Upper Bound on the Mass of Non-Rotating Neutron Stars

Details Upper Bound on the Mass of Non-Rotating Neutron Stars Upper Bound on the Mass of Non-Rotating Neutron Stars

Nov 1973

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973ap%26ss..25..117s&link_type=abstract

Astrophysics and Space Science, Volume 25, Issue 1, pp.117-131

Astronomy and Astrophysics

Astrophysics

20

Scientific paper

The problem of placing an upper bound on the mass of a non-rotating
neutron star is investigated under minimal assumptions on the equation
of state above nuclear densities. In particular causality (dp/dq<1)
is not assumed in this region. An upper bound of about five solar masses
is found.

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