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The evolution of hadron-collider experiments

JUN 01, 2013
High-energy accelerator beams colliding head-on have now completed the discovery of all the fundamental particles required by particle theory’s standard model. The search is on for new ones.

DOI: 10.1063/PT.3.2010

Paul Grannis
Peter Jenni

In particle-physics experiments, the discovery of increasingly more massive particles has brought deep understanding of the basic constituents of matter and the fundamental forces between them. Such discoveries are made possible by accelerator beams of ever more energetic particles.

Traditionally, such beams were directed at stationary targets. In that configuration, however, the total center-of-mass energy Ecm of a collision between a beam particle of energy Eb and a target particle grows only like √Eb. But Ecm is what limits the masses of particles a collision can produce.

One can get much more bang (Ecm) for the buck (Eb) by making counterpropagating particle beams collide head-on. In that case, Ecm grows much faster; for beams of equal mass and energy, it’s simply 2Eb. For almost half a century now, such colliding-beam accelerators—colliders—have been hurling beams of hadrons (protons, antiprotons, nuclei) or leptons (electrons, positrons) at each other with increasing vehemence.

In this article, we focus on hadron colliders and particularly on the experimental techniques that have evolved with them. Their crowning achievement to date is the Large Hadron Collider (LHC) at CERN, whose proton beams last year achieved an Ecm of 8 TeV, almost ten thousand times the 0.9-GeV mass of the proton. That collision energy sufficed to reveal a new particle that’s very likely to be the long-awaited Higgs boson (see Physics Today, September 2012, page 12 ).

Beginnings

The first hadron collider was the 1-km-circumference proton–proton (pp) Intersecting Storage Rings (ISR), 1 commissioned at CERN in 1971. Its beam energies ranged from 12 to 31 GeV. Experimenters set up particle detectors at eight points where the two countercirculating beams crossed each other. Experiments at the ISR revealed the logarithmic rise of the pp total scattering cross section at energies where it was expected to have leveled off. But the detectors were not, at first, adequately configured to study collisions that produced particles with large momentum components, pT, transverse to the collision axis. Only later was it fully realized how important high-pT events are for revealing new physics.

Ten years later, CERN’s Super Proton Synchrotron (SPS), until then a fixed-target accelerator, became the SppS, a proton–antiproton collider 2 with Ecm up to 630 GeV. The antiprotons (p) were produced by intense proton beams striking a metal target and then formed into a beam by magnets, collimators, and stochastic cooling—magnetic kicks based on feedbacks from detected beam fluctuations.

The two countercirculating beams were tethered in the collider’s 7-km-circumference tunnel by an array of 1.3-T bending magnets. By the end of 1983, the collaborations that ran the large UA1 and UA2 detectors at the collider’s beam-crossing points had discovered the heavy W± and Z0 bosons that mediate the weak interactions. 3

Before the end of the decade, Fermilab’s pp Tevatron collider 4 had raised Ecm to 1.8 TeV; eventually it reached 2 TeV. Containing the TeV beams in a 6-km-circumference ring required 4.2-T superconducting magnets. For two decades until the startup of CERN’s LHC in 2009, the Tevatron operated as the world’s highest-energy particle collider.

The LHC’s design Ecm is 14 TeV. Confining the 7-TeV proton beams to a preexisting 27-km tunnel necessitated the challenging development of 8.3-T superconducting bending magnets. 5 But before LHC construction began in 1998, there was a painful interlude across the ocean. The planned 87-km tunnel of the Superconducting Super Collider, a 40-TeV pp collider, was already under construction near Dallas, Texas, when that project was abruptly canceled by the US Congress in 1993.

Luminosity

Collision energy Ecm is by no means the whole story. The frequency of particle collisions must be high enough to yield significant numbers of interesting events, even for rare processes with minuscule cross sections. Total pp and pp cross sections at high energies are large—of order 100 millibarns (1 mb = 10−27 cm2). But interesting processes today have cross sections typically given in femtobarns (1 fb = 10−12 mb).

A crucial figure of merit for the collision rate at a beam-crossing point is the luminosity L, given by the event rate per unit scattering cross section. For example, if L is 106/(mb s) at a beam crossing in a collider, that crossing will produce a total of about 108 collisions every second. Luminosity depends on a beam’s diameter and current, and on how well the exquisitely thin collider beams are aimed at each other. Typically, L improves with time and experience.

Luminosity integrated over time determines how many rare events an extended collider run can record. It is often appropriate to quote integrated luminosity in events per femtobarn. A run of several months at one of the LHC detectors might produce an integrated luminosity of 10 fb−1. Such a run, encompassing 1015 pp collisions, would be expected to record only a few hundred Higgs bosons with discernible decay modes.

Detectors

Particle detectors at hadron collider detectors have evolved in size and complexity as technology has advanced and physics questions have changed. Each generation of detectors has built on previous experience. The size increases reflect both higher energies and the need for greater sophistication.

The early ISR experiments had rather specific physics goals that were addressed with detector designs still influenced by the fixed-target era. They offered only limited solid-angle coverage. But toward the end of the ISR period, the anticipation of new discoveries stimulated a new detector paradigm. One now had to study new massive, short-lived particles like the W and Z bosons and the top quark, all very much heavier than the proton. Their decay particles emerge over a large angular region, usually with large pT. That required detectors with more complete angular coverage.

So, starting with the SppS experiments, new general-purpose detectors followed more holistic designs, with cylindrical shells of subdetectors surrounding the evacuated beam pipe and the small collision region with nearly full 4π solid-angle coverage. The innermost “tracker” shells record the ionization trails of charged particles moving in a magnetic field; a track’s curvature in the field measures its momentum. Just beyond the trackers are the calorimeters, in which electrons, photons, and hadrons reveal their energies by interacting with material. Muons, which typically traverse calorimeters without interacting strongly, require a final outer shell.

Detector designs varied, depending on the physics emphasis and the available technology. Figure 1 gives a sense of the evolution and variety of collider detectors. Trackers have evolved from multiwire and drift chambers that measured ionization trails with resolutions of a few hundred microns, to silicon-microstrip and pixelated detectors with micron resolution. That much-finer resolution makes possible the measurement of tiny distances between the production and decay points of the very short-lived, heavy-quark hadrons that often identify rare processes.

PTO.v66.i6.38_1.f1.jpg

Figure 1. Evolution of detectors that record collisions at hadron colliders. (a) The 6-m-diameter detector of the R702 experiment at CERN’s Intersecting Storage Rings1 in the 1970s. (b) The 10-m UA1 detector17 at CERN’s SuperProton–AntiprotonSynchrotron collider a decade later. (c) The 12-m Collider Detector at Fermilab at the Tevatron in 2000 (http://www-cdf.fnal.gov/physics/techpub_run2.html). (d) The 24-m ATLAS detector18 at CERN’s Large Hadron Collider has been taking physics data since 2009.

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To optimize the measurement of telltale transverse momenta, many collider detectors get their magnetic fields from a surrounding solenoid aligned with the beam axis. Field intensities have increased from about 1 T in early collider days to 4 T in the Compact Muon Solenoid (CMS) at the LHC. 6 (See the cover of this issue.)

Calorimeters are designed to measure the energies of hadrons, electrons, and photons by fully containing and recording the energy they lose in showering cascades of collisions as they stop in absorbing material. Because showers generated by hadrons are typically much bigger than those generated by electrons and photons, electromagnetic and hadron calorimeters require quite different designs.

So-called sampling calorimeters alternate absorbing layers with layers of transparent plastic scintillator or ionizing liquid whose signals are proportional to the energy of the traversing particle. Alternatives to such layered configurations are calorimeters made entirely of scintillating crystals.

Muons, the only charged particles that survive beyond the calorimeters, are usually identified in surrounding low-cost ionization detectors. The almost complete solid-angle coverage by calorimeters and muon detectors in modern detectors makes it possible to spot “missing” transverse energy carried away by high-energy neutrinos—or by something altogether new.

Keeping up with collision rates

With increased luminosity, total collision rates grew from 105 per second at the SppS to 107/s at the Tevatron, and now 109/s at the LHC. Although the ability to log data for later offline analysis has grown with modern computing technology, the number of bytes required to describe a collision event has also grown so much that one simply cannot record more than a few hundred events per second.

Therefore, complex trigger systems have evolved to select the relative handful of potentially interesting events from the flood of all collisions. Reliable triggering is essential because a rejected event is lost forever. At the SppS, triggers mostly used fast-hardware indicators of high-energy leptons ℓ± (muons and electrons) to signal interesting events. But a smaller event stream was selected by more elaborate online analysis in microprocessors. Three-level triggering was introduced at the Tevatron collider: The first decision, based on a tracker, calorimeter, or muon information, was made in single-chip processors. Then microprocessor decisions combined data from several subdetectors. Finally, a “farm” of processors ran a simplified version of offline processing. Such multiple-level triggering reduced the stream of accepted events to 50 Hz at a dead-time cost of only 5%.

Despite the challenging demands of the very high LHC luminosities, ATLAS and CMS, the collider’s two large general-purpose detectors, have refined multi-level triggering to achieve efficient and manageable event-logging rates of a few hundred per second, with only about 1% dead time.

The changing physics landscape

Interesting high-energy collisions between hadrons are best understood as interactions between a constituent quark or gluon (collectively called partons) in one hadron with a parton in the other. Quantum chromodynamics (QCD), the theory of those strong interactions, can—in principle—predict the wide array of possible outcomes. When a head-on parton collision produces a large-angle scattering, QCD’s paradoxically increasing force with increasing separation prevents partons from emerging as free particles.

Instead, quarks and gluons scattered in head-on parton–parton collisions manifest themselves at the detectors as “jets,” collimated sprays of hadrons. Predicted by QCD, jets were hinted at in ISR data. But then the SppS gave spectacular visual demonstration of their existence. (See, for example, figure 2a.)

PTO.v66.i6.38_1.f2.jpg

Figure 2. Jets of hadrons produced in high-energy collisions. (a) The angular distribution of energy deposited in the segmented calorimeter of the UA2 detector at the SppS collider shows two jets emerging in roughly opposite directions from a pp collision. Polar and azimuthal angles refer to the beam axis. Histogram bar heights indicate energy deposited in individual calorimeter components. (b) Differential cross sections for jet production at three generations of hadron colliders are plotted as functions of transverse momentum pT, the jet’s momentum component perpendicular to the beam axis. At large pT, the cross section grows markedly7 with increasing collision energy Ecm.

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Measured over 10 orders of magnitude at increasing Ecm, the differential cross section for the production of high-pT jets, plotted in figure 2b, is in excellent agreement with QCD calculations. Those cross sections provide a detailed look at the momentum distributions of different partons within the proton. 7 The most energetic jets arise from quarks or gluons that happened to be carrying about half of the incident proton’s momentum—much more than their fair share.

The search for the W± and Z0 bosons predicted by unified electroweak theory was the primary motivation for building the SppS collider. Their discovery in the early 1980s via their decays

W± → ℓ±ν and Z → ℓ+,

where ν denotes a neutrino, gave convincing evidence that hadron colliders are indeed great discovery tools. The discoveries demonstrated, in particular, the usefulness of missing transverse energy for indirectly measuring an escaping neutrino’s pT. The missing-energy signature also played a major role in the discovery of the top quark (t) at the Tevatron collider in 1995. And it is now a mainstay in the search for dark matter at colliders.

Following the handful of W and Z events seen by the UA1 and UA2 detector teams at the SppS, the CDF and D0 collaborations at the Tevatron measured the W mass (80.39 GeV) to a precision of 0.02% from about a million events. 8 That was a striking achievement in the messy environment of a hadron collider, where every interesting collision also produces dozens of uninteresting particles. The LHC experiments benefit from tens of millions of W and Z bosons, which can be used both for detailed detector calibrations and for precision tests of the standard model of particle physics.

In the early 1990s, the top quark was urgently sought as the sixth and last quark required by the standard model. Null results had made it clear that it was very much heavier than the 5-GeV bottom quark (b). The SppS teams could not find it, but they set a lower limit of 69 GeV on its mass, mt. The eventual discovery of the top quark was a major highlight of the Tevatron program, first in tt pair production 9 and, 14 years later, in the much more elusive process of single-t production. 10

The CDF and D0 teams measured mt to be 173.2 GeV, nearly the mass of a gold nucleus. Unlike the five lighter quarks, the top quark decays (mostly to W + b) before it has had time to dress itself in hadronic garb. The impressively small 0.5% uncertainty in mt underscores the modern capacity for precision measurements in complex production and decay topologies involving hadron jets, charged leptons, and undetectable neutrinos. A typical tt production event at the Tevatron is depicted in figure 3. At the LHC’s even higher collision energy, tt pairs are produced much more profusely. The LHC detector teams are exploiting that profusion in searches for very massive new particles that would decay into top quarks.

PTO.v66.i6.38_1.f3.jpg

Figure 3. Beam’s-eye view of a top–antitop quark pair created at the center of the Tevatron’s D0 detector. One top quark decays to a W boson plus a bottom (b) quark, and that W promptly decays to a muon plus a neutrino. The other top quark also decays to W + b, but that W decays into two quarks that emerge as jets of hadrons at 8 and 10 o’clock. The lengths of the histogram bars around the cylindrical detector represent energy deposited by jets in azimuthal calorimeter segments surrounding the detector’s inner tracking layers. The isolated blue line at 2 o’clock is the W-decay muon, and the jet encompassing the muon at 4 o’clock was generated by the decay of a b quark. The magenta bar at 3 o’clock indicates the missing energy and direction of the escaped neutrino.

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Cross-section measurements for the production of b quarks were first done at the SppS. The UA1 team also reported the first observation of quantum oscillation between quark-flavor states of neutral B mesons, which carry b quarks (see Physics Today, November 2012, page 16 ). The analogous flavor oscillation of neutral K mesons, which carry the strange quark, has been known since the 1960s.

Such oscillation arises from the fact that the quark-flavor eigenstates of the mesons are linear superpositions of mass eigenstates with slightly different masses. At the Tevatron, the CDF and D0 teams collected large samples of neutral B mesons with decay lengths accurately determined in silicon-strip vertex detectors. Thus the teams were able to measure the very rapid (0.3-ps) oscillation of B0s mesons, a subclass of B mesons that also carry strange quarks. 11 The CDF result is shown in figure 4.

PTO.v66.i6.38_1.f4.jpg

Figure 4. Neutral Bs mesons oscillate between states B0s and B0s, distinguished by whether the meson’s bottom-flavored quark is a b or a b. The CDF collaboration’s measured asymmetry,11 defined as the fractional difference between the number of decays that do not manifest flavor change and those that do, is plotted against the time between the meson’s creation and its decay. The data combine many oscillation periods. The best-oscillation-fit curve has a periodicity of 0.35 ps.

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At the LHC, not only ATLAS and CMS but also the smaller LHCb detector, dedicated to b-quark physics, continue flavor-oscillation investigations with huge samples of B mesons. That superabundance permits searches for extremely rare B-decay modes that would be sensitive to new physics beyond the standard model. The new physics might, for example, elucidate the observed predominance of matter over antimatter in our universe (see the article by Helen Quinn in Physics Today, February 2003, page 30 ). As yet, however, the most precise LHCb measurements—including the recent first observation of the very rare B0s decay to two muons—are in good agreement with standard-model predictions. 12

For decades the search for the Higgs boson (H) has been a primary goal of hadron-collider experiments. It drove the designs for ATLAS and CMS, which have to cope with many rare collision signatures embedded in a huge background of ordinary hadronic debris. The much-heralded 125-GeV boson announced by the ATLAS and CMS teams 13 last 4 July has not yet exhibited any departure from standard-model predictions for the Higgs boson.

That discovery was a giant experimental step toward the completion of the standard model. Figure 5 shows a rare candidate in ATLAS for the low-background decay mode

PTO.v66.i6.38_1.f5.jpg

Figure 5. Searching for the Higgs boson at CERN’s Large Hadron Collider.13 (a) The ATLAS detector records a candidate for the rare Higgs decay H → Z0Z0 → e+eμ+μ. The penetrating μ± are recorded in muon-detector panels (green) far outside the calorimeter segments (yellow) that stop the e± (red) and record the energies they deposit. (b) The CMS detector’s evidence for Higgs decay to two high-energy photons (γ) is the bump around 125 GeV in the observed distribution of γγ invariant masses—the γγ pair’s energy in its center-of-mass frame. The red curve is the best fit to the Higgs-decay signal plus background.

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H → Z0Z0 → e+eμ+μ.

The figure also shows the CMS’s evidence for the more abundant two-photon decay mode H → γγ.

The Higgs discovery at the LHC exploited innovative analysis techniques developed at the Tevatron collider. In fact, corroborating evidence was found 14 in D0 and CDF for H → bb. That decay mode actually dominates in the standard model, but it offers poor mass resolution.

The standard model leaves fundamental questions open: What is the particle nature of dark matter (see Physics Today, May 2013, page 14 )? Why does the unification of the electromagnetic and weak forces by the Higgs field occur at a mass scale so much lower than the seemingly natural 1019-GeV scale of the Planck mass, √ℏc/G, where gravitational and quantum effects become comparable? What caused the cosmological matter–antimatter imbalance? Why are there three families of quark and lepton pairs with such disparate masses?

Theoretical suggestions for new physics beyond the standard model abound, each with proposed experimental signatures. A prominent example is supersymmetry, in which each standard-model boson is partnered with a new fermion—and vice versa. Supersymmetry could solve several of the standard model’s problems and provide a plausible dark-matter particle. The need to search for supersymmetric particles set important benchmarks for the design of the LHC detectors.

In searches for new high-mass phenomena, the key is the increase of Ecm. As yet, the colliders have yielded no definitive evidence of new physics beyond the standard model. But the scheduled 2015 increase in the LHC collision energy to its design value of 14 TeV holds out great hope for early sightings of terra incognita.

Analysis tools

Computing and communication tools have been revolutionized over the past four decades. The ISR experiments were analyzed on large mainframe computers. Their limited processing speeds and storage-disk capacity forced a certain simplicity in algorithms for reconstructing collision events. At the Tevatron and the LHC, computing advances brought fundamental changes that made it possible to decipher complex decay patterns despite the presence of hundreds of background particles.

A typical LHC event generates a megabyte of information. Although collider experiments have contributed importantly to computing advances such as massively parallel processing and grid computing, the progress of high-energy physics rests squarely on the advances made by the computing industry.

The advent of fast and cheap field-programmable gate arrays, digital-signal processors, and microprocessors has made possible the migration of computer intelligence to the detectors themselves. The detectors can now perform smart event selection and full reconstruction in real time. Those capabilities also allow the efficient collection of special event samples used for calibrations in situ.

Lasers and position monitors make it possible to align detector components with micron precision. Microprocessor farms, having replaced mainframe computers for offline analyses, allow parallel processing of events that keeps up with the data flood. Large storage disks hold massive calibration databases that significantly improve detector resolution.

In the later Tevatron runs and at the LHC, distributed-grid computing 15 has permitted globally connected farms to generate large sets of simulated Monte Carlo events. The event-simulation programs have become remarkably sophisticated. The yearly volume of data, real and simulated, produced by ATLAS and CMS reaches tens of petabytes.

The increasing complexity of experiments has necessitated new analysis tools. Sophisticated new algorithms improve particle tracking by recognizing true tracks in the presence of noise. Multivariate pattern-recognition algorithms now identify electrons and photons on the basis of the shapes and correlations of energy deposits in finely segmented calorimeters. New “particle flow” methods rely on high-precision tracking measurements of charged-particle momenta instead of calorimeter measurements and thus improve the determination of jet energies.

As physics goals have turned toward finding increasingly rare processes in the face of huge backgrounds, the old methods of simply selecting events based on a set of basic kinematic variables have become too inefficient. New multivariate techniques such as neural networks and decision trees have become common. 16 Although the use of such algorithms initially met with skepticism, they have been shown to be reliable and very useful. And new statistical techniques, based on both frequentist and Bayesian methods, have become commonplace for combining many related measurements and minimizing the impact of systematic uncertainties (see the article by Louis Lyons in Physics Today, July 2012, page 45 ).

Collaborations

Hadron-collider collaborations have grown spectacularly in four decades. Typical experimental collaborations at the ISR in the early 1970s were consortia of a dozen or so physicists from a few institutes. By the early 1980s, the largest ISR experiment involved some 90 scientists from 16 institutes. The UA1 experiment at the SppS grew to comprise 170 scientists from 19 institutes.

At the Tevatron that trend continued. The CDF and D0 collaborations each brought together about 600 scientists, and they marked the beginning of the large-scale globalization of high-energy physics experiments. For example, D0 involved 81 institutions in 18 countries on 4 continents.

Globalization became even more pronounced at the LHC. The ATLAS and CMS collaborations each have about 3000 scientists from some 200 institutions in about 40 countries. About one-third of the scientists are students, and many more are PhD physicists in their early careers. Those statistics underline the educational value of front-line science activity and its value in fostering understanding of how to work productively with colleagues from different backgrounds. The collaborations and the host laboratories have made conscious efforts to include scientists from emerging nations.

At the ISR and the earlier, fixed-target accelerators, collaborations ran with a minimum of formal organization. Decisions were made at frequent meetings of all the participating physicists. But with the growing sizes, complexities, and costs of experiments, it became necessary to formalize collaboration rules and working structures. On one hand, the collaborations are nowadays internally organized from the bottom up by democratically established bodies and working groups, with elected spokespersons and written governance documents. On the other hand, relationships with the host laboratories, collaborating institutions, and funding agencies are formalized with memoranda of understanding that specify rights and obligations of all partners in a top-down manner.

Each of the giant collaborations comprises many distinct projects for design, building, software development, and physics analysis. The experiments have evolved rather complex organizational structures, with coordinators at various levels to ensure that the parts fit together smoothly. But the real work on individual projects is typically carried out by groups of relatively few individuals working closely together, just as in the early days of high-energy physics.

Geographical dispersion brought the need for new communications mechanisms. In the old days, physicists had to be on site to interact effectively with colleagues. But in the early 1980s, the internet revolution introduced new collaboration modes. Electronic messaging meant that physicists in far-flung locations could exchange information quickly. Although periodic face-to-face gatherings remained necessary, electronic communication made it possible for distant collaborators to conduct complex, ongoing analyses. By the turn of the millennium, videoconferencing further buttressed collaboration at a distance. A typical collaboration discusses progress by conducting dozens of video meetings on most days, hampered only by the wide disparity of time zones.

The SppS, the Tevatron collider, and the LHC have each housed two comparably large general-purpose detectors. That duplication has been essential for independently confirming—or in some cases shooting down—new “discoveries.” The competition between the experiments is also a powerful stimulator of innovative analysis strategies. The competition can be intense because neither collaboration wants to be scooped on an important discovery. Without the friendly rivalry, progress would surely be slower.

Modern high-energy-physics collaborations are peculiar organizations in that they are self-organized around common goals, but with no traditional authority for setting salaries or conducting formal employee reviews. And yet they have been enormously successful in articulating goals and mobilizing the requisite effort over time spans measured in decades. Loyalty to the experiment often transcends loyalty to the employing institution. It is not uncommon for individuals to pass from graduate student to permanent scientist with several sequential employers while working on a single experiment. The collider collaborations also have distinct personalities, typically formed in their very early days and persisting even after the early participants have left the scene.

The increasingly large and complex hadron-collider experiments have brought many challenges, but the lessons learned from successive generations of experiments have made possible remarkable advances in our understanding of Nature. Big science is here to stay.

References

  1. 1. K. Johnsen, Proc. Natl. Acad. Sci. USA 70, 619 (1973). https://doi.org/10.1073/pnas.70.2.619

  2. 2. C. Rubbia, P. McIntyre, D. Cline, in Proceedings of the International Neutrino Conference, Aachen 1976, H. Faissner, H. Reithler, P. Zerwas, eds., Vieweg, Braunschweig, Germany (1977), p. 683;
    J. Gareyte, in 11th International Conference on High-Energy Accelerators, Geneva, Switzerland, July 7-11, 1980, W. S. Newman, ed., Birkhauser, Basel, Switzerland (1980), p. 79.

  3. 3. G. Arnison et al. (UA1 collaboration), Phys. Lett. B 122, 103 (1983); https://doi.org/10.1016/0370-2693(83)91177-2
    G. Arnison et al. (UA1 collaboration), Phys. Lett. B 126, 398 (1983); https://doi.org/10.1016/0370-2693(83)90188-0
    M. Banner et al. (UA2 collaboration), Phys. Lett. B 122, 476 (1983); https://doi.org/10.1016/0370-2693(83)91605-2
    P. Bagnaia et al. (UA2 collaboration), Phys. Lett. B 129, 130 (1983). https://doi.org/10.1016/0370-2693(83)90744-X

  4. 4. H. T. Edwards, Annu. Rev. Nucl. Part. Sci. 35, 605 (1985); https://doi.org/10.1146/annurev.ns.35.120185.003133
    S. Holmes, R. S. Moore, V. Shiltsev, J. Instrum. 6, T08001 (2011). https://doi.org/10.1088/1748-0221/6/08/T08001

  5. 5. L. Evans, P. Bryant, eds., J. Instrum. 3, S08001 (2008). https://doi.org/10.1088/1748-0221/3/08/S08001

  6. 6. S. Chatrchyan et al. (CMS collaboration), J. Instrum. 3, S08004 (2008). https://doi.org/10.1088/1748-0221/3/08/S08004

  7. 7. A. A. Bhatti, D. Lincoln, Annu. Rev. Nucl. Part. Sci. 60, 267 (2010). https://doi.org/10.1146/annurev.nucl.012809.104430

  8. 8. T. Aaltonen et al. (CDF collaboration), Phys. Rev. Lett. 108, 151803 (2012); https://doi.org/10.1103/PhysRevLett.108.151803
    V. M. Abazov et al. (D0 collaboration), Phys. Rev. Lett. 108, 151804 (2012). https://doi.org/10.1103/PhysRevLett.108.151804

  9. 9. F. Abe et al. (CDF collaboration), Phys. Rev. Lett. 74, 2626 (1995); https://doi.org/10.1103/PhysRevLett.74.2626
    S. Abachi et al. (D0 collaboration), Phys. Rev. Lett. 74, 2632 (1995). https://doi.org/10.1103/PhysRevLett.74.2632

  10. 10. V. M. Abazov et al. (D0 collaboration), Phys. Rev. Lett. 103, 092001 (2009); https://doi.org/10.1103/PhysRevLett.103.092001
    T. Aaltonen et al. (CDF collaboration), Phys. Rev. Lett. 103, 092002 (2009). https://doi.org/10.1103/PhysRevLett.103.092002

  11. 11. V. M. Abazov et al. (D0 collaboration), Phys. Rev. Lett. 97, 021802 (2006); https://doi.org/10.1103/PhysRevLett.97.021802
    A. Abulencia et al. (CDF collaboration), Phys. Rev. Lett. 97, 242003 (2006). https://doi.org/10.1103/PhysRevLett.97.242003

  12. 12. R. Aaij et al. (LHCb collaboration), Phys. Rev. Lett. 108, 101803 (2012). https://doi.org/10.1103/PhysRevLett.108.101803

  13. 13. G. Aad et al. (ATLAS collaboration), Phys. Lett. B 716, 1 (2012); https://doi.org/10.1016/j.physletb.2012.08.020
    S. Chatrchyan et al. (CMS collaboration), Phys. Lett. B 716, 30 (2012). https://doi.org/10.1016/j.physletb.2012.08.021
    See also the review by M. Della Negra, P. Jenni, T. S. Virdee, Science 338, 1560 (2012). https://doi.org/10.1126/science.1230827

  14. 14. T. Aaltonen et al. (CDF and D0 collaborations), Phys. Rev. Lett. 109, 071804 (2012). https://doi.org/10.1103/PhysRevLett.109.071804

  15. 15. J. Harvey, P. Mato, L. Robertson, in The Large Hadron Collider: A Marvel of Technology, L. Evans, ed., EPFL Press, Lausanne, Switzerland (2009), p. 229.

  16. 16. P. C. Bhat, Annu. Rev. Nucl. Part. Sci. 61, 281 (2011). https://doi.org/10.1146/annurev.nucl.012809.104427

  17. 17. C. Albajar et al. (UA1 collaboration), Z. Phys. C 48, 1 (1990). https://doi.org/10.1007/BF01565600

  18. 18. G. Aad et al. (ATLAS collaboration), J. Instrum. 3, S08003 (2008). https://doi.org/10.1088/1748-0221/3/08/S08003

More about the Authors

Paul Grannis is a Distinguished Research Professor of physics at the State University of New York at Stony Brook. Peter Jenni was a senior physicist at CERN in Geneva. He is now a guest scientist at the University of Freiburg in Germany.

This Content Appeared In
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Volume 66, Number 6

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The Week in Physics" is likely a reference to the regular updates or summaries of new physics research, such as those found in publications like Physics Today from AIP Publishing or on news aggregators like Phys.org.

Physics Today - Table of Contents
Physics Today - Whitepapers & Webinars
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