Right now: Trying to collide 25×25 bunches

Posted by Mike Anderson on 29 Jul 2010

As we speak there are 25 bunches of protons in both proton beams in the LHC.  See all those steps in the graph (red and blue lines)?  Each little step is one bunch being added, and each “big” step is 4 bunches being added.  So if you count the steps yourself you should get a total bunch count of 25 in each beam.  The red and blue lines correspond to the left-hand y-axis showing “Intensity”.

The energy of the proton beams is in black and goes with the right-hand y-axis, “Energy (GeV)”.  As I write this the protons are around 500-some GeV and being ramped up to 3500 GeV which should take about half an hour.

Once both beams are at 3500 GeV and they declare stable beams, it’s time to record some data with the most bunches in the LHC to date!

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ICHEP’s Biggest Day

Posted by Seth Zenz on 27 Jul 2010

Yesterday was, I suppose, the biggest and most formal day here at the 35th International Conference of High Energy Physics. I wore my suit, and took some ribbing from some of my colleagues for dressing up so much, but I’ve worn it for far less excuse and am not sorry in the slightest. It’s not every day, or even every ICHEP, that one hears an address from the President of the French Republic!

Mr. Sarkozy’s speech was great to hear. He is a very emotive, enthusiastic, and informal speaker, which made him relatively easy to understand for those in the audience (like me) with limited French. He didn’t claim to know the details of our work, and seemed to think we’re all a little weird, but spoke mostly about the importance of fundamental questions about the universe and his support for basic research. This was very well received indeed. He also talked a bit about the contributions of the French labs to the LHC and other projects, which is fair: France plays one of the central roles at CERN, and the French particle physics community has made significant contributions throughout the field. This is reflected in the excellent and informative conference that they’re hosting here in Paris.

ICHEP BanquetIf there was one thing I would ask to be improved for the next ICHEP, however, I wish there had been a bit more food at the banquet! You can see the banquet, which was held in the National Natural History Museum, at right. It was a very impressive museum — the main hall reminds me of the ATLAS cavern, and seems to be just about the same size — and the food was certainly varied and interesting. But the lines were long to get even a little of it, and we had to go out to dinner afterwards to be full.

Yesterday was also the final talk on the combined Tevatron Higgs results. Fermilab sent out the press release while we were still on coffee break, so I saw the excluded mass range on Twitter before going into the talk. (I overcame the temptation to shout out the answer at the start.) It was still a very entertaining talk, and obviously the details of how the measurement was done were as important to see as the final numbers. Of course, we all wish there had been more to see than mass limits in the expected range and a few possible tantalizing hints. We also had talks from the CERN’s Director for Accelerators and Technology on the LHC and from the spokespeople of the LHC experiments. Although we haven’t seen anything really new at the LHC yet, it’s clear that the accelerator and experiments are all making great progress in getting ready to make the exciting discoveries that we’ll see at future conferences!

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Particles and Searches

Posted by Regina on 23 Jul 2010

Lots of us bloggers have been talking about ICHEP which is going on this week. I’m not attending the conference, although some of the work I’ve been doing is :) .
Now I’ve been turning my attention back to my physics analysis.  As of about a week ago we have 200 nb-1 (now closer to 300 nb-1) of data – which is about 1/50th of what I hope to get for an analysis.

I briefly mentioned that I’ll be doing a search in a previous post. Now I’d like to share a bit what this particle beast is. A leptoquark carries quantum numbers for both quarks and leptons. It would decay by generation such that it mixes families of quarks and leptons. So why do we think it exists? In a word: Symmetry.

Physicists love symmetry (and symmetry breaking :) ). Symmetry in forces (like electricity and magnetism), symmetry in families and generations of particles, symmetries everywhere. Since the quarks and leptons in the Standard Model have the same family structure it seems like there should be something that ties them together, like leptoquarks.

Granted this is a bit of an oversimplification, theorists have put in lots of work into understanding how these particles work. And now I’m going to be looking for them.

I’ll be giving updates over the next few months explaining more about these particles over the coming weeks.

-Regina

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My First Day at ICHEP

Posted by Seth Zenz on 23 Jul 2010

This is my poster. There are many like it but this one is mine.
There are probably many blogs where you can read summaries of the ICHEP conference — or if not, there will be soon enough — so I’m going to limit myself to telling you about my day. Getting my poster printed and getting it to Paris in one piece was stressful, but uneventful in the end, and once I got to the conference things were easy. The poster session was the first evening, and you can see me at right standing in front of the thing, ready to explain what’s going on. (I will soon post more about the measurement shown in the poster, but here is the official ATLAS conference note, and here is an old summary of some of the concepts.) I didn’t get an overwhelming number of people asking questions — there were an awful lot of posters, which gave me a new perspective on how my work is one tiny facet of our overall effort to understand particle physics — but I did have a few good discussions with interested folks, and the psoter will be up all week.

As for the rest of the conference, I mostly went to the “early LHC experience” sessions, along with a few talks in the Standard Model session. I found the ATLAS and CMS measurments of the W and Z bosons interesting, but mostly because they show how the experiments are getting going. The theory of these particles is very well understood, and the experiments are consistent with it — in fact, if the experiments disagreed the theory at this point, we’d conclude that something had gone wrong with the experiments. When the detectors are solidly understood and working toward precision measurements, they may discover subtle differences from theoretical predictions in this area, but that will be years from now.

And now for another day of conference talks!

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ICHEP: what to watch for

Posted by Ken Bloom on 21 Jul 2010

At long last, the 35th International Conference on High Energy Physics begins tomorrow. It’s the largest particle-physics conference of the year, and the first major conference since the start of LHC operations at 7 TeV, If the US LHC blog has seemed to be a bit quiet lately, it might be because so many bloggers have been working hard to get results ready. Now, it’s highly unlikely that there will be any surprising LHC discoveries announced there; we just don’t have nearly enough data yet. But that doesn’t mean that this conference will be boring! Here are a few things that you might want to be watching for:

  • How well are the experiments keeping up with the LHC? The LHC has now delivered about 350 nb-1 of integrated luminosity to the experiments. What fraction of that data will the experiments show? This is a measure of the operational efficiency of the experiments, and of their ability to get the data through reconstruction and analysis. If the experiments are able to show a large fraction of the delivered data, then we can be optimistic about how quickly results will come out as the collision rates rise.
  • How competitive is the LHC with the Tevatron? The Tevatron experiments have collected a huge amount of data over the past nine years, and have an excellent understanding of how their detectors work. They will still be in the lead on many, many physics topics. (Disclaimer: I also work on one of the Tevatron experiments.) However, because of the LHC’s higher collision energy, there might be a few measurements for which the LHC can produce stronger results, even with a tiny amount of data. Will there be any such results, and what will they be?
  • How competitive is the Tevatron with the LHC? Everyone is eager to hear the latest limits on the standard-model Higgs boson from the Tevatron. The excluded Higgs masses are the ones that would have been the easiest for the LHC to see too. How much harder will new Higgs limits make it to find a Higgs at the LHC?
  • Any surprises from elsewhere? Let’s not forget that this conference covers all of particle physics, and there’s a lot more going on out there than just the LHC!
  • How tired do the presenters look? A lot of that 350 nb-1 came at the last minute — did everyone stay up all night to finish their data analysis?

I won’t be attending the conference, but I’ll try to provide some commentary from lovely Lincoln as events unfold. Good luck to all involved — this is going to be a lot of fun!

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It is possible to have a life outside of the lab.

Posted by Jake Anderson on 21 Jul 2010

“Get a life!” seems to be a tried and true TV line when talking to geeks, nerds and the like. I’d like to think I have one. It must be the birth of my third son that has me reflecting on a larger scale than usual, but I haven’t found that being a physicist has been a significant burden on my personal life.

I know there are stereo types of physicist spending day and night at the lab working. My wife often likes to tease me that when I get home late from work it isn’t because of anything she needs to worry about; I was engrossed in my work and lost track of time. I’ll admit that it has happened (ok more than once), but I don’t make a habit of it. Most of the people I work with keep regular, sane hours, and all have what seem to be normal personal/work lives. Sometimes we have to put in extra hours at the lab, like now as the ICHEP conference is upon us, but most jobs have deadlines and extra hours to meet them.

Physicists and scientists in general are often unfairly considered to lack a personal life. I’ll admit that I have met some, but the vast majority are able to relax and have some fun most days. In fact, I get to have fun just about all day everyday since I find physics fun most of the time in addition to having fun away from work, and isn’t that the measure of having a really good life.

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Almost There

Posted by Seth Zenz on 19 Jul 2010

The official ATLAS conference note describing the analysis I worked on was approved on Saturday morning. My poster was finalized, approved, and printed — possibly not in that order — just in the past few hours. Now the only challenge left is to get myself and my poster through a French air traffic controllers’ strike and to the Palais de Congrès by Thursday morning.

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That’s what I like to see

Posted by Mike Anderson on 18 Jul 2010

Stable proton beams colliding at some of the highest luminosities reached by the LHC so far!

Right now the luminosity is at 1030/cm2s.  Up until now, the luminosity collected these past few months has been at a luminosity around, at most, 1029/cm2s.

This is significant because this basically means that in about a day we can collect the same amount of data that we have collected over the past few months.  That’s why it’s so useful to do studies on increasing the luminosity rather than continuing to run at lower luminosities.

There’s a short term downside though: doing studies to increase luminosity makes it hard to get clean, stable beams for data taking.  It’s kind of like deciding whether you should buy a computer now, or wait a few months until prices come down and hardware is better.

The LHC has a balanced program of stable running and also doing studies to increase luminosity.  From the looks of it, it’s going well.

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LHC: Play along at home! (or, scoreboard watching)

Posted by Ken Bloom on 12 Jul 2010

OK, I’ll admit it — instead of writing blog posts or reviewing results that are headed for ICHEP or doing something else productive, I find myself all too easily distracted by information on the current status of the LHC. As the gallant accelerator physicists work to push the machine to higher beam intensities and collision rates, I’m eager to learn about each little bit of progress. It definitely has some meaning to me — the more collisions the LHC produces, the more the experiments can record, and the greater the chance that we will see any particular physics process take place. Especially as we get close to the big ICHEP conference, we are all curious about how much data we might record before then, because that will determine what measurements might possibly be ready. (Of course it’s also determined by how quickly we can push the data through data analyses, how well we can understand detector performance and so forth; let’s not put all of the burden on the LHC.)

It’s not like I can do anything to make the luminosity go up, but I feel better (or at least distracted) by knowing what’s going on at this minute. This is akin to scoreboard watching in baseball, where the outfielders in one game might have their eye on the scoreboard above them to see how the competition is doing. (In fact, back at the Cornell Electron Storage Ring, the display that showed the luminosity numbers for the past 24 hours was called the “scoreboard”, so the analogy fits.)

So, if you want to play along at home, here are a few Web pages you can keep an eye on. Some of these have been mentioned in previous posts on this blog, but it’s been a little while and I’ll give a few more details.

To know what’s happening right now, check out LHC Page 1, which gives the current machine status and the (very) short-term running plan. Here you’ll typically see plots of the amount of beam current and the beam energy in the LHC, and, during periods of collisions for “physics” (i.e. data-taking by the experiment as opposed to studies of collisions done to optimize machine performance) there will be plots of the observed instantaneous luminosity reported by each of the four experiments. (Instantaneous luminosity is a measure of collision rate; its units of inverse centimeter squared per second deserve explanation in a second post.) The experiment reports can also be seen on the LHC Operation page. At other times, it will show the status of preparing to go to collisions, such as “ramp” (increasing beam energy to 3.5 TeV) or “squeeze” (focusing the beams to increase the collision rate). There are also helpful short messages about what’s going on, such as “this fill for physics” or the somewhat unnerving “experts have been called.”

The medium term run plan can be seen on the LHC Coordination screen. Here you can see the goals for the coming week, what administrative limits are currently in place to protect the machine, and the planned activities for the next few shifts.

While the collision rate is interesting, what really counts is the “integrated luminosity”, or the total number of collisions that have taken place. Up-to-date charts can be found here; the data go back to March 30, the start of 3.5 TeV operations. You can see here that the integrated luminosity has been increasing exponentially in time (when the LHC is not in studies periods or technical stops). If the collision rate were the same all the time, the integral would only increase linearly, so this demonstrates just how quickly the LHC physicists are figuring out how to make the machine go.

That’s what I’ve been keeping an eye on. OK, all of you stop looking at Facebook, and distract yourselves with the LHC instead!

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The size of the proton

Posted by Christine Nattrass on 12 Jul 2010

There is a new measurement of the size of the proton and it turns out that protons are smaller than we thought they were.

At some point in your education you probably got introduced to the Bohr model of the atom.  The nucleus is made up of protons and neutrons, and electrons orbit around the nucleus.  In the Bohr model, electrons orbit the nucleus in circular orbits like the Earth orbits the Sun, but these orbits are only allowed to have some radii (which correspond to an integer number of de Broglie wave lengths).  Electrons can transition between these levels and when they do, they either absorb a photon (in the case of an electron being excited from, say, the ground state to an excited state) or emit a photon (in the case of an electron going from an excited state to a lower state.)  This is shown below:

The Bohr model isn’t exactly right – but it’s close enough to get some feel for what’s going on.  In a more precise quantum mechanical picture, the electron isn’t actually orbiting the nucleus – it’s smeared out in what we call a wave function.  The square of the wave function tells us how likely we are to find the electron in a given place.  The ground state orbital (the shape of the wave function of the electron in the atom) is spherical.  The lowest excited state has four different possible orbitals, one spherical (S) and three which are shaped like a dumbbell (P), a sort of 3D figure-8.

What you probably learned in school was that these S and P orbitals have exactly the same energy – and they almost do.  In a simple model, the nucleus is just a point particle – meaning it exists just at a single point, with no size in any dimension.  But protons aren’t point particles – they’re just very small.  In the S orbitals, the electron spends most of its time near the nucleus, but in the P orbitals, the electron spends less of its time near the nucleus.  This difference in how much time the electron spends near the nucleus leads to a very small shift in the energy of the orbitals, called the Lamb shift.  The Lamb shift is measured by measuring the photon emitted when an electron goes from the P to the S orbital in the second shell.  It depends on the mass of the electron and the size of the proton.  (Here’s the explanation of the Lamb shift on the experiment’s web site.)

In this new measurement, they looked at hydrogen with a muon (the heavier cousin of the electron) instead of an electron.  Because the muon is about two hundred times heavier than the electron, it spends more time near the nucleus than the electron, meaning it’s more sensitive to the Lamb shift than the electron.  Previously, the best measurement of the diameter of the proton was 0.877±0.007 femtometers (m) and this measurement measured it to be 0.8418±0.0007 fm.  A femtometer is 10-15 meters.  If you were a proton (you’re somewhere between 1-2m tall), this would mean traveling one millimeter would be like traveling from the Earth to the Sun (1011 m).  This measurement would be like finding out that you’re 5′5″ instead of 5′8″ by looking at how long it takes for you to walk between Milwaukee, WI and Chicago, IL (150 km) and Milwaukee, WI and Madison, WI (141 km)*.

The fact that this measurement is so far off from our expectations indicates one of the following:

  • The precise calculation we’re comparing to is flawed.The proton is actually a really complicated object – perhaps we forgot an important component.
  • The measurement has some flaw we haven’t figured out yet.  Maybe there was some systematic shift that wasn’t taken into account.
  • Our theory is flawed.  This could indicate some physics beyond the Standard Model – exactly what we’re looking for at the LHC.

We have to seriously consider the first two options, but the third would obviously be very exciting.

So why I am writing about this here?  First, it illustrates that there are other ways of studying fundamental particle physics than by slamming things together.  Second, it’s an interesting result that may hint at exciting new physics we’re hoping to see at the LHC.  Third, it’s a great segue into my next post…

*Yes, this analogy breaks down at some point.  Don’t take it too far.

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Track Jets for ICHEP

Posted by Seth Zenz on 09 Jul 2010

Along with many other particle physicists, I’ve been working hard lately to prepare results for the 35th International Conference on High Energy Physics, which will be held in Paris starting on July 22nd. That means I am again going through the complexities of reviewing my work with my (3000+) collaborators, to make sure that the work I’ve done is something we all have confidence in. After all, everyone’s name will be on it!

So far, things are going well, and it looks like (cross your fingers) the analysis will be out and ready. I just designed a poster this week, and some of the plots might also appear in one of the ATLAS talks given by one of my colleagues. The approval process has also been a great opportunity to get feedback — some of which has been included in the current analysis, and some of which will be added as we update and improve the results for a complete paper.

Momentum of raw track jets from the 900 GeV runI’ll be able to show you the latest results once the ICHEP conference starts, but for now I at least have some plots of track jets from last year’s 900 GeV run, one of which is shown here at right. You can click the image for more and bigger pictures, but I don’t promise that the text will be too comprehensible! I’ve written a more understandable explanation of the track jet analysis here. The plot on this page shows the momentum of track jets we found in the 900 GeV data (black points) and compares it to the momentum of simulated track jets (yellow graph). You can tell a few things from it: first, there are a lot more low-momentum jets than high-momentum jets, which is exactly what we expect; second, that the data and the simulation agree pretty well; third, that they don’t agree perfectly.

There are two basic reasons why data and simulation might not agree: one is that we aren’t simulating our detector accurately enough, and the other is that we’re not simulating the underlying physics that comes out of the collision well enough. Working out which is which, and coming up with our best guess as to what really happened when the protons collided, is the hard work of data analysis. How did it go? To find out, come see my poster at the ICHEP conference, or just stay tuned here!

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Independence day

Posted by Regina on 04 Jul 2010

Sorry for the hiatus, blog enthusiasts! I’m taking some time to catch-up while watching the fireworks out of my window on July 4th. Tis the season for summer conferences. The one in particular that I’m involved in is ICHEP (International Conference on High Energy Physics) is coming up at the end of July, which means all the papers have to be approved by ATLAS by the end of June (which just so happened to be last week – hooray independence  ;) ). This year the conference is in Paris and there we’ll show the first physics results from the LHC. ATLAS alone has over 40 papers submitted. In particular I’ve been looking at material mapping using photons.

So what is material mapping?… sounds like something cartographers do.
We have lots of computer simulations of the ATLAS detector. To double check to make sure we’ve taken into account every cable we look to see that the particles interact the way we expect them to. Photons, for example, when they to through material convert predictably into an electron/positron pair. When I say predictably, I mean based on the amount of material they go through. We find these electron/positron pairs because they have a displaced vertex (an electron/positron which are close to each other and when you draw a line back from their tracks the origin isn’t the main interaction point). The more material in the way, the faster they convert. So we make sure our Monte Carlo simulations predict where most of the conversions occur to make sure we understand the detector.

I’ll try to provide a link to show a picture of the material map once they have been approved for public viewing.

Until then, Happy July 4th!

Fireworks

Regina

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The W boson: mixing things up

Posted by Flip Tanedo on 02 Jul 2010

For those of you who have been following our foray into the particle content of the Standard Model, this is where thing become exciting. We now introduce the W boson and present a nearly-complete picture of what we know about leptons.

We’re picking up right where we left off, so if you need a refresher, please refer to previous installments where we introduce Feynman rules and several particles: Part 1, Part 2, Part 3, Part 4, Part 5

The W is actually two particles: one with positive charge and one with negative charge. This is similar to every electron having a positron anti-partner. Here’s the Particle Zoo’s depiction of the W boson:

Together with the Z boson, the Ws mediate the weak [nuclear] force. You might remember this force from chemistry: it is responsible for the radioactive decay of heavy nuclei into lighter nuclei. We’ll draw the Feynman diagram for β-decay below. First we need Feynman rules.


Feynman Rules for the W: Interactions with leptons

Here are the Feynman rules for how the W interacts with the leptons. Recall that there are three charged leptons (electron, muon, tau) and three neutrinos (one for each charged lepton).

In addition, there are also the same rules with the arrows pointing in opposite directions, for a total of 18 vertices. Note that we’ve written plus-or-minus for the W, but we always use the W with the correct charge to satisfy charge conservation.

Quick exercise: remind yourself why the rules above are different from those with arrows pointing in the opposite direction. Hint: think of these as simple Feynman diagrams that we read from left to right. Think about particles and anti-particles.

In words: the W connects any charged lepton to any neutrino. As shorthand, we can write these rules as:

Here we’ve written a curly-L to mean “[charged] lepton” and a νi to mean a neutrino of the ith type, where i can be electron/muon/tau.

Exercise: What are the symmetries of the theory? In other words, what are the conserved quantities? Compare this to our previous theory of leptons without the W.

Answer: Electric charge is conserved, as we should expect. However, we no longer individually conserve the number of electrons. Similarly, we no longer conserve the number of muons, taus, electron-neutrinos, etc. However, the total lepton number is still conserved: the number of leptons (electrons, muons, neutrinos, etc.) minus the number of anti-leptons stays the same before and after any interaction.

Really neat fact #1: The W can mix up electron-like things (electrons and electron-neutrinos) with not-electron-like things (e.g. muons, tau-neutrinos). The W is special in the Standard Model because it can mix different kinds of particles. The “electron-ness” or “muon-neutrino-ness” (and so forth) of a particle is often called its flavor. We say that the W mediates flavor-changing processes. Flavor physics (of quarks) is the focus of the LHCb experiment at CERN.

Exercise: Draw a few diagrams that violate electron number. [If it's not clear, convince yourself that you cannot have such effects without a W in your theory.]

Answer: here’s one example: a muon decaying into an electron and a neutrino-antineutrino pair. (Bonus question: what is the charge of the W?)

Remark (update 7 July): In the comments below Mori and Stephen point out that in the ‘vanilla’ Standard Model, leptons don’t have flavor-changing couplings to the W as I’ve drawn above. This is technically true, at least before one includes the phenomena of neutrino-oscillations (only definitively confirmed in 1998). In the presentation here I am assuming that such interactions take place, which is a small modification from the “most minimal” Standard Model. Such effects must take place due to the neutrino oscillation phenomena. We will discuss this in a future post on neutrino-less double beta decay.

Feynman Rules for the W: Interactions with other force particles

There are additional Feynman rules. In fact, you should have already guessed one them: because the W is electrically charged, it interacts with the photon! Thus we have the additional Feynman rule:

This turns out to only be the tip of the iceberg. We can replace the photon with a Z (as one would expect since the Z is a heavy cousin of the photon) to get another three-force-particle vertex:

Finally, we can even construct four force-particle vertices. Note that each of these satisfies charge conservation!

These four-force-particle vertices are usually smaller than any of the previous vertices, so we won’t spend too much time thinking about them.

Really neat fact #2: We see that the W introduces a whole new kind of Feynman rule: force particles interacting with other force particles without any matter particles! (In fancy words: gauge bosons interacting with other gauge bosons without any fermions.)

Remarks

  1. The most interesting feature of the W is that it can change fermion flavors, i.e. it can not only connect a lepton and a neutrino, but it can connect a lepton of one type with a neutrino of a different type. One very strong experimental constraint on flavor physics comes from the decay μ→eϒ (muon decaying to electron and photon). As an exercise, draw a Feynman diagram contributing to this process. (Hint: you’ll need to have a W boson and you’ll end up with a closed loop.)
  2. It is worth noting, however, that these flavor-changing effects tend to be smaller than flavor-conserving effects. In other words, a W is more likely to decay into an electron and an electron-neutrino rather than an electron and a tau-neutrino. We’ll discuss how much smaller these effects are later.
  3. W bosons are rather heavy—around 80 GeV, slightly lighter than the Z but still much heavier than any of the leptons. Thus, as we learned from the Z, it decays before it can be directly observed in a detector.
  4. The W was discovered at the UA1 and UA2 experiments at CERN in the 80s. Their discovery was a real experimental triumph: as you now know from the Feynman rules above, the W decays into a lepton and a neutrino—the latter of which cannot be directly detected! This prevents experimentalists from observing a nice resonance as they did for the Z boson a few months later. They used a slightly modified technique based on a quantity called “transverse mass” to search for a smeared-out resonance using only the information about the observed lepton. Generalizations of this technique are still being developed today to search for supersymmetry! (For experts: see this recent review article on LHC kinematics.)
  5. The W boson only talks to left-handed particles. This is a remarkable fact that turns out to be related to the difference between matter and antimatter. For a proper introduction, check out this slightly-more-detailed post.

Exercise: Now that we’ve developed quite a bit of formalism with Feynman rules, try drawing diagrams corresponding to W boson production at a lepton collider. Assume the initial particles are an electron and positron. Draw a few diagrams that produce W bosons. “Finish” each diagram by allowing any heavy bosons (Z, W) to decay into leptons.

What is the simplest diagram that includes a W boson? Is the final state observable in a detector? (Remember: neutrinos aren’t directly observable.) What general properties do you notice in diagrams that both (1) include a W boson and (2) have a detectable final state (at least one charged lepton)?

Can you draw diagrams where the W boson is produced in pairs? Can you draw diagrams where the W boson is produced by itself?

Hints: You should have at least one diagram where the W is the only intermediate particle. You should also play with diagrams with both the fermion-fermion-boson vertices and the three-boson vertices. You may also use the four-boson vertices, but note that these are smaller effects.

Remark: Try this exercise, you’ll really start to get a handle for drawing diagrams for more complicated processes. Plus, this is precisely the thought process when physicists think about how to detect new particles. As an additional remark, this is not quite how the W was discovered—CERN used proton-antiproton collisons, which we’ll get to when we discuss quantum chromodynamics.

Relating this to chemistry

Before closing our introduction to the W boson, let’s remark on its role in chemistry and simultaneously give a preview for the weak interactions of quarks. You’ll recall that in chemistry one could have β decay:

neutron → proton + electron + anti-neutrino

This converts one atom into an isotope of another atom. Let’s see how this works at the level of subatomic particles.

Protons and neutrons are made out of up and down type quarks. Up quarks (u) have electric charge +2/3 and down quarks (d) have electric charge -1/3. As we will see when we properly introduce the quarks, up and down quarks have the same relationship as electron-neutrinos and electrons. Thus we can expect a coupling between the up, down, and W boson.

A neutron is composed of two down quarks and an up quark (ddu) while a proton is composed of two up quarks and a down quark (uud). [Check that the electric charges add up to what you expect!] The diagram that converts a neutron to a proton is then:

Because the W boson is much heavier than the up and down quarks—in fact, it’s much heavier than the entire proton—it is necessarily a virtual particle that can only exist for a short time. One can imagine that the system has to ‘borrow’ energy to create the W so that the Heisenberg uncertainty principle tells us that it has to give back the energy very quickly. Thus the W can’t travel very far before decaying and we say that it is a “short range force.” Thus sometimes the weak force is called the weak nuclear force. Compare this to photons, which have no mass and hence are a “long range force.”

[We now know, however, that it is not intrinsically a nuclear force (in our theory above we never mentioned quarks or nuclei), and further its 'weakness' is related to the mass of the W making it a short-range force.]

Cheers!
Flip (USLHC)

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Anti-proton to proton ratio – ALICE’s 4th paper submitted!

Posted by Christine Nattrass on 29 Jun 2010

ALICE has just submitted its fourth paper, on the anti-proton to proton ratio in p+p collisions, to Physical Review Letters.  This is a really cool measurement because it is one way of quantifying how many of the particles we create in our collisions – as opposed to how many of the particles we see are remnants of the beam.

A proton has three valence quarks, two up quarks and one down quark.  The proton’s electric charge is +1.  An anti-proton has three valence anti-quarks, two anti-up quarks and one anti-down quark.  The anti-proton’s electric charge is -1.  The anti-proton is the proton’s anti-particle.  When a proton and an anti-proton come together, they annihilate.

A baryon has three valence quarks -  examples are protons (two up quarks and a down quark) and neutrons (two down quarks and an up quark).  There are many more exotic baryons – my favorites are the Λ (an up quark, a down quark, and a strange quark) and the Ω (three strange quarks) . A proton is a baryon, while an anti-proton is an anti-baryon.  Baryon number is the net number of baryons in a system and it is conserved in all processes we have observed in the laboratory.  In our p+p collisions, the baryon number is 2 because there are two incoming baryons.  Because the anti-proton is an anti-baryon, it had to be created in the collision.  Moreover, because there were no (net) anti-quarks in our incoming protons, all three anti-quarks in any anti-proton we see had to be created in the collision.  If we just look at protons, we can’t tell if they were created in the collision or if they are remnants of the beam.

Since anti-protons don’t exist prior to collision, one way of quantifying how many particles were created in the collisions, as opposed to how many are beam remnants, is their ratio.  If this is near zero, most of the particles we observe are remnants of the beam.  If this is near one, most of the particles we see were created in the collision.  At low energies, the anti-proton to proton ratio is closer to zero, but we expect it to be almost one at LHC energies.  Here you can see the collision energy dependence of the anti-proton to proton ratio (Figure 4 of the new paper):

The y-axis is the anti-proton to proton ratio.  The upper x-axis is the center-of-mass energy of the collision.  The different data points are measurements from different experiments.  The line shows a fit to the data.  The lower y-axis is a little more complicated – I’ve put an explanation below, but you can skip it and just look at the top x-axis.  You can see that the anti-proton to proton ratio is very close to one at LHC energies.  But of course, we have to quantify how close the anti-proton to proton ratio is to one.  Specifically, we measured it to be 0.957 ± 0.006(statistical) ± 0.014(systematic) at 0.9 TeV and 0.991 ± 0.005(statistical) ± 0.014(systematic) at 7 TeV.  Most of the work went into determining the uncertainty.  We could reduce the statistical uncertainty by just taking more data, but the systematic uncertainty is limited by the method and the experiment.

What do we learn from this measurement?  It helps us test and refine our understanding of baryon production in proton-proton collisions.  We can compare to models for proton and anti-proton production and this lets us constrain some models and exclude others.

To give a feel for how complicated it can be to do the measurement, I’ll explain one of the details that has to be considered to do this measurement right.  If we see an anti-proton, we’re pretty sure it was really created in the collision.  But we have billions and billions of protons in our detector.  A very fast particle created in the collision could knock a proton out of our detector.  If we measure a proton, how can we be sure that it didn’t come from our detector?  We have accurate enough charged particle tracking to see where the proton came from.  This figure (Figure 2 from the paper)

shows the distribution of the distance of closest approach (dca) of protons and anti-protons to the collision vertex.  Real protons and anti-protons created in the collision will mostly be close to the collision point (near a dca of 0), so this shows up as a peak around a dca of 0.  Our largest background is from protons knocked out of the beam pipe by a fast particle created in the collision.  These protons don’t get close to the collision vertex – their dca is larger.  This is why the proton peak on the left sits on top of a plateau.  But we can’t knock anti-protons out of the beam pipe – so we don’t see the same plateau under the anti-proton peak.  Protons knocked out of the beam pipe will also be slower on average than protons created in the collision.  This is why we see the plateau from protons knocked out of the beam pipe on the left (for protons with momentum p≈0.5 GeV/c) but we don’t see it on the right (for protons with roughly twice the momentum, p≈1.0 GeV/c).  To get an accurate anti-proton to proton ratio, we have to subtract off the protons knocked out of the beam pipe.  We can tell where particles travelling practically at the speed of light went to within a few mm – and we need to in order to do our measurements.

Isn’t that cool?  ALICE is a wonderful detector!

Explanation of the lower x-axis of the anti-proton to proton ratio plot:

This is the difference between the beam rapidity, y, and the rapidity where the measurement is done (|y|<0.5).  You can calculate the beam rapidity using

y = 1/2 ln((E+pz)/(E-pz))

where pz is the momentum along the beam axis and E=√(E2+m2) is the total energy.  If you plug in the numbers, you’ll see that the beam rapidity is about 7.6 for 900 GeV and about 9.6 for 7 TeV.  I have fudged over a detail, which is that it matters where we do the measurement.  If we look closer to the beam axis, we’ll see a lower anti-proton to proton ratio and we’ll get the highest anti-proton to proton ratio at rapidities close to zero (roughly perpendicular to the beam axis).

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On the border

Posted by Mike Anderson on 27 Jun 2010

The LHC ring crosses the France/Switzerland border in something like 6 places.  Unfortunately, since Switzerland isn’t in the EU, one needs to have both Euros and Swiss Francs when working and living near CERN.  The main site is just barely in Switzerland, while several other CERN sites are in France.  For example, our detector, CMS, is about 8 miles into France.

Vending machines do not take more than once kind of currency.  Also, border guards don’t take kindly to bringing wine or meat across the border.

As for the American dollars, I only happened to have those because I recently traded euros to someone who was moving to France permanently, while I was going back to the US within a week or so.

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