Erratum: Tests of General Relativity with GW150914 [Phys. Rev. Lett. 116 , 221101 (2016)]

Abstract

This Erratum reports an error found in the implementation of the code of the LIGO Scientific and Virgo Collaborations (LVC) as used in gravitational-wave-based estimations of possible deviations from the post-Newtonian (PN) terms expected in general relativity (GR).The error concerned the 0.5 PN term and affected the results previously published for GW150914 [1] in Ref. [2], for GW151226 [3] in Ref. [4], and for GW170104 in Ref. [5].We corrected the bug and present the reproduced results in this Erratum, as well as in the related Errata [6,7].The main conclusion, that the results are consistent with general relativity, remains.In Ref.[2], the test for the parameterized post-Newtonian [8] deviations from the expected GR values relied on creating non-GR waveforms [9-13] and using them as potential matches for the observed waveforms [14][15][16][17].In these waveforms, implemented in the frequency domain, freedom was introduced by allowing the phase coefficients describing different powers of the post-Newtonian parameter (equivalently, powers of the frequency) to assume a range of values, not only the particular values prescribed by GR.However, a coding bug was introduced, identically zeroing the deviations at 0.5 PN in the inspiral regime (as in GR).The 0.5 PN deviations were hence absent in the phasing formula, though not in the junction conditions that relate the inspiral regime to the intermediate regime.Any constraints obtained in [2,4,5] only resulted from the latter.This error affected the results of the non-GR parameter estimation (PE) [14] pipeline tests performed for finding bounds on possible PN deviations from GR.In particular, they affect the bounds on the single deviations in the 0.5 PN term and on the tests with multiple deviations together.These erroneous results appeared in Figs. 6 and 7 and Table I of [2], in Figs.7 and 8 of [4], and in Fig. 9 of the Supplemental Material of [5].The corrected versions of all of these have been produced.The corrections for Figs.6 and 7 and Table I of [2] appear below, while the others are available in [6,7].All these results are consistent with GR.The error, introduced by erroneous caching during the optimization of the waveform generation for efficient PE, has been corrected in commit [18] of the LALSuite [19] code.No subsequent LVC papers have been affected.FIG. 1.This is the corrected Fig. 6 of [2], comparing the 90% upper bounds on PN parameter deviations from GR obtained from the double pulsar PSR J0737 -3039 [22,23] to those obtained from the first gravitational wave GW150914.