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Numerical studies on core collapse supernova in self-interacting massive scalar-tensor gravity

Patrick Chi-Kit CheongDepartment of Physics, The Chinese University of Hong Kong, Shatin, New Territories, Hong KongTjonnie G. F. LiDepartment of Physics, The Chinese University of Hong Kong, Shatin, New Territories, Hong Kong
2019en
ABI

Abstract

We investigate stellar core collapse in scalar-tensor theory with a massive self-interacting scalar field. In these theories, strong long-lived inverse chirp signals could be induced during the stellar core collapse, which provides us with several potential smoking-gun signatures that could be found using current ground-based detectors. We show that the existence of self-interaction in the potential of the scalar field can significantly suppress spontaneous scalarization and the amplitude of the monopole gravitational-wave radiation. Moreover, this suppression due to self-interaction is frequency dependent and may be discernible in LIGO/Virgo's sensitive band. Therefore, self-interaction should be considered when constraining scalar-tensor coupling parameters with gravitational-wave detections. Alternatively, if such monopole gravitational-wave signals are detected, then one may be able to infer the presence of self-interaction.

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