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arxiv: 1204.4340 · v2 · pith:4RYZ7XNYnew · submitted 2012-04-19 · 🌀 gr-qc · astro-ph.HE· hep-ph· hep-th

Light scalar field constraints from gravitational-wave observations of compact binaries

Emanuele Berti , Leonardo Gualtieri , Michael Horbatsch , Justin Alsing This is my paper
classification 🌀 gr-qc astro-ph.HEhep-phhep-th
keywords observationsomegaboundscombinationgravitational-wavelightscalarsqrt
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Scalar-tensor theories are among the simplest extensions of general relativity. In theories with light scalars, deviations from Einstein's theory of gravity are determined by the scalar mass m_s and by a Brans-Dicke-like coupling parameter \omega_{BD}. We show that gravitational-wave observations of nonspinning neutron star-black hole binary inspirals can be used to set lower bounds on \omega_{BD} and upper bounds on the combination m_s/\sqrt{\omega_{BD}}$. We estimate via a Fisher matrix analysis that individual observations with signal-to-noise ratio \rho would yield (m_s/\sqrt{\omega_{BD}})(\rho/10)<10^{-15}, 10^{-16} and 10^{-19} eV for Advanced LIGO, ET and eLISA, respectively. A statistical combination of multiple observations may further improve these bounds.

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