general relativity and astrophysics in the hanyang relativity...
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GENERAL RELATIVITY AND ASTROPHYSICS GENERAL RELATIVITY AND ASTROPHYSICS
IN THE HANYANG RELATIVITY GROUPIN THE HANYANG RELATIVITY GROUP
In-Saeng Suh
행당웍샵 2012 (이철훈교수 정년퇴임 기념)
PROF. PROF. CHULCHUL H. LEEH. LEE
감사
약력
서울대
University of Notre Dame – Prof. William McGlinn
Coupled gravitational and electromagnetic perturbations
around a charged black hole
ICTP 연구원
육사교관
한양대학교 교수 – 상대론 그룹
한국 물리학회 천체물리분과 위원장 – 1대,2대
The 1st Italian-Korean Joint Symposium
on Relativistic Astrophysics (1987)
일반일반 상대론상대론 (1986)(1986)
HANYANGHANYANG RELATIVITY GROUP RELATIVITY GROUP
Ph.D. in Physics – 6 명
Master of Science in Physics - 16 명
General Relativity
Cosmology
Astrophysics Black Holes
Quark Stars
Neutron Stars
…
Topological/Nontopological Objects: Solitons, Textures
Numerical Relativity
…
SEUNGUNSEUNGUN YOONYOON
Gauged Nontopological Solitons and
Callan-Rubakov
EffectsCallan-Rubakov effect - catalyze baryon
decay
Calculated the cross-section for quark-to-lepton
transition due to the gauged NTS
Existence of stable gauged NTSs
ININ--SAENGSAENG SUHSUH
Cosmological Quark-Hadron Phase Transition
Quark-Gluon Plasma - Imperfect Fluid
Effects of Bulk viscosity on the evolution in the early
Universe
Curvature energy on the cosmological quark-hadron
phase transition
Temperature evolution and its effect on the Big-Bang
Nucleosynthesis
Primordial Magnetic Fields and neutrino degeneracy
Magnetars – Strongly magnetized neutron stars
Relativistic Hydrodynamics – Binary neutron stars
HEEILHEEIL KIMKIM
Two Objects in the early Universe: Texture and
Primordial Black Hole
Texture
Primordial Black Hole
Density Fluctuations amplification during the
cosmological quark-hadron phase transition
Numerical Hydrodynamics – Rapidly rotating neutron star
SEOKTAESEOKTAE KOHKOH
Gravitational Perturbations in the Early Universe 1) Inflation: Higgs inflation, nonminimally coupled scalar field
model, vector inflation, oscillating inflation, nonminimal hybrid inflation
2) linear perturbations and gravitational wave
3) non-Gaussianity and nonlinear perturbations
4) CMB
5) trans-Planckian physics
Late time accelerating universe 1) Dark energy
2) gravitational wave spectrum in an accelerating universe
3) Large scale structure
WONWOOWONWOO LEELEE
The Gravity Effect on the Decay of a False Vacuum
False vacuum bubble nucleation due to a nonminimally
coupled scalar field and dynamics after the nucleation
Creation of a black hole pair with a domain wall
Instanton solutions mediating tunneling between the
degenerate vacua and oscillating solutions in curved
space
CHANGHEONCHANGHEON OHOH
Properties of self-gravitating instanton solutions
and AdS soliton spacetimes
그때그때 그시절그시절……
그때그때 그시절그시절……
그때그때 그시절그시절……
PROF. WILLIAM PROF. WILLIAM MMCCGLINNGLINN INTERVIEWINTERVIEW
Thank you