# Gravitational radiation from binary systems in $f(R)$ gravity: A semi-classical approach

@inproceedings{Narang2022GravitationalRF, title={Gravitational radiation from binary systems in \$f(R)\$ gravity: A semi-classical approach}, author={Ashish Narang and Subhendra Mohanty and Soumya Jana}, year={2022} }

. The rate of energy loss and orbital period decay of quasi- stable compact binary systems are derived in f ( R ) theory of gravity using the method of a single vertex graviton emission process from a classical source. After linearising the f ( R ) action written in an equivalent scalar-tensor format in the Einstein frame, we identify the appropriate interaction terms between the massless spin-2 tensor mode, massive scalar mode, and the energy momentum tensor. The deﬁnition of the scalar ﬁeld…

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