General Relativity and Astrophysics in the Hanyang Relativity...
Transcript of General Relativity and Astrophysics in the Hanyang Relativity...
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