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Ellipsoidal figures of equilibrium

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254
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~4h 14min
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English
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Published 1969 Dover 5 views
ISBN
0300011164
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About Author

Subrahmanyan Chandrasekhar

Subrahmanyan Chandrasekhar (19 October 1910 – 21 August 1995) was an Indian-American theoretical physicist. He shared the 1983 Nobel Prize in Physics "for his theoretical studies of the physical processes of importance to the structure and evolution of the stars." His mathematical treatment of stellar evolution yielded many of the current theoretical models of the later evolutionary stages of massive stars. The Chandrasekhar limit describes the maximum mass of a white dwarf (1.44 solar masses). Above it, a stellar remnant will collapse to form a neutron star or black hole. Many concepts, institutions and inventions, including the Chandra X-Ray Observatory, are named after him.

Description

Classical investigations on the ellipsoidal figures of equilibrium of liquid masses are here enlarged by Chandrasekhar into a complete theory. The author develops and completes the basic ideas put forth in three fundamental papers by Dirichlet, Dedekind, and Riemann over a century ago, which have been all but ignored since that time. The various problems are solved by a method and a technique that are essentially elementary, and a number of common misconceptions and errors are corrected. After a historical introduction, the author goes on to discuss virial equations of the various orders and to describe his new method; potentials of homogeneous and heterogeneous ellipsoids (including theorems on a class of heterogeneous ellipsoids which enable the treatment of the subject without explicit use of ellipsoidal harmonics); Dirichlet's problem and Dedekind's theorem; Maclaurin spheroids; Jacobi and Dedekind ellipsoid; Riemann ellipsoids; Roche ellipsoids (Including Darwin ellipsoids).

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