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A Simple Equation of State of Matter at Super-Nuclear Densities∗

Published online by Cambridge University Press:  14 August 2015

Y. C. Leung  and
C. G. Wang
Y. C. Leung
Affiliation:
Southeastern Massachusetts University, North Dartmouth, Mass. 02747, U.S.A.
C. G. Wang
Affiliation:
Massachusetts Institute of Technology, Cambridge, Mass. 02139, U.S.A.

Abstract

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The qualitative features of the equation of state of matter at supernuclear densities are deduced through a careful examination of the nature of particle interactions at short distances and by the introduction of an ‘effective mass spectrum.’ it is found that the equation of state begins to take on a particularly simple form (the ‘asymptotic form’) at a relatively low matter density of 1017 g cm−3. A brief review of various approaches to calculate the equation of state for a neutron star is also given.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 53: Physics of Dense Matter , 1974 , pp. 93 - 104
Copyright
Copyright © Reidel 1974 

References

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