On the mass of rotating stars in Newtonian gravity and GR
classification
🌀 gr-qc
astro-ph.HE
keywords
newtonianmassoriginalrotatingalbeitappearsapproachcalculation
read the original abstract
We show how the correction to the calculation of the mass in the original relativistic model of a rotating star by Hartle [6], found recently [10], appears in the Newtonian limit, and that the correcting term is indeed present, albeit hidden, in the original Newtonian approach by Chandrasekhar [2].
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.