Of Particular Significance

Blog – Of Particular Significance

London, it seems, has much better weather this week than my home town of New York. Too bad I had to spend most of the day at a desk, working on my 20-minute Powerpoint presentation for tomorrow’s scientific meeting, on how to improve and expand the searches for supersymmetry at the Large Hadron Collider (LHC) so that they can cover variants of the theory that the standard searches for supersymmetry don’t address very well.  (You can read a bit more about what we do and don’t know right now about less popular variants of supersymmetry  by looking at this page and this one; this sequence of articles is still quite incomplete, thanks in part to certain pesky neutrinos.)

I expect an intense day tomorrow. The presentations will be short, leaving a lot of time for discussion.   It’s one of my favorite forms of scientific workshop — one where an exchange of ideas can actually lead to new policy and strategy.

Meanwhile, I have been getting great questions from non-experts in response to my “Summary and Open Space for Questions” post regarding the OPERA experiment’s early-arrival neutrinos.  A number of people have prefaced their comment with “this is probably a dumb question but…” Well, I have to say that I have scarcely seen a dumb question yet among the ones I’ve been receiving. (more…)

Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON September 28, 2011

[If you are a layperson interested in the faster-than-light neutrino claim, and you haven’t yet looked at yesterday’s “open-space’’ post and the list of excellent questions laypeople have asked in the comments, you definitely should.  And ask your own if you want. That post also gives an organized list of links to all my posts on the neutrino experiment so far.]

Now, here’s a problem: How should a particle physicist budget his or her time, when faced with the OPERA experiment, which has, say, a 1% chance of representing the most important discovery in decades, and a 99% chance of being wrong?  After all, life goes on at normal speed — and in particular, the Large Hadron Collider (LHC) is continuing to gather important data at an accelerating rate.  (more…)

Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON September 27, 2011

As befits our information age, and anything that has to do with Einstein, we are now deluged with a blizzard of detail, commentary, speculation, polemic, and downright silliness surrounding the recent OPERA experiment (the one which claims to find neutrinos arriving, after a trip from Western Switzerland to Central Italy, earlier than expected.) I aim to avoid adding to the confusion, and will only post what I feel is both clear and reliable.  Right now I have little new to say that fully satisfies both criteria.  However, later in this post you will find a summary of the posts I’ve put up so far, to help you navigate what’s already here.

One goal of this site is to create a space where lay people with a range of backgrounds can ask questions. While I deeply appreciate that many of my physics colleagues are reading my posts and some are commenting on them — along with highly educated non-physicists who’ve been asking very sensible questions and making insightful comments — my one concern right now is that the level of comments is so sophisticated that a person less familiar with the physics will feel intimidated about asking more elementary questions.  So I’d like to ask that the comments on this post be limited to those who feel there are some very, very basic points about the OPERA experiment, and the relevant background, that they just can’t follow.  (more…)

Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON September 26, 2011

This layperson’s explanation of to how to detect neutrinos is a companion post to the one that explains how to make a neutrino beam.

Neutrinos are passing through your body in vast numbers at all times. They are flooding out of the sun, from its central furnace, and even if it is nighttime where you are, those neutrinos are passing right through the earth and through your body as though the earth wasn’t even there. Cosmic rays (high energy particles flying in from deep space) often strike atoms in the high atmosphere and produce a number of neutrinos.  These too go right through you.

Almost always.  But a tiny, tiny fraction of these neutrinos do actually hit something. (more…)

Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON September 25, 2011

The OPERA experiment has now presented its results, suggesting that a high-energy neutrino beam has traveled 730 kilometers at a speed just a bit faster than the speed of light.  It is clear the experiment was done very carefully.  Many cross-checks were performed.  No questions were asked for which the speaker did not have at least a reasonable answer.

Some preliminary comments on the experiment (none of which is entirely well-informed, so caution…)

  • They have to measure times and distances to an accuracy of 1 part in a few hundred thousand. This is hard, not impossible, and they have worked with metrology experts to carry these measurements out.
  • The timing measurement is not direct; it has to be made in a statistical fashion. The proton beam pulses that make the neutrino beam pulses [read more about making neutrino beams here] are not sharp spikes in time, but are distributed in time over ten thousand nanoseconds. (Recall the measured early arrival of the neutrinos is only 60 nanoseconds.) And so one cannot measure, for each arriving neutrino, how long it took to travel. Instead one has to measure the properties of the proton beam pulses carefully, infer the properties of the neutrino pulses, measure the timing of the many arriving neutrinos, and work backwards to figure out how much time on average it took for the neutrinos to arrive. This sounds tricky. [Thanks to Ryan Rohm for calling my attention to this a few days ago; however, see his comment below.] That said, the experimenters do show some evidence that their technique works.  But this could be a weak point.
  • I am a bit concerned about the way in which statistical and systematic errors are combined. The theory for statistical errors is well-defined; one assumes random fluctuations. In combining two statistical errors E1 and E2, one says that the overall error is the square root of E1-squared + E2-squared.  This is called “adding errors in quadrature.”  But systematic errors are much less well-defined, and it is not clear you should combine them in quadrature, or combine them with statistical errors in quadrature. The OPERA experiment combines all errors in quadrature, and says they have a measurement at 6 standard deviations away from the speed of light. If you instead combined systematic errors linearly with statistical errors (E1+E2 instead of as above) you would get 4 standard deviations. If you combined all the systematic errors with each other linearly, and then with the statistical error linearly, you would get 2 standard deviations (though that is surely too conservative). All this is to say that this result is not yet so significant that different and more conservative treatments of the uncertainties would all give a completely convincing result. This is just something to keep in mind when evaluating such an exceptional claim; we need exceptional confidence.

Now, some brief comments on the theoretical implications, in addition to what I said in Tuesday’s and Thursday’s posts.

You may have heard some people say that neutrinos traveling faster than light would mean that Einstein’s theory is completely wrong and implies that instantaneous communication and even time travel would be possible. Balderdash! this is loose and illogical thinking. If Einstein’s theory were exactly correct AND neutrinos could travel faster than light, then this would follow. But if neutrinos travel faster than light, then Einstein’s theory is wrong at least in some part, and until you know exactly how it needs to be modified, you can draw no such conclusions.

As I emphasized in yesterday’s post, Einstein’s principles should be divided for current purposes into two parts:

  1. There is a universal speed limit.
  2. Light travels at this speed limit.

Observing that some neutrinos travel faster than light could mean there is no speed limit at all, or simply that light does not travel at the speed limit. And there are much more complex logical possibilities. Some of these would require only rather small (though still revolutionary) adjustments to current theoretical physics. Others would be more disruptive to current thinking. But it is certainly not true (as some physicists have said in public fora) that it requires going back to the drawing board as far as theoretical physics and Einsteinian relativity are concerned. It will depend on which of the various logical possibilities is actually operating. Hyperventilating about the impending collapse of existing theoretical physics is a tad inappropriate at this time.

In fact, over the years quite a few theorists (including very mainstream and well-respected scientists at major universities) have considered the possibility that Einstein’s principles might be slightly violated, and some of that work from the 1990s (and probably earlier [?]) suggested that studying neutrino properties would be a good way to look for signs of such violations. So it is not as though these issues have never come up before in theoretical physics… though I think it fair to say that everyone has viewed this exciting possibility as a long-shot.  (And most of us probably still do, until this experiment is confirmed.)

There is certainly more to say about the theoretical situation, but I am still learning about what the experts already know.

Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON September 23, 2011

Here’s a layperson’s explanation of how to make a beam of neutrinos, roughly speaking (the details depend on the individual experimental facility.)  (more…)

Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON September 23, 2011

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