Gravitational wave radiation from compact binary systems in the Jordan-Brans-Dicke theory
- 27 January 1999
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review D
- Vol. 59 (4), 044027
- https://doi.org/10.1103/physrevd.59.044027
Abstract
In this paper we analyze the signal emitted by a compact binary system in the Jordan-Brans-Dicke theory. We compute the scalar and tensor components of the power radiated by the source and study the scalar wave form. Eventually we consider the detectability of the scalar component of the radiation by interferometers and resonant-mass detectors.Keywords
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This publication has 26 references indexed in Scilit:
- Gravitational-wave versus binary-pulsar tests of strong-field gravityPhysical Review D, 1998
- Spherical neutron star collapse toward a black hole in a tensor-scalar theory of gravityPhysical Review D, 1998
- Gravitational waves in Brans-Dicke theory: Analysis by test particles around a Kerr black holePhysical Review D, 1997
- Scalar gravitational wave from Oppenheimer-Snyder collapse in scalar-tensor theories of gravityPhysical Review D, 1997
- Testing theories of gravity with a spherical gravitational wave detectorClassical and Quantum Gravity, 1996
- Tensor-scalar gravity and binary-pulsar experimentsPhysical Review D, 1996
- Collapse to black holes in Brans-Dicke theory. II. Comparison with general relativityPhysical Review D, 1995
- Scalar-type gravitational wave emission from gravitational collapse in Brans-Dicke theory: Detectability by a laser interferometerPhysical Review D, 1994
- Binary pulsars and relativistic gravityReviews of Modern Physics, 1994
- Gravitational radiation, close binary systems, and the Brans-Dicke theory of gravityThe Astrophysical Journal, 1989