Journal
PHYSICAL REVIEW D
Volume 99, Issue 12, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.99.124050
Keywords
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Funding
- International Postdoctoral Exchange Fellowship Program at Central China Normal University
- China Postdoctoral Science Foundation [2018M632895]
- European Union [MaGRaTh-646597]
- H2020-MSCA-RISE-2015 [StronGrHEP690904]
- COST Action CANTATA [CA-15117]
- INFN (iniziativa specifica QGSKY)
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We discuss the scalar mode of gravitational waves emerging in the context of F(R) gravity by taking into account the chameleon mechanism. Assuming a toy model with a specific matter distribution to reproduce the environment of detection experiment by a ground-based gravitational wave observatory, we find that the chameleon mechanism remarkably suppresses the scalar wave in the atmosphere of Earth, compared with the tensor modes of the gravitational waves. We also discuss the possibility to detect and constrain scalar waves by the current gravitational observatories and advocate a necessity of the future space-based observations.
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