Corresponding-states approach to nuclear and neutron-star matter
Publication
, Journal Article
Palmer, RG; Anderson, PW
Published in: Physical Review D
January 1, 1974
The properties of nuclear matter and dense neutron-star matter are studied by an approach which largely avoids the microscopic assumptions of nuclear-matter theory. The method is empirical, employing an extended form of the law of corresponding states to deduce the properties of nuclear systems from those of laboratory substances such as helium. It is possible to predict the solidification pressure and density, the compressibility, and the critical temperature of nuclear and neutron-star matter. As previously reported, a comparatively low solidification pressure is found for neutron-star matter, implying a solid core for most neutron stars. © 1974 The American Physical Society.
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Published In
Physical Review D
DOI
ISSN
0556-2821
Publication Date
January 1, 1974
Volume
9
Issue
12
Start / End Page
3281 / 3291
Related Subject Headings
- Nuclear & Particles Physics
- 5107 Particle and high energy physics
- 5101 Astronomical sciences
- 4902 Mathematical physics
- 0206 Quantum Physics
- 0202 Atomic, Molecular, Nuclear, Particle and Plasma Physics
- 0201 Astronomical and Space Sciences
Citation
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ICMJE
MLA
NLM
Palmer, R. G., & Anderson, P. W. (1974). Corresponding-states approach to nuclear and neutron-star matter. Physical Review D, 9(12), 3281–3291. https://doi.org/10.1103/PhysRevD.9.3281
Palmer, R. G., and P. W. Anderson. “Corresponding-states approach to nuclear and neutron-star matter.” Physical Review D 9, no. 12 (January 1, 1974): 3281–91. https://doi.org/10.1103/PhysRevD.9.3281.
Palmer RG, Anderson PW. Corresponding-states approach to nuclear and neutron-star matter. Physical Review D. 1974 Jan 1;9(12):3281–91.
Palmer, R. G., and P. W. Anderson. “Corresponding-states approach to nuclear and neutron-star matter.” Physical Review D, vol. 9, no. 12, Jan. 1974, pp. 3281–91. Scopus, doi:10.1103/PhysRevD.9.3281.
Palmer RG, Anderson PW. Corresponding-states approach to nuclear and neutron-star matter. Physical Review D. 1974 Jan 1;9(12):3281–3291.
Published In
Physical Review D
DOI
ISSN
0556-2821
Publication Date
January 1, 1974
Volume
9
Issue
12
Start / End Page
3281 / 3291
Related Subject Headings
- Nuclear & Particles Physics
- 5107 Particle and high energy physics
- 5101 Astronomical sciences
- 4902 Mathematical physics
- 0206 Quantum Physics
- 0202 Atomic, Molecular, Nuclear, Particle and Plasma Physics
- 0201 Astronomical and Space Sciences