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Burton DeWilde | USLHC | USA

Read Bio

Déménagement

Tuesday, November 1st, 2011

I’ve lived and worked at CERN for two years, and now I’m going away. This is a common story.

When I first moved here from Stony Brook, NY, I was a fresh PhD Candidate who had just finished up a hardware project, acquired a young new advisor, and started learning C++ in a serious way. I had no idea what research I would be doing at CERN.

I spent a couple of months thoroughly lost: in red tape and French bureaucracy; in a labyrinthine, nonsensically-numbered hodge-podge of office buildings and industrial warehouses; in a social scene dominated by physics and physicists; in supermarkets that close at 7pm, roads that go roundabout-to-roundabout, and conversations that start in one language and inevitably end in another.

With the return of beam in the LHC (after a well-publicized accident) came a new sense of urgency and purpose, for both CERN and myself. I remember how the pace of life on-site noticeably picked up, all of us marveling at the screens showing the beams’ status as we sped by on the way to a meeting, or a coffee. I got involved in the ATLAS 3D Pixel Collaboration. I took midnight shifts to help with data-taking on the prototype silicon sensors, jumped into software development on particle track reconstruction, and got started on a short-term analysis project to determine the hit resolution of the sensors, complete with smart, Swedish-made post-doc.

As with most “short-term” projects at CERN, mine became long-term, hindered by unforeseen complications in the data and, at all steps along the way, the analysis framework in which many of us do our work: ROOT. Complaining about this distinctly sadistic piece of software became a favorite pastime! And still is. In the end, my analysis was somewhat inconclusive — so it goes.

Fortunately, my group at Stony Brook was in the process of initiating a more cohesive, aggressive research program, and I got drafted by my advisor into an Exotics search for second-generation leptoquarks. I was able to help build our analysis framework from the ground up, and in the process learned how to code in Python. It was a revelation. Meanwhile, the LHC had begun its 2010 run, and it seemed like our dataset was doubling every other day! These were very exciting times. Nobody knew what we might find in all this data, be it supersymmetry or a Higgs Boson or, maybe maybe maybe, some sort of leptoquark.

The analysis went roughly as expected: An endless series of incremental changes, talks in weekly meetings, unanticipated crises, deadlines, plots, emails, interpersonal conflicts, and soul-crushing hoops to jump through on the way to publication. It was an awful lot of work and stress, all for the best null result in the world. Huzzah. To be honest, it was a bit disheartening that the LHC experiments hadn’t dropped a bombshell on the scientific community, like OPERA’s super-liminal neutrinos measurement or the discovery of a true “goldilocks” planet, but it certainly felt like something was just around the corner.

I went to Cambridge for a conference and Stanford for summer school, dated a native Genevois, visited Paris and Berlin and Rome, got trained as an ATLAS Pixel shifter, celebrated the holidays with friends and family back home, and had the chance to visit the ATLAS detector down in its pit during the annual winter shutdown.

For the LHC’s 2011 run, I basically picked up where I left off with my leptoquark search; it was meant to be a straightforward update. But, of course, nothing is ever as easy as we expect: the beams’ increased luminosity meant much more data but also challenges in simulating and effectively filtering out all the extra events; new software releases fixed some bugs but introduced others; new collaborators meant new interpersonal conflicts (or is it just me?!); and improvements to the analysis itself seldom worked out as nicely, or quickly, as we would have liked. Deadlines have a way of flying by… but that’s research! Or so I’m told.

Meanwhile, I visited New Orleans, Helsinki, and Zurich, got involved with LGBT CERN, filmed, edited, and co-produced a particle-physics-themed zombie movie, and started writing my thesis. ATLAS kept taking more and more data — until just a few days ago.

And that’s it! Two years at CERN. In less than a week, I’m going away — back to New York, to write my thesis full-time, hunt for jobs (decide what sort of job I’m hunting for…), and graduate. It’s hard looking back on a chapter in your life and assessing it for lessons learned and enduring connections made, accomplishments and moments of zen. While I have my share of regrets and what-ifs (why, why did I never finish learning French?!), I feel like I’ve come a long way these past two years. From slightly jaded, I-can’t-wait-to-start-my-analysis junior grad student to thoroughly jaded, I-can’t-wait-to-finish-my-analysis-and-get-out-of-here senior grad student. All these gray hairs must count for something.

Heads-up: This blog is about to get hardcore, thesis-style. But first… an international move, and a long series of good-byes.

Burton

Thesis Advice

Wednesday, September 7th, 2011

Well, I’ve finally started thinking about starting to start writing my PhD thesis. I’m told this is a big deal.

It is known that asking a grad student about the status of his or her thesis, or when he or she plans to graduate, is bad form — practically taboo — and until recently, I applied this golden rule equally to myself as well as people whom I didn’t want to aggravate. Alas, those care-free days are over! The harsh onset of fall (I see the clouds gathering for their annual, six-month layover), the obvious absence of summer students (CERN is notable for many reasons, not least of which is that, at the start of September, all the undergrads leave), and the near-completion of what I consider a polished analysis (my advisor would probably disagree) have all conspired to get me thinking more long-term. And this brought me, kicking and screaming, to my non-existent thesis.

Over the years, and particularly in the last week or so, I’ve accumulated a fair amount of “thesis advice” from more senior grad students and post-docs. Fun fact: Nobody wants to talk about their thesis while they’re writing it (unless to complain about how totally unfair life is), but once they finish, they suddenly become very eager to share their experience with others. This is what I have learned so far:

- Don’t start writing your thesis until you’ve completely finished your analysis and, ideally, published a paper on it. Then start with the analysis section, using your paper as a guide. Try not to plagiarize yourself.
- Write the experimental section of your thesis in the second year of grad school. What you learn about your detector will serve you well in your analysis. Try not to plagiarize others, as there are only so many ways to say “The LHC is a proton-proton collider with a center-of-mass energy of 7 TeV.”
- Why not dance it out?
- The hardest part of your thesis is just getting started. (CHECK!)
- The hardest part of your thesis is writing the introduction, so save it for last.
- The hardest part of your thesis is getting your committee to agree on a date for you to finish.
- Hide “Easter eggs” throughout your thesis, such as figures with dinosaurs used for scale, or phrases not normally seen in scientific writing. Find out how closely your advisor is reading.
- You can write a thesis in about six months.
- You can write a thesis in about three months.
- “I wrote my thesis in two months.”
- “I have to write my thesis in the next five weeks.”
- Start applying for jobs while you write your thesis, so by the time you’re done, you’ll have something to move on to. Don’t graduate before you have a job lined up — you can always delay! Some people do this for years…
- Your thesis title is important! Choose with care.

Okay. So what I’ve learned so far is this: Every thesis, and every person writing a thesis, is unique. What works for one doesn’t work for all. Inevitably, necessarily, you have to find a way through it that works for you, and doesn’t drive you (completely) crazy in the process. Talking to others — perhaps blogging about it? — can help, but in the end, your thesis is what you yourself make out of it.

Whew. The good news is, I have a working title! Leptoquarks: The Particles That Go Both Ways.

– Burton

The Sound of CERN (Now, with sound!)

Monday, August 1st, 2011

Hi, All!

I’ve been absent for a bit, competing in the twice-annual Race to a Conference Publication. It’s a full-out sprint that lasts for… five months. No comment on how I did,  but hey, here’s a fun quotation that is totally not at all in any way related:

I love deadlines. I like the whooshing sound they make as they fly by.

– Douglas Adams

Anywho! Last time I wrote about “The Sound of CERN,” as inspired by a reporter on the hunt for it, but I wasn’t able to share anything more than a description of those sounds. Well, I went out and did some field recordings of my own! So put on your headphones, and listen closely: This is what CERN sounds like. :)

TheSoundOfCern

In order: The ATLAS cooling towers, the CERN computing center, high-voltage power lines outside Building 40, a computer that’s working too hard, coffee machines at Restaurant 1, a conversation in French. Alas, I wasn’t able to track down the flock of sheep with bells on their necks — they have a few different grazing fields, and we only cross paths when I’m without a microphone. Better luck next time… when I’ll include video with the audio?

Burton :D

The Sound of CERN

Monday, June 27th, 2011

I recently had an encounter with an unusual reporter. He had been roaming about CERN in search of a story, and by chance that brought him far afield to the test beam control room at CERN’s SPS North Area where I was spending the day on shift with a colleague. Because of technical difficulties (or was it a worker’s strike?), the beam was off, and our devices under test weren’t taking any data, so when the reporter came by and asked to speak with us, it was an emphatic “Yes, but I need coffee first.”

Now, to be fair, it wasn’t the reporter himself that was unusual, it was the story he sought: “The Sound of CERN.” Um, what? This gentleman had been taking field recordings all over in hopes of piecing together an aural representation of the world’s largest particle physics laboratory, and now he wished to speak with us. After seeing — hearing! — so much of CERN’s infrastructure and equipment, all of it humming whirring beeping pulsing clicking, he had decided to widen the scope of his project to include the scientists inhabiting this soundscape. Sounded reasonable to me.

After my colleague rather eloquently explained the work we were doing at the test beam and why it mattered in the grander scheme of things, our conversation moved on to the reporter’s work. Why sound? Well, it’s awfully difficult for people to relate to fundamental physics on a visceral level, and intellectually isn’t much easier — there’s a reason we spend so much time in grad school! But understanding is facilitated whenever you can associate a concrete bit of sensory information with an abstract concept. What sound does a Higgs boson make when it decays into two W bosons? What color is an electron? (No, I’m not talking quantum chromodynamics…) If you could reach out and touch a proton, would it be soft like a plushy, or hard like a billiard, or squishy like a hard-boiled egg?

Or, in this reporter’s case, What does CERN sound like? Well, I will give you some hints — in words, until I acquire the means to record the audio myself:

  • like a room full of computers, fans blowing hard while merciless physicsts bang on their keyboards
  • like a 1.6 Tesla Morpugo magnet thrumming softly while a beam of 180 GeV pions passes through it at close to the speed of light
  • like a flock of sheep grazing in a field 100 m directly above the low-energy end of CERN’s accelerator complex, the bells on their necks chiming pleasantly
  • like the coffee machines in R1 dispensing liquid energy to tired grad students
  • like the electronic tone emanating from television screens once every forty seconds, indicating when the SPS is spilling beam your way
  • like water cascading down the inside of the ATLAS cooling towers at Point 1 on the LHC
  • like two people chatting excitedly as you pass them by, “… saw good agreement in the high-pT tails, but something strange …”
  • like this, maybe

Until next time — keep your eyes open and your ears tuned!

Burton

So You Want to Discover a New Particle (Pt. 2)

Sunday, May 22nd, 2011

Editor’s note: For those who missed it, here’s “So You Want to Discover a New Particle (Pt. 1)

Hi, Readers!

I went away for a bit to pursue some other extra-curriculars, but now I’m back — and the blog has a new home! Perhaps a new audience as well. Since this (my first) Quantum Diaries post is actually the second part in a series, and I am a shamefully sporadic poster, I suppose I owe you a synopsis:

• The Standard Model is boring, but new particles are not.
• If you’d like to discover a new particle, theorists have conveniently provided you with an expansive menu of possibilities.
• Choose your particle with great care. This involves physics-, politics-, and plushy-based considerations.

So, let’s assume you’ve done some research, sent some emails, formed (or joined) a research group, and selected the new particle you’d like to discover. Congrats. Now what? Well, your particle hasn’t been found yet probably because… it isn’t easy to find. :) There could be multiple reasons for this:

• It has a tiny production cross-section (the LHC produces it only once in a blue moon, as opposed to millions of times per second).
• It looks like other, already-discovered particles, so it blends right in with the (so boring!) Standard Model.
• It is produced and/or decays in such a way that our particle detectors have a tough time seeing it and measuring its properties.
• It is shielded from present detection by a future version of itself, traveling back in time to thwart your research plans (see here or here).

With the notable exception of that last one, the practical consequence is that you’re essentially looking for a needle in a haystack. Only sometimes the needle looks an awful lot like hay. And in some cases, the needle could actually be lying outside the haystack, in a place you aren’t even looking. We call this hay “background”; the needle, “signal.” Before you can even think about looking for your needle of interest, you first have to get to know the hay.

In general, the bulk of your background is made up of Standard Model processes that resemble your signal but are produced far more copiously. As an added complication, this can be split into two groups: “physics” backgrounds, which actually involve the same “final state” particles as your signal  — that is, those that are measured by the detector and then used to reconstruct the event; and “instrumental” backgrounds, which involve a different final state that is mis-measured by the detector such that it “fakes” looking like your signal. To make matters worse, it’s possible that non-Standard Model (new!) particles similar to your own could interfere with your analysis, adding an entirely theoretical component to your total background. Insidious! You must be aware that yours isn’t necessarily the only needle in this haystack.

(… As is often the case, one person’s trash is another person’s treasure. :) )

Assuming you did the research before choosing your particle, you already know the main backgrounds for your signal. Great! Now to study these background processes in a systematic, controlled manner, we use what are called “Monte Carlo” (MC) simulations, aka “fake data.” Although I won’t go into detail about how the MC is generated, I will say that it’s a sophisticated simulation representing our best guess at how the data should look based on both theoretical and experimental constraints. It involves random numbers, probability distributions, lots of computing power, and magic.

Most likely your backgrounds have already been simulated, and all you need to do is get them. Do so. Practically speaking, this is person- and experiment-specific, so I offer no details, but let’s just assume that you now have access to the MC simulated datasets for your main backgrounds — and so the fun can begin! Except it is now 2am, and my workweek is about to start. Nuts!

Next time: Examining your simulated haystack, comparing it to your simulated needle, and finding ways to effectively separate the two with an algorithmic baler.

– Burton

So You Want to Discover A New Particle (Pt. 1)

Tuesday, April 12th, 2011

Hi All,

Perhaps you’ve heard of the Standard Model of Particle Physics. (If you’ve been following Flip’s ongoing series, you’ve certainly heard a lot.) In a nutshell, the Standard Model is a theory describing the fundamental particles of matter and the forces that mediate their interactions, and it’s the theoretical framework in which we at CERN generally understand our experimental data. In the three decades since its formulation, the Standard Model has been extraordinarily successful and accurate in its predictions, and with the notable exception of the SM Higgs boson, all of the pieces to this particle puzzle are already in place.

The Standard Model is so boring.

However, for a variety of reasons that I’ll keep outside the purview of this post, we believe that there’s physics “beyond” the Standard Model. As with most things in high-energy physics (HEP), this has been given a practical acronym: BSM (Beyond the Standard Model) physics. Many BSM theories predict the existence of one or more new (non-SM) particles. Here’s a scandalously abridged list:

  • Supersymmetry (SUSY) predicts “superpartners” or “sparticles” corresponding to every current SM particle
  • in addition to the three generations of matter particles already observed, there could be a fourth, more massive generation consisting of two quarks and two leptons
  • because the SM Higgs just isn’t enough! Little Higgs, Fat Higgs, Composite Higgs, Hidden Higgs …
  • W’ and Z’
  • Leptoquarks

Theorists are very creative! This list could go on for quite a while… :)

Given that I’m an experimentalist, however, I’m more directly interested in how one goes about detecting these hypothetical particles. And as an entirely practical matter, the first thing you have to do is actually choose which of these particles you’ll be searching for. This isn’t as simple as it sounds! Here are some general issues to take into consideration when making your decision:

  • How much data is needed for a discovery? Or, alternatively, How large is the production cross-section? If your particle has a large production cross-section, it will be produced in copious amounts by the LHC, and therefore less data is required for you to find it. Since the LHC is still relatively young, and the number of collisions recorded by the experiments is only a tiny fraction of the expected total, many analyses — BSM searches especially! — are limited by statistics. We hope to have about 1 fb-1 of data by the end of this year. If you expect to be sensitive to your particle only with 100 fb-1, then you will be waiting an awfully long time…
  • Is the particle model-independent? It pays to be general. If your particle is entirely dependent on the viability of a particular BSM model, and that model is subsequently ruled out by experimental data, then where does that leave you? Back at the beginning, looking for a new particle to discover. Furthermore, the more general the particle, the less fine-tuned your analysis will be. Many BSM particles resemble each other, at least in a general sense, so you can imagine a situation where you’re so focused on finding one specific particle that you don’t notice another one lurking in the data.
  • Are other people already looking for your particle? Collaboration is essential in a field like ours, but do make sure that there’s room for you on this search before you barge in. Perhaps the other analysts are very territorial. Maybe there are simply too many of them already. Or could it be that you don’t want to share the Nobel Prize when you discover your new particle…? Ask around ahead of time, even email the folks in charge (“conveners”) to find out who is working on what. Given the aforementioned creativity of theorists, there’s sure to be particles still in need of analysts!
  • Is it available at The Particle Zoo? Just sayin.

In truth, these are only a few of the many considerations that go into choosing a new particle to search for. From pure theory to pure politics, this decision is not one to be taken lightly! Think carefully before setting your heart on (and devoting many months of work to) your new particle — then go for it.

– Burton :)

LHC FTW !!!

Tuesday, March 22nd, 2011

As I wrote just last week, the 2011 dataset is going to be huge. And as a promising sign of great things to come: The LHC has already surpassed its previous instantaneous luminosity record!

That means more data, faster. Keep it coming!

I swear I’m not just sitting at home, watching the OP Vistars web page refresh… which it does automatically, btw. You can even have a program announce changes in the beam status out loud! Just saying. :)

– Burton

LHC is GO!!!

Sunday, March 13th, 2011

Hi, all!

It feels like forever since the LHC last delivered proton-proton collisions (… in early November). There was a very productive stretch of heavy-ion collisions followed by the usual winter shutdown, and then a few weeks of machine development that ended… just now.

Yes: The first stable beam p-p collisions of the year are happening at this very moment! As always, you can see the LHC status live: here.

The 2011 dataset promises to be EPIC. Stay tuned — lots of physics to come!

– Burton :D

Playing Politics with Science

Monday, March 7th, 2011

Hi, folks!

As many of you are undoubtedly aware, the U.S. federal government is in the midst of a budget crisis. The prevailing wisdom in Washington is that deficits are out of control and will soon bring America to ruin; therefore, drastic budget cuts are necessary to ensure the nation’s future health and prosperity. Okay. Let’s take for granted that this is true. Let’s also ignore the official policies and recent acts of Congress that fly in the face of fiscal responsibility. We should probably also narrow our vision to the short-term — say, the next two years — to avoid unpleasant long-term realities.

Still with me? :)

This is now: The FY 2011 budget proposed by Republicans and passed in the House of Representatives would cut non-defense discretionary spending by roughly $60 billion compared to current funding levels. Unfortunately, science funding takes a particularly hard hit:

- Environmental Protection Agency: -$1.6 billion

- Department of Energy loans: -$1.4 billion

- Office of Science: -$1.1 billion

- National Institute of Health: -$1 billion

- Energy efficiency and renewable energy: -$899 million

- Centers for Disease Control and Prevention: -$755 million

- NASA: -$379 million

- National Oceanic and Atmospheric Administration: -$336 million

- National Institute of Standards and Technology: -$186 million

- National Science Foundation: -$139 million

Now, I am not an economist, but it seems clear that this is absolutely devastating. If the budget proposal is passed as-is, thousands of scientists will be laid off, operation of current experiments will be disrupted, and many new projects simply won’t receive funding. Cutting-edge research will be especially hurt — and yes, dear readers, that includes high-energy physics. (Recall the impending shutdown of Fermilab’s Tevatron, for lack of funding.) A wide swath of American scientific research will be stifled. Since basic research and resulting scientific innovations drive long-term economic growth, this is, at best, a short-sighted attempt at reducing our national debt. At worst, it is a self-destructive travesty of pandering and ineptitude that results when politics and reason become mutually exclusive.

I won’t force my position on this issue, but I will point you to a place where you can work the US budget out for yourself: http://public-consultation.org/exercise/. (See how easy public policy decision-making is when you aren’t beholden to the funders of your previous election campaign?) After that, perhaps you would be inclined to contact your elected officials to let them know what you think about all this: http://www.usa.gov/Contact/Elected.shtml.

By any measure, science is an excellent investment in the long-term success of our nation. It should not be a political punching bag. Make some noise, folks! This is serious.

– Burton

On Going Home(s)

Sunday, January 23rd, 2011

Hi, folks!

I’ve been absent for a while on account of switching jobs: from “graduate student/research assistant” to “plot-slash-table-making automaton.” The cynical among you may argue that these are essentially the same thing, but it helps me sleep at night to believe otherwise. Well. At any rate, I’ve had several blog post ideas sloshing around in my head for months now, and rather than age to perfection, they’ve gotten all… mushy. Here is your first serving of mushed thought.

I went home to Michigan for Christmas. Things were pretty much the same, modulo the effects of prolonged regional economic distress and the strange sensation that everything and everyone was larger than they should be (cars, portion sizes, distances to points of interest, family members). Naturally people wanted to know what I’d been up to, but I was mostly at a loss for words: How does one condense high-energy physics and la vie CERNoise into a quip or anecdote that connects with non-physicists?

“I work a lot.”

Surprisingly, that seemed to satisfy most questioners. Also: “Haven’t managed to destroy the world yet.” For more thorough and eloquent answers, I turned to CERN’s visitor center and gift shop, bringing home a few CERN/physics books as both gifts and conversational references. When a friend asked about “the Higgs Bassoon,” I pointed her to a fully illustrated children’s book showing the basics of the Standard Model and how physicists are able to study it. “No, it’s not a woodwind instrument, it’s a hypothetical fundamental scalar boson.” This was the same book I gifted to my mom; tomorrow, on her 50th birthday, I will be sending her a quiz to assess what she learned. I am a terrible son. My dad had mentioned to me a drinking buddy who fancied himself a physics enthusiast, so I gave my dad a more advanced but still brief introduction to particle physics in order to impress this guy and, one hopes, get a free drink or two out of the exchange. See? My field has practical applications. In related news, my grandma found the Higgs Boson.

The whole experience has underscored the importance of accurate, accessible communication between scientists and the general public. This US LHC blog is a nice venue for such conversations, right? :) But as for a much wider scale, let me just say that I’m incredibly thankful for all the science journalists and other folks out there engaged in outreach (Daisy, Bryan, Katie, …). We all benefit from your excellent metaphors.

I went home to New York for New Years. I was surprised to find that people in bars really like hearing about the LHC; I was not surprised to hear some call it the “Large Hardon Collider.” Emergency physics lessons ensued.

It’s easy to forget about (or at least willfully ignore) my institution, Stony Brook University, when it’s so far away, but since I was in the neighborhood, I swung by to say hello to my advisor and physics friends who don’t work at CERN. This was a dangerous move: advisors are pretty much obligated to request plots and tables from their advisees, and I quickly reverted to the automaton existence I’d left behind. Sigh. Absence really does make the heart grow fonder — will keep in mind next time I consider visiting.

Oh, one more thing before I get back to making last-minute plots for the ATLAS note I and my colleagues have been working on for some time (and will soon be submitting!) : Let’s please have a moment of silence for the Tevatron, a pioneer and workhorse in high-energy physics for the past two decades, whose funding won’t be extended beyond 2011.

It’s time for the LHC to really, really shine.

– Burton