Abstract
A previous thermodynamically consistent procedure for considering the finite volume effect of nucleons in nuclear matter is developed to be relativistic. Parameters are determined by fitting all five empirical data for normal nuclear matter. The resulting nuclear equations of state may be used in researches for neutron stars and for phase transitions between nuclear matter and quarkgluon plasma.
Similar content being viewed by others
References
Glendenning, N.K.: Nucl. Phys, A480, 597 (1988)
Rischke, D.H., Gorenstein, M.I., Stöcker, H., Greiner, W.: Z. Phys. C51, 485 (1991)
Zhang, Q.-R., Ma, B.-Q., Greiner, W.: J. Phys. G18, 2051 (1992)
Ma, B.-Q., Zhang, Q.-R., Rischke, D.H., Greiner, W.: Phys. Lett. B315, 29 (1993)
Zhang, Q.-R., Li, X.-G.: Z. Phys. A343, 337 (1992)
Zhang, Q.-R.: Acta Sci. Nat. Univ. Jilin [Suppl. (Physics)]xx1 (1992) (in Chinese)
See for example Huang, K.: Statistical mechanics. New York: Wiley 1963
See for example Pauli, W.: Theory of relativity. London: Pergamon Press 1958
See for example Weinberg, S.: Gravitation and cosmology. New York: Wiley 1972
Myers, W.D., Swiatecki, W.J.: Ann. Phys. (NY)84, 186 (1974)
Author information
Authors and Affiliations
Additional information
Partly supported by Science Foundation of Nuclear Industry, China
Rights and permissions
About this article
Cite this article
Zhang, Q.R. Relativistic and thermodynamically consistent treatment for the finite volume effect of nucleons in nuclear matter. Z. Physik A - Hadrons and Nuclei 351, 89–97 (1995). https://doi.org/10.1007/BF01292790
Received:
Revised:
Issue Date:
DOI: https://doi.org/10.1007/BF01292790