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Published August 15, 2023 | Published
Journal Article Open

Binary tree approach to template placement for searches for gravitational waves from compact binary mergers

Abstract

We demonstrate a new geometric method for fast template placement for searches for gravitational waves from the inspiral, merger and ringdown of compact binaries. The method is based on a binary tree decomposition of the template bank parameter space into nonoverlapping hypercubes. We use a numerical approximation of the signal overlap metric at the center of each hypercube to estimate the number of templates required to cover the hypercube and determine whether to further split the hypercube. As long as the expected number of templates in a given cube is greater than a given threshold, we split the cube along its longest edge according to the metric. When the expected number of templates in a given hypercube drops below this threshold, the splitting stops and a template is placed at the center of the hypercube. Using this method, we generate aligned-spin template banks covering the mass range suitable for a search of Advanced LIGO, Advanced Virgo and KAGRA data. The aligned-spin bank was generated in ∼24  hours using a single CPU core and produced 2 million templates. Our primary motivation for developing this algorithm is to produce a bank with useful geometric properties in the physical parameter space coordinates. Such properties are useful for population modeling and parameter estimation.

Copyright and License

© 2023 American Physical Society.

Acknowledgement

This research has made use of data, software and/or web tools obtained from the Gravitational Wave Open Science Center [37], a service of LIGO Laboratory, the LIGO Scientific Collaboration and the Virgo Collaboration. We especially made heavy use of the LVK Algorithm Library [38,39]. LIGO Laboratory and Advanced LIGO are funded by the United States National Science Foundation (NSF) as well as the Science and Technology Facilities Council (STFC) of the United Kingdom, the Max-Planck-Society (MPS), and the State of Niedersachsen/Germany for support of the construction of Advanced LIGO and construction and operation of the GEO600 detector. Additional support for Advanced LIGO was provided by the Australian Research Council. Virgo is funded, through the European Gravitational Observatory (EGO), by the French Centre National de Recherche Scientifique (CNRS), the Italian Istituto Nazionale di Fisica Nucleare (INFN) and the Dutch Nikhef, with contributions by institutions from Belgium, Germany, Greece, Hungary, Ireland, Japan, Monaco, Poland, Portugal, and Spain. This work was supported by National Science Foundation Awards No. OAC-1841480, No. PHY-2011865, and No. OAC-2103662. Computations for this research were performed on the Pennsylvania State University's Institute for Computational and Data Sciences gravitational-wave cluster, partially funded by OAC-2201445. C. H. acknowledges generous support from the Eberly College of Science, the Department of Physics, the Institute for Gravitation and the Cosmos, the Institute for Computational and Data Sciences, and the Freed Early Career Professorship.

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Additional details

Created:
October 16, 2023
Modified:
October 16, 2023