Tolman, Richard C. (1930) On the estimation of distances in a curved universe with a non-static line element. Proceedings of the National Academy of Sciences of the United States of America, 16 (7). pp. 511-520. ISSN 0027-8424. http://resolver.caltech.edu/CaltechAUTHORS:TOLpnas30b
See Usage Policy.
Use this Persistent URL to link to this item: http://resolver.caltech.edu/CaltechAUTHORS:TOLpnas30b
Introduction. - In two previous articles,(1,2) I have shown that there is a possibility of relating the annihilation of matter in the universe to the observed red shift in the light from the extra-galactic nebulae, by ascribing to the universe a line element of the general form ds^2 = - e^g(t)/[1 + r2/4R^2]^2 * (dx^2 + dy^2 + dz^2) + dt^2, where r is an abbreviation for √(x^2+y^2+z^2) and R is a constant.
|Additional Information:||Copyright © 1930 by the National Academy of Sciences. Communicated June 14, 1930.|
|Usage Policy:||No commercial reproduction, distribution, display or performance rights in this work are provided.|
|Deposited By:||Tony Diaz|
|Deposited On:||21 Aug 2006|
|Last Modified:||26 Dec 2012 08:59|
Repository Staff Only: item control page