ujjwal3097
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yes! you are right because there is no info about the video. Site just says if you want to set the reminder.e.bar.goum said:It's not clear, but I think so.
yes! you are right because there is no info about the video. Site just says if you want to set the reminder.e.bar.goum said:It's not clear, but I think so.
Daz said:Not long to go now... Here's a link to the youtube live feed:
Note the unit of strain on the y-axis. That is an incredibly small number. To detect that is truly amazing.bcrowell said:Here's the signal:
On September 14, 2015 at 09:50:45 UTC the two detectors of the Laser Interferometer Gravitational-Wave Observatory simultaneously observed a transient gravitational-wave signal. The signal sweeps upwards in frequency from 35 to 250 Hz with a peak gravitational-wave strain of 1.0×10−21. It matches the waveform predicted by general relativity for the inspiral and merger of a pair of black holes and the ringdown of the resulting single black hole. The signal was observed with a matched-filter signal-to-noise ratio of 24 and a false alarm rate estimated to be less than 1 event per 203 000 years, equivalent to a significance greater than 5.1σ. The source lies at a luminosity distance of 410+160−180Mpc corresponding to a redshift z=0.09+0.03−0.04. In the source frame, the initial black hole masses are 36+5−4M⊙ and 29+4−4M⊙, and the final black hole mass is 62+4−4M⊙, with 3.0+0.5−0.5M⊙c2 radiated in gravitational waves. All uncertainties define 90% credible intervals. These observations demonstrate the existence of binary stellar-mass black hole systems. This is the first direct detection of gravitational waves and the first observation of a binary black hole merger.
Could the majority of the traffic be due to this gravitational wave discovery?bcrowell said:Right now the PRL website appears to be overloaded and not responding
In the CERN seminar this was explained in more detail. They ran for 16 days (of coincidence time between the two detectors) and used this background data to estimate how often stronger signals occur. Their estimate is less than once in ~200.000 years (forgot the second digit). Compare that to 16 days of running time...bcrowell said:It's surprising that the signal from the best event is so clearly visible on a time-domain graph, if, as rumored, it was only 5 sigma over all.
websterling said:
mfb said:In the CERN seminar this was explained in more detail. They ran for 16 days (of coincidence time between the two detectors) and used this background data to estimate how often stronger signals occur. Their estimate is less than once in ~200.000 years (forgot the second digit). Compare that to 16 days of running time...
mjs said:Great news-big day for science!
I know its still early, but can someone say which theories are hurt, (and which ones are favored) the most by these new findings?
There is a class of quantum gravity approaches (based on a variant way of handling spin 2 quantization, put forward by a few Russian physicists), that had a specific prediction (yeah!) that collapse would stop signficantly before horizon formation (as I recall, close to the photon sphere of classical GR). Presumably this result (along with increasing reliability of horizon / mass observations) completely kills this approach (the downside of a specific prediction). It probably kills most any approache that suggests the QG effects diverge from classical GR outside the horizon.phyzguy said:Simple answer is that Einsteinian GR seems to describe the event to near perfection. The paper from LIGO says, "The agreement between the reconstructed waveforms using the two models is found to 94(+2;-3) %". This is the most stringent test yet of GR in the strong gravity regime. I'm not sure if this kills some alternatives to GR, but I think it will disfavor some of them.
JorisL said:I really enjoyed Rainer Weiss' explanation, let's hope the press has been paying attention.