Category Archives: Other Collider News

It’s (not) The End of the World

The December solstice has come and gone at 11:11 a.m. London time (6:11 a.m New York time). That’s the moment when the north pole of the Earth points most away from the sun, and the south pole points most toward it. Because it’s followed by a weekend and then Christmas Eve, it marks the end of the 2012 blogging season, barring a major event between now and year’s end. But although 11:11 London time is the only moment of astronomical significance during this day (clearly the universe does not care where humans set our international date line and exactly how we set our time zones, so destruction was never going to be at local midnight — something the media doesn’t seem to get) it obviously wasn’t the end of the world.

A lot of people do put a lot of stock in prophecy, including prophecies of the end of the world that nobody ever made (such as the one not made for today by the Mayans, through their calendar) and others that people made but were wrong (such as those made by Harold Camping last year and by many throughout history who preceded him.) If anyone were any good at prophecy they’d be able to use their special knowledge to become billionaires, so maybe we should be watching Bill Gates and Michael Bloomberg and the Koch brothers and people like that. I haven’t heard any rumors of them building bunkers or spaceships yet. Of course at the end of the year they may get a small tax hike, but that wouldn’t be the end of the world.

The Large Hadron Collider [LHC], meanwhile, has triumphantly reached the end of its first run of proton-proton collisions. Goal #1 of the LHC was to allow physicists at the ATLAS and CMS experiments to discover the Higgs particle, or particles, or whatever took their place in nature; and it would appear that, in a smashing success, they have co-discovered one.  But no Higgs particles, or anything like them, will be produced again until 2015. Although the LHC will run for a short while in early 2013, it will do so in a different mode, smashing not protons but the nuclei of lead atoms together, in order to study the properties of extremely hot and dense matter, under conditions the universe hasn’t seen since the earliest stages of the Big Bang that launched the current era of our universe.  Then it will be closed down for repairs and upgrades.  So until 2015, any additional information we’re going to learn about the Higgs particle, or any other unknown particle that might have been produced at the LHC, is going to be obtained by analyzing the data that has been collected in 2011 and 2012. The total amount of data is huge; what was collected in 2012 was about 4.5 times as much as in 2011, and it was taken at 8 TeV of energy per proton-proton collision rather than 7 TeV as in 2011. I can assure you there will be many new things learned from analyzing that data throughout 2013 and 2014.

Of course a lot of people prophesied confidently that we’d discover supersymmetry, or something else dramatic, very early on at the LHC. Boy, were they wrong! Those of us who were cautioning against such optimistic statements are not sure whether to laugh or cry, because of course it would have been great to have such a discovery early in the LHC program. But there was ample reason to believe (despite what other bloggers sometimes say) that even if supersymmetry exists and is accessible to the LHC experiments, discovering it could take a lot longer than just two years!  For instance, see this paper written in 2006 pointing out that the search strategies being planned for seeking supersymmetry might fail in the presence of a few extra lightweight particles not predicted in the minimal variants of supersymmetry. As far as I can tell at present, this very big loophole has only partly been closed by the LHC studies done up to now. The same loophole applies for other speculative ideas, including certain variants of LHC-accessible extra dimensions. I am hopeful that these loopholes can be closed in 2013 and 2014, with additional analysis on the current data, but until they are, you should be very cautious believing those who claim that reasonable variants of LHC-accessible supersymmetry (meaning “natural variants of supersymmetry that resolve the hierarchy problem”) are ruled out by the LHC experiments. It’s just not true. Not yet. The only classes of theories that have been almost thoroughly ruled out by LHC data are those predict on general grounds that there should be no observable Higgs particle at all (e.g. classic technicolor).

While we’re on the subject, I’ve been looking back at how I did on prophecy this year. It’s been a remarkably good year, probably my best ever — though admittedly I only made very easy (though not necessarily common) predictions. First, the really easy one:  I assured you, as did most of my colleagues, that 2012 would be the Year of the Higgs — at least, the Year of the Simplest Possible Higgs particle, called the “Standard Model Higgs”. It would be the year when Phase 1 of the Higgs Search would end — when we’d either find a Higgs particle of Standard Model type (or something looking vaguely like it), or, if not, we’d know we’d have to move to a more aggressive search in Phase 2, in which we’d look for more complicated versions of the Higgs particle that would have been much harder to find. We started the year with ambiguous hints of the Higgs particle, too flimsy to be sure of, but certainly tantalizing, at around a mass of 125 GeV/c2. In July the hints turned into a discovery — somewhat faster than expected for a Standard Model Higgs particle, because the rate for this particle to appear in collisions that produce two photons was higher than anticipated. The excess in the photon signal means either the probability for the Higgs particle to decay to photons is larger than predicted for a Higgs of Standard Model type, or both CMS and ATLAS experienced a fortunate statistical fluctuation that made the discovery easier. We still don’t know which it was; though we’ll know more by March, this ambiguity may remain with us until 2015.

One prophecy I made all the way back at the beginning of this blog, July 2011, was that the earliest search strategy for the Higgs, through its decays to a lepton, anti-lepton, neutrino and anti-neutrino, wouldn’t end up being crucial in the discovery; it was just too difficult. (In this experimental context, “lepton” refers only to “electron” or “muon”; taus don’t count, for technical reasons.) In the end, I said, it would be decays of the Higgs to two photons and to two lepton/anti-lepton pairs that would be the critical ones, because they would provide a clean signal that would be uncontroversial. And that prophesy was correct; the photon-based and lepton-based searches were the signals that led to discovery.

Now we’ve reached December, and the data seems to imply that except possibly for this overabundance of photons, which still tantalizes us, the various measurements of how the Higgs-like particle is produced and decays are starting to agree, to a precision which is still only moderate, with the predictions of the Standard Model for a Higgs of this mass. Fewer and fewer experts are still suggesting that this is not a Higgs particle. But it will be some years yet — 2018 or later — before measurements are precise enough to start convincing people that this Higgs particle is really of Standard Model type. Many variants of the Standard Model, with new particles and forces, predict that the difference of the real Higgs from a Standard Model Higgs may be subtle, with deviations at the ten percent level or even less. Meanwhile, other Higgs-like particles, with different masses and different properties, might be hiding in the data, and it may take quite a while to track them down. Many years of data collecting and data analysis lie ahead, in Phase 2 of the Higgs search.

Another prophecy I made at the beginning of the year was that Exotic Decays of the Higgs would be a high priority for 2012. You might think this prophesy was wrong, because in fact, so far, there have been very few searches at ATLAS, CMS and LHCb for such decays. But the challenge that required prioritizing these decays wasn’t data analysis; it was the problem of even collecting the data. The problem is that many exotic decays of the Higgs would lead to events that might not be selected by the all-important trigger system that determines which tiny fraction of the LHC’s collisions to store permanently for analysis! At the beginning of 2012 there was a risk that some of these processes would have been dumped by the trigger and irretrievably lost from the 2012 data, making future searches for such decays impossible or greatly degraded. At a hadron collider like the LHC, you have to think ahead! If you don’t consider carefully the analyses you’ll want to do a year or two from now, you may not set the trigger properly today. So although the priority for data analysis in 2012 was to find the Higgs particle and measure its bread-and-butter properties, the fact that the Higgs has come out looking more or less Standard Model-like in 2012 means that focusing on exotic possibilities, including exotic decays, will be one of the obvious places to look for something new, and thus a very high priority for data analysis, in 2013 and 2014. And that’s why, for the trigger — for the collection of the data — exotic decays were a very high priority for 2012. Indeed, one significant use of the new strategy of delayed data streaming at ATLAS and of data parking at CMS (two names for the same thing) was to address this priority. [My participation in this effort, working with experimentalists and with several young theorists, was my most rewarding project of 2012.]  As I explained to you, a Higgs particle with a low mass, such as 125 GeV/c2, is very sensitive to the presence of new particles and forces that are otherwise very difficult to detect, and it easily could exhibit one or more types of exotic decays.  So there will be a lot of effort put into looking for signs of exotic decays in 2013 and 2014! I’m very excited about all the work that lies ahead of us.

Now, the prophecy I’d like to make, but cannot — because I do not have any special insight into the answer — is on the question of whether the LHC will make great new discoveries in the future, or whether the LHC has already made its last discovery: a Higgs particle of Standard Model type. Even if the latter is the case, we will need years of data from the LHC in order to distinguish these two possibilities; there’s no way for us to guess. It’s clear that Nature’s holding secrets from us.  We know the Standard Model (the equations we use to describe all the known particles and forces) is not a complete theory of nature, because it doesn’t explain things like dark matter (hey, were dark matter particles perhaps discovered in 2012?), and it doesn’t tell us why, for example, there are six types of quarks, or why the heaviest quark has a mass that is more than 10,000 times larger than the mass of the lightest quarks, etc. What we don’t know is whether the answers to those secrets are accessible to the LHC; does it have enough energy per collision, and enough collisions, for the job?  The only way to find out is to run the LHC, and to dig thoroughly through its data for any sign of anything amiss with the predictions of the Standard Model. This is very hard work, and it will take the rest of the decade (but not until the end of the world.)

In the meantime, please do not fret about the quiet in the tunnel outside Geneva, Switzerland. The LHC will be back, bigger and better (well, at least with more energy per collision) in 2015. And while we wait during the two year shutdown, the experimentalists at ATLAS, CMS, and LHCb will be hard at work, producing many new results from the 2011 and 2012 proton collision data! Even the experiments CDF and DZero from the terminated Tevatron are still writing new papers. In short, fear not: not only isn’t the December solstice of 2012 the end of the world, it doesn’t even signal a temporary stop to the news about the Higgs particle!

—-

One last personal note (just for those with some interest in my future.)

End of the OPERA Story

In case you haven’t yet heard (check my previous post from this morning), neutrinos traveling 730 kilometers from the CERN laboratory to the Gran Sasso laboratory do arrive at the time Einstein’s special relativity predicts they would.

Of course (as the press mostly seems to forget) we knew that.  We knew it because

So the news from the Neutrino 2012 conference in Kyoto, on new data from May 2012 taken by OPERA and three nearby experiments, is no surprise to anyone who was paying attention back in March and early April; it’s exactly what we were expecting.

One thing that almost no one is reporting, as far as I can tell, is that CERN’s research director Sergio Bertolucci did not give the first talk on neutrino speeds in Kyoto.  That talk was given by Marcos Dracos, of OPERA.  Dracos presented both OPERA’s corrected 2011 results (with corrections based on the detailed investigation shown in March of the problems reported back in February) and also the new 2012 results, which were taken with a kind of short-pulse beams similar to that used in OPERA-2.  (A short pulse beam allows for a neutrino speed measurement to be made rather easily and quickly, at the expense of OPERA’s neutrino oscillation studies, which were the main purpose of building the OPERA experiment.)

Following Dracos’ talk, Bertolucci spoke next, and reported the results of the neighboring Borexino, LVD and ICARUS experiments on the May 2012 data, which along with OPERA are all bathed in the same CERN-to-Gran Sasso neutrino beam, and collected their data simultaneously.  All of the results are preliminary so the numbers below will change in detail.  But they are not going to change very much.  Here they are: neutrinos arrive at a time that differs from expectation by:

  • Borexino: δt = 2.7 ± 1.2 (stat) ± 3 (sys) ns
  • ICARUS: δt = 5.1 ± 1.1 (stat) ± 5.5 (sys) ns
  • LVD: δt = 2.9 ± 0.6 (stat) ± 3 (sys) ns
  • OPERA: δt = 1.6 ± 1.1 (stat) [+ 6.1, -3.7] (sys) ns

(Here “ns” means nanoseconds, and ”stat” and “sys” mean statistical and systematic uncertainty.)  The original OPERA result was an early arrival of about 60 nanoseconds, about six standard deviations away from expectations.  You see that all the experiments are consistent with zero early/late arrival to about 1 standard deviation — almost too consistent, in fact, for four experiments.

So there is no longer any hint of any evidence whatsoever of a problem with the predictions of special relativity, and in particular with the existence of a universal speed limit.

A summing up is called for, but I want to write that carefully.  So unless something else comes up, that’s all for today.

Guess What?! Neutrinos Travel Just Below the Speed of Light

Five out of five experiments agree: neutrinos do not travel faster than the speed limit.

Or more precisely: to within the uncertainties of current measurements, neutrino speed, for neutrinos with energies far larger than their masses, is experimentally indistinguishable from the speed of light in vacuum.  This is just as expected in standard Einsteinian special relativity, which would predict they move just below light speed, by an amount too small to measure with current experiments.

http://press.web.cern.ch/press/PressReleases/Releases2011/PR19.11E.html

Based on data taken in May 2012 using a beam of neutrinos sent from the CERN laboratory to the Gran Sasso lab, the four experiments ICARUS, LVD, Borexino and even OPERA (the source of  all the excitement) find results consistent with the speed of light, with uncertainties (at one-standard-deviation) about 10 times smaller than OPERA’s original measured deviation of neutrino speed from the speed of light.  The new results are consistent with ICARUS’s result from 2011 data.  Moreover, OPERA’s mistaken result from September and November 2011 — a claimed six standard deviations away from the expected speed — has now been corrected, following their detective work presented in March.  Even MINOS, a U.S. experiment, has revised their older result, which was previously slightly discrepant from the speed of light by a small amount (two standard deviations), and they find now that their data too are quite consistent with neutrinos traveling with light speed, though with much less precision in the measurement.

And so with a final quintet, sung in unison, this melodramatic comic OPERA buffa comes to a close.  As with all classic operatic comedies, there’s been crisis, chaos, and a good bit of hilarity, all the while with wise voices speaking reason to no avail, but in the end the overzealous are chastened, the righteous are made whole, everyone (even the miscreant) is happy, and all is well with the world.

Curtain!! Applause!!  Science Triumphant!!

Favorable review to follow when time permits.

A Violation of Lepton Universality?

A brief mention today of a new measurement from the BABAR experimental collaboration, which tests lepton universality (to be explained below) and finds it wanting.

The Basic Story (Slightly Oversimplified)

Within the Standard Model of particle physics (the equations that describe and predict the behavior of all of the known particles and forces), the effects of the weak nuclear force on the three leptons — the electron, the muon and the tau — are all expected to be identical. This called “lepton universality”. Continue reading

OPERA’s Timing Issue Confirmed? Yes!

[QUICK UPDATE April 2: I've now finished an article giving more details of how OPERA, with LVD's help, solved the mystery.]

[UPDATE March 31 2 a.m.: following study of the slides from a mini-workshop recording the results of investigations by OPERA and LVD, I now have the information to remove all the guesswork from my original post; you'll see outdated information crossed out and newer and more precise information written in orange.  I've also added figures from the talks.]

March 30 5:30 p.m. Two main scientists at OPERA, one leading the OPERA team as a whole and the other leading the neutrino speed measurement, resigned their leadership positions today.  The suggestion from the press is that this is due to personal and scientific conflicts within the OPERA experiment, rather than due directly to the errors made in the neutrino speed experiment; but of course the way the measurement was publicized by OPERA caused serious internal conflicts at the time and are surely part of the issue.    [Oh, and meanwhile, back over at the CERN lab, some good news: collisions at the Large Hadron Collider with 8 TeV of energy per collision were achieved this afternoon.]

The mystery surrounding OPERA, the Gran Sasso experiment which (apparently through a technical problem) measured that neutrinos sent from the CERN lab to the Gran Sasso lab in Italy arrived earlier than expected by 60 nanoseconds, seems to be on the verge of being is resolved.  Statements made by an OPERA scientist in the Italian language press, pointed out to me by commenters (Titus and A.K.), seem to imply that OPERA has more or less confirmed that the problematic fiber optic cable (along with the clock problem, to a lesser extent) was responsible for a 60 nanosecond (billionth-of-a-second) shift in the timing, creating the false result.  We do not yet have official information from OPERA about this, but talks given at a mini-workshop a couple of days ago make clear that this is the case.

The way this was done if I/we understand the Italian correctly is something like is the following  with all details still very uncertain. Continue reading

Taking Stock: Where is the Higgs Search Now?

Today, we got new information at the Moriond conference on the search for the Higgs particle (in particular, Phase 1 of the search, which involves the search for the simplest possible Higgs particle, called the “Standard Model Higgs”) from the Tevatron and the Large Hadron Collider [LHC], the Tevatron’s successor.  With those results in hand, and having had a little time to mull them over, let me give you a short summary.  If you want more details, read today’s earlier post and yesterday’s preparatory post.

Before I do that, let me make a remark.  There is a big difference between healthy skepticism and political denialism.  I get the impression that some people who are writing or reading other blogs misinterpret my caution with regard to experimental results as being somehow a political and unreasonable bias against the Higgs particle being present, either at a mass of 125 GeV/c2 or at all.  That’s ridiculous.  All that is going on is that I simply am not convinced yet by the data.  I’m a careful scientist… period.  And you’ll see that I’m consistent; later in this post I will advise you not to over-react negatively to what ATLAS didn’t see.

What happened today at the Moriond conference?

What did we learn?

The Tevatron experiments see a combined 2.2 standard deviation [2.2 ``sigma''] excess in their search, consistent with a Standard Model Higgs particle with a mass anywhere in the range of 115 to 135 GeV/c2.  This is not inconsistent with the Higgs hints that we saw in December from the LHC experiments.  Here I am being perhaps overly careful in not saying, more positively, “it is consistent with the Higgs hints…” only because this measurement is intrinsically too crude to allow us to narrow in on 124-126 GeV, where ATLAS and CMS see their hints.  In short, the Tevatron measurement could, in the end, turn out to indicate a Higgs at a different mass than the one indicated by the current ATLAS and CMS hints.  Anyway, it’s a minor and mostly a semantic point.

The results from ATLAS were a bit of a shock.  In all three processes on which ATLAS reported, CMS has presented results already, and in each case CMS saw a small excess (1 standard deviation [1"sigma"], which is  small indeed.)  But ATLAS reported today that it sees essentially no excess in any of the three, and even a deficit in one of them for low mass.  This has a big effect.

  • First, it allows ATLAS to exclude a Standard Model Higgs all the way up to 122 GeV/c2 (except for a little window 1 GeV/c2 wide centered at 118) and down to 129 GeV/c2.  The only large window left for the Standard Model Higgs particle is 122-129, more or less centered around the hint at 126 GeV/c2 that they saw in December.
  • But second, the significance of the December hint, when combined with the new data that shows no excesses in these three new processes, drops by about a full standard deviation.  That’s a pretty big drop.

What does it all mean?

I think it basically means, roughly, status quo.  We got some positive information and some negative information today, and none of it is that easy to interpret.  So I think we are roughly where we were before, except that we probably no longer have to worry about any Standard Model Higgs below 122 GeV/c2.  Before today we had a decent hint of a Standard Model-like Higgs particle with a mass around 125 GeV/c2; we still have it.  Let me explain what I mean.

There are easy (relatively!) searches for the Higgs, and there are hard ones.  The easy searches are the ones where the backgrounds are relatively simple and the signal is a narrow peak on a plot.  There are two:

  1. Higgs decaying to  photons
  2. Higgs decaying to two lepton/anti-lepton pairs (often called “four leptons” for short)

Results on these were presented by both ATLAS and CMS back in December.  The hard searches are the ones where the backgrounds are rather complicated and the signal is quite broad, so that a mistake in estimating a background can either create a fake signal or hide a real one.    There are three (mainly) for a lightweight Higgs:

  1. Higgs decaying to a lepton, an anti-lepton, a neutrino and an anti-neutrino
  2. Higgs decaying to a tau lepton/anti-lepton pair
  3. Higgs decaying to a bottom quark/anti-quark pair

These are the three that ATLAS reported on today (where they saw no sign of a Higgs signal), and that CMS presented back in December (and saw a small excess in all three.)  [ATLAS presented a result on the first one in December, but only using part of their data; it showed a small excess at the time, but not now.]  The third process is the main one in which CDF and DZero reported an excess today, though the first one also plays a role in interpreting that excess.

In other words, everything we learned today had to do with the difficult searches — the ones that are hard to perform, hard to interpret, and hard to check.  And everything we learned was 1 or 2 sigma information; not very compelling even statistically.

For this reason,

  • I would not conclude that the new Tevatron results make the 125 GeV Higgs case much stronger
  • I would not conclude that the new ATLAS results make the 125 GeV Higgs case much weaker

For the same reason, when I explained why I was skeptical of the evidence back in December, I told you that in my view the CMS excesses in the difficult searches did not make the case for a 125 GeV Higgs much more compelling.  Since the easy searches at CMS do not show as large excesses as ATLAS’s do, I wasn’t really comfortable with the whole case from CMS.   Their case improved in January, when they added a bit more information from their easy search for two photons.

If, like me, you discount the difficult Higgs searches somewhat relative to the easy Higgs ones, then almost nothing has changed, as far as the current Higgs hints, after today’s up and down information.  The excess in the two easy searches at ATLAS is still there, and there are excesses at CMS at least in the two-photon search.  Even from the beginning, I gave you good reasons to think the ATLAS’s easy-search excesses were a bit larger than they should be, probably due to an upward statistical fluctuation in the background.    Conversely I think now that one should not overstate how bad today’s ATLAS news is for the Higgs hints.  It’s still quite reasonable to think there may be a Standard Model Higgs there at 125 GeV/c2.  There’s some evidence in its favor, and it’s certainly not ruled out at this point. (Whereas now, almost all other masses are.)

So as usual I advise patience and calm and no hyperventilating; the 2012 data will settle the issue.  Either there is a Standard Model Higgs with a mass within a few percent of 125 GeV/c2 , or we’ll soon be fanning out in Phase 2 of the Higgs search, looking for all the other types of Higgs particles that might be out there.