Of Particular Significance

Author: Matt Strassler

Many of you, learning of the OPERA experiment’s claim (whose plausibility is dropping rapidly) of maybe-faster-than-light neutrinos, may have wondered (a) how do physicists know so much about neutrinos, and (b) what was the OPERA experiment originally designed to do?  [Hint: Only as a side project did the OPERA experiment set out to measure the speed of the neutrinos, and that’s why its design was by no means ideal for that purpose. ]

I’ve written an article that tries to explain the answer.  It describes how there are multiple ways to classify neutrinos that are mutually exclusive, and this leads to a strange, and scientifically crucial, quantum effect called “neutrino oscillations.”  After you’ve read the article, I hope you’ll have the language to understand this description of what the OPERA experiment was originally designed to do:   Its original goal was to study a particular effect of neutrino oscillations, by sending muon-neutrinos traveling through the earth for 730 kilometers, oscillating as they go, (more…)

Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON October 5, 2011

Unbelievable; yet again, for the fourth or fifth time since July, something related to high-energy physics hits the front pages. This time it’s not a shocking claim of a novel phenomenon, but a thoroughly expected Nobel prize awarded for the field’s greatest discovery of the 1990s: that not only is the universe expanding (as Edwin Hubble discovered in 1929), it is expanding more and more rapidly. The teams in which the prize-winners participated used Type Ia supernovas to make the first direct observations indicating that the universe is dominated by something like a “cosmological constant”, often now called “dark energy”.  [What these terms really mean deserves a longer article.]

It is interesting, given the historical juxtaposition of this award with the chaos and media circus of ten days ago, to compare this result with the OPERA experiment’s claim that neutrinos arrive earlier than expected. (more…)

Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON October 4, 2011

Two weeks ago, a colloquium; last week, a workshop talk; and this week starts with yet another presentation, in the form of a “seminar”.  In academic departments, especially the sciences, the term in this context refers to a talk, usually an hour long, about one’s recent research, given to the graduate students, postdoctoral researchers and faculty in one’s sub-discipline. Seminars are pretty common; I’ve given as many as a dozen in a year, and most institutions host one or two every week.

The topics of today’s talk? (more…)

Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON October 3, 2011

[If you are a layperson interested in the faster-than-light neutrino claim, and you haven’t yet looked at my recent “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 my main posts on the neutrino experiment.]

Today is a sad day in American particle physics.  It is the day that Fermilab will shut down the Tevatron, once the world’s leading particle accelerator, which discovered and measured the mass and other properties of the top quark (the sixth discovered, and by far the heaviest), tested the Standard Model of particle physics in very great detail (confirming that everything I wrote in this post about the known particles is correct to the available precision of the experiment), and looked hard for the Higgs particle before being overtaken by the Large Hadron Collider.   (more…)

Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON September 30, 2011

For me, one of the great pleasures of scientific research is the small, focused “workshop”, where a few scientists (typically 20 — 40 faculty, postdoctoral researches and students) assemble for a day or two to discuss a particular topic in detail. Presentations are typically short and often quite informal, and there’s lots of time for discussion built in to the schedule. The best workshops, of course, are those where the quality of the science and the knowledge, experience and skill of the participants is exceptional. I was fortunate to enjoy such a workshop yesterday at Imperial College in London, one of Britain’s finest scientific institutions.  About half the participants were experimentalists from the CMS experiment at the Large Hadron Collider (LHC) and the other half theorists like myself (one of whom is also on the ATLAS experiment at the LHC.)

Another great pleasure in doing science, at least in my field, is its international nature. The participants from yesterday’s workshop included scientists from at least seven countries and three continents, many of whom are now working in a country that is not their native land. Add to this diversity of cultures, appearances and accents some lively personalities, good senses of humor, and high quality science, and you have the ingredients for a very serious workshop that is a very serious form of fun, followed by much less serious fun when the workshop is over and everyone who can stick around goes out to a pub, a restaurant, and then another pub. (more…)

Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON September 30, 2011

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

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