Implications of Tachyon-Like Matter for Superdense Stars

Details Implications of Tachyon-Like Matter for Superdense Stars Implications of Tachyon-Like Matter for Superdense Stars

Jun 1972

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972phrvd...5.2936b&link_type=abstract

Physical Review D, vol. 5, Issue 12, pp. 2936-2938

Computer Science

Sound

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Scientific paper

A new equation of state of superdense matter is proposed. It is derivable by treating superdense matter as a perfect, degenerate tachyon gas. Yet the velocity of sound in the medium, 0<=β2<12, which this equation leads to, satisfies the inequality β. 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.

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