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- W2075316411 abstract "The formalism of a relativistically covariant saturating chiral field theory of nuclear matter is developed in the mean field approximation, and some of the properties are studied. The theory possesses the normal saturated state of nuclear matter. The finite temperature properties are examined. A normal gas-liquid phase equilibrium region exists below T ≈ 23MeV. The maximum mass for a neutron star is calculated, and it lies well above the lower bound set by observation. In the high-temperature regime, there is a second minimum in the free energy, on which branch the effective baryon mass is very small. However, this branch is everywhere mechanically unstable, and so is not a realizable state of the theory. Above a certain critical temperature there is in fact no stable state at low baryon density. There is no density or temperature regime where chiral symmetry is restored." @default.
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- W2075316411 date "1986-04-01" @default.
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- W2075316411 title "Phase transitions in a saturating chiral theory of nuclear matter" @default.
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