DaleSpam said:
I agree. After looking at the paper it is clear that this cannot be explained simply by photon mass, but that still leaves a lot of possibilities:
1) tachyonic neutrinos (not likely due to stellar observations)
2) SR violation (not likely due to large number of more sensitive experiments)
3) Experimental error (most likely, but would have to be subtle)
4) Change to standard model (somewhat likely, this is the primary purpose of doing particle physics after all)
#4 is impossible. There is no way that a change to the SM of particle physics will let you have a neutrino interaction 60 ns before it arrives. (Or, alternatively, have it begin to travel 60 ns before it's produced. Or some combination)
xts said:
I may agree only partially. They do not measure intervals. They measure space-time co-ordinates of production point (using CERN ref. frame) and space-time co-ordinates of detection (using Gran-Sasso frame). In order to calculate interval they must transform those results to common frame. There are lots of possible errors to be made in this process, especially that neither of lab frames is inertial.
The way you would like to do this is have the light and the neutrinos start together and go through the same path. Of course that's impossible. So instead what you do is you set up a triangle, with light (well, radio) emerging from one point and being detected at the source and destination points. If you work this out, you will discover that the interval between the source and destination is independent of their relative motion.
SR/GR effects only matter in this problem if you have the radio pulse, wait (using local clocks to measure how much time elapses) and then do the experiment. The drift between a clock at CERN and one at LNGS is probably around 20-30 ns per day. But anyone who has used a GPS navigator knows that it syncs much more often than this - a few seconds at most. So these effects are completely zeroed out by the way the measurement is constructed.
xts said:
They use wavelenghtshifter fibres to collect light from scintillating plates. According to CERN Particle Detector BriefBook (http://rkb.home.cern.ch/rkb/PH14pp/node203.html#202 ) WLS blur the readout by 10-20ns, scintillator itself by single nanoseconds, photomultiplier - next single nanoseconds.
I do this for a living. Remember, for timing what matters is the rise time, not the total signal formation time. You get the worst timing in a calorimetric configuration, because there you want to collect all the light. This way, you have a total signal formation time around 60 ns (say 45-120 ns, depending on the detector) and can usually time in the leading edge to better than 5 ns. That is already good enough, but in a tracking configuration, using constant fraction discriminators, 1 ns is doable. OPERA claims 2.3 ns.
If I were charged with straightening this out, I'd be looking at the software for the Septentrio PolaRx2e. This is the specialized GPS receiver they had to use, and the desire to measure nanosecond-level timing over distances of hundreds of kilometers is probably not a common application. Uncommon applications means less well-tested software. I would also re-do the tunnel survey: GPS tells you where the antenna is. Finally, I'd redo the CERN survey. (GPS tells you where the antenna is) Both of those surveys should be done by independent teams who do not have access to the original surveys.