Journal
PHYSICAL REVIEW D
Volume 106, Issue 4, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.106.043009
Keywords
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Funding
- United States National Science Foundation (NSF)
- Science and Technology Facilities Council (STFC) of the United Kingdom
- Max-Planck-Society (MPS)
- State of Niedersachsen/Germany
- Australian Research Council
- European Gravitational Observatory (EGO)
- French Centre National de Recherche Scientifique (CNRS)
- Italian Istituto Nazionale di Fisica Nucleare (INFN)
- Dutch Nikhef
- NSF [DGE-2039656]
- National Science Foundation [2012086]
- Simons Foundation [216179]
- Center for New Scientists at the Weizmann Institute of Science
- Ruth and Herman Albert Scholarship Program for New Scientists
- Canadian Institute for Advanced Research (CIFAR) program on Gravity and the Extreme Universe
- Simons Foundation Modern Inflationary Cosmology initiative
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In this study, we report the detection of ten new binary black hole mergers using data from the third observing run of advanced LIGO and advanced Virgo. Some of these events reveal interesting astrophysical scenarios and provide insights into the parameter space of black hole mergers.
We report the detection of ten new binary black hole (BBH) mergers in the publicly released data from the first half of the third observing run (O3a) of advanced LIGO and advanced Virgo. We identify candidates using an updated version of the search pipeline described in Venumadhav et al. [Phys. Rev. D 100, 023011 (2019)] (the IAS pipeline [T. Venumadhav et al., Phys. Rev. D 101, 083030 (2020).]) and compile a catalog of signals that pass a significance threshold of astrophysical probability greater than 0.5 (following the GWTC-2.1 [R. Abbott et al. (The LIGO Scientific Collaboration, the Virgo Collaboration), arXiv: 2108.01045.] and 3-OGC [A. H. Nitz et al., Astrophys. J. 922, 76 (2021).] catalogs). The updated IAS pipeline is sensitive to a larger region of parameter space, applies a template prior that accounts for different search volume as a function of intrinsic parameters, and uses an improved coherent detection statistic that optimally combines the data from the Hanford and Livingston detectors. Among the ten new events, we observe interesting astrophysical scenarios including sources with confidently large effective spin parameters in both the positive and negative directions, high-mass black holes that are difficult to form in stellar collapse models due to (pulsational) pair instability, and low-mass mergers that bridge the gap between neutron stars and the lightest observed black holes. We infer source parameters in the upper and lower black hole mass gaps with both extreme and near-unity mass ratios, and one of the possible neutron star-black hole (NSBH) mergers is well localized for electromagnetic (EM) counterpart searches. We detect all of the GWTC-2.1 BBH mergers with coincident data in Hanford and Livingston except for three loud events that get vetoed, which is compatible with the false-positive rate of our veto procedure, and three that fall below the detection threshold. We also return to significance the event GW190909_114149, which was reduced to a subthreshold trigger after its initial appearance in GWTC-2 [R. Abbott et al., Phys. Rev. X 11, 021053 (2021).]. This amounts to a total of 42 BBH mergers detected by our pipeline's search of the coincident Hanford-Livingston O3a data.
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