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Published April 1, 1928 | public
Journal Article Open

On the equilibrium between radiation and matter in Einstein's closed universe

Abstract

In two preceding articles,(1) the principles of thermodynamics have been expressed in a form suitable for applications in general relativity, and then applied to Einstein's closed universe, employing a set of coordinates in which the line element assumes the form ds^2 = -R^2dX^2 - R^2 sin^2 X(dθ^2 + sin^2 θdp^2) + dt2.

Additional Information

Copyright © 1928 by the National Academy of Sciences. Communicated February 28, 1928.

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August 21, 2023
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