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Accurate inspiral-merger-ringdown gravitational waveforms for nonspinning black-hole binaries including the effect of subdominant modes

Mehta, Ajit Kumar and Mishra, Chandra Kant and Varma, Vijay and Ajith, Parameswaran (2017) Accurate inspiral-merger-ringdown gravitational waveforms for nonspinning black-hole binaries including the effect of subdominant modes. Physical Review D, 96 (12). Art. No. 124010. ISSN 2470-0010. http://resolver.caltech.edu/CaltechAUTHORS:20171212-102720355

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Abstract

We present an analytical waveform family describing gravitational waves (GWs) from the inspiral, merger, and ringdown of nonspinning black-hole binaries including the effect of several nonquadrupole modes [(ℓ = 2,m = ±1),(ℓ = 3,m = ±3),(ℓ = 4,m = ±4) apart from (ℓ = 2,m = ±2)]. We first construct spin-weighted spherical harmonics modes of hybrid waveforms by matching numerical-relativity simulations (with mass ratio 1–10) describing the late inspiral, merger, and ringdown of the binary with post-Newtonian/effective-one-body waveforms describing the early inspiral. An analytical waveform family is constructed in frequency domain by modeling the Fourier transform of the hybrid waveforms making use of analytical functions inspired by perturbative calculations. The resulting highly accurate, ready-to-use waveforms are highly faithful (unfaithfulness ≃10^(−4)–10^(−2)) for observation of GWs from nonspinning black-hole binaries and are extremely inexpensive to generate.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1103/PhysRevD.96.124010DOIArticle
https://journals.aps.org/prd/abstract/10.1103/PhysRevD.96.124010PublisherArticle
https://arxiv.org/abs/1708.03501arXivDiscussion Paper
Additional Information:© 2017 American Physical Society. Received 15 August 2017; published 11 December 2017. We are indebted to the SXS Collaboration for making a public catalog of numerical-relativity waveforms. We thank K. G. Arun, Bala Iyer, Sascha Husa, Mark Hannam, and Nathan Johnson-McDaniel for very useful discussions. P. A., A. K. M., and V. V. acknowledge support from the Indo-US Centre for the Exploration of Extreme Gravity funded by the Indo-US Science and Technology Forum (IUSSTF/JC-029/2016). In addition, P. A.’s research was supported by the AIRBUS Group Corporate Foundation through a chair in “Mathematics of Complex Systems” at the International Centre for Theoretical Sciences (ICTS), by a Ramanujan Fellowship from the Science and Engineering Research Board (SERB), India, by the SERB FastTrack fellowship SR/FTP/PS-191/2012, and by the Max Planck Society through a Max Planck Partner Group at ICTS. V. V.’s research was supported by NSF Grant No. PHY-1404569 to Caltech and the Sherman Fairchild Foundation. Computations were performed at the ICTS clusters Mowgli, Dogmatix, and Alice. This document has LIGO preprint number LIGO-P1700160-v3.
Group:LIGO
Funders:
Funding AgencyGrant Number
Indo-US Science and Technology ForumIUSSTF/JC-029
AIRBUS Group Corporate FoundationUNSPECIFIED
Science and Engineering Research Board (SERB)SR/FTP/PS-191/2012
Max Planck SocietyUNSPECIFIED
NSFPHY-1404569
Sherman Fairchild FoundationUNSPECIFIED
Other Numbering System:
Other Numbering System NameOther Numbering System ID
LIGO DocumentLIGO-P1700160
Record Number:CaltechAUTHORS:20171212-102720355
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20171212-102720355
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:83823
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:12 Dec 2017 21:41
Last Modified:12 Dec 2017 21:41

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