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    First Constraints on Compact Binary Environments from LIGO-Virgo Data

    Giada Caneva Santoro1,*, Soumen Roy2,3,†, Rodrigo Vicente1,‡, Maria Haney2, Ornella Juliana Piccinni1, Walter Del Pozzo4, and Mario Martinez1,5

    • 1Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology, UAB Campus, E-08193 Barcelona, Spain
    • 2Nikhef, Science Park 105, 1098 XG Amsterdam, The Netherlands
    • 3Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, Princetonplein 1, 3584 CC Utrecht, The Netherlands
    • 4Dipartimento di Fisica “Enrico Fermi,” Università di Pisa and INFN Sezione di Pisa, Pisa I-56127, Italy
    • 5Catalan Institution for Research and Advanced Studies (ICREA), E-08010 Barcelona, Spain

    • *gcaneva@ifae.es
    • †soumen.roy@nikhef.nl
    • ‡rvicente@ifae.es

    Phys. Rev. Lett. 132, 251401 – Published 17 June, 2024

    DOI: https://doi.org/10.1103/PhysRevLett.132.251401

    Abstract

    The LIGO-Virgo analyses of signals from compact binary mergers observed so far have assumed isolated binary systems in a vacuum, neglecting the potential presence of astrophysical environments. We present here the first investigation of environmental effects on each of the events of GWTC-1 and two low-mass events from GWTC-2. We find no evidence for the presence of environmental effects. Most of the events decisively exclude the scenario of dynamical fragmentation of massive stars as their formation channel. GW170817 results in the most stringent upper bound on the medium density (≲21  g/cm3). We find that environmental effects can substantially bias the recovered parameters in the vacuum model, even when these effects are not detectable. We forecast that the Einstein Telescope and B-DECIGO will be able to probe the environmental effects of accretion disks and superradiant boson clouds on compact binaries.

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