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2014

A Time Domain Waveform for Testing General Relativity

Huwyler, Cédric, Porter, Edward K., Jetzer, Philippe

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Gravitational-wave parameter estimation is only as good as the theory the waveform generation models are based upon.

It is therefore crucial to test General Relativity (GR) once data becomes available.
Many previous works, such as studies connected with the ppE framework by Yunes and Pretorius, rely on the stationary phase approximation (SPA) to model deviations from GR in the frequency domain.
As Fast Fourier Transform algorithms have become considerably faster and in order to circumvent possible problems with the SPA, we test GR with corrected time domain waveforms instead of SPA waveforms.

A Time Domain Waveform for Testing General Relativity · Around

Built on

Damour T, Iyer B R and Sathyprakash B S 2000 Phys. Rev. D
2000
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Arun K G, Iyer B R, Qusailah M S S and Sathyprakash B S 2006 Phys. Rev. D
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Pan Y, Buonanno A, Baker J G, Centrella J, Kelly B J, McWilliams S T, Pretorius F and van Meter J R 2008 Phys. Rev. D
2008
Earlier work this paper cites.
Yunes N and Pretorius F 2009 Phys. Rev. D
2009
Earlier work this paper cites.

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Cornish N, Sampson L, Yunes N and Pretorius F 2011 Phys. Rev. D
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Sampson L, Yunes N and Cornish N 2013 Phys. Rev. D
2013
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Sampson L, Cornish N and Yunes N Phys. Rev. D
Cited in the paper.

Then

Blanchet L 2014 Living Reviews in Relativity
2014
Closest in time.
Lang R N 2014 Phys. Rev. D
2014
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Huwyler C, Porter E and Jetzer P 2014 in preparation
2014
Closest in time.

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