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Ken Bloom | USLHC | USA

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Your summer travel options

Friday, June 14th, 2013

Now that summer is fully here, are you feeling that old wanderlust, the desire to hit the open road? Well then, there are a lot of interesting places to go on the physics conference circuit between now and Labor Day. There are many fabulous locations on the menu, and who knows, you might get to hear the first public presentation of an exciting new physics result. While it’s true that what many would consider the most glamorous stuff from the LHC has already been pushed out (at the highest priority), you can be assured that scientists are hard at work on new results, and of course there are many other particle-physics experiments that are doing important work. So, find your frequent-flyer card and make sure you’ve changed the oil, and let’s see where you might be headed this summer:

  • 2013 Lepton Photon Conference, San Francisco, CA, June 24-29, hosted by SLAC. This is definitely the most prestigious conference this year; it is the international conference that is the odd-numbered year complement to the ICHEP meetings that are held in even-numbered years. Last year’s ICHEP saw the announcement of the observation of the Higgs boson, and if someone wants to make a big splash this year, they will do it at Lepton Photon. I have previously discussed how ICHEP works; the Lepton Photon series has a similarly storied history, but is slightly different in format, in that there are only plenary overview talks rather than a series of shorter, more focused presentations. San Francisco is always a great destination, and a fine place to consider the physics of the cable car and plate tectonics.
  • 2013 European Physical Society Conference on High Energy Physics, Stockholm, Sweden, July 18-24. If results aren’t ready in time for Lepton Photon, they could be ready in time for EPS. This conference also appears in odd-numbered years, and with a format that has both parallel and plenary sessions, there are many opportunities for younger people to present their work. It is probably the premier particle-physics conference in Europe this year. Thanks to the tilted axis of the earth, and the position of Stockholm at 59 degrees north of the equator, you’ll be able to enjoy 17 hours and 40 minutes of daylight each day at this conference…starting at 4 AM each morning.
  • Community Summer Study 2013, aka Snowmass on the Mississippi, Minneapolis, MN, July 29-August 6. This isn’t really a conference, but it is the culmination of the year-long effort of the US particle-physics community to define its long-range plan. With the discovery of the Higgs boson and important developments neutrino physics, we have better clues on what we should be trying to study in the future. Now we have to understand what facilities are best for this science, and what the technical barriers are to building and exploiting them. But we have to realize that we’re working with a finite budget, and we’ll have to do some hard thinking to understand how to set priorities. You might think that Minneapolis doesn’t have much on San Francisco or Stockholm, but my wife is from there, so I have traveled there many times and I think it’s a great place to visit. You can contemplate the balancing forces and torques on the “Spoonbridge and Cherry” sculpture at the Walker Art Center, or the aerodynamics of Mary Tyler Moore’s hat on the Nicollet Mall.
  • 2013 Meeting of the American Physical Society Division of Particles and Fields, Santa Cruz, CA, August 13-17. Like the EPS conference, DPF also meets in odd-numbered years and is a chance for the US particle physics community to gather. It’s one of my favorite conferences, with a broad program of particle physics and neither too big or too small. It is especially friendly to younger people presenting their own work. Measurements that weren’t ready for the earlier conferences could still get a good audience here. Yes, you might have gone to nearby San Francisco in June, but Santa Cruz has a totally different feel, and you can study the hydrodynamics that power the redwood trees that are all over the campus.

    And you might ask, where am I going this summer? I’d love to get to all of these, but I have another destination this summer — I will be moving my family to Geneva for a sabbatical year at CERN in July. It’s a little disappointing to be missing some of the action in the US, but I’m looking forward to an exciting year. I will be returning to the US for the Snowmass workshop, where I’m co-leading a working group, but that’s about it for conferences for me this summer. That will still be plenty exciting, and I’ll do my best to report all the news about it here.

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  • Place your bets: 25 or 50?

    Thursday, May 23rd, 2013

    Note to readers: this is my best attempt to describe some issues in accelerator operations; I welcome comments from people more expert than me if you think I don’t have things quite right.

    The operators of the Large Hadron Collider seek to collide as many protons as possible. The experimenters who study these collisions seek to observe as many proton collisions as possible. Everyone can agree on the goal of maximizing the number of collisions that can be used to make discoveries. But where the accelerator physicists and particle physicists might part ways over just how those collisions might best be delivered.

    Let’s remember that the proton beams that circulate in the LHC are not a continuous current like you might imagine running through your electric appliances. Instead, the beam is bunched — about 1011 protons are gathered in a formation that is about as long as a sewing needle, and each proton beam is made up of 1380 such bunches. As the bunches travel around the LHC ring, they are separated by 50 nanoseconds in time. This bunching is necessary for the operation of the experiments — it ensures that collisions occur only at certain spots along the ring (where the detectors are) and the experiments can know exactly when the collisions are occurring and synchronize the response of the detector to that time. Note that because there are so many protons in each beam, there can be multiple collisions each time two bunches pass by each other. At the end of the last LHC run, there were typically 30 collisions that occurred per bunch crossing.

    There are several ways to maximize the number of collisions that occur. Increasing the number of protons in each bunch crossing will certainly increase the number of collisions. Or, one could imagine increasing the total number of bunches per beam, and thus the number of bunch crossings. The collision rate increases like the square of the number of particles per bunch, but only linearly with the number of bunches. On the face of it, then, it would make more sense to add more particles to each bunch rather than to increase the number of bunches if one wanted to maximize the total number of collisions.

    But the issue is slightly more subtle than that. The more collisions that occur per beam crossing, the harder the collisions are to interpret. With 30 collisions happening at the same time, one must contend with hundreds, if not thousands, of charged particle tracks that cross each other and are harder to reconstruct, which means more computing time to process the event. With more stuff going on each event, the most important parts of the event are increasingly obscured by everything else that is going on, degrading the energy and momentum resolution that are needed to help identify the decay products of particles like the Higgs boson. So from the perspective of an experimenter at the LHC, one wants to maximize the number of collisions while having as few collisions per bunch crossing as possible, to keep the interpretation of each bunch crossing simple. This argument favors increasing the number of bunches, even if this might ultimately mean having fewer total collisions than could be obtained by increasing the number of protons per bunch. It’s not very useful to record collisions that you can’t interpret because the events are just too busy.

    This is the dilemma that the LHC and the experiments will face as we get ready to run in 2015. In the current jargon, the question is whether to run with 50 ns between collisions, as we did in 2010-12, or 25 ns between collisions. For the reasons given above, the experiments generally prefer to run with a 25 ns spacing. At peak collision rates, the number of collisions per crossing is expected to be about 25, a number that we know we can handle on the basis of previous experience. In contrast, the LHC operators generally to prefer the 50 ns spacing, for a variety of operational reasons, including being able to focus the beams better. The total number of collisions delivered per year could be about twice as large with 50 ns spacing…but with many more collisions per bunch crossing, perhaps by a factor of three. This is possibly more than the experiments could handle, and it could well be necessary to limit the peak beam intensities, and thus the total number of collisions, to allow the experiment to operate.

    So how will the LHC operate in 2015 — at 25 ns or 50 ns spacing? One factor in this is that the machine has only done test runs at 25 ns spacing, to understand what issues might be faced. The LHC operators will re-commission the machine with 50 ns spacing, with the intention of switching to 25 ns spacing later, as soon as a couple of months later if all goes well. But then imagine that 50 ns running works very well outset. Would the collision pileup issues motivate the LHC to change the bunch spacing? Or would the machine operators just like to keep going with a machine that is operating well?

    In ancient history I worked on the CDF experiment at the Tevatron, which was preparing to start running again in 2001 after some major reconfigurations. It was anticipated that the Tevatron was going to start out with a 396 ns bunch spacing and then eventually switch over to 132 ns, just like we’re imagining for the LHC in 2015. We designed all of the experiment’s electronics to be able to function in either mode. But in the end, 132 ns running never happened; increases in collision rates were achieved by increasing beam currents. This was less of an issue at the Tevatron, as the overall collision rate was much smaller, but the detectors still ended up operating with numbers of collisions per bunch crossing much larger than they were designed for.

    In light of that, I find myself asking — will the LHC ever operate in 25 ns mode? What do you think? If anyone would like to make an informal wager (as much as is permitted by law) on the matter, let me know. We’ll pay out at the start of the next long shutdown at the end of 2017.

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    Shutdown? What shutdown?

    Sunday, March 24th, 2013

    I must apologize for being a bad blogger; it has been too long since I have found the time to write. Sometimes it is hard to understand where the time goes, but I know that I have been busy with helping to get results out for the ski conferences, preparing for various reviews (of both my department and the US CMS operations program), and of course the usual day-to-day activities like teaching.

    The LHC has been shut down for about two months now, but that really hasn’t made anyone less busy. It is true that we don’t have to run the detector now, but the CMS operations crew is now busy taking it apart for various refurbishing and maintenance tasks. There is a detailed schedule for what needs to be done in the next two years, and it has to be observed pretty carefully; there is a lot of coordination required to make sure that the necessary parts of the detector are accessible as needed, and of course to make sure that everyone is working in a safe environment (always our top priority).

    A lot of my effort on CMS goes into computing, and over in that sector things in many ways aren’t all that different from how they were during the run. We still have to keep the computing facilities operating all the time. Data analysis continues, and we continue to set records for the level of activity from physicists who are preparing measurements and searches for new phenomena. We are also in the midst of a major reprocessing of all the data that we recorded during 2012, making use of our best knowledge of the detector and how it responds to particle collisions. This started shortly after the LHC run finished, and will probably take another couple of months.

    There is also some data that we are processing for the very first time. Knowing that we had a two-year shutdown ahead of us, we recorded extra events last year that we didn’t have the computing capacity to process in real time, but could save for later analysis during the shutdown. This ended up essentially doubling the number of events we recorded during the last few months of 2012, which gives us a lot to do. Fortunately, we caught a break on this — our friends at the San Diego Supercomputer Center offered us some time on their facility. We had to scramble a bit to figure out how to include it into the CMS computing system, but now things are happily churning away with 5000 processors in use.

    The shutdown also gives us a chance to make relatively invasive changes to how we organize the computing without potentially disrupting critical operations. Our big goal during this period is to make all of the computing facilities more flexible and generic. For the past few years, particular tasks have often been bound to particular facilities, in particular those that host large tape archives. But that can lead to inefficiencies; you don’t want to let computers remain idle at one site just while another site is backed up because it has particular features that are in demand. For instance, since we are reprocessing all of the data events from 2012, we also need to reprocess all of the simulated events, so that they match the real data. This has typically been done at the Tier-1 centers, where the simulated events are archived on tape. But recently we have shifted this work to the Tier-2 centers; the input datasets are still at the Tier 1′s, but we read them over the Internet using the “Any Data, Anytime, Anywhere” technology that I’ve discussed before. That lets us use the Tier 2′s effectively when they might have been otherwise idle.

    Indeed, we’re trying to figure out how to use any available computing resource out there effectively. Some of these resources may only be available to us on an opportunistic basis, and taken away from us quickly when they are needed by their owner, on the timescale of perhaps a few minutes. This is different from our usual paradigm, in which we assume that we will be able to compute for many hours at a time. Making use of short-lived resources requires figuring out how to break up our computing work into smaller chunks that can be easily cleaned up when we have to evacuate a site.

    But computing resources include both processors and disks, and we’re trying to find ways to use our disk space more efficiently too. This problem is a bit harder — with a processor, when a computing job is done with it, the processor is freed up for someone else to use, but with disk space, someone needs to actively go and delete files that aren’t being used anymore. And people are paranoid about cleaning up their files, in fear of deleting something they might need at an arbitrary time in the future! We’re going to be trying to convince people that many files on disk aren’t getting accessed, and it’s in our interest to automatically clean them up to make room for data that is of greater interest, with the understanding that the deleted data can be restored if necessary.

    In short, there is a lot to do in computing before the LHC starts running again in 24 months, especially if you consider that we really want to have it done in 12 months, so that we have time to fully commission new systems and let people get used to them. Just like the detector, the computing has to be ready to make discoveries on the first day of the run!

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    Higgs to light video comes to light

    Thursday, January 31st, 2013

    Just a quick note here on something that isn’t really mine: CMS has now released some video footage from the internal meetings where the results of the search for a Higgs particle decaying to a pair of photons (light) were first presented to the collaboration. I think it’s pretty interesting to watch this little bit of science history.

    Here is the context: the Higgs searches were done “blind”, in that every little bit of the analysis was done without examining the actual detector data sample where the Higgs might be observed. Using simulations and data samples that are similar to, but not actually, the data in question are used to design the Higgs search, to understand what the experimental uncertainties are, and to give an expectation of what would be seen in the data if there were a Higgs (or not). Everyone avoids looking at the key data samples to avoid biasing the search based on what is seen. (The fear is that if you see a small signal, you might start to make changes in the analysis to enhance the signal…which could turn out to be a statistical fluctuation in the end.)

    Then, in the late stages of the data analysis, we finally take a look at the “signal” sample. Of course, someone has to be the first person to do this, which means that for a brief moment, that’s the only person in the world who knows a new scientific fact. And then there is a lot of suspense for everyone else! In the video, someone who was among the first to see the result, just hours beforehand, is presenting it to the rest of the collaboration. You can certainly see how excited the presenters are about that moment.

    I suppose there isn’t any suspense now, since we know what the answer is, but try to put yourself in the mindset of the audience in the room…and enjoy!

    CMS video Higgs unveiling

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    It’s a wrap: proton Run 1 ends

    Sunday, December 16th, 2012

    On Monday at 6 AM CERN time, the LHC ended its collisions of protons for 2012, and in fact until 2015, when the “long shutdown” for energy upgrades is completed. [There will be heavy-ion collisions in early 2013, but the details are beyond my expertise.] Here’s what appeared on the LHC status screen:

    It’s the end of an era for the LHC, the end of what we might someday call “Run 1″, the period of first beams at (relatively) low energies, when we got our first glimpse of a new energy scale, and gathered just enough data to see the first glimmerings of (maybe) the Higgs boson. Considering how long we waited for the start of Run 1 — nearly twenty years from the first concepts for the the LHC and its detectors — it is rather amazing that we’re now at the end of the run, after a mere three years.

    Still, it’s been a great three years. Here is the plot that captures the whole story:

    LHC integrated luminosity summary

    This is the integrated luminosity recorded by CMS, essentially the number of collisions that the experiment observed, year by year. Remember all the excitement of the first data in 2010? That turned out to be a tiny amount of data compared to what we have recorded since; while we made very good use of it at the time, it was just hinting at the future success of the LHC. And even after the great advances in 2011, by the start of June 2012 we had recorded more data this year than we had in all of last year. Once again, all the experimenters thank the LHC team for the excellent performance of this still new machine.

    The last few days of the proton run were spent looking towards the future. Since there won’t be any more proton collisions for two years, it’s important to do some tests that can guide our thinking about how to operate the LHC in 2015. So far, the LHC has run with “50 ns bunch spacing”; that is, the minimum time between bunch crossing is 50 nanoseconds. (Remember, the LHC beam is not continuous, but “bunched”, with a large number of protons close together in the beam, followed by a 50-foot gap before the next bunch in the beam.) This week, the LHC experimented with 25 ns bunch spacing, and even allowed the experiments to take a little bit of data in this mode on Saturday night and Sunday morning. Obviously, with the shorter bunch spacing, you can have beam collisions happening twice as often, and that means that you could potentially achieve the same total number of collisions with fewer protons per bunch. That’s good for the experiments, as each event that we record will have fewer collisions in it, making it easier for us to reconstruct what went on. With 25 ns spacing, we’d probably need less computing capacity and calibration and the like would be easier. But from the accelerator perspective, it is easier to operate the LHC with 50 ns spacing, and the machine operators can’t guarantee that they could provide as much integrated luminosity at 25 ns spacing as the could with 50 ns. Thus, it was important to take some time to understand how to operate the LHC this way. It’s ultimately up to the LHC managers to decide what the best mode for operations is. From the experiment side, it would be easier for us to have 25 ns spacing, but we wouldn’t want to do that at the cost of less data, and perhaps missing a chance of a discovery as a results.

    Meanwhile, what does a 3000-member collaboration do with itself when there is no data to record? (Besides sending and reading email.) Quite a lot. First, there are a number of upgrades, repairs and improvements to be made on the detector in the next two years. There is a carefully choreographed dance to be performed in the collision hall, where the CMS detector must be opened up for access to the different components, and the schedule for all the work to be done could be pretty tight. There are also preparations to be made for how we analyze the data in 2015. The environment will be a lot like in 2010: we’ll be at a new beam energy, and in a physics environment that we’ve never seen before, so we’ll have to be ready for anything that might appear in the data. And we will continue our studies of the fabulous three years of data already recorded. During the past three years, the collaborations have released multiple papers on particular topics, with increases in the amounts of data analyzed each time and improvements in analysis techniques. But the next round of papers will use the full dataset, and there won’t be any “next” papers. The analysis techniques then must be the best possible; there won’t be another shot for improvements, as the next word will be the final word, at least until 2015. This too will take a lot of effort from the scientists.

    Congratulations to everyone on a successful Run 1, and let’s look ahead to a busy shutdown and an exciting Run 2 beyond!

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    Foxes, hedgehogs and particle physicists

    Sunday, November 11th, 2012

    I’m just back from a trip to CERN, which was mostly for a week of meetings about how well the computing for the CMS experiment is doing and how it could be done better. But meanwhile, the collaboration was also working through the scrutiny of new measurements that are targeted to be released for the Hadron Collider Physics conference that starts tomorrow (I guess today, given the time zone) in Tokyo. Obviously I can’t discuss these results yet. So instead I’ll spend a little time on philosophy, which I admit makes this a much less interesting post. But bear with me.

    In case you’ve been hiding under a rock for the last week, you should know that Nate Silver of the FiveThirtyEight blog made another successful prediction of a presidential election outcome, state by state. I’ve written about Nate Silver’s work here before, because I admire his adoption of what I think is a particle-physics kind of approach to making predictions.

    So, being in a Nate Silver kind of mood as I headed off on my trip, I bought a e-copy of his new book, “The Signal and the Noise,” to read on the plane. I’m not sure that I’d call it a great work of literature, but Silver does have some very interesting things to say about how to make predictions. In one section he reminds us of the classic Isaiah Berlin essay, “The Hedgehog and the Fox.” And in case you have been hiding under a different rock, that refers to a quote from Archilochus, who observed that “the fox knows many things, but the hedgehog knows one big thing.” Hedgehogs view the world through the prism of a single big conceptual framework, while foxes don’t believe that’s possible and are willing to be more flexible in their approaches. Silver asserts that it’s the foxes of the world who make better predictions. You have to be willing to try many different approaches and integrate many different tactics to make a good prediction, and, perhaps most importantly, to be prepared to adapt to new information and to change your ideas when your current framework isn’t working,

    This got me thinking: are particle physicists foxes or hedgehogs? I would say some of both. Our hedgehog-ness is in our belief in physical law. That’s a big idea that is unavoidable. It is true that our knowledge of physics is always subject to revision in the face of new information, but we believe that in circumstances that have already been well-explored through experiment, physical laws hold without question. Certainly the much-revered standard model of particle physics is taken as a given in regimes where it has been thoroughly tested. And at the very least, we believe in physical law as a big, consistent framework at least as an ideal, if not something that we can truly realize.

    But in terms of our approaches to experiment, we have to be foxes. I can say this about some of the results that will be shown at the HCP conference — these are hard measurements, and to get them done, we’ve had to use every trick in the book. A huge variety of techniques have been brought to bear to wring every last bit of useful information out of the data, and it has taken a gargantuan effort from a large team of people. I always come out of the detailed presentations of a measurement somewhat stunned by its complexity. We’re also always on the lookout for new and better tricks. No matter how good an idea sounds on paper, if it isn’t effective in making a measurement, or is less effective than other ideas, then you abandon it and find something better. It’s this flexibility and willingness to evolve and change that helps us do this work.

    As a younger person, I saw myself as at least an aspiring hedgehog, hoping to find the one big idea that would pull everything together and give me a complete grasp of the world. But I’ve come to realize that life, and science, is more complicated than that, and you have to be a fox just to get through it all.

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    “Snowmass” (Not Snowmass)

    Saturday, October 13th, 2012

    Every so often, perhaps once or twice a decade, particle physics in the United States comes to some kind of a crossroads that requires us to think about the long-term direction of the field. Perhaps there is new experimental data that is pointing in new directions, or technology developments that make some new facility possible, or we’re seeing the end of the previous long-term plan and it’s time to develop the next one. And when this happens, the cry goes up in the community — “We need a Snowmass!”

    Snowmass refers to Snowmass Village in Colorado, just down the road from Aspen, the home of the Aspen Center for Physics, a noted haunt for theorists. During the winter, Snowmass a ski resort. During the summer, it’s a mostly empty ski resort, where it’s not all that expensive to rent some condos and meeting rooms for a few weeks. Over the past few decades there have been occasional “summer studies” held at Snowmass, typically organized by the Division of Particles and Fields of the American Physical Society (and sponsored by a host of organizations and agencies). It’s a time for the particle-physics community to come together for a few weeks and spend some quality time focusing on long-range planning.

    The last big Snowmass workshop was in 2001. At the time, the Fermilab Tevatron was just getting started on a new data run after a five-year shutdown for upgrades, and the LHC was under construction. The top quark had been discovered, but was not yet well characterized. We were just beginning to understand neutrino masses and mixing. The modern era of observational cosmology was just beginning. A thousand physicists came to Snowmass over the course of three weeks to plot the future of the field. (And I was a lot younger.) Flash forward eleven years: the Tevatron has been shut down (leaving the US without a major high-energy particle collider), the LHC is running like gangbusters, we’re trying to figure out what dark energy is, and just in the past year two big shoes have dropped — we have measured the last neutrino mixing angle, and, quite famously, observed what could well be the Higgs boson. So indeed, it is time for another Snowmass workshop.

    This week I came to Fermilab for a Community Planning Meeting for next year’s Snowmass workshop. Snowmass 2013 is going to be a bit different than previous workshops in that it will not actually be at Snowmass! Budgetary concerns and new federal government travel regulations have made the old style of workshop infeasible. Instead, there will be a shorter meeting this summer hosted by our colleagues at the University of Minnesota (hats off to thee for having us), so this time we won’t have as much time during the workshop to chew over the issues, and more work will have to be done ahead of time. (But I suspect that we’re still going to call this workshop “Snowmass”, just as the ICHEP conference was “the Rochester conference” for such a long time, even if it’s now the “Community Summer Study”.)

    This Snowmass is being organized along the three “frontiers” that we’re using to classify the current research efforts in the field — energy, intensity and cosmic. As someone who works at the LHC, I’m most familiar with what’s going on at the energy frontier, and certainly there are important questions that have only come into focus this year. Did we observe the Higgs boson at the LHC? What more do we have to know about it to believe that it’s the Higgs? What are the implications of not having observed any other new particles yet for particle physics and for future experiments? The Snowmass study will help us understand how we answer these questions, and specifically what experiments and facilities are needed to do so. There are lots of interesting ideas that are out there right now. Can the LHC tell us what we need to know, possibly with an energy or luminosity upgrade? Is this the time to build a “Higgs factory” that would allow us to study measure Higgs properties precisely? If so, what’s the right machine for that? Or do we perhaps need an accelerator with even greater energy reach, something that will help us create new particles that would be out of reach of the LHC? What kind of instrumentation and computing technologies are needed to make sense of the particle interactions at these new facilities? The intensity and cosmic frontiers have equally big and interesting questions. I would posit that the scientific questions of particle physics have not been so compelling for a long time, and that it is a pivotal time to think about what new experiments are needed.

    However, we also have the bracing reality that we are looking at these questions in a budget environment that is perhaps as constrained as it has ever been. Presentations from our champions and advocates at the Department of Energy and the National Science Foundation, the agencies that fund this research (and that sponsor the US LHC blog) were encouraging about the scientific opportunities but also noted the boundary conditions that arise from the federal budget as a whole, national research priorities, and our pre-existing facilities plan. It will continue to be a challenge to make the case for our work (compelling as it may be to us, and to someone who might be interested in looking at the Quantum Diaries site) and to envision a set of facilities that can be built and used given the funding available.

    The first (non-native) settlers of Snowmass, Colorado, were miners, who were searching for buried treasure under adverse conditions. They were constrained by the technology of the time, and the facilities that were available for their work. I shouldn’t suggest that what we are doing is exactly like mining (it’s much safer, for one thing), but hopefully when we go to Snowmass (or really “Snowmass”) we will be figuring out how to develop the technology and facilities that are needed to extract an even greater treasure.

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    The LHC sneaks along, part 2

    Saturday, September 1st, 2012

    It’s Labor Day weekend. You’ve probably been on vacation sometime in the past month. So have a lot of physicists (and a lot of bloggers). But the LHC hasn’t been on vacation, by any means. As we last saw, the accelerator was running flat out to produce enough collisions to give us a shot at a Higgs-boson observation. Now we know that it worked; the Higgs results that the CMS and ATLAS experiments released had made use of data that had been collected through the middle of June, and that was enough to claim a discovery. But here’s what’s happened since:

    (This plot is a direct link from the LHC luminosity page; it will get updated to the latest version if you read this post sometime later.) Since a technical stop in late June, the LHC has roughly doubled the number of collisions provided. In fact, about a week ago the LHC achieved its highest collision rate ever, which should allow us to accelerate the production of integrated luminosity. We have three months left in the proton-proton run (before a one-month heavy-ion run, and then a two-year shutdown), and we can be optimistic about how much more data we might record in that time.

    What are the implications of doubling the size of the dataset? Here is a totally unofficial, totally back-of-the-envelope estimate. In a perfect world, uncertainties due to counting statistics, i.e. the amount of data you are using to make a measurement, fall like the square root of the number of events. Thus, a doubling of the data should result in reducing your uncertainties by a factor of the square root of two, or about 1.4. In our imperfect world, it’s a lot more complicated than that — the uncertainty on a measurement comes from more than just counting statistics. But let us suspend disbelief for a moment and consider the case of the measurement of the probabilities for the presumed Higgs boson to decay into its various final states. Here are the CMS measurements, based on the data that was in hand for the publications that have been submitted:

    A value of one on the x axis would constitute a measurement in agreement with the predictions of the standard model. With the uncertainties shown here, you would say that at the very least the measurements do not disagree with the predictions. But now imagine those same error bars reduced by 40%, while the central values stay in the same place. Then the probability to decay to photons would start to look discrepantly large, while that for taus would look discrepantly small, and that would start getting really interesting — perhaps the “Higgs” we’re observing is not the standard-model Higgs.

    Of course, this is pure speculation — when the additional data is incorporated into the analysis, all the points might start moving closer to the expected values. But the additional data we are recording will help make the picture more clear no matter what. 2012 has already been an exhilarating year, but as we head into the final one-third of it, we can imagine that it will get more exciting still, thanks to the excellent operation of the Large Hadron Collider.

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    The destiny of boson observation papers

    Thursday, August 2nd, 2012

    On Tuesday, CMS and ATLAS submitted their papers on their observation of a new boson to the journal Physics Letters B. These are surely the most significant publications of the LHC experiments to date, and, without airing too much internal laundry, you can imagine that the content and the phrasing of the papers was very thoroughly discussed within the collaborations. Within CMS, the length of all the comments submitted during collaboration review was longer than the paper itself. You will also notice that CMS and ATLAS came up with slightly different titles; one says that a boson was observed, the other says that a particle (spin unspecified) was observed in a search for the Higgs boson. And for sure neither one says that what is observed is the Higgs boson; as has been discussed in many other posts, we’re very far away from being able to make any confident statements about that.

    We can expect that these papers will soon be accepted for publication (in fact, sooner than you might think), and then go on to be fixtures of the scientific literature of particle physics, cited many times over in future papers. Which got me thinking — what are the most highly cited papers in particle physics, and where might the “Higgs” observation papers end up in that list? (Note how he takes pains to put “Higgs” in quotation marks!)

    Now, you’ve heard me sing the praises of the Particle Data Group before, but now let me put in a word for the people at INSPIRE, which has recently succeeded SLAC’s SPIRES database as the repository of publication information in our field. I wouldn’t be able to put my CV together or brag about my crazy-big h-index without them. Not only do they track every paper by author, they also keep track of paper citations. How often a paper is cited is a measure of the impact of the paper on the field.

    It’s not hard to generate a list of the most cited papers tracked by INSPIRE. And the results may surprise you! A few observations:

    1. The most cited papers are theory papers, not papers that describe measurements. The number one paper, with 8414 citations, is by Juan Maldacena, describing a major breakthrough in string theory. (Don’t ask me to explain it, though!) This paper is only 14 years old. Number two, at 7820, is Steven Weinberg’s paper that was among the first to lay out the electroweak theory. It’s from 1967, predating the Maldacena paper by more than thirty years. And number three, at 6784, is by Kobayashi and Maskawa, explaining how a third generation of quarks could straightforwardly accommodate the phenomenon of CP violation; it’s from 1973.
    2. That famous paper by Peter Higgs? Only #95, with 2043 citations.
    3. The first experimental paper that shows up, at #4, is actually an astrophysics paper, the first results from the WMAP satellite, which among other things really nailed down the age of the universe for the first time. There are in fact many highly-cited papers on experimental results on cosmology. This is of course partly a function of the kind of papers that INSPIRE tracks.
    4. The first experimental papers that show up are actually compendia of results, from the PDG. They release a new review every two years, so many of them are on the list.
    5. The most-cited paper on a single experimental measurement is at #27, with 3769 citations. It’s the Super-Kamiokande paper from 1998 that showed the first evidence of the oscillation of atmospheric neutrinos.

    So while it’s true that these observation papers will be among the most highly cited from the LHC experiments, the evidence already suggests that they will be pikers compared to many other publications in the literature. (So was it worth all that effort on what the title should be?) It will be interesting to watch…if nothing else, it will surely be one of the most cited papers that I am an author on, and it is definitely an achievement that we can be proud of.

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    Landmarks

    Wednesday, July 11th, 2012

    landmark (n): 1. An object or feature of a landscape or town that enables someone to establish their location. 2. An event, discovery, or change marking an important stage or turning point in something.

    Several times in his ICHEP 2012 closing presentation today, CERN Director General Rolf Heuer referred to ICHEP 2012 as a “landmark” conference. This inspired me to take a look at the dictionary definition of “landmark.”

    Indeed, the conference seems to fulfill both definitions of the word. First, we have very much defined the location of the field of particle physics. The new particle observed this week, which at the moment appears to have the properties of the Higgs boson, now establishes that the standard model of electroweak symmetry breaking, the main working theory of particle physics for forty years, is correct. Many speakers at the conference who were not explicitly talking about the Higgs still needed to talk about the model, and they all noted with some relief that what they wrote down about the Higgs potential and so forth is now known to be true. (Implicit in all this is the usual scientific caveat that “true” only means “not yet shown to be false,” but please bear with me.) Of course we have long assumed and hoped that it was true, given how much supporting evidence there was for the model all along. But now we know our location: we have a theory that works.

    (I should note that while all the attention lately has been on the Higgs, there has been another major advance this year, and that is the measurement of the neutrino mixing angle θ13 at the Daya Bay nuclear reactor experiment in China, with confirmation in other experiments. This establishes that all elements of the neutrino-mixing matrix are non-zero, allowing for the possibility of CP violation in that system. So our colleagues in the neutrino sector also have a landmark measurement to show for themselves.)

    And most definitely this observation, and the conference where we first learned about it, is also a landmark in the second sense. We now turn our attention to what this discovery means. What are the next set of questions to ask, and how do we go about asking them? Our first job is to do our very best to characterize the “Higgs boson.” Once its mass is established, the standard model fully specifies all of its other properties. Does it decay to the right final states as often as it is supposed to? Various extensions to the standard model predict different values for these “branching ratios.” Does it have the right spin? We know that the spin must be an even integer, but we don’t know if it is zero as predicted. The LHC will continue taking data into February of next year, before a two-year long shutdown. We’re going to need every ounce of data we can get, and all the cleverness we can muster, to answer these questions as accurately as we can. It will keep us busy during the data drought that is about to come.

    I have been spending a lot of time this week thinking about what comes next, especially in terms of future facilities. The LHC is going to be the workhorse of Higgs physics for some time, but it will have its limits. Alas, there are some bad-news landmarks from this conference too: so far, there is no evidence at all for any other new particles beyond the Higgs at this mass scale — no supersymmetry, no exotic fermions or bosons, nothing. We can’t exclude the possibility that even the 13 TeV LHC that will start to run at the end of 2014 might not have enough energy to produce any other new particles. Heuer talked a little about the “high-energy LHC,” which he also noted is really a completely new machine in the same LHC tunnel, but it’s hard to imagine that this happens before 2030. Can we do something else in the meantime? Are there revolutionary, game-changing ideas that we can bring to the table? And, as a writer from the United States, I have to ask — can we build this machine at home?

    Big questions for what we hope is a big new era of particle physics! This ICHEP, the first in the Southern Hemisphere, will truly be remembered as a landmark. I would like to take this opportunity to thank our hosts for all of their work in hosting this remarkable conference in an equally remarkable location.

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