Of Particular Significance

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Shoichi Sakata would have been 100 years old this year, and a conference celebrating his achievements in high-energy physics and beyond is underway here in Nagoya. The university president made brief introductory remarks, describing how, right after the war, Sakata introduced a democratically-inspired culture into the physics department, insisting on the right of young researchers to choose their own research paths independent of senior faculty, and permanently impacting the culture of physics (and beyond) at Nagoya University. There followed a talk reviewing Sakata’s most important work, including central contributions to the understanding of the muon, many of the hadrons, and the first two neutrinos. Unfortunately for Sakata, English publication of one of his most important papers (correctly identifying the muon as a decay product of an electrically-charged pion) was delayed by the war; another of his ideas (concerning the nature of hadrons) inspired many important developments, but was not itself correct; and a third idea (suggesting two neutrinos, which could oscillate one into the other) arrived just a bit too late to predict an experimental result. On top of this, he died young, before he was 60.   Consequently, outside Japan he is not so widely known today.  But here he casts a long shadow. Indeed, Professor Maskawa’s brief address at the opening of the Inaugural Conference of the Kobayashi-Maskawa Institute (earlier this week) was entirely devoted to lauding his mentor.

Professor Fumihiko Sakata, standing in front of his father's memorial stone, thanks the assembled dignitaries (including, from left, Nagoya University president Hamaguchi and Nobel Prize winners Maskawa and Kobayashi.)

Tucked in among today’s talks, another ceremony, this one to unveil a memorial stone outside the Kobayashi-Maskawa Institute, in Sakata’s honor.

Unfortunately I cannot stay for the last day of the conference. An amusing feature of my journey home: I depart Tokyo at 5 pm on October 28th and arrive in New York City at 5 pm on October 28th.

Picture of POSTED BY Matt Strassler

POSTED BY Matt Strassler

ON October 27, 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

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

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

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

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

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

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