Physics
Scientific paper
Sep 1978
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978gregr...9..801v&link_type=abstract
General Relativity and Gravitation, vol. 9, Sept. 1978, p. 801-807.
Physics
5
Astronomical Models, Einstein Equations, Space-Time Functions, Universe, Eigenvectors, Field Theory (Physics), Homogeneity, Isotropic Media, Mathematical Models
Scientific paper
The metric for the standard static Einstein model of the universe can be expressed in coordinates for which a congruence of spacelike world lines of the model will be twisting. A method of 'shifting the twist' has been devised by which the twist on spacelike world lines is shifted onto the timelike world lines. The model universe then becomes Goedel's model. A combined Einstein-Goedel model containing a parameter epsilon is obtained. Switching epsilon from +1 to -1 will effect the shift of twist in the world lines and lead from the Einstein model to the Goedel model.
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