- Neutrinos --- Oscillations --- Quantum chromodynamics --- Hadron interactions --- Flavor --- Dark matter (Astronomy) - Congresses --- Atomic clocks - Congresses --- Symmetry (Physics) - Congresses --- Electroweak interactions - Congresses --- Particles (Nuclear physics) - Flavor - Congresses --- Neutrinos - Congresses --- Oscillations - Congresses --- Quantum chromodynamics - Congresses --- Hadron interactions - Congresses
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Superconducting Super Collider --- Quantum chromodynamics --- Electroweak interactions --- Monte Carlo method --- Particles (Nuclear physics) --- Nuclear counters --- Chromodynamique quantique --- Interactions électrofaibles --- Monte-Carlo, Méthode de --- Particules (Physique nucléaire) --- Détecteurs nucléaires --- Congresses --- Congrès --- Interactions électrofaibles --- Monte-Carlo, Méthode de --- Particules (Physique nucléaire) --- Détecteurs nucléaires --- Congrès --- Superconducting Super Collider - Congresses --- Quantum chromodynamics - Congresses --- Electroweak interactions - Congresses --- Monte Carlo method - Congresses --- Particles (Nuclear physics) - Congresses --- Nuclear counters - Congresses
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539.12 <063> --- 530.1 --- Elementary and simple particles (charge less than 3 including alpha-rays, beta-rays, gamma-rays as individual particles or as radiation)--Congressen --- Basic principles of physics --- 530.1 Basic principles of physics --- 539.12 <063> Elementary and simple particles (charge less than 3 including alpha-rays, beta-rays, gamma-rays as individual particles or as radiation)--Congressen --- Quantum chromodynamics --- Congresses --- Particles (Nuclear physics) --- Quantum electrodynamics --- Particules (physique nucléaire). --- Électrodynamique quantique. --- Chromodynamique quantique. --- Quantum chromodynamics - Congresses
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539.12 <063> --- 539.12 <063> Elementary and simple particles (charge less than 3 including alpha-rays, beta-rays, gamma-rays as individual particles or as radiation)--Congressen --- Elementary and simple particles (charge less than 3 including alpha-rays, beta-rays, gamma-rays as individual particles or as radiation)--Congressen --- Particles (Nuclear physics) - Congresses --- Unified field theories - Congresses --- Quantum chromodynamics - Congresses --- Particles (Nuclear physics) --- Unified field theories --- Quantum chromodynamics
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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.
Quantum chromodynamics -- Congresses. --- Gravitational waves --- Black holes (Astronomy) --- Neutron stars --- General relativity (Physics) --- Astronomy & Astrophysics --- Physical Sciences & Mathematics --- Astrophysics --- Astronomy - General --- Neutron stars. --- Gravitational waves. --- Gravitational radiation --- Gravity waves (Astrophysics) --- Frozen stars --- Relativistic theory of gravitation --- Relativity theory, General --- Physics. --- Mathematical physics. --- Astronomy. --- Astrophysics. --- Cosmology. --- Astronomy, Astrophysics and Cosmology. --- Mathematical Applications in the Physical Sciences. --- Numerical and Computational Physics. --- Gravitational fields --- Radiation --- Waves --- Compact objects (Astronomy) --- Stars --- Pulsars --- Gravitational collapse --- Gravitation --- Physics --- Relativity (Physics) --- Numerical and Computational Physics, Simulation. --- Natural philosophy --- Philosophy, Natural --- Physical sciences --- Dynamics --- Physical mathematics --- Astronomical physics --- Astronomy --- Cosmic physics --- Mathematics
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