Abstract:
A second-order virial equation of state for a symmetric system of nucleons (N=Z) interacting through a deuteronlike force is established. The dependence of the virial coefficient on temperature and the square-well parameters is discussed. The isotherms are analyzed, and it is shown that the gas-liquid phase transition takes place at a much lower density than that commonly assumed to be the characteristic density of nuclear matter. © 1978 The American Physical Society.
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Citas:
---------- APA ----------
(1978)
. Phase transitions in nuclear matter at finite temperatures. Physical Review A, 18(3), 1266-1271.
http://dx.doi.org/10.1103/PhysRevA.18.1266---------- CHICAGO ----------
Hernández, E.S.
"Phase transitions in nuclear matter at finite temperatures"
. Physical Review A 18, no. 3
(1978) : 1266-1271.
http://dx.doi.org/10.1103/PhysRevA.18.1266---------- MLA ----------
Hernández, E.S.
"Phase transitions in nuclear matter at finite temperatures"
. Physical Review A, vol. 18, no. 3, 1978, pp. 1266-1271.
http://dx.doi.org/10.1103/PhysRevA.18.1266---------- VANCOUVER ----------
Hernández, E.S. Phase transitions in nuclear matter at finite temperatures. 1978;18(3):1266-1271.
http://dx.doi.org/10.1103/PhysRevA.18.1266