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Physicists did a lot of planning for data analysis before the LHC ever ran, and we’ve put together a huge number of analyses since it started. We’ve already looked for most of the things we’ll ever look for. Of course, many of the things we’ve been looked for haven’t shown up yet; in fact, in many cases including the Higgs, we didn’t expect them to show up yet! We’ll have to repeat the analysis on more data. But that’s got to be easier than it was to collect and analyze the data the first time, right? Well, not necessarily. We always hope it will be easier the second or third time around, but the truth is that updating an analysis is a lot more complicated than just putting more numbers into a spreadsheet.

For starters, every time we add new data, it was collected under different conditions. For example, going from 2011 to 2012, the LHC beam energy will be increasing. The number of collisions per crossing will be larger too, and that means the triggers we use to collect our data are changing too. All our calculations of what the pileup on top of each interesting collision looks like will change. Some of our detectors might work better as we fix glitches, or they might work worse as they are damaged in the course of running. All these details affect the calculations for the analysis and the optimal way to put the data together.

But even if we were running on completely stable conditions, there are other reasons an analysis has to be updated as you collect more data. When you have more events to look at, you might be interested in limiting the events you look at to those you understand best. (In other words, if an analysis was previously limited by statistical uncertainties, as those shrink, you want to get rid of your largest systematic uncertainties.) To get all the power out of the new data you’ve got, you might have to study new classes of events, or get a better understanding of questions where your understanding was “good enough.”

So analyzing LHC data is really an iterative process. Collecting more data is always presenting new challenges and new opportunities that require understanding things better than before. No analysis is ever the same twice.

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Chamonix 2012

Sunday, February 19th, 2012

At the start of each calendar year, the CERN management holds a workshop in Chamonix to discuss the LHC run plan for the coming year and beyond. This year’s meeting was held two weeks ago, and this past week CERN announced the outcomes. Now, after last year’s Chamonix, the plan came out differently than many of us had been expecting. But this year’s workshop results were consistent with this year’s rumors.

There is a clear physics goal for this year: both CMS and ATLAS should each individually be in a position to discover the standard-model Higgs boson, if it exists. There are two ways that the LHC will try to make this possible. The first is to deliver as many collisions (i.e. as much integrated luminosity) as the LHC can manage. The integrated luminosity target for this year is fifteen inverse femtobarns for each experiment, three times as much as was delivered last year. It will still be a challenge to discover the Higgs with that much data; the experiments will have to run efficiently and the experiments will have to be as clever as ever. But it is possible. CERN is also prepared to extend the LHC run if necessary to meet this luminosity target. This is important, as the LHC will enter a long shutdown after 2012, so this year is our last shot for a while at making a discovery, of a Higgs or anything else. We should remember that last year’s target was a mere one inverse femtobarn, yet we got five times that. Can we hope that the LHC will outperform expectations again this year?

The second way to improve our chances of discovery is to raise the energy of the beams. The production rate for the Higgs and many other hypothetical particles increases with beam energy. Thus the LHC will run with 4 TeV per beam rather than the 3.5 TeV of last year. The operational experience of the past two years gives the LHC physicists confidence that this beam energy will be safe for the machine. This means that the LHC will probably never run at 3.5 TeV/beam again; the data we have recorded will now be unique in human history. It means that we’ll have to think about how to juggle resources so that people can look at both the old and the new data, and how to properly archive it for future use. Also, all sorts of measurements that we have made before at the LHC become new again: we can ask how does the production rate for phenomenon X change as you change the beam energy from 3.5 TeV to 4 TeV.

One change that the experiments had hoped for, but will not come to pass, was a change in the time interval between collisions. It was 50 ns during 2011, and it will stay that way. That means that we are now expecting an average of 30 simultaneous proton-proton collisions per beam crossing. Had the bunch spacing been reduced to 25 ns, we could have hoped to record a similar amount of data, but with much simpler events. However, the LHC experts weren’t sure that they could provide as much integrated luminosity at 25 ns spacing as at 50 ns; it is a very different way to operate the machine. Integrating data is the need for the year, so 50 ns it is. The experiments have shown that they can handle the complex events, although it would be a stretch to call it a pleasant experience.

Finally, the plan for the longer term was sketched out. The LHC will enter a “long technical stop” (as CERN likes to put it) at the end of the year, which will go on for twenty months. Given that we’ll need some time afterwards to re-commission the accelerator and the detectors, it’s probably two years from “physics to physics.” This will give the machine and the experiments time to implement some needed and useful upgrades and repairs. On the machine side, this includes the preparations to run the LHC at much closer to the design energy. That is 7 TeV per beam, although it is sounding like 6.5 TeV/beam is much more likely to be the safe operating point. At this point, we can only guess what the particle physics landscape will look like, but a higher-energy LHC will allow us to explore it thoroughly.

That’s the plan — let’s get ready to re-start the search for new physics in under two months!

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As discussed in this blog post in Scientific American (see blog post here) the Tevatron experiments may have a few last interesting things to say when it comes to the Higgs Boson at the March meetings.

At the American Association for the Advancement of Science meeting Collider Detector at Fermilab (CDF) spokes person Rob Roser said that we can expect “something interesting” coming from the Tevatron in the coming month.

Now normally I don’t get into the excitement of “hints” of the Higgs because now it seems you can’t sneeze with out causing a “3-sigma” deviation in you data. However, if we are to take the last results from the LHC seriously and there is an intriguing deviation around 125 GeV for the Higgs search the data from the Tevatron might be very well suited to being sensitive to seeing evidence for the Higgs.

Atlas results for the search for the Higgs boson with an intriguing "peak" around 125 GeV

For me, this only goes back to a debate that was going on almost a year ago, and this was whether or not we should extend the run of the Tevatron. One of the more compelling arguments that was made was exactly the scenario that is playing out and goes something like this…

“If the Higgs is low mass as other experimental results suggest then the Tevatron is well posed to be sensitive to the Higgs mass and can provide a completely independent discovery of this elusive particle and aid in measuring many of the properties of the Higgs and unlock many of the mysteries to the universe and the origins of mass.”

However, this didn’t compel enough people to make this happen, so we are left with this opportunity for the Tevatron to contribute to the Higgs search at a maximum of 3-sigma confirmation due to limited data samples.

Now of course this whole discussion is predicated on the fact that the Higgs lives in a low mass range (if it lives anywhere) all of which is not proven anywhere yet…

So this is just to say that the Tevatron is/was a great experiment and is still actively contributing to the discovery process unfolding every day in High Energy Physics and we should all stay tuned for this possible independent confirmation or refutation of the claims of where the Higgs boson may live.

Some great posts about the Higgs from my fellow bloggers:

Why do we expect a Higgs Boson? Part II Unitarization of Vector Boson Scattering

It Might Look Like a Higgs, But Does it Really Sing Like One?

 

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Error Control in Science

Friday, February 17th, 2012

Scientists are subject to two contradictory criticisms. The first is that they are too confident of their results, to the point of arrogance. The second is that they are too obsessed about error control–all this nonsense about double blind trials, sterilized test tubes, lab coats and the like. It evidently has not occurred to the critics that the reason scientists are confident of their results is that they have obsessed over error control. Or conversely they obsess over error control so they can be confident of their results.

Now, most people outside science, do not realize a scientist’s day job is error control. There is this conception of scientists having brilliant ideas, going into immaculate labs where they effortlessly confirm their results to the chagrin of their competitors. That is, of course, when they are not plotting world domination like Pinky and the Brain.  But scientists neither spend their time plotting world domination (be with you in a minute Brain) nor doing effortless experiments. But rather they are thinking about what might be wrong; how do I control that error? As for theorists, they must be a part of a wicked and adulterous generation[1] because they are always seeking after a sign–a minus sign that is.

So what do scientists do to control errors? There are very few arrows in their quiver. Really only three: care in doing the experiment or calculation, care in doing the experiment or calculation, and care in doing the experiment or calculation. Well actually there are two others: peer review and independent repetition. Let’s take the first three first: care, care, and care. As previously noted, scientists are frequently criticized here. Why do double blind studies when we have Aunt Martha’s word for it that Fyffe’s Patented Moose Juice cured her lumbago? Well actually, testimonials are notoriously unreliable. A book[2] I have, had an example of from the early 1900’s of testimonials for cures for consumption and then had the dates the person died of consumption. The death was frequently quite close to the date of the testimonial. So no, I will not trust Aunt Martha’s testimonial[3]. To quote Robert L. Park: The most important discovery of modern medicine is not vaccines or antibiotics, it is the randomized double-blind test, by means of which we know what works and what doesn’t. This has now carried over into subatomic physics where blind analyses are common. By blind, I mean that the people doing the analysis cannot tell how close they are to the expected answer (the theoretically predicted answer or the results of a previous experiment) until most of the analysis has been completed. Otherwise, as one of my experimental colleagues said: data points are like sheep, they travel in flocks. Even small biases can influence the results. Blind analysis is just one example of the extremes scientists go to, to ensure that their results are reliable. All this rigmarole that scientists go through is one of the reasons life expectancy increased by about 30 years between 1900 and 2000, perhaps the major reason. The lack of this care is the reason I distrust alternative medicine.

We now move on to the other two aspects of error control: peer review and independent replication of results. Both of these depend on the results being made public. Since these are crucial to error control, results that have not been made available for scrutiny should be treated with suspicion. Peer review has been discussed in the previous post and is just the idea that new results should be run past the people who are most knowledgeable so they can check for errors.

Replication is, in the end, the most important part of error control. Scientists are human, they make mistakes, they are deluded, and they cheat. It is only through attempted replication that errors, delusions, and outright fraud can be caught. And it is very good at catching them. In the next post, I will go into the examples but it is a good practice not to trust any exciting new result until it has been independently confirmed. However replication and reproducibility are not simple concepts. I go out doors and it is nice and sunny, I go out twelve hours later and it is dark and cold. The initial observation is not reproduced. I look up, I see stars. An hour later I go out and the stars are in different places. And the planets, over time, they wander hither, thither and yon. In a very real sense the observations are not reproduced. It is only within the context of model or paradigm that we can understand what reproducible means. The models, either Ptolemaic or Newtonian, tell us where to look for the planets and we can reproducibly check they are where the models say they should be at any given time. Reproducibility is always checking against a model prediction.

Replication is also not just doing the same things over and over again. Then you would make the same mistakes and get the same results over and over again. You do things differently, guided by the model being tested, to see if the effect observed is an artifact of the experimental procedures or real. Is there really a net energy gain or have you just measured a hot spot in your flask. The presence of the hot spot can be reproduced, but put in a stirrer to test the idea of energy gain and, damn, the effect went away. Another beautiful model was slain by an ugly observation. Oh, well, happens all the time.

So science advances, we keep testing our previous results in new and inventive ways. The wrong results fall by the wayside and are forgotten. The correct ones pile up and we progress. To err is human, to control errors–science.

Additional posts in this series will appear most Friday afternoons at 3:30 pm Vancouver time. To receive a reminder follow me on Twitter: @musquod.


[1] Matthew 12:39,16:4

[2] Pseudoscience and the Paranormal, Terence Hines, Prometheus Books, Buffalo (1988).

[3] My grandfather died of consumption.

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Releasing LHCb results

Thursday, February 16th, 2012

Winter conference season [*] is upon us, which means everybody is busy preparing new results. Today, instead of talking about the physics itself, I’m going to discuss the process around it; namely the procedure which the results of an LHCb analysis [**] need to go through before being released.

There are two ways in which analysis results are released: either through a conference note, meaning it is a preliminary result, or to a paper. I’m only going to discuss the former because I’m currently going through that procedure at the moment, though as a referee of the analysis and not a proponent.

The preliminary result approval procedure is constantly in flux, but currently, it looks something like this:
which is a simplified (and coloured) version of what can publicly be accessed on the LHCb editorial board webpage.

I think the most important points to note are the levels of the scrutiny that each analysis goes through before release. When I say that “everybody is busy preparing new results”, I’m not just referring to the people who are performing the specific analyses which are being released, I also include all the assigned analysis referees and editorial board members, and the physics coordinator as well as interested members of the collaboration, who can review the public notes and attend the approval presentations.

Believe me when I tell you that there have been/will be lot of extra emails and meetings this month due to all the paper and conference note reviews and approval presentations… Here’s looking forward to the Moriond conferences where the new results will be presented!

——————————————————————————–
[*] Winter conference season for experimental particle physics refers to the cluster of conferences held in February and March every year. The most well known of these are Aspen, Lake Louise, La Thuile and Moriond. Yes, these conferences are held annually at ski resorts. The conference organisers are understanding enough to give participants time to take advantage of the location, with sessions in the morning and evening, but none in the afternoon. I personally call these conferences “skiing conferences”. I have never been to any of them, but I would love to some day. They sound like the perfect combination of work and fun.

[**] I should probably mention that all experimental particle physics collaborations have some sort of publication procedure, most of which involve some sort of detailed internal document, followed by the public document.

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The EMMA accelerator ring

Working with an international team, three physicists from Brookhaven Lab have helped to demonstrate the feasibility of a new kind of particle accelerator that may be used in future physics research, medical applications, and power-generating reactors. The team reported the first successful acceleration of particles in a small-scale model of the accelerator in a paper published in Nature Physics.

The device, named EMMA and constructed at the Daresbury Laboratory in the UK, is the first non-scaling fixed field alternating gradient accelerator, or non-scaling FFAG, ever built. It combines features of several other accelerator types to achieve rapid acceleration of subatomic particles while keeping the scale — and therefore, the cost — of the accelerator relatively low.The technology is of particular interest to Brookhaven physicists who want to accelerate muons, heavier but short-lived relatives of electrons, to study the fundamental laws of physics. Brookhaven physicist Scott Berg, who worked on the conceptual design and commissioning of the new machine, as well as tests of its performance, explains:

Colliding beams of muons can let us study the fundamental laws of physics at the highest energies and smallest length scales — beyond what any existing accelerators are capable of. Accelerating muons can also produce an intense beam of neutrinos, another type of subatomic particle, enabling detailed studies of their properties.

See the full story here.

Karen McNulty Walsh, BNL Media & Communications Office

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La face cachée du CERN

Wednesday, February 15th, 2012

La plupart des gens associent le CERN avec le Grand Collisionneur de Hadrons (LHC). Pourtant,  on y retrouve aussi de nombreuses expériences certes moins connues mais très diversifiées.

Près d’un millier de scientifiques travaillent sur des expériences allant de l’antimatière à des thérapies anti-cancer, en passant par la formation des nuages et la production de radioisotopes.

Déjà en 2011, l’expérience ALPHA a fait les manchettes en réussissant à conserver de l’antihydrogène pendant plus de quinze minutes. Antiparticules et particules sont produites en quantités égales dans les accélérateurs de hautes énergies. Mais comme nous vivons dans un monde fait de matière, confiner de l’antimatière n’est pas une mince affaire.  Il faut l’empêcher d’entrer en contact avec la matière, sinon les deux s’annihileront. Habituellement, une «bouteille magnétique» est utilisée pour le confinement. Il s’agit d’un espace délimité par de puissants champs magnétiques et opéré dans un vide absolu pour éviter cette rencontre. Il faut au préalable réussir à combiner un antiproton avec un antiélectron (appelé «positon») à très basse température. Ainsi, les antiatomes formés ont aussi peu d’énergie que possible afin qu’on puisse les piéger, soit moins de 0.5 0K ou -272.5 0C.

Malgré tout, maintenant que les techniques de confinement ont été améliorées en 2011, le but des expériences ALPHA, ASACUSA, et ATRAP est maintenant de voir si ces antiatomes ont les mêmes propriétés que les atomes de matière, la même spectroscopie par exemple. Une nouvelle expérience AEgIS démarrera cette année et tentera de vérifier si la constante gravitationnelle g de l’antihydrogène est la même que celle de la matière.

Entre temps, l’expérience CLOUD essaie de résoudre une vieille énigme: comment se forment les aérosols dans l’atmosphère? Toutes les gouttelettes de nuages apparaissent sur des aérosols, de toutes petites particules liquides ou solides en suspension dans l’air. Mais la formation de ces aérosols demeure un mystère. Pour y répondre, on utilise une chambre à température contrôlée contenant de l’air pur où on introduit des traces de vapeurs d’éléments chimiques. Et surprise, on constate que l’ammoniaque et l’acide sulfurique, les deux composants chimiques aéroportés soupçonnés d’être responsables de la formation de tous les aérosols, contribuent à peine à expliquer la formation d’un dixième à un millième des taux observés dans l’atmosphère. Le programme pour 2012 est donc clair : identifier les éléments manquants et poursuivre l’étude de l’effet des rayons cosmiques (simulés avec des faisceaux de pions) sur la formation de ces aérosols.

Beaucoup d’activité aussi du côté de la thérapie hadronique, une technique de pointe utilisée dans la lutte contre le cancer. Des protons et autres ions légers remplacent les photons des rayons X utilisés en radiothérapie. Le défi est de détruire les cellules cancérigènes sans affecter les cellules des tissus sains. Contrairement aux rayons X, les protons et ions de carbone déposent pratiquement toute leur énergie à la fin de leur parcours au lieu de la disséminer tout le long du trajet. Il est donc possible d’apporter de grandes quantités d’énergie là où on en a besoin, sans abimer les autres cellules en chemin.

Énergie déposée par différentes particules en fonction de la distance parcourue lorsqu’elles pénètrent la matière, par exemple un tissus humain. Les protons et les ions de carbone déposent la majorité de leur énergie à une profondeur bien précise, alors que les photons des rayons X conventionnels la dépose tout au long de leur parcours, endommageant les tissus sains avant d’atteindre la tumeur.

Le CERN a joué un rôle de catalyseur dans la formation du Réseau Européen de Recherche en Thérapie Hadronique (ENLIGHT) établi en 2002 pour faciliter la coordination des efforts européens. Durant les années 90, un groupe du CERN a développé la conception d’un accélérateur de particules pour la thérapie hadronique appelé PIMMS  (Proton Ion Medical Machine Study). Ce travail a servi de base pour plusieurs autres versions. Le CERN soutient aussi le vaste projet MedAustron en Autriche et planifie d’exploiter son expertise en technologie des accélérateurs pour développer une seconde génération d’appareils dédiés à la thérapie hadronique.

L’expérience ACE a testé la même idée avec des antiprotons. L’avantage est qu’ils détruisent plus de cellules malignes avec l’énergie supplémentaire libérée lors de l’annihilation des antiquarks de l’antiproton avec les quarks des protons et neutrons de la tumeur. Ces travaux seront complétés cette année.

Et puis il y a ISOLDE, un centre qui utilise un petit accélérateur du CERN (le booster du Proton Synchroton) pour produire des noyaux “exotiques” pour presque tous les éléments chimiques en ajoutant des protons à des noyaux stables. Ces radioisotopes sont ensuite utilisés par une cinquantaine d’expériences pour étudier le structure du noyau, l’astrophysique nucléaire, les symétries fondamentales, la physique atomique et de l’état solide, et des applications en biologie.

D’autres scientifiques utilisent des faisceaux de neutrons de n_TOF pour en autres tenter de transmuter des déchets radioactifs en éléments de plus courtes durées de vie, voire même les rendre stables et inoffensifs.

Les équipes de CAST et OSQAR elles sont  la recherche d’axions, paraphotons et caméléons, toutes des particules hypothétiques proposées par différentes théories pour expliquer la mystérieuse matière noire. Depuis une décennie déjà, ces chercheur-e-s ne cessent d’ajouter de nouvelles hypothèses sur leur liste de : « à trouver » sans risquer de chômer de si tôt.

Et comme des millions de personnes l’ont appris l’an dernier, le CERN fournit aussi des faisceaux de neutrinos à plusieurs expériences situées au laboratoire du Gran Sasso en Italie, dont OPERA où la troublante annonce de la mesure de neutrinos voyageant apparemment plus vite que la lumière a envoyé une onde de choc tout autour de la planète. Deux autres expériences du Gran Sasso se préparent en ce moment à vérifier ces résultats dans les mois à venir.

Voilà donc quelques unes des nombreuses expériences en cours au CERN en plus du programme du LHC. Ensemble, elles font du CERN un endroit valant la peine de garder à l’œil. Alors suivez nous sur Twitter @CERN.

Pauline Gagnon

Pour être averti-e lors de la parution de nouveaux blogs, suivez-moi sur Twitter: @GagnonPauline ou par e-mail en ajoutant votre nom à cette liste de distribution

 

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The hidden face of CERN

Wednesday, February 15th, 2012

Most people associate CERN with the Large Hadron Collider (LHC). But lesser known although extremely diversified research activities are also ongoing at CERN.

About a thousand physicists are working on experiments ranging from antimatter studies to cancer therapy, cloud formation and radioisotope production.

Already in 2011, the ALPHA experiment made the headlines when they managed to trap antihydrogen atoms for more than fifteen minutes. Antiparticles and particles are produced in equal amounts in high energy accelerators. But since we live in a world made of matter, it is no small feat to prevent antiparticles from annihilating with particles of matter and vanishing. Usually, a magnetic “bottle” is used as the trap  This is a space confined by strong magnetic fields and operated in a high vacuum to keep antimatter from encountering any matter. First hurdle: one has to combine an antiproton with an antielectron (called “positron”) at low temperature to form antihydrogen atoms that are sluggish enough to be able to trap them (less than 0.5 K or -272.5 0C).

Nevertheless, having improved their antihydrogen production techniques in 2011, the goal of the ALPHA, ASACUSA, and ATRAP experiments is now to see if these antiatoms have the same properties as their counterpart of matter, the same spectroscopy for example. A new experiment AEgIS will come online this year with the long-term goal of measuring the gravitational constant g with antihydrogen to see if it is the same g as matter experiences.

Meanwhile, the CLOUD experiment is attempting to solve a long-standing enigma: how do aerosol particles form in the atmosphere? All cloud droplets form on aerosols — tiny solid or liquid particles suspended in the air – but how these aerosols form or “nucleate” remains a mystery. To find out, a chamber with a carefully controlled temperature is used to introduce traces of various chemical vapours into an initially “pure” atmosphere. Surprise: ammonia and sulphuric acid, the two airborne chemicals thought to be responsible for all aerosol formation, can account for only one tenth to one thousandth of the rate observed in nature. The goal for 2012 is clear: identify the missing elements and pursue studies on the influence of cosmic rays (simulated using a pion beam) on the aerosol formation rate.

Lots of developments are happening in hadron therapy, a cutting-edge cancer therapy technique where protons and other light ions are used instead of X-rays photons as in conventional radiotherapy treatment. The challenge is to destroy cancer cells without affecting the neighbouring healthy tissue. Contrary to X-rays, protons and other ions deposit nearly all their energy at a specific point near the end of their path instead of all along their path. This means one can bring large amounts of energy exactly where needed without causing damage along the way.


Energy deposited by different particles as they penetrate matter such as human tissue. Protons and carbon ions deposit most of their energy at a specific depth, whereas photons used in conventional X-rays tend to leave energy all along their path, damaging healthy tissue.

CERN acted as a catalyst in the formation of the European Network for Research in Light-Ion Hadron Therapy (ENLIGHT) in 2002 , which was established to coordinate European efforts in radiation therapy using light-ion beams. During the 1990s a group at CERN developed designs for a hadron therapy accelerator in the Proton Ion Medical Machine Study(PIMMS). This basic work has been incorporated into several of the subsequent designs. CERN is currently supporting the MedAustron therapy project in Austria and is also planning to exploit its accelerator technology and expertise in developing a second generation design for hadron therapy.

The ACE experiment has also tested the idea of using beams of antiprotons for hadron therapy, with the added advantage of blasting more malignant cells because of the amount of energy released when the antiquarks of the antiproton annihilate with the quarks of protons or neutrons from one of the cancer cells. This work is nearly completed and will be finished this year.

Much is also ongoing at the ISOLDE facility, which uses protons from a small CERN accelerator (the Proton Synchroton Booster) to produce “exotic” nuclei from most chemical elements by adding protons to stable nuclei. The radioisotopes are then used by more than 50 experiments to study nuclear structure, nuclear astrophysics, fundamental symmetries, atomic and condensed-matter physics, and for applications in life sciences. Some scientists pursue research using neutron beams from the n_TOF facility in the hope of transforming long-lived radioactive waste from nuclear power plants into shorter-lived or stable, non-radioactive elements.

Others at the CAST and OSQAR experiments are hot on the tail of “axions”, “paraphotons” and “chameleons”, some of the many hypothetical and rather exotic particles proposed by theorists to explain the nature of dark matter. For the past decade, these experimentalists have been adding new tricks to their experiments every few years to test new hypotheses and axions of heavier masses. More ideas keep these experiments’ “dance-cards” full all the time.

As millions of individuals have heard, CERN also supplies a neutrino beam to several experiments at the Gran Sasso Laboratory in Italy, including OPERA where puzzling results on muon neutrinos apparently travelling faster than the speed of light were reported last year. Two separate experiments at Gran Sasso are now setting up to cross-check this result in the coming months.

Much more is happening but it is impossible to do every one justice in a short overview. These are just a few of the many activities ongoing at CERN besides the LHC programme. All together, they make CERN a place well worth keeping an eye on in 2012, so follow us on Twitter @CERN.

Pauline Gagnon

To be alerted of new postings, follow me on Twitter: @GagnonPauline or sign-up on this mailing list to receive and e-mail notification.

 

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Hi everyone—it’s time that I wrap up some old posts about the Higgs boson. Last December’s tantalizing results may end up being the first signals of the real deal and the physics community is eagerly awaiting the combined results to be announce at the Rencontres de Moriond conference next month. So now would be a great time to remind ourselves of why we’re making such a big deal out of the Higgs.

Review of the story so far

Since it’s been a while since I’ve posted (sorry about that!), let’s review the main points that we’ve developed so far. See the linked posts for a reminder of the ideas behind the words and pictures.

There’s not only one, but four particles associated with the Higgs. Three of these particles “eaten” by the W and Z bosons to become massive; they form the “longitudinal polarization” of those massive particles. The fourth particle—the one we really mean when we refer to The Higgs boson—is responsible for electroweak symmetry breaking. A cartoon picture would look something like this:

The solid line is a one-dimensional version of the Higgs potential. The x-axis represents the Higgs ”vacuum expectation value,” or vev. For any value other than zero, this means that the Higgs field is “on” at every point in spacetime, allowing fermions to bounce off of it and hence become massive. The y-axis is the potential energy cost of the Higgs taking a particular vacuum value—we see that to minimize this energy, the Higgs wants to roll down to a non-zero vev.

Actually, because the Higgs vev can be any complex number, a more realistic picture is to plot the Higgs potential over the complex plane:

 

Now the minimum of the potential is a circle and the Higgs can pick any value. Higgs particles are quantum excitations—or ripples—of the Higgs field. Quantum excitations which push along this circle are called Goldstone bosons, and these represent the parts of the Higgs which are eaten by the gauge bosons. Here’s an example:

Of course, in the Standard Model we know there are three Goldstone bosons (one each for the W+, W-, and Z), so there must be three “flat directions” in the Higgs potential. Unfortunately, I cannot fit this many dimensions into a 2D picture. :-) The remaining Higgs particle is the excitation in the not-flat direction:

Usually all of this is said rather glibly:

The Higgs boson is the particle which is responsible for giving mass.

A better reason for why we need the Higgs

The above story is nice, but you would be perfectly justified if you thought it sounded like a bit of overkill. Why do we need all of this fancy machinery with Goldstone bosons and these funny “Mexican hat” potentials? Couldn’t we have just had a theory that started out with massive gauge bosons without needing any of this fancy “electroweak symmetry breaking” footwork?

It turns out that this is the main reason why we need the Higgs-or-something-like it. It turns out that if we tried to build the Standard Model without it, then something very nefarious happens. To see what happens, we’ll appeal to some Feynman diagrams, which you may want to review if you’re rusty.

Suppose you wanted to study the scattering of two W bosons off of one another. In the Standard Model you would draw the following diagrams:

There are other diagrams, but these two will be sufficient for our purposes. You can draw the rest of the diagrams for homework, there should be three more that have at most one virtual particle. In the first diagram, the two W bosons annihilate into a virtual Z boson or a photon (γ) which subsequently decay back into two W bosons. In the second diagram it’s the same story, only now the W bosons annihilate into a virtual Higgs particle.

Recall that these diagrams are shorthand for mathematical expressions for the probability that the W bosons to scatter off of one another. If you always include the sum of the virtual Z/photon diagrams with the virtual Higgs diagram, then everything is well behaved. On the other hand, if you ignored the Higgs and only included the Z/photon diagram, then the mathematical expressions do not behave.

By this I mean that the probability keeps growing and growing with energy like the monsters that fight the Power Rangers. If you smash the two W bosons together at higher and higher energies, the number associated with this diagram gets bigger and bigger. If  these numbers get too big, then it would seem that probability isn’t conserved—we’d get probabilities larger than 100%, a mathematical inconsistency. That’s a problem that not even the Power Rangers could handle.

Mathematics doesn’t actually break down in this scenario—what really happens in our “no Higgs” theory is something more subtle but also disturbing: the theory becomes non-perturbative (or “strongly coupled”). In other words, the theory enters a regime where Feynman diagrams fail. The simple diagram above no longer accurately represents the W scattering process because of large corrections from additional diagrams which are more “quantum,” i.e. they have more unobserved internal virtual particles. For example:

In addition to this diagram we would also have even more involved diagrams with even more virtual particles which also give big corrections:

And so forth until you have more diagrams than you can calculate in a lifetime (even with a computer!). Usually these “very quantum” diagrams are negligible compared to the simpler diagrams, but in the non-perturbative regime each successive diagram is almost as important as the previous. Our usual tools fail us. Our “no Higgs theory” avoids mathematical inconsistency, but at the steep cost of losing predictivity.

Now let me be totally clear: there’s nothing “wrong” with this scenario… nature may very well have chosen this path. In fact, we know at least one example where it has: the theory of quarks and gluons (QCD) at low energies is non-perturbative. But this is just telling us that the “particles” that we see at those energies aren’t quarks and gluons since they’re too tightly bound together: the relevant particles at those energies are mesons and baryons (e.g.pions and protons). Even though QCD—a theory of quarks and gluons—breaks down as a calculational tool, nature allowed us to describe physics in terms of perfectly well behaved (perturbative) “bound state” objects like mesons in aneffective theory of QCD. The old adage is true: when nature closes a door, it opens a window.

So if we took our “no Higgs” theory seriously, we’d be in an uncomfortable situation. The theory at high energies would become “strongly coupled” and non-perturbative just like QCD at low energies. It turns out that for W boson scattering, this happens at around the TeV scale, which means that we should be seeing hints of the substructure of the Standard Model electroweak gauge bosons—which we do not. (Incidentally, the signatures of such a scenario would likely involve something that behaves somewhat like the Standard Model Higgs.)

On the other hand, if we had the Higgs and we proposed the “electroweak symmetry breaking” story above, then this is never a problem. The probability for W boson scattering doesn’t grow uncontrollably and the theory remains well behaved and perturbative.

Goldstone Liberation at High Energies

The way that the Higgs mechanism saves us is somewhat technical and falls under the name of the Goldstone Boson Equivalence Theorem. The main point is that our massive gauge bosons—the ones which misbehave if there were no Higgs—are actually a pair of particles: a massless gauge boson and a massless Higgs/Goldstone particle which was “eaten” so that the combined particle is massive. One cute way of showing this is to show the W boson eating Gold[stone]fish:

Indeed, at low energies the combined “massless W plus Goldstone” particle behaves just like a massive W. A good question right now is “low compared to what?” The answer is the Higgs vacuum expectation value (vev), i.e. the energy scale at which electroweak symmetry is broken.

However, at very high energies compared to the Higgs vev, we should expect these two particles to behave independently again. This is a very intuitive statement: it would be very disruptive if your cell phone rang at a “low energy” classical music concert and people would be very affected by this; they would shake their heads at you disapprovingly. However, at a “high energy” heavy metal concert, nobody would even hear your cell phone ring.

Thus at high energies, the “massless W plus Goldstone” system really behaves like two different particles. In a sense, the Goldstone is being liberated from the massive gauge boson:

Now it turns out that the massless W is perfectly well behaved so that at high energies. Further, the set of all four Higgses together (the three Goldstones that were eaten and the Higgs) are also perfectly well behaved. However, if you separate the four Higgses, then each individual piece behaves poorly. This is fine, since the the four Higgses come as a package deal when we write our theory.

What electroweak symmetry breaking really does is that it mixes up these Higgses with the massless gauge bosons. Since this is just a reshuffling of the same particles into different combinations, the entire combined theory is still well behaved. This good behavior, though, hinges on the fact that even though we’ve separated the four Higgses, all four of them are still in the theory.

This is why the Higgs (the one we’re looking for) is so important: the good behavior of the Standard Model depends on it. In fact, it turns out that any well behaved theory with massive gauge bosons must have come from some kind of Higgs-like mechanism. In jargon, we say that the Higgs unitarizes longitudinal gauge boson scattering.

For advanced readers: What’s happening here is that the theory of a complex scalar Higgs doublet is perfectly well behaved. However, when we write the theory nonlinearly (e.g. chiral perturbation theory, nonlinear sigma model) to incorporate electroweak symmetry breaking, we say something like: H(x) = (v+h(x)) exp (i π(x)/v). The π’s are the Goldstone bosons. If we ignore the Higgs, h, we’re doing gross violence to the well behaved complex scalar doublet. Further, we’re left with a non-renormalizable theory with dimensionful couplings that have powers of 1/v all over the place. Just by dimensional analysis, you can see that scattering cross sections for these Goldstones (i.e. the longitudinal modes of the gauge bosons) must scale like a positive power of the energy. In this sense, the problem of “unitarizing W boson scattering” is really the same as UV completing a non-renormalizable effective theory. [I thank Javi S. for filling in this gap in my education.]

Caveat: Higgs versus Higgs-like

I want to make one important caveat: all that I’ve argued here is that we need something to play the role of the Higgs in order to “restore” the “four well behaved Higgses.” While the Standard Model gives a simple candidate for this, there are other theories beyond the Standard Model that give alternate candidates. For example, the Higgs itself might be a “meson” formed out of some strongly coupled new physics. There are even “Higgsless” theories in which this “unitarization” occurs due to the exchange of new gauge bosons. But the point is that there needs to be something that plays the role of the Higgs in the above story.

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par Nathalie Aubin et Sylvie Massiot, artistes de la compagnie Nukku Matti

Les zéolithes, le pic du spectre, disséquer les gonades, les nématodes, anaérobie, enzymatique, l’étuve agitante, interaction, j’ai du temps de faisceau, le pouième, la désintégration double béta des états excités, la soupe de quark, la magicité du noyau, TeV, KeV… Des mots imaginaires ? Non, le vocabulaire bien spécifique des scientifiques : leur « jargon » comme on dit. Parce que ces mots nous amusent, parce que les phénomènes qu’ils décrivent nous fascinent, et parce qu’ils nous inspirent tout simplement, nous venons de plonger dans l’univers de l’infiniment petit pour la création d’un spectacle sur la structure de la matière et les particules élémentaires. Nous terminons tout juste la deuxième phase : la prise de données…

Les comédiennes interprètent une chanson devant un instrument de physique du CENBG. Photo : Service audiovisuel de Bordeaux 1

Pour ce faire, nous nous sommes immergées, durant cinq jours, dans le monde de la recherche fondamentale et de la physique des particules. Notre expérience s’est déroulée plus précisément au Centre d’Etudes Nucléaires de Bordeaux Gradignan (CENBG). Nous y avons passé une semaine exceptionnelle et nous avons découvert un univers extraordinaire… Christine Marquet, chercheuse au CENBG, nous a ouvert les portes d’un monde jusqu’alors invisible à nos yeux. Ici les chercheurs tentent de percer les mystères par la réflexion, la collaboration, l’échange de savoir, l’invention et la construction d’instruments insolites pour le néophyte. L’ensemble des professionnels s’est mis à notre portée sans compter son temps, ni son énergie pour partager ses connaissances et ses questionnements.

Ainsi, chercheurs, ingénieurs, techniciens nous ont parlé de noyaux exotiques, de mécanique, d’électronique, de chimie chaude, d’astrophysique, de biologie, d’informatique, de particules mais aussi de la place de la recherche dans notre société, de l’importance de la collaboration internationale, de la question de la rentabilité incompatible avec le principe même de la recherche fondamentale. Nous avons collecté beaucoup de données qu’il va nous falloir analyser et trier, mais comme le dit Stéphane, un physicien du CENBG : « le résultat n’est pas toujours là où on l’attend ».

Toutefois cette semaine d’immersion confirme notre envie de transmettre au plus grand nombre l’enthousiasme dans lequel nous avons été plongées. Notre souhait le plus cher est de réussir à traduire dans ce spectacle la même passion, la même curiosité, la même envie de partage que les chercheurs nous ont montrée.


Vidéo de la « Prise de données » (réalisation : Service audiovisuel de l’Université Bordeaux 1)

Pour le moment intitulé « Parce que 12 », ce nouveau spectacle sera en tournée cet automne. Le projet est soutenu par : l’IDDAC, le CENBG, le CNRS/IN2P3, l’Université Bordeaux 1, la Communauté de Communes du Vallon de l’Artolie, la ville de Villenave de Rions. Pour suivre l’évolution du projet, rendez-vous sur la rubrique “Création 2012” de notre site web !

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