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Inverse-Chirp Imprint of Gravitational Wave Signals in Scalar Tensor Theory

The scalar tensor theory contains a coupling function connecting the quantities in the Jordan and Einstein frames, which is constrained to guarantee a transformation rule between frames. We simulate the supernovae core collapse with different choices of coupling functions defined over the viable region of the parameter space and find that a generic inverse-chirp feature of the gravitational waves in the scalar tensor scenario.

preprint2020arXivOpen access
Chao-Qiang GengHao-Jui KuanLing-Wei Luo
astro-ph.COgr-qc
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Chao-Qiang GengHao-Jui KuanLing-Wei Luo

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