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Steve Myers and the LHC: an unexpected journey

Happiness as the LHC

The origins of the LHC trace from the early 1980s, in the days when construction of the tunnel for the Large Electron–Positron (LEP) collider was just getting under way. In 1983, Steve Myers was given an unexpected opportunity to travel to the US and participate in discussions on future proton colliders. He recalls: “None of the more senior accelerator physicists was available, so I got the job.” This journey, it turned out, was to be the start of his long relationship with the LHC.

Myers appreciated the significance for CERN of the discussions in the US: “We knew this was going to be the future competition and I wanted to understand it extremely well.” So he readied himself thoroughly by studying everything on the subject that he could. “With the catalyst that I had to prepare myself for the meeting, I looked at all aspects of it,” he adds. After returning to CERN, he thought about the concept of a proton collider in the LEP tunnel and wrote up his calculations, together with Wolfgang Schnell. “Wolfgang and I had many discussions and then we had a very good paper,” he says.

The paper (LEP Note 440) provided estimates for the design of a proton collider in the LEP tunnel and was the first document to bring all of the ideas together. It raised many of the points that were subsequently part of the LHC design: 8 TeV beam energy, beam–beam limitation (arguing the case for a twin-ring accelerator), twin-bore magnets and the need for magnet development, problems with pile-up (multiple collisions per bunch-crossing) and impedance limitations.

After Myers’ initial investigations, the time was ripe to develop active interest in a future hadron collider at CERN

After Myers’ initial investigations, the time was ripe to develop active interest in a future hadron collider at CERN. A dedicated study group was established in late 1983 and the significant Lausanne workshop took place the following year, bringing experimental physicists together with accelerator experts to discuss the feasibility of the potential LHC. Then began the detailed preparation of the project design.

In the meantime in the US, the Superconducting Super Collider (SSC) project had been approved. Myers was on the accelerator physics subcommittee for both of the major US Department of Energy reviews of the SSC, in 1986 and 1990. He recalls that the committee recommended a number of essential improvements to the proposed design specification, which ultimately resulted in spiralling costs, contributing to the eventual cancellation of the project. “The project parameters got changed, the budget went up and they got scrapped in the end.”

The LHC design, being constrained by the size of the LEP tunnel, could not compete with the SSC in terms of energy. Strategically, however, the LHC proposal compensated for the energy difference between the machines by claiming a factor-10 higher luminosity – an argument that was pushed hard by Carlo Rubbia. “We went for 1034 and nobody thought we could do it, including ourselves! But we had to say it, otherwise we weren’t competitive,” Myers says, looking back. It now gives Myers enormous satisfaction to see that the LHC performance in the first run achieved a peak stable luminosity of 7.73 × 1033 cm–2 s–1, while running at low energy. He adds confidently: “We will do 1034 and much more.”

The decision to use a twin-ring construction for the LHC was of central importance because separate rings allow the number of bunches in the beam to be increased dramatically. To date, the LHC has been running with 1380 bunches and is designed to use twice that number. For comparison, Myers adds: “The best we ever did with LEP was 16 bunches. The ratio of the number of bunches is effectively the ratio of the luminosities.”

Design details

LEP Note

At CERN, it was difficult to make significant progress with the LHC design while manpower and resources were focused on running LEP. Things took off after the closure of LEP in 2000, when there was a major redeployment of staff onto the LHC project and detailed operational design of the machine got under way. The LHC team, led by Lyn Evans, had three departments headed by Philippe Lebrun (magnets, cryogenics and vacuum), Paulo Ciriani (infrastructure and technical services) and Myers (accelerator physics, beam diagnostics, controls, injection, extraction and beam dump, machine protection, radio frequency and power supplies).

Myers makes a typical understatement when asked about the challenges of managing a project of this size: “You do your planning on a regular basis.” This attitude provides the flexibility to exploit delays in the project in a positive way. “Every cloud has a silver lining,” he comments, illustrating his point with the stark image of thousands of magnets sitting in car parks around CERN. A delay that was caused by bad welds in the cryogenic system gave the magnet evaluation group the benefit of extra time to analyse individual magnet characteristics in detail. The magnets were then situated around the ring so that any higher-order field component in one is compensated by its neighbour, therefore minimizing nonlinear dynamic effects. Myers believes that is one of the reasons the machine has been so forgiving with the beam optics: “You spend millions getting the higher-order fields down, so you don’t have nonlinear motion and what was done by the magnet sorting gained us a significant factor on top of that.”

When asked about the key moments in his journey with the LHC, he is clear: “The big highlight for us is when the beam goes all of the way round both rings. Then you know you’re in business; you know you can do things.” To that end, he paid close attention to the potential showstoppers: “The polarities of thousands of magnets and power supplies had to be checked and we had to make sure there were no obstacles in the path of the beam.” During the phase of systematically evaluating the polarities, it turned out that only about half were right first time. There were systematic problems to correct and even differing wiring conventions to address. In addition, a design fault in more than 3000 plug-in modules meant that they did not expand correctly when the LHC was warmed up. This was a potential source of beam-path obstacles and was methodically fixed. These stories illustrate the high level of attention to detail that was necessary for the successful switch-on of the LHC on 10 September 2008.

The low point of Myers’ experience was, of course, the LHC accident on 19 September 2008, which occurred only a matter of hours after he was nominated director of accelerators and technology. The incident triggered a shutdown of more than a year for repairs and an exhaustive analysis of what had gone wrong. During this time, an unprecedented amount of effort was invested in improvements to quality assurance and machine protection. One of the most important consequences was the development of the state-of-the-art magnet protection system, which is more technically advanced than was possible at the time of the LHC design. The outcome is a machine that is extremely robust and whose behaviour is understood by the operations team.

Steve Myers

In November 2009 the LHC was ready for testing once again. The first task was to ramp up the beam energy from the injection energy from the Super Proton Synchrotron of 0.45 TeV per beam. The process is complicated in the early stages by the behaviour of the superconducting magnets but the operations team succeeded in achieving 1.18 TeV per beam and established the LHC as the highest-energy collider ever built. By the end of March 2010, the first collisions at 7 TeV were made and from that point on the aim was to increase the collision rate by introducing more bunches with more protons per bunch and by squeezing the beam tighter at the interaction points. Every stage of this process was meticulously planned and carefully introduced, only going ahead when the machine protection team were completely satisfied.

In November 2009, when the LHC was ready to start up, both the machine and its experiments were thoroughly prepared for the physics programme ahead. The result was a spectacular level of productivity, leading to the series of announcements that culminated in the discovery of a Higgs boson. By the end of 2011 the LHC had surpassed its design luminosity for running with 3.5 TeV beams and the ATLAS and CMS experiments had seen the first hints of a new particle. The excitement was mounting and so was the pressure to generate as much data as possible. At the start of 2012, given that no magnet quenches had occurred while running with 3.5 TeV beams, it was considered safe to increase the beam energy to 4 TeV. With a collision rate of 20 MHz and levels of pile-up reaching 45, the experiments were successfully handling an almost overwhelming amount of data. Myers finds this an amazing achievement, as he says, “nobody thought we could handle the pile-up,” when the LHC was first proposed. He views the subsequent discovery announcement at CERN on 4 July 2012 as one of the most exciting moments of his career and, indeed, in the history of particle physics.

Reflecting on his journey with the LHC, Myers is keen to emphasize the importance of the people involved in its development, as well as the historical context in which it happened. In his early days at CERN in the 1970s, he was working with the Intersecting Storage Rings (ISR), which he calls “one of the best machines of its time”. As a result, “I knew protons extremely well,”he says. The experience he gained in those years has, in turn, contributed to his work on the LHC.

In the following years of building and operating LEP – as the world’s largest accelerator – many young engineers developed their expertise, just as Myers had on the ISR. “I think that’s why it worked so well,” he says, “because these guys came in as young graduates, not knowing anything about accelerators and we trained them all and they became the real experts, in the same way as I did on the ISR.” He sums up the value of this continuum of young people coming into CERN and becoming the next generation of experts: “That for me is what CERN is all about.”

The LHC’s first long run

From the first 3.5 TeV collisions in March 2010 to the start of the first long shutdown in March 2013, the LHC went through three years of improving performance. This led in 2012 to the discovery of a Higgs boson, which made headlines around the world and brought many accolades to CERN, including the 2013 EPS-HEPP prize (EPS-HEP2013: these are good times for physics). This issue takes a look behind the scenes at what underpinned the successful operation of the LHC during this first long run. With thanks to Theresa Harrison, Warwick University, for her editorial work with the authors of these articles. Thanks also to Jesse Karjalainen, IOP Publishing, for his work on the design of what will be his last issue of CERN Courier as he heads for pastures new after six years.

Networks Geeks: How They Built the Internet

By Brian E Carpenter
Springer
Paperback: £15 €21.09 $19.99
E-book: £11.99 €15.46 $9.99

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In Network Geeks, Brian Carpenter weaves the history of the early internet into an entertaining personal narrative. As head of CERN’s computer-networking group throughout the 1980s, he is well placed to describe the discussions, the splits, the technical specifications and countless acronyms that made up the esoteric world of networking in the early days of the internet in Europe. Just don’t expect to be spared the technical details.

Carpenter joined CERN in 1971, at a time when computers filled entire rooms, messages were relayed by paper tape or punched card and numerous local networks ran bespoke software packages around the laboratory. Simplifying the system brought Carpenter into the world of the internet Engineering Task Force – the committee charged with overseeing the development of standards for internet technology.

I enjoyed the fictional account of a meeting of the Task Force in 1996, which gives a vivid idea of the sheer number of technical issues, documents and acronyms that the group tackled. That year, traffic was doubling every 100 days. Keeping up with the pace of change and deciding which standards and protocols to use – TCP/IP or OSI? – were emotive issues. As with any new technology, there was lobbying, competition and elements of luck. Nobody knew where the internet would lead.

Carpenter’s enthusiasm is the strength of Network Geeks. He recounts his early interest in science – a childhood of Meccano and Sputnik – with an easy nostalgia and his memories of informal meetings with often-bearded computer scientists show genuine warmth. But it is no easy read. The autobiographical narrative jumps jarringly between lyrical descriptions of the author’s youth and the rather mundane details of computer networking. At times I felt I was drowning in specifics when I was really hoping for a wider view, for implications rather than specifications.

Networks Geeks reminded me that the evolution of technology can be as much down to politics and luck as to scientific advances. It gave me a great overview of the climate in the early days on the internet. At the same, the heavy layers of jargon also reminded me why I’m no computer scientist.

A Journey with Fred Hoyle (2nd Edition)

By Chandra Wickramasinghe and Kamala Wickramasinghe (ed.)
World Scientific
Paperback: £28
E-book: £21

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Fred Hoyle was undoubtedly among the most original thinkers of his time and one of the leading figures of 20th-century physics. From the purely scientific viewpoint, his name is associated with at least three ideas: the synthesis of heavy nuclear elements in the cores of supernovae (developed in collaboration with William Fowler, Margaret and Geoffrey Burbidge); the steady-state model of the universe (formulated together with Hermann Bondi and Thomas Gold); and some of the early applications of anthropic arguments to astrophysics and cosmology. Hoyle also contributed to many other fields – such as stellar structure, planetary formation, galactic dynamics and the origin of large-scale magnetism – where his creative imagination often made the difference.

A Journey with Fred Hoyle – now in a second edition that incorporates relevant developments that have occurred since the original was published in 2005 – is a respectful, lively and at times exciting tribute to an independent thinker, a capable teacher and an inventive scientist. It is an extremely well written collection of scientific memoirs and an intriguing journey in the realm of scientific controversies, which often accompany the achievements of those who like to think a little differently. The author started his PhD under the guidance of Hoyle in the early 1960s and was still collaborating with him in 2001 when Hoyle passed away. His narration begins in Cambridge where, from the mid-1950s to the mid-1960s, three disciplines thrived serendipitously: biology (with the monumental discovery of James Watson and Francis Crick of the famous double helix structure of genetic material); cosmology and astrophysics (with the work of Hoyle at the institute of astronomy and of Martin Ryle with the radio-astronomy group) and particle physics (with the Lucasian professorship of Paul Dirac).

The Cambridge atmosphere probably inspired a quest for the unification between astrophysics and biology – a field that later became known as astrobiology and gained funding and respect from the whole scientific community. The starting observation made by Hoyle and Wickramasinghe was that interstellar clouds are not made of ice, as originally thought in the 1950s and early 1960s, but rather of carbon. By analysing the way that interstellar dust dims starlight the authors proposed, in a crescendo, that the carbon was part of complex organic molecules and, eventually, bacteria or even viruses. This combination of science and inventiveness led to the theory of panspermia, i.e. the hypothesis that life exists throughout the universe distributed in meteorites and asteroids.

Is it really true that life on the Earth came from the cosmos? This is probably not the most relevant question. What matters here is to appreciate that the current success of astrobiology started – amid inevitable controversies – from the analysis of organic compounds in interstellar space. This is an interesting book and worth reading for those who like to follow the complicated fate of successful ideas. Recalling the title of Hoyle’s autobiography, we could say that “home” for scientists is, sometimes, “where the wind blows”.

Feynman’s Tips on Physics: Problem-Solving Supplement to the Feynman Lectures on Physics

By Richard P Feynman, Michael A Gottlieb and Ralph Leighton
Basic Books
Paperback: £11.99 $16.99

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Originally published in hardback not long ago (Addison Wesley 2006), Feynman’s Tips on Physics is now available as a slim paperback, complete with some additional material. It is essentially a collection of four “lost” lectures and could be thought of as four chapters that somehow didn’t make it into The Feynman Lectures on Physics – the well known three-volume set by Feynman and colleagues Robert Leighton and Matthew Sands. To complement these, Michael A Gottlieb and Ralph Leighton (Robert’s son) have added a fifth chapter with selected problems from Exercises in Introductory Physics by Leighton Sr and Rochus Vogt. To set the scene, they also include a “memoir” by Sands on the origins of the famous three books in their distinctive red covers and – new for this edition – three interviews, with Leighton Sr, Vogt and Feynman himself.

The first thing to say is that the scientific level of the four lectures is far below that of the other published lectures. The first lecture, “Prerequisites”, is an elementary reminder about the importance of learning basic calculus and vector algebra and it is unlikely that anyone reading this review will find anything new. Perhaps the main point of interest is Feynman’s discussion on how to deal with not being the top member of a group comprised of many talented people. This might provide some inspiration to bright high-school students who go from being top of their class to no longer being at the top at a good university.

The second lecture, “Laws and Intuition” attempts to explain to students the importance of having a feel for the material and using physical intuition to back up mathematical calculations. This could help students, who far too often, in my experience, just want to know “what formula to use”.

“Problems and Solutions”, the third lecture, is pitched at a slightly more advanced level. It would be suitable for a good high school student or first-year university student and covers a range of interesting topics from satellite motion to rockets (including ion and photon propulsion) as well as a couple of simple particle-physics examples: electrostatic deflection of a proton beam and the determination of the charged-pion mass.

Last, “Dynamical Effects and Their Applications”, is essentially about gyroscopes. It contains little mathematics and the technology is quite dated but it is fun to read. In fact, even the datedness of some of the material has its charm. Feynman says: “Computing is mostly analogue at the moment, but it is likely that it’ll turn into digital – in a year or two, probably – because that has no errors in it.” How things have changed since 1962!

While there is not much here for the practising physicist, it is a quick and easy read and contains many interesting things about the history of The Feynman Lectures in Physics in the introduction (and the surprising statement that there are more than 170 errors in the 3 volume set). As such, it is worth the hour or two that it will take to read – and, after all, it is Feynman. While it is unlikely to find much use as a reference work, it would make a nice gift for someone about to start studying physics – but together with the full 3-volume set.

Handbook of Radioactivity Analysis (3rd edition)

By M L’Annunziata (ed.)
Academic Press
Hardback: €120
E-book: €129

9780123848734

Updated and much expanded, the new edition of this authoritative text provides the principles, practical techniques and procedures for accurately measuring radioactivity, from the low levels encountered in the environment to higher levels measured, for example, in radioisotope research, nuclear medicine and nuclear power. The book describes the basic principles of radiation detection and measurement and the preparation of samples; assists in the selection and use of appropriate radiation detectors; and presents state-of-the-art methods of analysis. Fundamentals of radiation properties, radionuclide decay and methods of detection provide the foundation of the analytical procedures. It is also suitable as a teaching text for university and training courses.

Strong in the rain

Strong in the Rain
By Lucy Birmingham and David McNeil
Palgrave Macmillan
Hardback: £17.99 $27.00
E-book: $12.99

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Some dates will remain in the public consciousness forever, given their cultural impact. Personally, these would include 11 September 2001 (the attacks on the twin towers in New York), 7 July 2005 (the London Underground bombings) and 11 November (Armistice Day, commemorating the end of the First World War).

On 11 March 2011 the Tohoku earthquake occurred approximately 70 km off the coast of Japan. It was the most powerful earthquake ever to hit Japan and the fifth most powerful to be recorded since records began in 1900. The earthquake triggered powerful tsunami waves that reached heights of up to 40 m. The Japanese National Police Agency subsequently confirmed 15,883 deaths, ensuring that this date will live long in the Japanese cultural memory.

Strong in the Rain brings together six stories from people affected by the tragic events associated with the earthquake/tsunami on 11 March. The book is described as “part history, part science” and the authors use the experiences of the six people in the book, in addition to their own, to paint a tale of heroes and villains.

The book gets off to a slow start but the reading becomes gripping once the stories move on to the tales of the six central protagonists. It delves into the Japanese cultural strengths and weaknesses in equal measure, from the lack of information provided regarding the nuclear meltdown at the Fukushima Daiichi to the best qualities of the Japanese spirit and character, which are embodied in the town mayor who changes press coverage of the nuclear meltdown with a heartfelt plea uploaded to YouTube.

Living somewhere like the UK it is hard to picture the epic scale of this disaster but the authors weave between the stories of the protagonists to make you feel like you were there. The book manages to be both heart-breaking and uplifting in equal measure and the title Strong in the Rain – taken from a famous Japanese poem – becomes an apt description of the events that unfold.

Some books portraying historical events have the potential to become dated but I believe that Strong in the Rain will stand up well to the test of time. This is mainly because of the human stories within the book that leave you questioning how you might have behaved under similar stress. What would you leave and who would you save? What does it take to be a hero? It also leaves you thinking how important learning from the past is to save us all in the future. I would heartily recommend this book and will be lending it to all of my friends.

Materia Strana (Strange Matter)

Materia Strana (Strange Matter)
By J J Gómez Cadenas, translated from the original Materia Extraña, published by Espasa Calpe
Edizioni Dedalo
Paperback: €16

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CERN has attracted the attention of a number of writers as a stage for their thrillers and in most cases they have been assisted on the scientific background by friends or by interviews with key CERN scientists. In Dan Brown’s Angels & Demons, CERN’s science portfolio was an excuse for writing a science-fiction novel in which special effects overshadow reality to create shocking situations. Bruno Arpaia’s L’Energia del Vuoto (Vacuum’s Energy) was more respectful of CERN’s science, providing detailed scientific descriptions but with the risk of breaking the rhythm of the novel. By contrast, J J Gómez Cadenas has been gifted with a rare combination of talents: he is a good writer and a professional particle physicist. As a result, Materia Strana is a powerful thriller based on an almost realistic scientific case that fits well with an engaging narration.

The possible existence of stable strange matter in the universe was put forward by Edward Witten and independently by Álvaro De Rújula and Sheldon Glashow in 1984. Some neutron stars could, indeed, be strange stars. The possibility that high-energy ion–ion collisions could create chunks of strange matter that would have a tendency to grow exponentially in size was debated when the Relativistic Heavy-Ion Collider started operating in the US. The probability of this happening has been calculated to be negligibly low but in Materia Strana it is assumed to be much higher – dangerously high for a high-luminosity, ion–ion LHC at CERN.

This is the main theme around which a truly international thriller develops involving Irene, the gifted young theoretician with Iranian roots and Héctor, an amazing experimental physicist from the US with multiple backgrounds as a boxer, soldier and scientist, who becomes involved in a highly dangerous mission in Iran – as well as with Irene. There is also Friedrich, the powerful but unscrupulous head of the large experiment that is likely to bring him the Nobel prize; Helena, the hyper-efficient, fighting and bright director-general of CERN; and Boiko, a natural-born killer, who escaped to Geneva from the horrors of Chernobyl and Grozny. The deadly fight between Hector and Boiko has the intensity of the pages of Khaled Hosseini’s The Kite Runner. Intermixed with dreams and ghosts crossing the border between life and death, these stories provide the texture for a decent thriller where good wins eventually over evil, although with a heavy toll.

The particle at the End of the Universe

The Particle at the End of the Universe
By Sean Carroll
Oneworld
Hardback: £16.99
Paperback: £9.99

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In his latest book, Sean Carroll, author of the brilliant From Eternity to Here, has produced an accessible read aimed at the layperson interested in an up-to-date account of the state of particle physics and, in particular, the discovery of the Higgs boson. Carroll is well placed to offer the reader an in-depth view of the world of particle physics, being close enough to give a personal account yet maintaining the perspective of an onlooker. As a result he is a superb advocate of the case for “Big Science”, which he demonstrates to full effect in both the opening and closing chapters of the book, beginning with several snapshots of physicists celebrating the milestones that led up to the announcement of the major discovery at CERN on 4 July 2012.

By interweaving the scientific concepts with chapters on historical, social and political aspects of particle physics, Carroll dilutes the hard bits with human interest, appealing to the widest possible audience. He conveys the central importance of the Higgs discovery before going into the theory in any detail, so that we get an idea of what the fuss is about. He explains that the particle at the end of the universe is not a reference to the Higgs boson’s location in space or time but rather its location in our understanding, as the final piece of the Standard Model. This marks the end of the journey to describe our everyday surroundings and the beginning of a new era of full discovery. The theme is developed further when Carroll gets into his stride with dark matter, supersymmetry and string theory, demonstrating how the Higgs particle can act as a portal for exploring as yet unreachable phenomena.

True to the headline-grabbing comments of intrigue and drama in high-energy physics on the cover, the book recounts the chequered history of accelerators: the engineering challenges and the agonies of having your machine switched off when a major discovery could be just around the corner; or the frustrations of not getting the machine built at all, as with the Superconducting Super Collider. In this way, the account does justice to the magnitude and achievements of the LHC and its experiments.

What is meant by the “discovery” of a particle is also explained clearly, together with the issues concerning the timing and control of such announcements, especially given the high level of public interest. Concerning the difficulties of apportioning credit, Carroll proposes that scientific collaborations should be allowed to win the Nobel prize and that “Whoever gets that rule change implemented might deserve the Nobel Peace Prize”.

A couple of errors should be mentioned: the Higgs boson is repeatedly credited with distinguishing the electron from the neutrino and the up quark from the down, etc. The important qualification that this statement holds true only for the left-handed components of these particles is mentioned only latterly. Also, there is an unfortunate sign error in the diagram of Fleming’s left-hand rule – not a big deal in itself but enough to undermine confidence in the book for some readers, perhaps giving the impression that it has been rushed into print.

With this book Carroll consolidates his position as an exceptionally talented writer of difficult physics concepts for the layperson. He weaves together fascinating facts, amusing anecdotes and insightful analogies. In storyteller style, with colourful characters and thrilling plots, he propels the reader along the journey that particle physics has made in our lifetime. The layperson can empathize with the emotional highs and lows of research, the patience and tenacity required to bring a project like the LHC to completion and the laudable level of co-operation that the particle-physics community demonstrates to other large and complex organizations – to quote: “If only the United Nations could work like CERN, the world would be a better place.”

Council updates European Strategy for Particle Physics

On 30 May, at a special meeting hosted by the European Commission in Brussels, the CERN Council formally adopted an update to the European Strategy for Particle Physics. Since the original European strategy was put into place seven years ago, the LHC has begun routine operation, producing its first major results at centre of mass energies of 7 TeV and 8 TeV, and the global particle-physics landscape has evolved with new neutrino and precision measurements. The updated strategy takes these changes into account and charts a leading role for Europe in a field that is increasingly globalized.

An important issue for the strategy is to ensure that Europe stays at the forefront of particle physics research, which pays dividends in terms of knowledge, innovation, education and training. CERN, in close collaboration with research institutions in its member states and under the guidance of the CERN Council, will co-ordinate future European engagement with global particle-physics projects in other regions.

The strategy emphasizes that Europe and the European particle-physics community should exploit the LHC to its full potential over many years via a series of planned upgrades. Alongside the LHC, the community should also be open to engaging in large particle-physics projects outside Europe and continuing to develop novel techniques for global future accelerator projects. European particle physics should maintain a healthy base in fundamental physics research, with universities and national laboratories contributing to a strong European focus through CERN. Last but not least, the community should continue to invest substantial effort in communication, education and outreach activities to engage global publics with science.

• The updated strategy is reproduced in full in a new brochure Accelerating science and innovation: societal benefits of European research in Particle Physics: http://cds.cern.ch/record/1551933. For the original statement, see http://council.web.cern.ch/council/en/EuropeanStrategy/ESParticlePhysics.html.

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