The comoving coordinate frame for differentially rotating, relativistic bodies.

Details The comoving coordinate frame for differentially rotating, relativistic bodies. The comoving coordinate frame for differentially rotating, relativistic bodies.

Apr 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976gregr...7..371a&link_type=abstract

General Relativity and Gravitation, Volume 7, Issue 4, pp.371-381

Physics

3

Scientific paper

A first-order, ordinary differential equation is derived that can in principle be integrated for any assumed rotation law Ω = Ω(r) within a relativistic, perfect-fluid body. The solution of this equation reduces the number of unknown metric functions appearing in the line element for the spacetime of such differentially rotating bodies to three. In the case of rigid rotation this is equivalent to a result of Harrison.

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