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

Hanna, C., Kennington, J., Sakon, S., Privitera, S., Fernandez, M., Wang, J., et al. (2023). Binary tree approach to template placement for searches for gravitational waves from compact binary mergers. Physical Review D, 108(4): 042003. doi:10.1103/PhysRevD.108.042003.

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 Urheber:
Hanna, Chad, Autor
Kennington, James, Autor
Sakon, Shio, Autor
Privitera, Stephen1, Autor           
Fernandez, Miguel, Autor
Wang, Jonathan, Autor
Messick, Cody, Autor
Pace, Alex, Autor
Cannon, Kipp, Autor
Joshi, Prathamesh, Autor
Huxford, Rachael, Autor
Caudill, Sarah, Autor
Chan, Chiwai, Autor
Cousins, Bryce, Autor
Creighton, Jolien D. E., Autor
Ewing, Becca, Autor
Fong, Heather, Autor
Godwin, Patrick, Autor
Magee, Ryan, Autor
Meacher, Duncan, Autor
mehr..
Affiliations:
1Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_1933290              

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Schlagwörter: General Relativity and Quantum Cosmology, gr-qc, Astrophysics, Instrumentation and Methods for Astrophysics, astro-ph.IM
 Zusammenfassung: 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 non-overlapping 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 data. The aligned-spin bank required ~24
CPU-hours and produced 2 million templates. In general, we find that other
methods, namely stochastic placement, produces a more strictly bounded loss in
match between waveforms, with the same minimal match between waveforms
requiring about twice as many templates with our proposed algorithm. Though we
note that the average match is higher, which would lead to a higher detection
efficiency. Our primary motivation is not to strictly minimize the number of
templates with this algorithm, but rather to produce a bank with useful
geometric properties in the physical parameter space coordinates. Such
properties are useful for population modeling and parameter estimation.

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Sprache(n):
 Datum: 2022-09-222023
 Publikationsstatus: Erschienen
 Seiten: -
 Ort, Verlag, Ausgabe: -
 Inhaltsverzeichnis: -
 Art der Begutachtung: -
 Identifikatoren: arXiv: 2209.11298
DOI: 10.1103/PhysRevD.108.042003
 Art des Abschluß: -

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Titel: Physical Review D
  Andere : Phys. Rev. D.
Genre der Quelle: Zeitschrift
 Urheber:
Affiliations:
Ort, Verlag, Ausgabe: Lancaster, Pa. : American Physical Society
Seiten: - Band / Heft: 108 (4) Artikelnummer: 042003 Start- / Endseite: - Identifikator: ISSN: 0556-2821
CoNE: https://pure.mpg.de/cone/journals/resource/111088197762258