Obese neutron stars

K. Brecher, George J Caporaso

Research output: Contribution to journalArticlepeer-review

95 Scopus citations


WE show here that non-rotating, spherically symmetric, general relativistic 'neutron' stars of mass ≥ 3M̂ are consistent with the known laws of physics. In particular, for the 'bag' model of hadrons, we find M max ≃ 3M̂. The maximum mass for polytropic equations of state is found to be ≃5 M̂.

Original languageEnglish (US)
Pages (from-to)377-378
Number of pages2
Issue number5542
StatePublished - 1976
Externally publishedYes

ASJC Scopus subject areas

  • General


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