activity
19982026
most citedExotic modes of excitation in atomic nuclei far from stability

543 citations · 4.2k across the 85 of their papers we have counts for

collaborators

85 papers

nucl-th2026

Outer-crust equations of state for neutron stars

P. S. Koliogiannis, N. Paar

The equation of state of the outer crust of neutron stars is sensitive to nuclear mass predictions and provides a direct connection to the properties of nuclei throughout the nucli…

nucl-th2026

Universal relation between dipole polarizability of finite nuclei and neutron-star compactness

P. S. Koliogiannis, T. Ghosh, E. Yuksel +1

The nuclear equation of state, which determines the structure and properties of neutron stars, remains subject to substantial theoretical uncertainties, leading to model dependence…

nucl-th2024

The axially-deformed relativistic quasiparticle random phase approximation based on point-coupling interactions

A. Ravlić, T. Nikšić, Y. F. Niu +2

Collective nuclear excitations, like giant resonances, are sensitive to nuclear deformation, as evidenced by alterations in their excitation energies and transition strength distri…

nucl-th2023

Finite temperature effects in magnetic dipole transitions

Amandeep Kaur, Esra Yüksel, Nils Paar

Finite temperature effects in electromagnetic transitions in nuclei contribute to many aspects of nuclear structure and astrophysically relevant nuclear reactions. While electric d…

nucl-th2023

Electric dipole transitions in the relativistic quasiparticle random phase approximation at finite temperature

Amandeep Kaur, Esra Yüksel, Nils Paar

Finite temperature results in various effects on the properties of nuclear structure and excitations of relevance for nuclear processes in hot stellar environments. Here we introdu…

nucl-th2023

Global properties of nuclei at finite-temperature within the covariant energy density functional theory

Ante Ravlić, Esra Yüksel, Tamara Nikšić +1

In stellar environments nuclei appear at finite temperatures, becoming extremely hot in core-collapse supernovae and neutron star mergers. However, due to theoretical and computati…