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High Magnetic Fields: Science and Technology, Volumes 1 and 2

by Fritz Herlach and Noboru Miura (eds), World Scientific. Hardback ISBN 9810249640 (vol 1) and 9810249659 (vol 2), £41 ($55) each.

These are the first two volumes of a three-volume set intended to provide a comprehensive review of experiments in very strong magnetic fields, which can be generated only with special magnets. Volume 1 is devoted to magnet technology and experimental techniques, while volumes 2 and 3 contain reviews of the different areas of research where strong magnetic fields are an essential tool. Volume 3 is scheduled to appear in autumn 2004.

Renormalization Methods: A Guide For Beginners

by W D McComb, Oxford University Press. Hardback ISBN 0198506945, £39.95 ($74.50).

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Occupying a gap between standard undergraduate and more advanced texts on quantum field theory, this book covers a range of renormalization methods, including mean-field theories and high-temperature and low-density expansions. It proceeds by easy steps to the epsilon expansion, ending up with the first-order corrections to critical exponents beyond mean-field theory. Macroscopic systems are also included, with particular emphasis on fluid turbulence. Requiring only the basic physics and mathematics known to most scientists and engineers, the material should be accessible to readers other than theoretical physicists.

Gauge Theories in Particle Physics, Volume 2

by Ian Aitchison and Anthony Hey, Institute of Physics Publishing. Paperback ISBN 0750309504, £29.99 ($45).

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Subtitled “QCD and the Electroweak Theory”, this is the second volume of the third edition of a highly successful textbook, which has now been substantially enlarged and updated. It builds on the foundations laid in volume 1, which led up to quantum electrodynamics, and deals with the other two gauge theories of the Standard Model: quantum chromodynamics (QCD) and electroweak theory. It includes new chapters on QCD, as well as extensions to the discussion of weak interaction phenomenology.

The Cold Wars – A History of Superconductivity

by Jean Matricon and Georges Waysand, Rutgers University Press. Hardback ISBN 0813532949, $65; paperback ISBN 0813532957, $26.

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After carefully investigating the behaviour of matter under new conditions, physicists then try to explain what they find. So it happened with cryogenics. It is much easier to light fires than to invent refrigerators, so the physics of high temperatures was initially much more familiar. However, the laws governing the behaviour of hot gases when extrapolated backwards suggested that something strange should happen if matter could be cooled to -273 °C, “absolute zero” on the new Kelvin temperature scale. Fourteen billion years after the Big Bang, the natural universe is screened from absolute zero by the all-permeating cosmic background radiation at 2.7 K, the faint echo of the Big Bang, and only recently have laboratory experiments descended the last few rungs of the temperature ladder. But such a natural barrier was long unsuspected, and in the second half of the 19th century one gas after another was liquefied triumphantly in the quest to approach absolute zero. However, helium remained stubbornly gaseous until Kamerlingh Onnes established a purpose-built laboratory in Leiden.

After setting this scene, The Cold Wars (what “wars”?) charts the progress of cryogenic physics after the liquefaction of helium at 4.2 K in 1908 opened up a new frontier. Painstakingly probing the behaviour of materials at these temperatures, Onnes discovered the phenomenon of superconductivity – the virtual disappearance of electrical resistance. The origins of this phenomenon, and its interplay with magnetic fields, long remained a mystery. Meanwhile, physicists noticed that liquid helium itself behaved bizarrely below about 2.2 K – becoming a superfluid with almost no viscosity. With the emergence of quantum ideas in the 1920s, attention focused on the possible link between superfluidity and Bose-Einstein condensation – when particles sink into the lowest possible quantum energy state, creating new types of matter. Thirty years later, John Bardeen, Leon Cooper and Robert Schrieffer suggested that pairs of electrons could account for the mystery of superconductivity.

The Cold Wars enthusiastically traces the history of cryogenic physics and superconductivity, with its triumphs and disappointments, and is a good introduction to an intriguing subject. However, it does not venture into the elegant modern quantum theory of phase transitions, which satisfyingly relates to a wider range of phenomena. Superfluid helium is still some way from absolute zero, and only in the past decade have physicists been able to achieve total Bose-Einstein condensation and demonstrate what happens when all particles accumulate into a single energy state, but this too is beyond a strictly superconducting horizon.

A major area for applications of superconductivity is in the powerful magnets that guide charged-particle beams in modern accelerators, but the book only covers this in passing and does not mention the world’s largest superconducting project – the 27 km LHC ring using superfluid helium that is now being constructed at CERN. (The only reference to particle-physics developments is an achievement of high magnetic fields at Fermilab “in 1963” – which was before plans for that US laboratory had even been drawn up.)

The Cold Wars is the English translation, with French government support, of La guerre du froid (Editions Seuil). The book concludes with the emergence of the new cuprate “high-temperature” superconductors. The search for superconductivity at still higher temperatures and the explanation of how this happens remains a glamorous research focus, and a final chapter updates these developments beyond what could have been described in the original 1994 edition.

La physique du XXe siècle

By Michel Paty, EDP Sciences, Collection Sciences et histoires. Paperback ISBN 286883518X, €34.

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The title Michel Paty has chosen for his book, La physique du XXe siècle (Physics of the 20th century), is an ambitious one. Summarizing the main advances in physics over the past 100 years in 276 pages, as well as demonstrating their impact on other fields of science, seems like an impossible task. Indeed, the author himself, a physicist and science historian, questions whether it is possible to single out the 20th century’s most important and most characteristic developments in science in general and physics in particular. He takes up the challenge all the same, painting a general panorama of physics in the 20th century.

He begins by reviewing the main concepts of physics, describing the historical background to them, and the men and women associated with them. These include relativity, quantum physics, atoms and states of matter, the nucleus, elementary particles, fundamental fields, dynamic systems and phase transitions. He then turns to fields closely related to physics, namely geophysics, astrophysics, cosmology and, more generally, the search for the origins of the universe. At the end, he examines the subject of physics and the associated methods, and comes back to the emergence of Big Science in the 20th century. Finally, in his conclusion, he describes the lessons to be learnt from the past and looks to the future with confidence.

For the student or curious novice, Paty’s book can quickly become a reference manual, whose use will vary according to individual requirements. It provides the reader with a general introduction to the main fields of physics research and helps him or her along with historical references. The photographs (essentially portraits), boxes, diagrams and tables, which are simple and well chosen, offer an alternative means of getting to grips with the subject. Finally, a detailed bibliography invites the reader to further exploration. Paty has thus essentially met the challenge he set himself, as his book opens up the door to those who wish to enter the universe of physics.

Neutrino Physics

by Kai Zuber, Institute of Physics. Hardback ISBN 0750307501, £80.00 ($125.00).

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This excellent introduction to neutrino physics describes, in 14 chapters and more than 400 pages, the past, present and future experiments and essential developments in one of the most exciting fields of fundamental physics today. Ranging from “Important historical experiments” to “Neutrinos in cosmology”, it is perfect that this comprehensive overview on neutrino physics was published shortly after the Nobel Prize for Physics was awarded to two neutrino physicists, Raymond Davis and Masatoshi Koshiba, for their pioneering contributions to astrophysics, in particular for the detection of cosmic neutrinos.

Neutrinos – first postulated in the 1930s and detected in 1956 by Clyde Cowan and Fred Reines – are one of the most fundamental particles in the universe, but they are also one of the least understood. The author, Kai Zuber from Oxford University, begins with some personally selected historical milestones and theoretical background. He then proceeds to give the fundamental properties of the neutrino, address the questions of neutrino mass, and looks at the place of the neutrino within and beyond the Standard Model. Zuber continues with a discussion of the role of neutrinos in modern astroparticle physics and ends with neutrinos in cosmology and the problem of dark matter, thus covering the full range of neutrino physics. It is remarkable that Zuber describes, over many chapters, not only neutrino experiments, detectors and spectrometers in operation, but also those that are at present under construction or planned, such as the KATRIN experiment and the neutrino factory.

The book ends with a summary and personal outlook, a comprehensive list of references and a detailed index. All of this helps the reader to enjoy a fascinatingly written overview of this exciting field of physics, where “you always have to expect the unexpected”. The only weak point is that some of the figures are of poor quality, making it difficult to see what is shown.

Neutrino Physics is a textbook at a level that is suitable for graduate students in physics and astrophysics. It can be highly recommended to anyone interested in this field, and to any advanced student who wants to learn more about this research topic and who needs to understand neutrino physics.

New protocol accords CERN wider international status

CERN’s member states have adopted a new protocol on the privileges and immunities of the organization. This brings CERN into line with other European intergovernmental organizations, such as the European Space Agency and the European Southern Observatory, which already enjoy international status in all their member states.

The protocol, which is also open for signature to non-member states that have agreements with CERN, will simplify the movement of personnel and materials between countries involved in projects with CERN. The privileges and immunities granted to CERN are similar to those granted to other international organizations. The protocol will also facilitate any future enlargement of the organization.

CERN already benefits from international status in its two host states, France and Switzerland. Switzerland accorded this status in 1955, as did France after the CERN site was extended across the Franco-Swiss border in 1965. With the new protocol, all member states that sign will recognize CERN’s international status.

When it comes into force, the protocol will have important effects for the organization’s activities in other countries, particularly those involving contractors or collaborators in other research institutes. For example, by establishing specific privileges and immunities, it will make easier the movement of personnel between countries involved in projects in which CERN is a partner. It will also exempt CERN’s purchasing activities from tax (in particular VAT) and customs duties, and thus simplify the transfer of equipment and materials between the various countries that can be involved in a single contract – with the effect of reducing the costs often incurred through successive taxations as goods move between countries.

The protocol also has an important symbolic value for the future of CERN, as it is open for signature not only to CERN’s member states, but also to other states that collaborate with CERN, either as associate member states or through co-operation agreements. “Although this seems symbolic today,” explains CERN’s director-general Robert Aymar, “I believe that in the future, with the increasing globalization of particle physics, this will become a valuable tool in helping CERN to remain a powerful force in science.”

Nine member states signed the protocol in a ceremony at CERN on 18 March, bringing to 11 (with France and Switzerland) the number of member states that have now agreed to grant full international status to CERN. The other nine have set in motion procedures that will allow them to sign in the near future. It will come into force once it has been signed and ratified by 12 member states other than the host states.

Smaller institutes look to gain from scientific fallout

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Large laboratories obtain scientific data in vast quantities and usually use this material for rapid research being driven by competition. The majority of important results are collected in as short a time as possible. When new data appear older data lose their importance and are abandoned or placed at the disposal of smaller labs that could make use of them.

This has been the case in the past with data obtained at laboratories such as CERN, Fermilab and JINR, which came in such quantities that they could not be exhaustively analysed by the researchers there. The data were therefore given to various universities and other smaller laboratories, which over a long period of time have analysed the events in question and sometimes made valid discoveries.

More recently, data from the CDF and D0 experiments at Fermilab have become available via the web. A more leisurely analysis phase is also happening with data obtained from experiments at LEP, whose activity is slowing down. Thus it gives the possibility of allowing researchers at smaller scientific institutions to follow up the work and make new findings. For example, institutes in the “Post L3” collaboration are currently analysing some LEP data in their own time and have no obligation to provide results by a specific deadline.

The pictures made in the late 1960s with the CERN 2 m hydrogen bubble chamber show the possible importance of this approach. Its films ended up in various universities, either for further analysis or for didactic purposes, because bubble-chamber pictures are useful for students. Consequently, during the 1970s, the University of Bucharest and JINR in Dubna obtained 125,000 pictures courtesy of CERN. The pictures were found to contain a number of interesting items that had earlier been overlooked because in the principal analysis they had been viewed with different criteria in mind.

In one particular example, V M Karnauhov, V I Moroz, C Coca and A Mihul were able to report on finding a resonance in π–p interactions at 16 GeV, having a mass of 3520 ± 3 MeV/c2 and a width of 7 +20-07MeV with eight standard deviations (Karnauhov et al. 1992). At the time this seemed very strange, as most physicists were not particularly interested as the resonance corresponded to a five-quark particle (uud ccbar), which did not fit then into any theoretical framework.

During the past year, however, evidence for several exotic resonances has been reported. A real “gold rush” for similar phenomena – the “pentaquarks” – has begun, even though there are few, if any, irrefutable theoretical explanations. Their masses have not yet been calculated due to the lack of a theoretical basis. These include the Θ* (1540 MeV and a width of 17 MeV) and the Ξ (1862) baryon with S = -2, which have still to be established with high accuracy. They appear like states of five quarks (pentaquarks), i.e. four quarks and one antiquark, so yielding a system without colour, which is necessary to be observable.

The 2 m bubble-chamber data suggested long ago that at least one more baryonic exotic state was found with a mass of 3520 ± 3 MeV/c2, a width of 7 +20-07 MeV and S = 0. This was a pentaquark baryon with neutral strangeness. The essential difference between the Θ*and Ξ (1862) and what was found long ago is that the old resonance was formed by quarks including a ccbar pair, while the new ones contain s (sbar) quarks, giving a substantial difference in the final mass. Other teams have also reported possible sightings of pentaquarks in data from the 2 m chamber, and now the H1 experiment at DESY has evidence for a uuddcbar state with a mass of 3100 MeV/c2.

So what can we learn from this experience? The distribution of data to smaller institutions, which perhaps have more time to follow different or unfashionable lines of analysis, must continue. Besides the benefits that this activity can bring to the institutes themselves, the long-term process also has the benefit of bringing fresh minds to the analysis as younger physicists, who may bring new approaches, replacing older ones.

The Grid should also be able to overcome some of the difficulties of the past. It aims at providing a global computing facility, which will allow the smaller laboratories to participate in the primary research. However, the Grid is being developed to provide enormous computing power; it will not be able to provide the thinking time that is necessary for the best job to be done. This can only be provided by the researchers performing long-term analysis generally in the smaller laboratories.

OECD committee endorses future linear collider

Ministers meeting at the end of January for the Committee for Scientific and Technological Policy of the OECD (Organisation for Economic Cooperation and Development) have acknowledged the importance of ensuring access to large-scale research infrastructures in high-energy physics and of the long-term vitality of the field. The ministers also noted the worldwide consensus of the scientific community in choosing an electron-positron linear collider as the next accelerator-based facility to complement and expand on discoveries that are likely to emerge from the Large Hadron Collider (LHC) at CERN. They agreed that the planning and implementation of such a large, multi-year project should be carried out on a global basis, and should involve consultations among not only scientists but also representatives of science funding agencies from interested countries.

At their previous meeting in 1999, the ministers had endorsed the creation of the OECD Global Science Forum, which provided a useful venue for consultations among senior science policy officials and programme managers, and was a valuable mechanism for bringing together government officials with representatives of scientific communities. Now, at the January 2004 meeting, the ministers were in a position to devote their attention to the forum’s work concerning high-energy physics. In particular the ministers endorsed the statement prepared by the forum’s Consultative Group on High-Energy Physics and noted several important points that were articulated in the group’s report. These included the need to have large, next-generation facilities funded, designed, built and operated as global-scale collaborations; the need to educate, attract and train young people in the fields of high-energy physics, astrophysics and cosmology; and the need for a strong international R&D collaboration and studies of the various issues required to realize the next major accelerator facility on the consultative group’s roadmap – a next-generation electron-positron collider with a significant period of concurrent running with the LHC.

CERN strengthens links with AMS experiment

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CERN and the collaboration behind the Alpha Magnetic Spectrometer (AMS) experiment have signed a new memorandum of understanding (MOU) for the execution of the experiment, which will take place not at CERN, or elsewhere on Earth, but in space. The new MOU foresees the establishment at CERN of the experiment’s Payload Operations and Control Centre, and the Science Operations Centre. CERN will also provide areas for the assembly and testing of the AMS detector, as well as offices for users and secretarial support.

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AMS is a major international collaboration that is led by Sam Ting of MIT. The principal goal of the AMS experiment, which will be located on board the International Space Station, is to look for antiparticles in the primary cosmic radiation of outer space. Other objectives of the experiment include searching for dark matter and carefully analysing details of the cosmic-ray spectrum. The detector will be equipped with a powerful superconducting magnet and sophisticated detectors for precision tracking, particle identification and photon detection.

AMS has been a “recognized experiment” at CERN since 1997. The new MOU, which is a significant upgrade of the previous agreement, has a duration of five years and can be renewed.

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