activity
20242026
collaborators

7 papers

astro-ph.HE2026

Accuracy and Applicability of the Hartle-Thorne and Komatsu-Eriguchi-Hachisu Methods for Modeling Rotating Neutron Stars

Hyukjin Kwon, Kenta Yoshimura, Tsuyoshi Miyatsu +2

Neutron stars, which are composed of extremely dense nuclear matter, serve as natural laboratories to study nuclear interactions beyond the terrestrial experiments. Recent research…

nucl-th2026

A dual description of quarks and baryons: Quarkyonic matter within a relativistic quark model

Tsuyoshi Miyatsu, Myung-Ki Cheoun, Koichi Saito

We investigate quarkyonic matter within a relativistic quark model by combining the dual quarkyonic picture with the quark-meson coupling (QMC) model. Using relativistic gaussian q…

nucl-th2025

Constraining the nuclear equation of state from terrestrial experiments and neutron star observations using relativistic mean-field models

Tsuyoshi Miyatsu, Myung-Ki Cheoun, Kyungsik Kim +1

We investigate the nuclear equation of state (EoS) for isospin-asymmetric matter using a new set of RMF interactions with the - and - mixing, referred to as the OME…

nucl-th2025

Quarkyonic Quark-Meson Coupling Model for Nuclear and Neutron Matter

Koichi Saito, Tsuyoshi Miyatsu, Myung-Ki Cheoun

We unite the dual quarkyonic model with the quark-meson coupling (QMC) model to construct a novel nuclear model based on the quark degrees of freedom, which can cover a wide range…

nucl-th2025

Equation of state for hyperonic neutron-star matter in SU(3) flavor symmetry

Tsuyoshi Miyatsu, Myung-Ki Cheoun, Kyungsik Kim +1

Using a relativistic mean-field model calibrated to finite-nucleus observables and bulk properties of dense nuclear matter, we investigate hyperonic neutron-star matter within an S…

nucl-th2024

Novel features of asymmetric nuclear matter from terrestrial experiments and astrophysical observations of neutron stars

Tsuyoshi Miyatsu, Myung-Ki Cheoun, Kyungsik Kim +1

The accurate measurement of neutron skin thickness of Pb by the PREX Collaboration suggests a large value of the nuclear symmetry energy slope parameter, , whereas the s…