Theories of Gravity with Structure-Dependent γ's

Details Theories of Gravity with Structure-Dependent γ's Theories of Gravity with Structure-Dependent γ's

Nov 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975phrvl..35.1188c&link_type=abstract

Physical Review Letters, Volume 35, Issue 18, November 3, 1975, pp.1188-1189

Physics

4

Scientific paper

A gauge theory for the Lorentz connection of a space-time describes geometries of stars with variable parametrized post-Newtonian parameter γ its value depends explicitly on the structure of a star: The value of γ for a neutron star is different from that for the solar system (|γsolar-1|<=10-2). Because of the absence of a "local parity invariance" γ is positive for ordinary stars and γ is negative for sources of gravity consisting of antimatter.

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