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Soft Multihadron Dynamics

by W Kittel and E A De Wolf, World Scientific. Hardback ISBN 9812562958 £60 ($98).

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This book comprehensively covers the development and status of soft (i.e. non-perturbative) phenomena encountered in the production of (multi-) hadronic final states by high-energy collisions of various particles. Phenomenological models used to describe the data are in general inspired by quantum chromodynamics (QCD) and the book often crosses between soft and hard (perturbative) QCD. Postgraduate students, researchers and academics interested in multihadron production will find this useful reading.

The QCD Vacuum Hadrons and Superdense Matter, 2nd edition

by Edward V Shuryak, World Scientific. Hardback ISBN 9812385738 £75 ($101). Paperback ISBN 9812385746 £43 ($58).

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This book is invaluable for particle and nuclear physicists and comprises extensive lecture notes on non-perturbative quantum chromodynamics. The original edition from 1988 had a review style. In this edition the outline remains, but the text has been rewritten and extended. As well as incorporating new developments, this edition has benefited from several graduate courses taught by the author at Stony Brook during the past decade. The text now includes exercises and about 1000 references to major works, arranged by subject.

Modeling Black Hole Evaporation

by Alessandro Fabbri and José Navarro-Salas, Imperial College Press. Hardback ISBN 1860945279 £34 ($55).

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This book gives a detailed and pedagogical presentation of the Hawking effect and its physical implications, and then discusses the backreaction problem, especially in relation to exactly solvable semiclassical models that analytically describe black-hole evaporation. The book aims to link the general relativistic viewpoint on black-hole evaporation and the new CFT-type approaches. The discussion on backreaction effects is valuable for graduate students and researchers in gravitation, high-energy physics and astrophysics.

A cosmic vision for world science

Many developed countries face the challenge of encouraging more young people to take up science to ensure future innovation to benefit society. However, there is a related and equally important challenge – to promote a scientific infrastructure to aid the academic and career ambitions of members of under-represented and economically disadvantaged groups, as well as scientists from developing countries, to increase their participation in scientific and technical fields worldwide.

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Severe constraints on resources, which are a common feature in developing countries, mean that research there does not usually consist of designing and making equipment for a new experiment at the forefront of the field. In many schools, colleges and universities laboratories either do not exist or are poorly equipped. Consequently, the brain drain of bright young scientists from developing to developed countries seems to be the norm, and further intellectually impoverishes the developing world. Collaborative programmes between scientists from developed and developing countries are urgently needed.

The Abdus Salam International Centre for Theoretical Physics (ICTP) in Trieste has set an international example by providing both a forum and practical support for collaboration in theoretical physics between developing and developed countries. It has also supported indigenous physics programmes in developing countries. Importantly, the director of ICTP, Katepalli Sreenivasan, plans to include experimental physics in the programme. CERN has also taken a significant step to foster a relationship with physicists from developing countries that does not require large cash contributions to CERN, but instead encourages the production of detector components at the home laboratories. This lets physicists from developing countries participate in frontier research.

The Pierre Auger Collaboration is involved in Vietnam in developing experimental work to understand the universe at the highest energies. The Vietnam Auger Training Laboratory (VATLY) at the Institute for Nuclear Science and Techniques in Hanoi was inaugurated as a training ground for future experimentalists in astroparticle physics and related areas, and an exact replica of the water Cherenkov detector used in the Pierre Auger Observatory has been installed at VATLY. More recently, the atmospheric muon spectrum was measured in Vietnam for the first time. The phenomenology of neutrino oscillation is also being studied at this laboratory. Indeed, a Vietnamese community for experimental particle physics is developing well – in 2001 a group from the Institute of Physics in Ho Chi Minh City joined the D0 collaboration at Fermilab.

In many areas of research, leading-edge science is expensive and there are few support networks for disadvantaged groups. However, cost-effective projects to investigate the nature of ultra-high-energy cosmic rays (UHECR) are already being developed for high schools and could provide an ideal vehicle for such an effort. These projects demonstrate the basic elements of research and technology, with modern detectors, fast electronics, GPS timing, computerized data acquisition and data analysis. Perhaps just as importantly, they also teach social skills such as collaborative effort, organization, long-term planning and teamwork.

Efforts to bring the developing world into such projects have already begun. For example, the collaboration behind the Mixed Apparatus for Radar Investigation of Cosmic-rays of High Ionization project has established contact with the Maseno University in Kisumu, Kenya, the University of Zambia in Lusaka and the University of Rio de Janeiro in Brazil, to investigate the hypothesis that some forms of lightning are induced by cosmic rays. The collaboration is also working with Rio de Janeiro to deploy detectors that register UHECR showers and meteors in high-school-based receivers.

These are just two examples of the diverse topics related to the “cosmic connection” between research and education in both the developed and developing world. These include not only the astrophysics and particle physics of cosmic rays, but also topics in biology (e.g. the effects of natural radiation), mathematics, computer science and programming, chemistry, and environmental and Earth sciences (e.g studying the chemistry of ozone and how that could affect the transmission of cosmic rays).

The educational paradigm created by the networks of cosmic-ray arrays in high schools is one that can be employed in many areas. In geophysics, for example, one could use distributed arrays of seismometers to study geological activity over a large area. A specific example is the project BAMBI, which promotes the construction of an amateur array of radio telescopes distributed over a large area to study the radio sky at 4 GHz and search for signs of extraterrestrial intelligence. Such large-area, national and international school-based detector networks could aid and encompass other efforts throughout the world including developing countries, where it could provide entry to the global scientific community.

Theoretical Nuclear and Subnuclear Physics, 2nd edition

by John Dirk Walecka, World Scientific. Hardback ISBN 9812387951 £60 ($98). Paperback ISBN 9812388982 £29 ($48).

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This second edition is a revised and updated version of the original comprehensive text on nuclear and subnuclear physics, first published in 1995. It maintains the original goal of providing for graduate students a clear, logical, in-depth and unifying treatment of modern nuclear theory, ranging from the non-relativistic many-body problem to the Standard Model of the strong, electromagnetic and weak interactions. Researchers will also benefit from the updates on developments and the bibliography. This edition incorporates new chapters on the theoretical and experimental advances made in nuclear and subnuclear physics in the past decade.

Lattice Gauge Theories: An Introduction, 3rd edition

by Heinz J Rothe, World Scientific. Hardback ISBN 9812560629 £51 ($84). Paperback ISBN 9812561684 £29 ($48).

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This broad introduction to lattice gauge field theories, in particular quantum chromodynamics, serves as a textbook for advanced graduate students, and also provides the reader with the necessary analytical and numerical techniques to carry out research. Although the analytic calculations can be demanding, they are discussed in sufficient detail that the reader can fill in the missing steps. The book also introduces problems currently under investigation and emphasizes numerical results from pioneering work.

Field Theory, the Renormalization Group and Critical Phenomena: Graphs to Computers, 3rd edition

by Daniel J Amit and Victor Martín-Mayor, World Scientific. Hardback ISBN 9812561099 £52 ($86). Paperback ISBN 9812561196 £27 ($44).

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Linking field-theory methods and concepts from particle physics with those in critical phenomena and statistical mechanics, this book starts from the latter point of view. In this way, it introduces quantum field theory to those already grounded in the concepts of statistical mechanics and advanced quantum theory. Non-perturbative methods and numerical simulations are introduced in this third edition, with new chapters on real-space methods, finite size scaling, Monte Carlo methods and numerical field theory. There are sufficient exercises in each chapter for use as a textbook in a one-semester graduate course.

300 questions à un astronome

de Anton Vos, Presses Polytechniques et Universitaires Romandes. Broché ISBN 2880746566, €26.

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Comment l’eau est-elle apparue sur Terre? Peut-on voyager dans le temps? Est-il possible de créer un trou noir en laboratoire? Voici quelques-unes des 300 questions qui apparaissent dans ce livre.

Comme on peur le lire dans l’avant-propos, le livre est né sur l’Internet, sur le site de l’Observatoire astronomique de l’Université de Genève. Un espace y avait été ouvert pour que les internautes posent directement leurs questions aux astronomes. A partir de ces questions/réponses, Anton Vos, journaliste scientifique a réalisé cet ouvrage. Ces deux aspects apparaissent très clairement dans le livre. Les questions sont très directes et pratiques, une caractéristique typique des sites où le public est invité à intervenir. D’autre part, un énorme travail de journaliste a été réalisé pour simplifier le contenu, ce qui rend la lecture très agréable.

Avant de lire le livre, j’ai formulé une question dans ma tête pour vérifier que l’ouvrage contenait vraiment “tout ce que vous avez toujours voulu savoir sur l’astronomie”, comme la quatrième de couverture l’annonçait. J’ai trouvé ma question ainsi qu’une réponse pertinente.

Pour conclure, la structure du livre se prête à des approches de lecture différentes: on peut le picorer ou le lire de bout en bout, sans que la compréhension s’en ressente. De quelque manière que vous le lisiez, vous aurez appris beaucoup de choses sur l’astronomie et sans trop de difficultés.

Chern-Simons Theory, Matrix Models, and Topological Strings

by Marcos Mariño, Oxford University Press. Hardback ISBN 0198568495 £49.50.

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One of the most important examples of string theory/gauge theory correspondence relates Chern-Simons theory – a topological gauge theory in three dimensions that describes knot and three-manifold invariants – to topological string theory. This book gives the first coherent presentation of this and other related topics. After an introduction to matrix models and Chern-Simons theory, it describes the topological string theories that correspond to these gauge theories and develops the mathematical implications of this duality for the enumerative geometry of Calabi-Yau manifolds and knot theory. It will be useful reading for graduate students and researchers in both mathematics and physics.

Quand le Ciel nous bombarde: Qu’est-ce que les rayons cosmiques?

de Michel Crozon, Editions Vuibert. Broché ISBN 2711771539, €28.

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Sous un titre évocateur des grandes offensives aériennes des années quarante, voici un nouveau compendium du rayonnement cosmique. Ces corpuscules naturellement accélérés depuis le fin fond de l’univers jusqu’à des énergies susceptibles de faire pâlir d’envie le physicien moderne, ont été mis en évidence voici bientôt un siècle grâce aux pacifiques ballons de l’Autrichien Viktor Hess.

Plus tard une foule d’autres pionniers tels que Robert Millikan et Carl Anderson traquèrent le mystérieux rayonnement. Ils furent suivis en Europe par Pierre Auger et Louis Leprince-Ringuet avec son école du Pic du Midi de Bigorre, lesquels ne tardèrent pas à se tourner vers l’exploitation des appareillages d’un CERN pas encore adulte. Aujourd’hui la chasse aux rayons cosmiques dispose de vastes installations de détection comparables de par leur ampleur à celles ceinturant le futur accélérateur européen LHC. Implantés dans les entrailles du globe, sous les glaces du Pole Sud, en Méditerranée, voire en de profondes mines, ces instruments tentent d’expliquer l’origine de corpuscules extra-galactiques dont l’énergie peut frôler les 1020 électronvolts.

L’ouvrage survole l’essentiel des expériences réalisées avant et depuis la guerre afin de mieux connaître ces messagers célestes. Au fil de 240 pages bien illustrées, l’auteur situe cette expérimentation dans le contexte des développements de la physique corpusculaire. Son approche n’en demeure cependant pas liée aux seuls développements théoriques. Elle décrit aussi l’outillage de plus en plus perfectionné mis en œuvre: émulsions, compteurs Geiger-Müller, ballons, chambres à brouillard ou à bulles, détecteurs souterrains ou sondes embarquées sur satellites.

L’auteur qualifie son travail d’ouvrage de vulgarisation. Toutefois, à destination du lecteur plus féru de détails technico-scientifiques, l’usage de caractères d’imprimerie différents permet occasionnellement de passer à un registre plus avancé. Le livre ne manque d’ailleurs pas d’autres atouts, à commencer par une table des matières commodément située en début de volume, et un lexique bien charpenté. En contrepartie il faut se satisfaire de quelques inconvénients tels que la sempiternelle orthographe d’électronvolt en deux mots ou, moins mineure, l’absence d’index.

En bref, le lecteur avide de science et désireux de mieux cerner la physique des corpuscules de hautes énergies pourra assouvir sa curiosité grâce à cette incursion dans le royaume de la plus gigantesque des machine accélératrices de particules: l’univers lui-même.

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