Published April 1, 1928
| public
Journal Article
Open
On the equilibrium between radiation and matter in Einstein's closed universe
- Creators
- Tolman, Richard C.
Chicago
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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.Files
TOlpnas28c.pdf
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Additional details
- Eprint ID
- 4369
- Resolver ID
- CaltechAUTHORS:TOLpnas28c
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2006-08-21Created from EPrint's datestamp field
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2019-10-02Created from EPrint's last_modified field