Tension between implications from PREX-2 data and gravitational tidal response on dense matter equation of state
Recently an improved value of neutron skin thickness of 208 Pb was reported in Lead Radius EXperiment-2 (PREX-2) to be R skin = R n R p = (0.283 0.071) fm which corresponds to high estimations of nuclear symmetry energy ( E sym ) and its slope ( L sym ). The updated values of E sym and L sym commens...
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Published in | EPJ Web of conferences Vol. 279; p. 10003 |
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Main Authors | , |
Format | Journal Article |
Language | English |
Published |
EDP Sciences
2023
|
Online Access | Get full text |
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Summary: | Recently an improved value of neutron skin thickness of
208
Pb was reported in Lead Radius EXperiment-2 (PREX-2) to be
R
skin
=
R
n
R
p
= (0.283 0.071) fm which corresponds to high estimations of nuclear symmetry energy (
E
sym
) and its slope (
L
sym
). The updated values of
E
sym
and
L
sym
commensurating to the neutron star observable estimations lie exterior to the astrophysical observed range. The higher values of
L
sym
at
n
0
deduced from recent PREX-2 data correlates to matter being easily deformable (yielding higher radius values) around intermediate matter densities leading to higher values of Λ̃ creating a tension between the terrestrial and astrophysical observations. In this study, we exploit this tension to constrain the Δ-scalar meson coupling parameter space. |
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ISSN: | 2100-014X 2100-014X |
DOI: | 10.1051/epjconf/202327910003 |