ScholarWorks@Soongsil University: Cheoun, Myung-Ki

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Cheoun, Myung-Ki (천명기)

College of Natural Sciences (Department of Physics)

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Neutron stars:5||Nuclear astrophysics:4||Nucleosynthesis:4||GamowTeller transition:3||Strong magnetic field:3||asymmetry:3||Strangeness:3||rpprocess:2||sprocess:2||Novae:2||Neutral current:2||HU (hounsfield unit):2||Abundance:2||Xray bursts:2||abundances:2||supernovae: general:2||Neutrino detectors:2||Black holes:2||γray bursts:2||Neutrino oscillations:2||chargedcurrent:2||Heavyion nuclear reactions:2||Neutrinoinduced reaction:2||Optical model:2||Magic numbers:2||Heavyion reaction:2||Rare isotope beams (RIB):2||double beta decay:2||Deformed nuclei:2||Neutron halos:2||Relativistic quantum approach:2||elementary particles:2||Neutron skins:2||Gamma detectors (scintillators, CZT, HPGe, HgI etc):2||Isomers(Isomeric states):2||Sterile neutrino:2||Supernova neutrinos:2||modified gravity:2||neutralcurrent:2||Supernovae:2||neutrino experiments:2||neutrino properties:2||neutrino scattering:2||neutrino theory:2||Neutronstar:2||neutrinos:2||Big Bang Nucleosynthesis:2||nuclear reactions:2||Tscore:2||nucleosynthesis:2||Coulomb dipole excitation:2||The elements:2||primordial nucleosynthesis:2||Proton halos:2||quasielastic region:2||Thermonuclear reactions:2||Threshold anomaly:2||rprocess:2||Total fusion cross section:2||AGB(asymptotic giant branch):2||Google Trends:1||Group research:1||Hdibaryon:1||Halo nuclei:1||Heavy ion collision:1||Hubble expansion rate:1||Hyperonnucleon interactions:1||Isospinasymmetric nuclear matter:1||Landau level:1||Liquid scintillator:1||Longrange nuclear potential:1||Loosely bound nuclei:1||Loosely bound nucleus:1||M1 spin transition:1||MDCT (multidetector computed tomography):1||Magnetar:1||Magnetic field:1||Magnetic fields:1||Magnetic moment:1||Manybody nucleon system:1||Modified gravity:1||Multipole amplitudes:1||Negatively charged massive particle:1||Neutrino and antineutrino emissions:1||Neutrino detector:1||Neutrino emission:1||Neutrino source from decay at rest:1||Neutrinoinduced reaction on C12:1||Neutrinoinduced reactions:1||Neutrinos:1||Neutronproton pairing correlation:1||Neutronrich nuclei:1||Ni isotopes:1||Nilsson basis:1||Nonlocal potential:1||Nonlocality factor:1||Nuclear Physics:1||Nuclear mass model:1||Nuclear matter:1||Nuclear physics:1||Nuclear symmetry energy:1||Nucleosynthesis
network calculation:1||Numerical simulation:1||OMEG:1||Optical model approach:1||PREX2 and CREX experiments:1||Pairing Energies:1||Pairing Matrix Elements:1||Pairing correlations:1||Parity violation:1||Photon vortex:1||Physics education:1||Presidential Election:1||Protoneutron star:1||Protoneutron stars:1||Pygmy dipole resonance:1||Quantum approach:1||Quantum hadrodynamics:1||Quantum synchrotron radiation:1||Quasi Particle Random Phase Approximation:1||Quasielastic region:1||Quasiparticle RPA:1||Quasiparticle random phase approximation (QRPA):1||Quasielastic data:1||Quasielastic region:1||Quasiparticle random phase approximation:1||RAON:1||RISP:1||RPA:1||Radiation dominated era:1||Rare isotope accelerator:1||Relativistic HartreeFock approximation:1||Relativistic meanfield models:1||SU(2) symmetry breaking:1||Scintillators, scintillation and light emission processes (solid, gas and liquid scintillators):1||Shell evolution:1||Starquakes:1||Symmetry Energy:1||Symmetry energy:1||Tensor Force:1||The proton and the neutron point density distributions:1||Traditional Polls:1||Trigger algorithms:1||Weak and electromagnetic form factors:1||Winner:1||Wong&apos:1||WoodsSaxon Potential:1||Xparticle:1||astroparticle physics:1||atomic processes:1||axial vector current:1||big bang nucleosynthesis:1||chiral Ward identities:1||cosmology:1||dark matter:1||deformed QRPA:1||dense matter:1||density dependence:1||early universe:1||electromagnetic form factors:1||electron antineutrino source:1||equation of state:1||gauged linear sigma model:1||longitudinal structure function:1||magnetic field:1||magnetic fields:1||massive stars:1||meson masses:1||meteorites, meteors, meteoroids:1||neutrino detectors:1||neutrinonucleus scattering:1||neutron stars:1||nuclear reactions, nucleosynthesis, abundances:1||parity violation:1||pion weakproduction:1||plasmas:1||quasielastic scattering:1||quasiparticle RPA:1||radioactive contamination:1||relativistic meanfield:1||s formula:1||short baseline neutrino disappearance:1||stars: abundances:1||stars: neutron:1||sterile neutrinos:1||strange axial form factor:1||strange form factors:1||strange quark:1||suppression:1||timeamplitude analysis:1||weak and electromagnetic form factors:1||weak pionproduction:1||감마선 폭발체:1||검은구멍:1||결합 진동자:1||골밀도:1||구글 트렌드:1||느린중성자포획과정:1||느슨하게 묶인 핵:1||다중 검출 전산화단층촬영:1||당선인:1||대통령선거:1||마법수:1||문턱비정상:1||물리 교육:1||빠른양성자포획과정:1||빠른중성자포획과정:1||수치 시뮬레이션:1||신성:1||아이소머:1||양성자 달무리핵:1||엑스선 폭발체:1||열핵반응:1||예측:1||원소:1||전통적인 여론조사:1||점근거성계열:1||존재비:1||중성자 달무리핵:1||중성자 피부핵:1||중성자별:1||중이온핵반응:1||천체핵물리학:1||초신성:1||핵반응 네트워크:1||핵조성:1||핵질량 모델:1||핵합성:1||$\chi^{2}$ analysis:1||희귀동위원소빔:1||$\chi^{2}$ 분석법:1||Asymmetric nuclear matter:1||Axion:1||Axion production:1||BCS:1||BMD (bone mineral density):1||Baryons:1||Bigbang nucleosynthesis:1||Binding energies:1||Bound state wave function:1||Bruckner Gmatrix:1||C03:1||C04:1||C12:1||C32:1||C43:1||CENS:1||CENuM:1||CaMoO4:1||Cascade baryon:1||Charge conserving reaction:1||Charge density distribution:1||Charge exchange reaction:1||Cosmology:1||Coulomb and Electromagnetic transitions:1||Coulomb and electromagnetic transitions:1||Coulomb excitation potenial:1||Coulomb quadrupole excitation:1||Coupled oscillators:1||Coupledchannel:1||Coupledchannel method:1||Coupledchannels method:1||Cyclotron:1||D10:1||D14:1||D41:1||Dark matter:1||Deformed Nuclei:1||Deformed Quasiparticle RPA:1||Density dependence:1||Densitydependent form factor:1||Detector control systems (detector and experiment monitoring and slowcontrol systems, architecture, hardware, algorithms, databases):1||Direct Urca:1||Double Beta Decay:1||Eﬀective Lagrangian method:1||Equations of state of neutronstar matter:1||Exclusive reaction:1||Exotics:1||Explosive nucleosynthesis:1||Forecasting:1||Functional Schrodinger picture formalism:1||Gamow Teller Transition:1||GamowTeller Transition:1||GamowTeller strength:1||Gamowteller transition:1||Giant Monopole and Pygmy Dipole Resonances:1||Giant dipole resonance:1||Giant monopole resonance:1||Glitches:1||

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