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Properties of hadron matter. II - Dense baryon matter and neutron stars.In this article we have provided certain details of a nuclear-matter computation, based on the Brueckner-Bethe-Goldstone theory of nuclear reaction, which leads to an equation of state for matter in the density region of 10 to 500 trillion g/cu cm. We also explore the possibilities that at very high baryon densities or for very short baryon separations, the net baryon-baryon interaction may be negligible so that the results of dynamical models, like the statistical bootstrap model and the dual-resonance model, may be applicable to the study of dense baryon matter. Several plausible equations of state are constructed, and their effect on the limiting mass of the neutron star is examined.
Document ID
19720030891
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Leung, Y. C.
(Southeastern Massachusetts University North Dartmouth, Mass., United States)
Wang, C. G.
(MIT Cambridge, Mass., United States)
Date Acquired
August 6, 2013
Publication Date
December 15, 1971
Publication Information
Publication: Astrophysical Journal
Volume: 170
Subject Category
Space Sciences
Accession Number
72A14557
Funding Number(s)
CONTRACT_GRANT: NGL-22-009-015
Distribution Limits
Public
Copyright
Other

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