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Title:
Observable effects of a scalar gravitational field in a binary pulsar
Authors:
Eardley, D. M.
Affiliation:
AA(Yale University, New Haven, Conn.)
Publication:
Astrophysical Journal, vol. 196, Mar. 1, 1975, pt. 2, p. L59-L62. (ApJL Homepage)
Publication Date:
03/1975
Category:
Astrophysics
Origin:
STI
NASA/STI Keywords:
Binary Stars, Black Holes (Astronomy), Gravitational Waves, Neutron Stars, Pulsars, Stellar Gravitation, Astronomical Models, Gravitational Constant, Gravitational Fields, Relativistic Effects, Scalars
DOI:
10.1086/181744
Bibliographic Code:
1975ApJ...196L..59E

Abstract

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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