Pressure-density Relation
Pressure-Density Relation is a theoretical construct in nuclear physics that specifies the functional dependence of pressure on matter density within neutron star interiors, distinguishing itself from other equation-of-state models by directly encoding the compressibility and thermodynamic stability of dense nuclear matter under extreme conditions.
343
Publications
18.6K
Citations
902
Authors
395
Institutions
Publications per year
2017–2026
55
Parents
343
THE EQUATION OF STATE FROM OBSERVED MASSES AND RADII OF NEUTRON STARS
The Astrophysical Journal · 2010 · 923 citations · Full text
Natural Sciences, Astronomy, Physics +17
1–5 of 343
902
Universidad Michoacana de San Nicolás de Hidalgo, Mexico
7 publications · 145 citations
7
h-index
5
h-index
5
h-index
Universidad Michoacana de San Nicolás de Hidalgo, Mexico
4 publications · 96 citations
4
h-index
4
h-index
1–5 of 902
395
Los Alamos National Laboratory
Los Alamos, United States
10 h-index
19 publications
708 citations

Lawrence Livermore National Laboratory
Livermore, United States
9 h-index
32 publications
1.1K citations
Massachusetts Institute of Technology
Cambridge, United States
8 h-index
14 publications
1.2K citations

Universidad Michoacana de San Nicolás de Hidalgo
Morelia, Mexico
8 h-index
23 publications
471 citations
The University of Tokyo
Tokyo, Japan
7 h-index
13 publications
579 citations
Institut Laue-Langevin
Grenoble, France
7 h-index
10 publications
642 citations

Centre National de la Recherche Scientifique
Paris, France
7 h-index
17 publications
942 citations
Princeton University
Princeton, United States
6 h-index
13 publications
925 citations
1–8 of 395
18 publications · 967 citations
16
h-index
PRC · 18 publications · 893 citations
15
h-index
PRD · 12 publications · 602 citations
12
h-index
ApJ · 12 publications · 1.3K citations
11
h-index
11 publications · 437 citations
11
h-index
1–5