Dingle, Herbert (1933) Values of Tvµ and the Christoffel symbols for a line element of considerable generality. Proceedings of the National Academy of Sciences of the United States of America, 19 (5). pp. 559-563. ISSN 0027-8424. http://resolver.caltech.edu/CaltechAUTHORS:DINpnas33
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In the general theory of relativity the mechanical properties of any region of the universe are expressed by the energy-momentum tensor, Tvµ, which is itself calculable from the form of the line element, ds2 = gµvdxµdx4, applicable to that region. The expressions for Tvµ in the most general case, in which all the gµv are arbitrary functions of the four coordinates, x1, x2, x3, x4, are exceedingly complicated, but considerable simplification is introduced if it is assumed that gµv(µ ≠ v) = 0.
|Additional Information:||© 1933 by the National Academy of Sciences. Communicated March 20, 1933.|
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|Deposited By:||Tony Diaz|
|Deposited On:||14 Feb 2007|
|Last Modified:||14 Nov 2014 19:19|
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