Chang-Hwan Lee

TL;DR: In this article, the authors used the relativistic Boltzmann-Uehling-Uhlenbeck (RBUU) transport code to estimate the properties of nuclear matter that can be created from low-energy heavyion collisions at RAON.

TL;DR: Cho et al. as discussed by the authors applied the eFM method to several nonspinning binary systems and find that the error bounds in eFM are qualitatively in good agreement with the MCMC results of Rodriguez et al in all mass regions.

TL;DR: In this paper, the cooling of neutron stars with relativistic and non-relativistic models of dense nuclear matter is investigated, focusing on the effects of uncertainties originated from the nuclear models, the composition of elements in the envelope region, and the formation of superfluidity in the core and the crust of the neutron stars.

TL;DR: In this paper , the authors show that the vector manifestation of the STAR peripheral collisions can be reconstructed from following their pion decay products back to the vertex where they are formed, and that the measured ρ 0 /π − ratio can be reproduced in these special circumstances only because the flash at which the ρ -mesons go on-shell is equal to the freeze-out temperature.

TL;DR: In this article, the authors used binary stellar evolution to argue that binaries with at least one black hole dominate the rate of compact-object mergers and two phenomena generally attributable to such mergers, gamma-ray bursts and gravity-wave bursts, are therefore likely to originate from near the event horizon of a black hole.