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Seth Zenz | USLHC | USA

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Can the LHC Run Too Well?

Friday, February 3rd, 2012

For CMS data analysis, winter is a time of multitasking. On the one hand, we are rushing to finish our analyses for the winter conferences in February and March, or to finalize the papers on analyses we presented in December. On the other, we are working to prepare to take data in 2012. Although the final decisions about the LHC running conditions for 2012 haven’t been made yet, we have to be prepared both for an increase in beam energy and an increase in luminosity. For example, the energy might go to 8 TeV center-of-mass, up from last year’s 7. That will make all our events a little more exciting. But it’s the luminosity that determines how many events we get, and thus how much physics we can do in a year. For example, if the Higgs boson exists, the number of Higgs-like events we’ll see will go up, and so will the statistical power with which we can claim to have observed it. If the hints we saw at 125 GeV in December are right, our ability to be sure of its existence this year depends on collecting several times more events in 2012 than we got in 2011.

We’d many more events over 2012 if the LHC simply kept running the way it already was at the end of the year. That’s because for most of the year, the luminosity was increasing over and over as the LHC folks added more proton bunches and focused them better. But we expect that the LHC will do better, starting close to last year’s peak, and then pushing to ever-higher luminosities. The worst-case we are preparing for is perhaps twice as much luminosity as we had at the end of last year.

But wait, why did I say “worst-case”?

Well, actually, it will give us the most interesting events we can get and the best shot at officially finding the Higgs this year. But increased luminosity also gives more events in every bunch crossing, most of which are boring, and most of which get in the way. This makes it a real challenge to prepare for 2012 if you’re working on the trigger, because have to sift quickly through events with more and more extra stuff (called “pileup”). As it happens, that’s exactly what I’m working on.

Let me explain a bit more of the challenge. One of the triggers I’m becoming responsible for is trying to find collisions containing a Higgs decaying to a bottom quark and anti-bottom quark and a W boson decaying to an electron and neutrino. If we just look for an electron — the easiest thing to trigger on — then we get too many events. The easy choice is to ask only for higher-energy electrons, but beyond a certain points we start missing the events we’re looking for! So instead, we ask for the other things in the event: the two jets from the Higgs, and the missing energy from the invisible neutrino. But now, with more and more extra collisions, we have random jets added in, and random fluctuations that contribute to the missing energy. We are more and more likely to get the extra jets and missing energy we ask for even though there isn’t much missing energy or a “Higgs-like” pair of jets in the core event! As a result, the event rate for the trigger we want can become too high.

How do we deal with this? Well, there are a few choices:

1. Increase the amount of momentum required for the electron (again!)
2. Increase the amount of missing energy required
3. Increase the minimum energy of the jets being required
4. Get smarter about how you count jets, by trying to be sure that they come from the main collision rather than one of the extras
5. Check specifically if the jets come from bottom quarks
6. Find some way to allocate more bandwidth to the trigger

There’s a cost for every option. Increasing energies means we lose some events we might have wanted to collect — which means that even though the LHC has produced more Higgs bosons, it’s counterbalanced by us seeing fewer of the ones that were there. Being “smarter” about the jets means more time spent by our trigger processing software on this trigger, when it has lots of other things to look at. Asking for bottom quarks not only takes more processing, it also means the trigger can’t be shared with as many other analyses. And allocating more bandwidth means we’d have to delay processing or cut elsewhere.

And for all the options, there’s simply more work. But we have to deal with the potential for extra collisions as well as we can. In the end, the LHC collecting much more data is really the best-case scenerio.

Location, Location, Location

Thursday, January 19th, 2012

If I had to pick one thing that’s definitely better on my old experiment, ATLAS, than on my new experiment, CMS — and especially if I had to pick something I could write publicly without getting into trouble — it would be this: the ATLAS detector is across the street from the rest of CERN. I’m not sure how that was decided, but once you know that, you know where CMS has to be: on the other side of the ring, 5 or 6 miles away. That’s because the detectors have the same goals and need the same beam conditions; two opposite points on the LHC are where a duplicate performance is easiest. The pre-existing caverns from the LEP collider, whose tunnel the LHC now uses, probably also helped determine where the detectors are.

In any case, it used to be that when I wanted to work on my detector, I had only to go across the street. Now I have to drive out of Switzerland and several miles into France. Except, I don’t like driving. So I’ve been working on alternate means of transportation. A few months ago I walked. Last night I had to go to downtown Geneva, so I took the bus. It’s actually pretty good, although the bus stop is a mile away from CMS. There’s also the shift shuttle, which runs from the main CERN site to CMS every 8 hours via a rather roundabout route. And I can bike, once the weather gets better and I get myself a little more road-worthy. To be honest, every option for getting here is much slower than driving, but I enjoy figuring out ways to get places enough that I’m going to keep trying for a while.

I have plenty of chances to try, because I’ll be here in the CMS control room a lot of the time over the next few weeks. Right now, I’m learning and helping with the pixel detector calibration effort. (We’re changing the operating temperature, so all the settings have to be checked.) Soon I’ll be learning to take on-call shifts. So the more I stay here, the more I learn. I got here this morning, and I won’t leave tonight until about 11 pm. I could take the shift shuttle back — or maybe I’ll just get a ride.

Numerical Family Connections

Wednesday, December 21st, 2011

Just a brief random thought at the start of the first winter break in my life where I’m not visiting or living with my parents… Whenever I need the number π — that is, the ratio between a circle’s circumference and its diameter — in computer analysis code I’m writing, I always write it out like this:

3.141592654

That’s not exactly π, but it’s quite close. What I really should do is look up where it’s already defined in the math library I’m using, but this is more than accurate enough for any reasonable purpose. It’s too many digits, in fact, although I know a few more. So why do I always write out exactly that many places? Well, after thinking about it for a minute a little while ago, I remembered the answer: it’s the number of digits of π my dad taught me when I was a kid.

Walking Across the LHC

Monday, November 28th, 2011

About a month ago, I walked back to Saint-Genis-Pouilly, France from the CMS experiment site after my last meeting of the day, which basically amounts to walking the width of the LHC ring: about 6 miles. Here are a few pictures from the walk:

More pictures, and commentary, on Google+…

Have we Found the Higgs Yet?

Monday, November 21st, 2011

Along with a bunch of important people who actually know how to give interviews, I answer that question in this video:

The video goes along with this Nature News article. You may also be interested in the recent combined ATLAS and CMS Higgs result, which uses only the first half of this year’s data.

By the way, when I talk about a “minimal Higgs, that only does the part we know that something like the Higgs has to do,” I’m referring to the so-called fermiphobic Higgs. It plays the usual role of the Standard Model Higgs boson in breaking electroweak symmetry, but doesn’t couple to quarks and leptons (i.e. fermions). We already know from the way the weak and electromagnetic forces work that the relationship between them has its origins in something like the Higgs — but we have less reason to be certain that the same particle takes care of quark and lepton masses too. This version of the Higgs boson is more difficult to find, but perfectly sensible, and we’ll probably hear a lot more about it in coming years if we don’t have a big discovery this year or next.

My Science Scout Badges

Thursday, November 10th, 2011

For translations, click or roll over each badge, or see the web page of the Order of the Science Scouts of Exemplary Repute and Above Average Physique.

Wild West Week at CERN

Tuesday, October 25th, 2011

"The Buffalo Head is back in R1, that is all." -- John PenwellFrom time to time, the company that runs the CERN restaurants sets up a theme week. This week they are hosting one of their most elaborate: the Wild West. As you can see at left, they have wheeled a buffalo head into the restaurant. A few more decorations are below.

For Europeans, the Wild West seems to be one of the commonly referenced themes from American culture. Perhaps they think that it reflects our national character even in the present day, or perhaps it’s just a very striking setting. I can’t quite imagine the Fermilab cafeteria putting up the equivalent — French Revolution Week, perhaps, complete with guillotine — but it’s all in good fun.

Faster-than-Light Neutrinos: Case Not Closed Yet

Wednesday, October 19th, 2011

To start, let me say that there are extremely strong reasons to believe that the OPERA experiment’s measurement of neutrinos travelling faster than light is flawed. We knew that from the moment it came out, because it contradicts General Relativity (GR), which is an extraordinarily well-tested theory. Not only that, but the most obvious ways to modify GR to allow the result to be true give you immediate problems that contradict other measurements. To my knowledge, there’s no complete theoretical framework that makes predictions consistent with existing tests of GR and allows the OPERA result to be right.

But in my view of how experimental physics is done, history has shown us that once in a great while, something is discovered that nobody thought of and nobody can fit into the existing theoretical mold. The measurements that led to the discovery of GR in the first place provide a good example of this. Such shifts are extremely rare, but I don’t like the idea of ignoring a result because it doesn’t fit with the theories we have.

No, we have to address the measurement itself, and satisfy ourselves that there really was a mistake. There are many ideas for what might have gone wrong, and as far as I know, the discussion is ongoing. I’m not an expert on it, but I know enough to disagree with some of the blogosphere discussion lately that has pronounced that the case is closed. There seem to be two categories of claims going around:

  1. Articles that point out that the OPERA result is inconsistent with other measurements, as in this piece by Tommaso Dorigo (who is, incidentally, my colleague now that I’ve joined CMS). These are of course correct within the context of GR or any straightforward modifications thereof, as I said right at the start of this post. The question is whether there’s some modification that can accomodate the results consistently, and that’s a very hard thing to exclude. (There is some good discussion in the comments of Tommaso’s post about this, in fact.)
  2. Articles that the OPERA result has been refuted because someone posted an idea on the arXiv server. A current example is this preprint, which asserts that a 60 nanosecond delay might be explained by OPERA having made a relatively trivial mistake in their GPS calculations. Of course, it’s possible that a trivial mistake has been made. But I’m not inclined to consider it definitive, especially because the author has already partially backpedaled upon learning more about how GPS works.


It’s great that people are sending ideas for what might have gone wrong with the result, or how it might be explained. But let’s wait for the discussion to settle down — and, indeed, for OPERA to finalize their paper — before we conclude that the case is closed. I do expect the result to be disproven, but what I want to see is one of these things:

  1. OPERA finds that there really was a problem with their measurement, revises it, and the “superluminal” effect goes away.
  2. Another experiment makes the same measurement, and gets a result consistent with GR.


Either way, I’ll consider the case closed, but there’s no reason to get ahead of ourselves. Doing science usually doesn’t mean knowing the answer in time for tomorrow’s news.

Lost in Acronym Translation

Thursday, October 13th, 2011

My first impression, once I got myself properly into the CMS databases and joined the requisite forty or so mailing lists, was that CMS has a lot more acronyms than I was used to. Particularly jarring were the mysterious PVT (“Physics Validation Team”) meetings, and the many occurrences of “PU” (“pileup“) always looked to me like “Princeton University” until I realized that made no sense in context.

But then I remembered all the acronyms on ATLAS, and learned that “PU” has gotten more common there too now that the increasing pileup is a frequent subject of discussion. (I really wasn’t paying attention generally to either ATLAS or CMS for the year where I did my analysis and wrote my thesis.) So although the culture of acronym use may be a bit different, it’s really just a matter of translating from one experiment’s terms to another.

For example, I recently learned that a JSON (“JavaScript something something”) file indicates which LumiSections (not an acronym, oddly) are good in a set of runs — in other words, for which times are the recorded data for all parts of CMS in good shape? On ATLAS, it would have been a GRL (“good run list”) indicating which LumiBlocks were good.

I still think that acronyms are thrown around in conversation a bit more on CMS than on ATLAS. Fortunately, there is a public list of CMS acronyms to help me. I’m sure I’ll figure them out eventually.

Turning to the Dark Side

Monday, October 3rd, 2011

“So, you’ve turned to the dark side?” I’ve heard it surprisingly often, usually from my new colleagues on CMS. “Yes,” I reply. “My hate makes me powerful.”

We’re just kidding, of course.

I’ve been asked more seriously, on a number of occasions, why I switched from working with ATLAS to working with CMS. There are several ways I can answer that one:

1. Why not? ATLAS and CMS both look for the same exciting things at the LHC: the Higgs boson, supersymmetry, and all sorts of other new physics. They have roughly similar capabilities and, for the most part, conceptually similar designs. So I should be happy to work on either one.

2. It came with the job. Being happy to work on either experiment means I applied to some groups working on ATLAS and some on CMS. The job I ended up with is with Princeton, and they have a CMS group, so…

3. It’s good for our field to exchange techniques and expertise between experiments.

4. It’s good for me to know people from both collaborations and learn different ways of doing things, and good to be forced into doing something completely different than what I did as a graduate student.

So why would switching be a bad idea? Well, mostly, it’s harder. There is more logistics to deal with to get started as a postdoc — on top of the logistics of starting a job — and a lot of time spent learning new software and new organization. And it will take me quite a bit longer to be in a position where I know enough and people have enough confidence in my work to give me significant responsibilities. But all of this, I hope, is transitory.

In the end, neither experiment is the dark side. They do compete with each other — as intended, to keep everyone working hard — but they’re more like opposing sports teams than opposite sides of the Force. You may despise the team across town much of the time, but without them you couldn’t play baseball. And once in a while, players get traded.