54 citations · 189 across the 16 of their papers we have counts for
16 papers
Quantum Field Theoretic Treatment of Pion Production via Proton Synchrotron Radiation in Strong Magnetic Fields: Effects of Landau Levels
Tomoyuki Maruyama, Myung-Ki Cheoun, Toshitaka Kajino +3
We study pion production from proton synchrotron radiation in the presence of strong magnetic fields. We derive the exact proton propagator from the Dirac equation in a strong magn…
Asymmetric Neutrino Production in Strongly Magnetized Proto-Neutron Stars
Tomoyuki Maruyama, Myung-Ki Cheoun, Jun Hidaka +6
We calculate the neutrino production cross-section through the direct URCA process in proto-neutron star matter in the presence of a strong magnetic field. We assume isoentropic co…
Neutron stars in a perturbative gravity model with strong magnetic fields
Myung-Ki Cheoun, Cemsinan Deliduman, Can Güngör +4
We investigate the effect of a strong magnetic field on the structure of neutron stars in a model with perturbative gravity. The effect of an interior strong magnetic field…
Updates of the nuclear equation of state for core-collapse supernovae and neutron Stars: effects of 3-body forces, QCD, and magnetic fields
G J Mathews, M Meixner, J P Olson +7
We summarize several new developments in the nuclear equation of state for supernova simulations and neutron stars. We discuss an updated and improved Notre-Dame-Livermore Equation…
Rapid Spin Deceleration of Magnetized Proto-Neutron Stars via Asymmetric Neutrino Emission
T. Maruyama, J. Hidaka, T. Kajino +5
We calculate the spin deceleration of proto-neutron stars by asymmetric neutrino absorption in the context of a fully relativistic mean field theory. We calculate for the first tim…
Relativistic Mean-Field Treatment of Pulsar Kick from Neutrino Propagation in Magnetized Proto-Neutron
Tomoyuki Maruyama, Nobutoshi Yasutake, Myung-Ki Cheoun +3
We make a perturbative calculation of neutrino scattering and absorption in hot and dense hyperonic neutron-star matter in the presence of a strong magnetic Field. We calculate tha…