Of Particular Significance

Author: Matt Strassler

[UPDATE 10/23/11: Blog traffic indicates that far more of you are reading this post than the one that follows.  That’s too bad, because in my opinion the more interesting information was in the second talk from CMS on the subject, not the first.  But also it’s too bad because you’re not reading my very clear statement of what this small excess does and doesn’t mean.  So I’ve decided to copy that statement into this post.  Here is my view, as stated 10/20/11.

But before we begin, maybe I should make my own opinion perfectly clear to the reader.   How high does this story rate on the scale?

  • Particle physicists perhaps should be interested, maybe even intrigued, but definitely not excited.  As do most small excesses, this one will probably disappear as more data becomes available.
  • Other scientists should basically ignore this.  The excess will probably disappear soon enough.
  • I can’t see why the general public should pay any heed to this, as the excess will probably disappear — with the exception of those who are specifically curious as to why particle physicists are paying close attention.  Those of you who are in this category have a nice opportunity to learn why multi-lepton searches are a powerful, though tricky, way to look for new physics.

I go on in that post to talk about why I think this; you can read about it there.  So — buyer beware…  The original post now follows (and please note words like “minor” and “somewhat”.  They are not there by accident.  Bloggers: .)]

Finally, something at the Large Hadron Collider (LHC) that does not seem to agree that well with the predictions of the equations of the Standard Model of particle physics. Of course, we should not be surprised that it has taken a while for even a minor discrepancy of this type to see the light of day; as I emphasized in this article, there is always a tendency, during the early and middle years of an experiment, for the results that agree with expectations to appear first, while the results that don’t agree get extra scrutiny and take longer. For this very reason, many outside the Large Hadron Collider experiments have been waiting with great curiosity for the results of the search for “multileptons”:  very rare proton-proton collisions which produce directly three or more of electrons, positrons (i.e. anti-electrons), muons, anti-muons, taus and/or anti-taus. These searches have been noticeably late. (more…)

Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON October 19, 2011

Another experiment has weighed in on superluminal neutrinos — indirectly.  The ICARUS experiment has measured the energy spectrum of neutrinos traveling from CERN to Gran Sasso.  They confirm that the Cohen-Glashow effect, which I described in some detail here,  is not occurring in the beam of neutrinos that OPERA is also using.  The distribution of neutrino energies in the beam is undistorted.   If standard Cerenkov processes take place, then these neutrinos are not traveling faster than light.

At least one blogger has said this refutes the OPERA experiment.  Hmmm… for my part, I don’t think it really changes the situation much at all.  It only checks something that we were already pretty sure of. As I explained in my post on the subject, Cohen-Glashow emission would have had a big effect on the OPERA neutrino beam, one that OPERA itself would have detected.   That was Cohen and Glashow’s main point.  OPERA didn’t see any hint of such an effect.  All ICARUS has done, as far as I can tell,  is confirm that indeed there’ s no such effect, to significantly higher precision.  If you want to say that ICARUS has refuted OPERA, you really have to say that OPERA refuted itself first… that the experiment was self-contradictory.

What’s the loophole?  It’s small, but it’s still there.  We already knew, both from Cohen-Glashow emission and from the calculation of Giudice et al. that OPERA almost certainly cannot be right unless relativity is altered in such a way as to shut off Cerenkov-like processes at high energy.  That loophole may well be too narrow for any decent modification of relativity to get through.  But I don’t think ICARUS’s result changes the location or nature of the loophole.

UPDATE: In a question below it was asked whether sterile neutrinos [new types of neutrino-like particles that aren’t affected by the weak nuclear force and therefore would not have large Cohen-Glashow emission] could also pose an acceptable loophole, by oscillating with ordinary neutrinos.  I can’t make a clean argument against it without going a calculation, so for now I have to say that, though I’m dubious, I am not sure that loophole is closed yet.

UPDATE: I hadn’t had time when I first put this post up to explain why ICARUS and OPERA are measuring the same neutrino beam.  Both experiments are in the Gran Sasso lab, quite near each other.  By the time the neutrinos arrive at Gran Sasso, the beam of neutrinos is quite spread out — a couple of kilometers wide, I believe — so the Gran Sasso experiments are sitting in the same neutrino beam.  We can expect other Gran Sasso experiments to weigh in with their own observations over time.

UPDATE: Here’s a picture comparing my sketch (from my  post ten days ago on Cohen-Glashow emission) of what CG emission predicts for the OPERA beam (an effect that OPERA itself would have seen)  to the measurement from ICARUS.  Note the peak and the tail, marked by the black arrow and violet arrow on both plots; if Cohen-Glashow emission were operating, the tail would be gone and the peak would have shifted to the left.

Left: Sketch of how CG emission would have strongly distorted the beam at OPERA, in a way that OPERA itself would have detected. The red curve is expectation, the green curve is what CG emission would have done to the beam. In this way, Cohen-Glashow argued, OPERA is self-contradictory. Right: The ICARUS experiment, sitting in the same beam, confirms that data (blue points) and expectation (red curve) for the distribution of neutrino energies agree, with a peak at 20 GeV (black arrow) and a tail extending far higher (violet arrow). This observation rules out any significant amount of Cohen-Glashow emission, constraining any theoretical attempt to explain OPERA's result.

Comments welcome.

Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON October 19, 2011

There is clearly some confusion regarding the degree of scepticism that physicists are manifesting toward the OPERA experiment’s claim of faster-than-light neutrinos.  I’ve seen various statements, even by physicists, that suggest this level of doubt has to do with “protection of the establishment”, perhaps similar to a political oligarchy with a vested interest in defending its turf.  I disagree with this point of view.  While there certainly is a level of politics in any human endeavor, including science, I don’t think that’s what’s going on here at all.

For one thing, everyone should keep in mind that the best thing that could possibly happen to high-energy physics would be for OPERA to be correct!  The possibilities for new discoveries, both experimental and theoretical, and for technological advances currently unforeseeable, might be enormous — as they were when classical Newtonian mechanics had to be improved and extended by the introduction of quantum mechanics.  Revolutions are wonderful things — and I certainly have a vested interest in having one happen on my watch.

However, false revolutions are another matter.  And of course they are much more common than real ones.

The reasons for the intense scepticism about OPERA are both general and specific.  The general reasons stem from the track record of experiments on the frontiers of science, which is pretty dismal.  This is not because experimentalists are careless or foolhardy (well, occasionally this happens) but because doing first-of-a-kind experiments, using new and clever methods and the latest technology, is extremely difficult, and prone to unforeseen problems.  And statistical flukes can always happen, too.  Everyone who has worked in high-energy physics for a while knows that the vast majority of exciting results, even from the best experimentalists, simply don’t hold up over time.  I made an informal list over the weekend of false alarms that have occurred during the nearly 30 years that I’ve been following or actually doing high-energy physics, and came up with nearly two dozen separate incidents — and I keep thinking of new ones.  [I may do some writing later this week about how some of these “discoveries” went awry.]  Meanwhile I can think of only three actual discoveries that survived, one of which (the top quark) was expected, one of which (neutrino oscillations) was pretty exciting but not unexpected, and only one of which really violated the prejudices of my field.  The last — the only real shocker to occur during my career — won this year’s Nobel Prize: the discovery that the universe’s expansion is accelerating instead of decelerating.

The specific reasons for distrusting OPERA are, I think, of three subtypes.  And they don’t have much to do with Einstein and his theories being somehow a sacred cow.  First, there is concern about OPERA as an experiment.  Remember OPERA’s main purpose was to study neutrino oscillations; it was not designed for measuring neutrino speeds. Consequently there are things that make OPERA’s measurement harder than it would be for an experiment whose design was optimized for tests of Einstein’s speed limit.  Second, there are some issues surrounding the experimental technique used by OPERA, including those I discussed after the original OPERA presentation: the complexity of the measurements of times and distances, the employment of rather long pulses of neutrinos to detect very short time shifts, and the use of an aggressive statistical technique in a context where, in my view, they ought to have done something much more conservative.  And finally, there are the theoretical arguments (I’ve written about two of them here and here) that show that it is very difficult to accommodate OPERA’s result within any minor adjustment of Einstein’s relativity, such as those that have been often discussed in the past (see Professor Alan Kostelecky’s webpage for some information on the many previous suggestions), and also difficult to make major adjustments to relativity for neutrinos without running afoul of constraints on such adjustments from prior experiments on electrons and photons.   This is not blind scepticism; it is reasoned scepticism.  Nor is it close-mindedness; it still leaves the door open.

It’s interesting to compare this situation with what happened when the accelerating universe was discovered.  Scepticism also ran very high, but the arguments against the claim were weaker than those against OPERA’s.  First, the observers had the measurement of the deceleration or acceleration of the universe as a primary goal, and their methods were optimized for that purpose.  Second, it was not easy to find fault with their observational techniques — though there were still plenty of proposals for ways they might have been fooled by astronomical effects, or even by the effect of a new particle. Third, although there was a strong theoretical prejudice in the particle physics community against an accelerating universe, there was no calculation anyone could do to argue the result was in strong conflict with previous experiments — no obstructions from prior data to match the ones that have been raised for OPERA.  Fourth, there had even been arguments by astrophysics theorists, as far back as 1995, arguing that data from other sources suggested the universe was accelerating.  And fifth, the claim came from two independent groups of scientists, who had come to the same conclusion.  So the scepticism, while high in some quarters (including mine), never rose to the levels that we see now with OPERA.

Of course, the clincher for the accelerating universe had nothing to do with any of this.  Confirmation came from additional, complementary data — from other experiments, such as those observing the cosmic microwave background radiation (the dim glow leftover from the hot Big Bang).  In the end, scientific evidence spoke louder than even the most vocal scientists.

Perhaps OPERA’s result will be confirmed, perhaps not.  But no one should be complaining about the current high level of scientific scepticism.   Experimentalists and theorists who are pointing out potential problems with OPERA are just doing their job, forcing this experimental result, like any other, to run a gauntlet of obstacles to prove its worth.  No radical claim enters into the great books of scientific knowledge without passing a series of draconian tests, of a sort that recalls the ordeals suffered in childhood fairy-tales. For this is how science, a process beset with human frailty, protects itself from harm.

Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON October 17, 2011

From the very existence of this website, you may rightly infer that I feel some members of the scientific community ought to commit to educating the public about the content and process of science. At a minimum, since my research, and that of my colleagues, is largely paid for by taxpayers, the public has the right to know and understand what it is getting for its money. Also, science underpins our technological society, and yet it seems mysterious and frightening to a good many people, so it’s important that the subject be demystified. And finally, it’s wonderful and exciting stuff, so it’s a real shame if the public knows little about it.

Aside from this site, another way I communicate ideas to the public is through public lectures. I’ve given a number of talks for laypeople in the past (some video clips from one of them are available), mostly at bars. Perhaps a little beer makes people more at ease when facing concepts such as hadrons and Higgs particles. It also perhaps makes them comfortable asking questions; I find the question and answer session is the most interesting and challenging part of the event. There are always some really great questions; it’s impressive how far self-educated non-experts can go. I do think it’s a lot easier to educate yourself now about high-energy physics and related fields than it was when I was a teenager; you can go read Lisa Randall’s most recent book, or watch the excellent pedagogical lectures by physicists such as Lenny Susskind (one of my mentors) or Sean Carroll (from Cosmic Variance).

I’ll be trying something new today, (more…)

Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON October 16, 2011

Today I’m at SUNY Stony Brook (SUNY = State University of New York) out on Long Island, to give a talk to the particle physics theorists there (and whoever else shows up.) One topic I’ll cover involves the still very mysterious measurements made by the CDF and DZero experiments (at Fermilab’s Tevatron collider) that suggest an asymmetry in the production of top quarks. You can read about that mystery here. Obviously one would want to make a similar measurement at the LHC (more…)

Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON October 13, 2011

A couple of months back I wrote an article explaining intuitively why most types of particles decay.  If you read that article you may be left wondering why a few types of particles, including the ones out of which we’re made, don’t decay.  An answer to that question has now arrived, in the form of a new article:“Most Particles Decay – Yet Some Don’t!”.  I hope you find it useful, and as always feel free to ask me to clarify points that don’t make sense to you.

Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON October 12, 2011

Here’s another major strike against the OPERA experiment’s claim of superluminal neutrinos, in addition to the Cohen-Glashow argument I described last week. It comes from a very natural place: the weak nuclear force. The theory (i.e. the equations) that we use, with great success, to predict the behavior of the weak nuclear force inextricably links some of the properties of neutrinos and charged leptons (electrons, muons and taus.) Because of this linkage, you simply can’t make neutrinos travel faster than light without making electrons do it too — by a smaller amount, to be sure, but still bigger than a part in a billion. And it turns out the effect is large enough that it should already have been detected by existing experiments, putting OPERA’s result further in doubt. (more…)

Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON October 11, 2011

Among the many tricky concepts which the layperson has to grapple with when learning about particle physics is something called “virtual particles”, which show up in cute pictures called “Feynman diagrams” along with “real particles”.  In most books for the public, some words are mumbled about the uncertainty principle and how virtual particles are particles that exist for a short time and then disappear.  Well, this isn’t really wrong, and it is the language that physicists use.  But I have found that the language is so misleading for non-experts that it leads to many confusions among my readers.   For this reason, I’ve taken a different tack in this pedagogical article, with the thinking that the most important thing for a layperson to understand about virtual particles is that they really are not particles at all, despite the name, and they don’t behave that much like them.  They are more of a generalized disturbance in a field, while a real particle, a nice ripple in a field, is a special one.

Why would you want to read this article?  Because in addition to the Cohen-Glashow argument against the OPERA experiment’s result on superluminal neutrinos, which appeals to a process similar to Cerenkov radiation, there’s a more powerful, but more subtle, argument that involves virtual particles.  I’ll explain that in my next post.

Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON October 10, 2011

While I was busy with last week’s LHC workshop in London, a very interesting and short paper appeared, written by two of the world’s experts on violations of “Lorentz invariance”, the symmetry of space and time that underlies Einstein’s theory of special relativity. The authors, both from Boston University, are Andrew Cohen, who is highly regarded within the community for several significant contributions to high-energy physics, including his co-authorship of the key papers that led to the theory of a composite Higgs field known as “Little Higgs”, and Sheldon Glashow (formerly at Harvard), Nobel Prize winner for his work on the weak nuclear force, and famous for many other contributions of nearly equal importance.  In the 1990s, Glashow, with the late great physicist Sidney Coleman, (highly respected not only for his exceptional theoretical research but also for his beautiful scientific writing and extraordinary teaching ability), wrote two important papers on violations of Lorentz invariance. It was they (to the best of my knowledge) who pointed out the enormous value of Cerenkov radiation in testing Einstein’s relativity principles. (I’ve just written a new short article on Cerenkov radiation, and there I briefly explain how Coleman and Glashow used it previously to test Lorentz invariance.)

What Cohen and Glashow did last week was to generalize this idea to point out a new physical phenomenon (new at least to me) and use it to argue that OPERA’s result is self-inconsistent. They argue that the very effect of faster-than-light travel that OPERA claims to observe would have caused distortions in its neutrino beam that clearly were not observed. Moreover, Cohen and Glashow also pointed out that at least two other experiments studying higher energy neutrinos put even stronger constraints on the possibility of anything similar to what OPERA observed. (more…)

Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON October 6, 2011

In case you are interested, I’ve written a short article about Cerenkov radiation, explaining very briefly what it is, why it is so useful in particle physics experiments, and how it can be used to test Einstein’s theory of relativity.

Coming later today or tomorrow: a new set of comments on OPERA and neutrinos that arrive before they were expected.

Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON October 6, 2011

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