Observable effects of a scalar gravitational field in a binary pulsar

Details Observable effects of a scalar gravitational field in a binary pulsar Observable effects of a scalar gravitational field in a binary pulsar

Mar 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...196l..59e&link_type=abstract

Astrophysical Journal, vol. 196, Mar. 1, 1975, pt. 2, p. L59-L62.

Astronomy and Astrophysics

Astronomy

64

Binary Stars, Black Holes (Astronomy), Gravitational Waves, Neutron Stars, Pulsars, Stellar Gravitation, Astronomical Models, Gravitational Constant, Gravitational Fields, Relativistic Effects, Scalars

Scientific paper

It is remarked that the Dicke-Brans-Jordan theory of gravitation predicts dipole gravitational radiation from certain binary systems that contain a neutron star or black hole, causing decay of the orbit. Further, it predicts that the true rate of a pulsar clock should vary with distance from a binary companion (other than a black hole). At least one of these effects would be observable in PSR 1913+16.

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