Measuring properties of primordial black hole mergers at cosmological distances: Effect of higher order modes in gravitational waves

نویسندگان

چکیده

Primordial black holes (PBHs) may form from the collapse of matter overdensities shortly after big bang. One identify their existence by observing gravitational wave (GW) emissions merging PBH binaries at high redshifts $z\ensuremath{\gtrsim}30$, where astrophysical binary (BBHs) are unlikely to merge. The next-generation ground-based GW detectors, Cosmic Explorer and Einstein Telescope, will be able observe BBHs with total masses $\mathcal{O}(10\ensuremath{-}100){M}_{\ensuremath{\bigodot}}$ such redshifts. This paper serves as a companion Ng et al. [Astrophys. J. Lett. 931, L12 (2022)], focusing on effect higher-order modes (HoMs) in waveform modeling, which detectable for these redshift BBHs, estimation source parameters. We perform Bayesian parameter obtain measurement uncertainties without HoM modeling sources different masses, mass ratios, orbital inclinations observed network detectors. show that including HoMs model reduces up factor two, depending exact then discuss implications identifying PBHs improved single-event measurements, expand investigation dependence relative abundance between BBH mergers originating first stars primordial shown (2022)].

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ژورنال

عنوان ژورنال: Physical review

سال: 2023

ISSN: ['0556-2813', '1538-4497', '1089-490X']

DOI: https://doi.org/10.1103/physrevd.107.024041