Gravitational Wave Radiation from Compact Binary Systems in the Jordan-Brans-Dicke Theory
M. Brunetti, E. Coccia, V. Fafone, F. Fucito
TL;DR
This paper investigates gravitational wave emissions from compact binary systems within the Jordan-Brans-Dicke theory, focusing on scalar and tensor radiation components and their detectability by current gravitational wave detectors.
Contribution
It provides a detailed analysis of scalar and tensor gravitational wave components in Jordan-Brans-Dicke theory and assesses their potential detectability.
Findings
Scalar radiation component is significant in Jordan-Brans-Dicke theory.
Tensor component aligns with predictions of general relativity.
Detectability of scalar waves depends on detector sensitivity.
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 waveform. Eventually we consider the detectability of the scalar component of the radiation by interferometers and resonant-mass detectors.
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