NASA NTRS · 19760017020
The relativistic equations of stellar structure and evolution
Abstract
The general relativistic equations of stellar structure and evolution are reformulated in a notation which makes easy contact with Newtonian theory. A general relativistic version of the mixing-length formalism for convection is presented. It is argued that in work on spherical systems, general relativity theorists have identified the wrong quantity as total mass-energy inside radius r.
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Thorne, K. S.. 1975-01-01. The relativistic equations of stellar structure and evolution. https://ntrs.nasa.gov/citations/19760017020
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