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Title: Observational prospects of self-interacting scalar superradiance with next-generation gravitational-wave detectors

Journal Article · · Classical and Quantum Gravity

Abstract Current- and next-generation gravitational-wave observatories may reveal new, ultralight bosons. Through the superradiance process, these theoretical particle candidates can form clouds around astrophysical black holes and result in detectable gravitational-wave radiation. In the absence of detections, constraints—contingent on astrophysical assumptions—have been derived using LIGO-Virgo-KAGRA data on boson masses. However, the searches for ultralight scalars to date have not adequately considered self-interactions between particles. Self-interactions that significantly alter superradiance dynamics are generically present for many scalar models, including axion-like dark matter candidates and string axions. We implement the most complete treatment of particle self-interactions available to determine the gravitational-wave signatures expected from superradiant scalar clouds and revisit the constraints obtained in a past gravitational-wave search targeting the black hole in Cygnus X-1. We also project the reach of next-generation gravitational-wave observatories to scalar particle parameter space in the mass-coupling plane. We find that while proposed observatories have insufficient reach to self-interactions that can halt black hole spin-down, next-generation observatories are essential for expanding the search beyond gravitational parameter space and can reach a mass and interaction scale of 10 13 –10 −12 eV / c 2 and 10 17 GeV, respectively.

Sponsoring Organization:
USDOE
Grant/Contract Number:
SC0024375
OSTI ID:
2482570
Journal Information:
Classical and Quantum Gravity, Journal Name: Classical and Quantum Gravity Journal Issue: 2 Vol. 42; ISSN 0264-9381
Publisher:
IOP PublishingCopyright Statement
Country of Publication:
United Kingdom
Language:
English

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