Integrating Einstein Field Equations in Observational Coordinates with Cosmological Data Functions: Nonflat Friedmann-Lemaître-Robertson-Walker Cases

Details Integrating Einstein Field Equations in Observational Coordinates with Cosmological Data Functions: Nonflat Friedmann-Lemaître-Robertson-Walker Cases Integrating Einstein Field Equations in Observational Coordinates with Cosmological Data Functions: Nonflat Friedmann-Lemaître-Robertson-Walker Cases

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001apj...549..716a&link_type=abstract

The Astrophysical Journal, Volume 549, Issue 2, pp. 716-720.

Astronomy and Astrophysics

Astronomy

12

Cosmology: Theory, Relativity

Scientific paper

In this paper we use the integration scheme for the exact spherically symmetric Einstein field equations in observational coordinates recently developed by Araújo and Stoeger, and input data functions for area distance and galaxy number counts that would be obtained if the universe were exactly represented by nonflat Friedmann-Lemaître-Robertson-Walker models.

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