Of Particular Significance

Blog – Of Particular Significance

The most important thing that happened this week in Berkeley, California was definitely not the news of a  small and probably ephemeral excess of multi-lepton events at the Large Hadron Collider‘s CMS experiment — and probably not even the disconcerting earthquakes on (near?) the strained Hayward fault — it was the (public but not yet peer-reviewed) report from the Berkeley Earth Team, a group of mostly non-climate scientists [mostly from physics] who went back to analyze and check the data that climate scientists have been studying for years.  Go look at their website; it’s for you.

My understanding is that the scientific director, Richard Muller, organized the team because he was highly skeptical that climate scientists were treating their data properly. His agenda seems to have been largely scientific rather than political.  Though I did not share his point of view, I found it understandable. In my field we have often seen data mis-analyzed, even though high-energy physics is a largely apolitical domain. It is not easy, even with full scientific integrity, to avoid all sources of bias. With something that has enormous policy implications, such as climate change, there was some concern among serious scientists that error and/or group-think bias could set in within even a large community. The idea of having a largely independent review by scientifically experienced non-experts was a good one.

Well, in science, when you see vocal skeptics starting to come around to the point of view of those they previously criticized, you know the climate is changing.

I doubt we’ll ever have a more independent review than the Berkeley Earth Team has just given us. I don’t know all the scientists on the team, but I am confident at least that Saul Perlmutter (who just won the Nobel Prize) is of the highest integrity.  The team included only scientists who had not taken a public position on climate change, and their funding sources are very broad-based.  Moreover, unlike climate scientists, who could be subjected to the accusation of letting a vested interest in obtaining funding bias their science toward a prevailing viewpoint, some members of this team had to give up time from their own personal research, thereby reducing their funding opportunities, in order to participate in this endeavor. None of them has much obviously to gain — no probability of scientific recognition, prizes, funding, or even thanks — especially Muller, who in confirming what he expected the team would likely refute has burned plenty of bridges in the interest of honesty.

I’m definitely not qualified to comment on the details of climate science, and I haven’t read the report.  All I have to go on right now is the two-page summary of the results reported here:

http://berkeleyearth.org/Resources/Berkeley_Earth_Summary_20_Oct

which I highly recommend you personally read.  It has subtleties and details that the press is not capturing.

Nevertheless, it seems to me at this early stage that the report’s main result — that where it has so far come to conclusions, it agrees with what many climate scientists have long been saying — represents a success story for science, one worth noting. It confirms yet again that preconceptions and funding sources do not automatically determine scientific results. And it confirms also that it is possible, over time, to obtain consensus about nature — that even while the US Congress witnesses ideology placed before the nation’s best interest, the collective scientific process still manages to put the integrity of science first, and a scientist’s pride second.

Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON October 24, 2011

For those of you wondering about this new and interesting hint of a possible (but still very doubtful) new physical phenomenon in the data from the CMS experiment at the Large Hadron Collider (LHC), here’s the summary of the situation.  [UPDATE: 10/22/11 very slightly reworded and reordered for clarity and proper emphasis]

  • Proton-proton collisions that produce three or more charged leptons and/or anti-leptons (“multi-leptons” for short) have long been seen as an excellent but very tricky place to look for new physics.   I have written an explanatory article as to why they are so good (to the point of being sometimes called “golden”), but also why they are tricky; there’s some fool’s gold in there.
  • On Wednesday and Thursday the CMS experiment gave two presentations  (here are my detailed comments, showing some tables and plots, on talks #1 and on #2) at a workshop in Berkeley, CA, giving two perspectives on a single set of multi-lepton events, obtained from data collected through August. They finds a small excess — more events than expected — but too small for CMS to claim to have seen anything significant.  [And Nota Bene: CMS has made no claims there is an excess, because the evidence is very weak by the stringent standards used (for good reason) in particle physics.]
  • Indeed, it must be remembered that small excesses of this type occur regularly in science, just from statistical fluctuations or from errors by experimentalists or theorists (remember the Higgs hints from earlier in the year, which were stronger, but have so far gone unconfirmed.)  And the excess seen here does not look particularly different from a statistical fluctuation.  So we should not be surprised if this hint goes away with more data from CMS, or when ATLAS reports their own studies.
  • But the excess is still large enough to intrigue theoretical particle physicists and motivate some consideration of what new physics, if any, might cause such an excess, and how to look for it more efficiently.
  • Two moderate earthquakes occurred in Berkeley, before and after the second talk.  Draw your own conclusions.      [joke…!]
  • Some of the plots shown at the second talk suggest that any such excess would most likely have to come from rather lightweight particles (well below 500 GeV) that do not carry the strong nuclear force.  (The reasoning is explained in my post following the second talk.) The logic is not airtight, but a number of other simple possibilities clearly wouldn’t fit the data at all.
  • Supersymmetry theorists will be quick to point out that supersymmetry has particles of the right type (charginos and neutralinos) and many variants of supersymmetry predict such a signal, though typically a bit smaller.  (You can read about how supersymmetry does that here; note especially Figure 2.)
  • However, many other classes of models of new physics can have light-weight particles with no strong forces, and associated multi-lepton events; such events are very generic and do not depend on anything special to supersymmetry.
  • So far I am aware of nothing in the data that would point toward or away from any one of these classes of models, so one cannot draw any conclusions.
  • We will know a lot more by March, when analysis of about 2.5 times the current data set will be possible.
Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON October 21, 2011

So now the second shoe drops, and the earth shakes a bit (3.9 earthquake just outside Berkeley prior to this talk.)  Yesterday we had the first report from the CMS experiment’s search for multi-lepton events at the LHC (Large Hadron Collider).  (See yesterday’s post.)  The emphasis yesterday was on events that show evidence of  substantial momentum and energy carried off by undetectable particles such as neutrinos (such evidence involves an imbalance of momentum among the detectable particles, or `missing energy’ as it is often [misleadingly] called).  Today the emphasis is on events with large overall energy (not exactly true but close enough for the moment), including both the energy of detectable particles (the leptons and any jets from quarks or gluons)  and the evident energy of anything undetectable.  One could already tell from yesterday’s table of event rates that today’s talk at the Berkeley supersymmetry workshop would be worth paying attention to. (more…)

Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON October 20, 2011

[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

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