Reality Check
Penultimate Amazing
How science works includes that scientists test science!
Observation of Gravitational Waves from a Binary Black Hole Merger was published on 11 February 2016 and had a 5.1 sigma signal. The data is available and presumably scientists have been analyzing the data to see whether the signal is really that good. A year and a half later we have one pre-print from a group casting doubts on the signal.
On the time lags of the LIGO signals by Creswell,von Hausegger, Jackson, Liu, Naselsky. In short they find a correlation in the noise in the 2 detectors that matches the time lag between the signals.
Described at Was It All Just Noise? Independent Analysis Casts Doubt On LIGO's Detections where a possible flaw is that they use methods based on tutorials from the LIGO website, not the higher quality methods used by LIGO in their papers.
A Response to “On the time lags of the LIGO signals” by a member of the LIGO collaboration
ETA: The above blog article points out something that I did not know
Observation of Gravitational Waves from a Binary Black Hole Merger was published on 11 February 2016 and had a 5.1 sigma signal. The data is available and presumably scientists have been analyzing the data to see whether the signal is really that good. A year and a half later we have one pre-print from a group casting doubts on the signal.
On the time lags of the LIGO signals by Creswell,von Hausegger, Jackson, Liu, Naselsky. In short they find a correlation in the noise in the 2 detectors that matches the time lag between the signals.
Described at Was It All Just Noise? Independent Analysis Casts Doubt On LIGO's Detections where a possible flaw is that they use methods based on tutorials from the LIGO website, not the higher quality methods used by LIGO in their papers.
A Response to “On the time lags of the LIGO signals” by a member of the LIGO collaboration
There are a number of reasons why this conclusion is incorrect: 1. The frequency-domain correlations they are seeing arise from the way they do their FFT on the filtered data. We have managed to demonstrate the same effect with simulated Gaussian noise. 2. LIGO analyses use whitened data when searching for compact binary mergers such as GW150914. When repeating the analysis of Creswell et al. on whitened data these effects are completely absent. 3. Our 5-sigma significance comes from a procedure of repeatedly time-shifting the data, which is not invalidated if correlations of the type described in Creswell et al. are present.
ETA: The above blog article points out something that I did not know
This analysis rules out signals not travelling at the speed of light, anything else is some noise transient.We first look through all our data to look for loud events within the 10ms time-window corresponding to the light travel time between the two observatories. Then we look again. Except the second time we look we shift ALL of the data from Livingston by 0.1s. This delay is much larger than the light travel time so if we see any interesting “events” now they cannot be genuine astrophysical events, but must be some noise transient. We then repeat this process with a 0.2s delay, 0.3s delay and so on up to time delays on the order of weeks long. In this way we’ve conducted of order 10 million experiments. For the case of GW150914 the signal in the non-time shifted data was louder than any event we saw in any of the time-shifted runs—all 10 million of them.
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