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Detecting Scalar Fields with Extreme Mass Ratio Inspirals

Maselli, Andrea; Franchini, Nicola; Gualtieri, Leonardo; Sotiriou, Thomas P.

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Authors

Andrea Maselli

Nicola Franchini

Leonardo Gualtieri

THOMAS SOTIRIOU Thomas.Sotiriou@nottingham.ac.uk
Professor of Gravitational Physics



Contributors

Abstract

We study extreme mass ratio inspirals (EMRIs), during which a small body spirals into a supermassive black hole, in gravity theories with additional scalar fields. We first argue that no-hair theorems and the properties of known theories that manage to circumvent them introduce a drastic simplification to the problem: The effects of the scalar on supermassive black holes, if any, are mostly negligible for EMRIs in vast classes of theories. We then exploit this simplification to model the inspiral perturbatively and we demonstrate that the scalar charge of the small body leaves a significant imprint on gravitational wave emission. Although much higher precision is needed for waveform modeling, our results strongly suggest that this imprint is observable with Laser Interferometer Space Antenna, rendering EMRIs promising probes of scalar fields.

Citation

Maselli, A., Franchini, N., Gualtieri, L., & Sotiriou, T. P. (2020). Detecting Scalar Fields with Extreme Mass Ratio Inspirals. Physical Review Letters, 125(14), Article 141101. https://doi.org/10.1103/PhysRevLett.125.141101

Journal Article Type Article
Acceptance Date Aug 31, 2020
Online Publication Date Sep 30, 2020
Publication Date Sep 30, 2020
Deposit Date Oct 1, 2020
Publicly Available Date Oct 5, 2020
Journal Physical Review Letters
Print ISSN 0031-9007
Electronic ISSN 1079-7114
Publisher American Physical Society
Peer Reviewed Peer Reviewed
Volume 125
Issue 14
Article Number 141101
DOI https://doi.org/10.1103/PhysRevLett.125.141101
Keywords General Physics and Astronomy
Public URL https://nottingham-repository.worktribe.com/output/4935369
Publisher URL https://journals.aps.org/prl/abstract/10.1103/PhysRevLett.125.141101

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