Non-static cylindrically symmetric fields in general projective relativity

Details Non-static cylindrically symmetric fields in general projective relativity Non-static cylindrically symmetric fields in general projective relativity

Jan 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.163...41s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 163, no. 1, Jan. 1990, p. 41-48. Research supported by the Council of Scie

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Einstein Equations, Field Theory (Physics), Gravitation Theory, Relativity, Computational Astrophysics, Space-Time Functions, Universe

Scientific paper

Exact solutions are obtained for the vacuum field equations of Arcidiacono's (1986) General Projective Relativity (GPR) for the nonstatic Einstein-Rosen metric. Consideration is given to the vacuum field of GPR in a nonstatic cylindrically-symmetric space-time. Solutions for the case of GPR with n = 0 are obtained and used to get solutions of GPR with n not equal to 0. Specific emphasis is given to the singular behavior of the Riemann curvature invariant R and Kretschmann curvature invariant S.

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