Stable masses and radii of super dense baryon stars

Stable masses and radii of super-dense baryon stars are computed from the isostatic relativistic equations of star equilibrium, using an equation of state for 45 baryon species and using the proton-proton interaction energy derived from high energy elastic scattering up to 30 GeV. Masses for an inte...

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Bibliographic Details
Published in:Physics letters. B 1969-01, Vol.30 (6), p.400-401
Main Authors: Libby, L.M., Thomas, F.J.
Format: Article
Language:English
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Summary:Stable masses and radii of super-dense baryon stars are computed from the isostatic relativistic equations of star equilibrium, using an equation of state for 45 baryon species and using the proton-proton interaction energy derived from high energy elastic scattering up to 30 GeV. Masses for an interval of radius 5 × 10 4 cm < r < 10 5 cm, are unstable, so that a generate star losing mass and approaching r of 5 × 10 4 cm suffers a partial collapse to half radius.
ISSN:0370-2693
1873-2445
DOI:10.1016/0370-2693(69)90470-5