CAU Scholar's Space: Kang, Gungwon

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Kang, Gungwon (강궁원)

자연과학대학 (물리학과)

Research Area: 수치상대론, 중력파 물리, 천체물리, Numerical relativity, Gravitational wave physics, Astrophysics

Tel 02-820-5893
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gravitational waves:41||Gravitational waves:10||stars: neutron:10||LIGO:6||gammaray burst: general:5||Gravitational wave astronomy:4||stars: black holes:4||black holes:4||methods: data analysis:4||Gravitational wave sources:3||Electromagnetic counterparts:3||Neutron stars:3||detector characterization:3||GW150914:3||Gravitationalwave detectors:3||Data analysis:3||binaries: close:3||binaries: general:3||E02:2||Pulsars:2||methods: observational:2||neutrinos:2||black hole physics:2||numerical relativity:2||catalogs:2||pulsars: general:2||F30:2||F32:2||stars: massive:2||Virgo:2||surveys:2||ISM: supernova remnants:2||LIGO/neutron stars:1||Laser interferometer:1||Multicolour:1||NINJA:1||Neutrino astronomy:1||Neutron stars (1108):1||Pulsars: General:1||Radio transient sources:1||Resonance bar detector:1||Rotating black holes:1||Scientific databases:1||Spherically symmetric numerical code:1||Stars: Neutron Supporting Material: MachineReadable Table:1||Statistical analysis:1||Stellar mass black holes:1||Stellar populations:1||Supernova remnants (1667):1||Supernovae:1||Twobody problem:1||Underground experiments:1||Vibration isolation:1||Xrays: binaries:1||accretion, accretion disks:1||binary black holes:1||compact binary coalescences:1||compact object mergers:1||control:1||cosmic explorer:1||cosmology: observations:1||cryogenic laser interferometer:1||data analysis:1||data analysis: algorithms and implementation:1||galaxies: nuclei:1||gravitational radiation detectors:1||gravitational wave astronomy:1||gravitational wave detector:1||gravitational wave detectors:1||gravitationalwave astronomy:1||interferometers:1||long duration transient:1||neutron star equation of state:1||neutron stars:1||optics:1||parameter estimation:1||pulsars:1||sapphire:1||seismic isolation:1||stars:1||stars: kinematics and dynamics:1||stars: magnetars:1||statistical:1||systematic errors:1||underground:1||vibration isolation:1||Astrophysical black holes:1||waveform models:1||Astrophysics:1||Bayesian inference:1||Black holes:1||Data representation and management:1||Eddingtoninspired gravity:1||Equation of state:1||F31:1||F33:1||F34:1||GWOSC:1||Gammaray bursts:1||General relativistic hydrodynamics:1||General relativity:1||Gravitation:1||Gravitational Waves:1||Gravitational collapse:1||Gravitational wave astronomy (675):1||Gravitational wave detectors:1||Gravitational waves (678):1||Gravitational waves / experiments:1||Gravitationalwave detector:1||Gravity:1||Groundbased detectors:1||High energy astrophysics:1||History of gravitationalwave detection:1||Hubble constant:1||Ideal gas:1||Interferometer:1||Intermediatemass black holes:1||KAGRA:1||LIGOVirgo:1||

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84, Heukseok-ro, Dongjak-gu, Seoul, Republic of Korea (06974)02-820-6194

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