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Catalog variance of testing general relativity with gravitational-wave data

Costantino Pacilio1,2,*, Davide Gerosa1,2,3, and Swetha Bhagwat3

  • 1Dipartimento di Fisica “G. Occhialini”, Universitá degli Studi di Milano-Bicocca, Piazza della Scienza 3, 20126 Milano, Italy
  • 2INFN, Sezione di Milano-Bicocca, Piazza della Scienza 3, 20126 Milano, Italy
  • 3School of Physics and Astronomy and Institute for Gravitational Wave Astronomy, University of Birmingham, Birmingham, B15 2TT, United Kingdom

  • *costantino.pacilio@unimib.it

Phys. Rev. D 109, L081302 – Published 29 April, 2024

DOI: https://doi.org/10.1103/PhysRevD.109.L081302

Abstract

Combining multiple gravitational-wave observations allows for stringent tests of general relativity, targeting effects that would otherwise be undetectable using single-event analyses. We highlight how the finite size of the observed catalog induces a significant source of variance. If not appropriately accounted for, general relativity can be excluded with arbitrarily large credibility even if it is the underlying theory of gravity. This effect is generic and holds for arbitrarily large catalogs. Moreover, we show that it cannot be suppressed by selecting “golden” observations with large signal-to-noise ratios. We present a mitigation strategy based on bootstrapping (i.e. resampling with repetition) that allows assigning uncertainties to one’s credibility on the targeted test. We demonstrate our findings using both toy models and real gravitational-wave data. In particular, we quantify the impact of the catalog variance on the ringdown properties of black holes using the latest LIGO/Virgo catalog.

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