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  Effective-one-body waveforms for binary neutron stars using surrogate models

Lackey, B., Bernuzzi, S., Galley, C. R., Meidam, J., & Broeck, C. V. D. (2017). Effective-one-body waveforms for binary neutron stars using surrogate models. Physical Review D, 95: 104036. doi:10.1103/PhysRevD.95.104036.

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Datensatz-Permalink: http://hdl.handle.net/11858/00-001M-0000-002D-AC95-E Versions-Permalink: http://hdl.handle.net/11858/00-001M-0000-002E-0816-8
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 Urheber:
Lackey, Benjamin1, Autor              
Bernuzzi, Sebastiano, Autor
Galley, Chad R., Autor
Meidam, Jeroen, Autor
Broeck, Chris Van Den, Autor
Affiliations:
1Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, escidoc:1933290              

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Schlagwörter: General Relativity and Quantum Cosmology, gr-qc
 Zusammenfassung: Gravitational-wave observations of binary neutron star systems can provide information about the masses, spins, and structure of neutron stars. However, this requires accurate and computationally efficient waveform models that take <1s to evaluate for use in Bayesian parameter estimation codes that perform 10^7 - 10^8 waveform evaluations. We present a surrogate model of a nonspinning effective-one-body waveform model with l = 2, 3, and 4 tidal multipole moments that reproduces waveforms of binary neutron star numerical simulations up to merger. The surrogate is built from compact sets of effective-one-body waveform amplitude and phase data that each form a reduced basis. We find that 12 amplitude and 7 phase basis elements are sufficient to reconstruct any binary neutron star waveform with a starting frequency of 10Hz. The surrogate has maximum errors of 3.8% in amplitude (0.04% excluding the last 100M before merger) and 0.043 radians in phase. The version implemented in the LIGO Algorithm Library takes ~0.07s to evaluate for a starting frequency of 30Hz and ~0.8s for a starting frequency of 10Hz, resulting in a speed-up factor of ~10^3 - 10^4 relative to the original Matlab code. This allows parameter estimation codes to run in days to weeks rather than years, and we demonstrate this with a Nested Sampling run that recovers the masses and tidal parameters of a simulated binary neutron star system.

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 Datum: 2016-10-152017
 Publikationsstatus: Im Druck publiziert
 Seiten: 17 pages, 11 figures, submitted to PRD
 Ort, Verlag, Ausgabe: -
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 Identifikatoren: arXiv: 1610.04742
DOI: 10.1103/PhysRevD.95.104036
URI: http://arxiv.org/abs/1610.04742
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Titel: Physical Review D
  Andere : Phys. Rev. D.
Genre der Quelle: Zeitschrift
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Ort, Verlag, Ausgabe: Lancaster, Pa. : American Physical Society
Seiten: - Band / Heft: 95 Artikelnummer: 104036 Start- / Endseite: - Identifikator: ISSN: 0556-2821
CoNE: http://pubman.mpdl.mpg.de/cone/journals/resource/111088197762258