Amanote Research
Register
Sign In
The Symmetry Energy, Neutron Skin Thickness and Isovector Dipole Response of Neutron-Rich Nuclei
EPJ Web of Conferences
- France
doi 10.1051/epjconf/20158801008
Full Text
Open PDF
Abstract
Available in
full text
Categories
Astronomy
Physics
Date
January 1, 2015
Authors
A. Horvat
N. Paar
Publisher
EDP Sciences
Related search
Symmetry Energy, Neutron Star Crust and Neutron Skin Thickness
Few-Body Systems
Optics
Atomic
Molecular Physics,
Symmetry Energy Effects on Isovector Properties of Neutron Rich Nuclei With Thomas-Fermi Approach
HNPS Proceedings
Bootstrap Technique to Study Correlation Between Neutron Skin Thickness and the Slope of Symmetry Energy in Atomic Nuclei
Acta Physica Polonica B
Astronomy
Physics
Structure of Neutron-Rich Nuclei
Crossover From Skin-Mode to Proton-Neutron-Mode in E1 Excitations of Neutron-Rich Nuclei
Neutron Skin Thickness From the Measured Electric Dipole Polarizability inNi68,Sn120, andPb208
Physical Review C
Symmetry Energy at Subnuclear Densities and Nuclei in Neutron Star Crusts
Physical Review C
Production and Study of Neutron-Rich Nuclei Using the LICORNE Directional Neutron Source
Acta Physica Polonica B
Astronomy
Physics
Number-Projected Isovector Neutron-Proton Pairing Effect in Odd Mass Nuclei
Journal of Theoretical and Applied Physics
Astronomy
Physics