A Static Theory of the Stability of the Equilibrium

Details A Static Theory of the Stability of the Equilibrium A Static Theory of the Stability of the Equilibrium

Jan 1971

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1971ap%26ss..10..165c&link_type=abstract

Astrophysics and Space Science, Volume 10, Issue 1, pp.165-177

Astronomy and Astrophysics

Astrophysics

Scientific paper

A static relativistic theory of the stability of the equilibrium of an isentropic spherically-symmetric star is deduced from the properties of a functionu which is solution of a second-order differential equation, and which is related to the model by means of the formulau = ∂m(v, ϱc)/∂ϱc, wherem is the mass-energy inside the coordinate volumev and ϱc is the central mass-energy density.

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