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Implications of tachyon-like matter for superdense stars.Derivation of a new equation of state of superdense matter by treating superdense matter as a perfect, degenerate tachyon gas. Model calculations for superdense stars based on this equation of state are presented. By appropriately choosing a certain parameter, dynamical stability can be achieved for arbitrarily large central densities. Also, a somewhat larger than usual value for the maximum mass is obtained.
Document ID
19720053049
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Bhatia, M. S.
(Bowie State College Bowie, Md., United States)
Pande, L. K.
(Delhi University Delhi, India)
Date Acquired
August 6, 2013
Publication Date
June 15, 1972
Publication Information
Publication: Physical Review D - Particles and Fields
Subject Category
Space Sciences
Accession Number
72A36715
Distribution Limits
Public
Copyright
Other

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