The nuclear symmetry energy and the neutron skin thickness in nuclei
IntroductionWe investigate possible correlations between the stiffness of the symmetry energy at saturation density, the so-called L parameter, and the neutron skin thickness of 48Ca and 208Pb, for which the recent measurements from the CREX and PREX I + II experiments at the Thomas Jefferson Labora...
Saved in:
Main Authors: | G. F. Burgio, H. C. Das, I. Vidaña |
---|---|
Format: | Article |
Language: | English |
Published: |
Frontiers Media S.A.
2024-12-01
|
Series: | Frontiers in Astronomy and Space Sciences |
Subjects: | |
Online Access: | https://www.frontiersin.org/articles/10.3389/fspas.2024.1505560/full |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Novel features of asymmetric nuclear matter from terrestrial experiments and astrophysical observations of neutron stars
by: Tsuyoshi Miyatsu, et al.
Published: (2025-02-01) -
Intersections of ultracold atomic polarons and nuclear clusters: how is a chart of nuclides modified in dilute neutron matter?
by: Hiroyuki Tajima, et al.
Published: (2024-02-01) -
Unveiling radii and neutron skins of unstable atomic nuclei via nuclear collisions
by: Masaomi Tanaka, et al.
Published: (2024-12-01) -
Probing the Equation of State of Neutron Stars with Captured Primordial Black Holes
by: Qing Gao, et al.
Published: (2024-01-01) -
Equation of State Independent Determination on the Radius of a 1.4 M⊙ Neutron Star Using Mass–Radius Measurements
by: Chun Huang
Published: (2024-01-01)