Phenomenological aspects of new gravitational forces. III. Slowly rotating astronomical bodies

Details Phenomenological aspects of new gravitational forces. III. Slowly rotating astronomical bodies Phenomenological aspects of new gravitational forces. III. Slowly rotating astronomical bodies

Dec 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987phrvd..36.3694n&link_type=abstract

Physical Review D (Particles and Fields), Volume 36, Issue 12, 15 December 1987, pp.3694-3699

Mathematics

Logic

7

Scientific paper

In this paper we expand the phenomenological quantum-gravity formalism developed previously and study the gravitational interaction of a slowly rotating body. We investigate in detail the β2 effects of (the massive) vector and scalar partners of the graviton, as well as those due to standard tensor gravity. An application to Eötvös experiments shows that the vector and scalar coupling constants would have to be unexpectedly large for β2 terms to account for postulated effects. We close with a short discussion on other possible applications.

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