Frequency Domain Binary Black Hole Gravitational Waveforms with Higher Multipoles

Document #:

LIGO-G1700815-v2

Document type:

G - Presentations (eg Graphics)

Abstract:

This talk discusses a general method for estimating contributions to gravitational-wave signals from non-precessing black hole binaries beyond the leading quadrupole order. The method is based on the stationary phase approximation, and it uses the Kerr quasi-normal mode spectrum and phenomenological observations in order to extend known relationships between gravitational multipoles. This method is applied to an existing leading quadrupole order frequency-domain waveform model tuned to Numerical Relativity (known as PhenomD) in order to yield a higher multipole inspiral-merger-ringdown gravitational-wave model. I analyze the performance of this model in terms of mismatches against numerical simulations of binary black hole mergers, and I illustrate examples of its use in parameter estimation.

Files in Document:

• Pannarale_Amaldi12_PhenomHM.pdf (file is not accessible)

Topics:

• Compact Binaries
• Modelling

Authors:

• Francesco Pannarale
• Lionel London
• Sebastian Khan
• Edward Fauchon-Jones
• Mark Hannam
• Sascha Husa
• Chinmay Kalaghatgi
• Francisco Forteza
• Frank Ohme

Associated with Events:

Amaldi 12 held on 09 Jul 2017 in Hilton Hotel, Pasadena, CA