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Inverse-Chirp Imprint of Gravitational Wave Signals in Scalar Tensor Theory
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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.
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Cited by 2 Pith papers
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Rapidly Rotating Neutron Star Collapse in Massive Scalar-Tensor Theories
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Axisymmetric stability of neutron stars as extreme rotators in massive scalar-tensor theory
Differentially rotating scalarized neutron stars with enormous angular momentum are axisymmetrically stable up to the turning point of their mass sequence, beyond which they collapse to black holes, confirming the tur...
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