activity
20112026
most citedConstraining the Symmetry Parameters of the Nuclear Interaction

506 citations · 1.6k across the 31 of their papers we have counts for

collaborators

33 papers

nucl-th2026

Constraining hyperonic relativistic mean-field models with rapidly rotating neutron stars

Gihwan Nam, Prashant Thakur, Yeunhwan Lim +1

Motivated by the recent mass measurement of the black-widow pulsar PSR~J09520607 with , we investigate how the masses of heavy, rapidly rotating millisec…

nucl-th2025

Universal Relation for the Neutron Star Maximum Mass within Relativistic Mean-Field Theories

Gihwan Nam, Yeunhwan Lim, Jeremy W. Holt

We obtain a universal relation for the neutron star maximum mass arising from a particular combination of the saturation density (), the effective mass (), and (when pres…

nucl-th2025

Sensitivity of neutron drip lines and neutron star properties to the symmetry energy

Yeunhwan Lim, Jeremy W. Holt

We investigate the influence of the nuclear symmetry energy and its density slope parameter on the neutron dripline and neutron star properties using a semi-classical liquid drop m…

nucl-th2023★ 20 cited

Symmetry energy and neutron star properties constrained by chiral effective field theory calculations

Yeunhwan Lim, Achim Schwenk

We investigate the nuclear symmetry energy and neutron star properties using a Bayesian analysis based on constraints from different chiral effective field theory calculations usin…

nucl-th2023

Realistic evaluation of Coulomb potential in spherical nuclei and test of the traditional approach

L. Xayavong, Y. Lim

A realistic evaluation of Coulomb potential has been made for some selected nuclei using the available model-independent data for the charge density and the recent development of C…

nucl-th2022★ 1 cited

Neutron star radii, deformabilities, and moments of inertia from experimental and ab initio theory constraints on the 208Pb neutron skin thickness

Yeunhwan Lim, Jeremy W. Holt

Recent experimental and ab initio theory investigations of the 208Pb neutron skin thickness are sufficiently precise to inform the neutron star equation of state. In particular, th…