A precise response function for the magnetic component of Gravitational Waves in Scalar-Tensor Gravity
Christian Corda

TL;DR
This paper refines the response function for the magnetic component of gravitational waves in Scalar-Tensor Gravity, highlighting its significance at high frequencies and its potential to distinguish alternative theories from General Relativity.
Contribution
It provides a corrected, more precise response function for the magnetic component of GWs in Scalar-Tensor Gravity, emphasizing its importance in high-frequency detection and theory differentiation.
Findings
Corrected the magnetic response function in Scalar-Tensor Gravity.
Demonstrated the significance of magnetic components at high frequencies.
Showed the magnetic component's relevance in both GTR and alternative theories.
Abstract
The important issue of the magnetic component of gravitational waves (GWs) has been considered in various papers in the literature. From such analyses, it resulted that such a magnetic component becomes particularly important in the high frequency portion of the frequency range of ground based interferometers for GWs which arises from standard General Theory of Relativity (GTR). Recently, such a magnetic component has been extended to GWs arising from Scalar-Tensor Gravity (STG) too. After a review of some important issues on GWs in STG, in this paper we re-analyse the magnetic component in the framework of STG from a different point of view, by correcting an error in a previous paper and by releasing a more precise response function. In this way, we also show that if one neglects the magnetic contribution considering only the low-frequency approximation of the electric contribution, an…
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