By T W Donnelly, J A Formaggio, B R Holstein, R G Milner and B Surrow
Cambridge University Press
This textbook aims to present the foundations of both nuclear and particle physics in a single volume in a balanced way, and to highlight the interconnections between them. The material is organised from a “bottom-up” point of view, moving from the fundamental particles of the Standard Model to hadrons and finally to few- and many-body nuclei built from these hadronic constituents.
The first group of chapters introduces the symmetries of the Standard Model. The structure of the proton, neutron and nuclei in terms of fundamental quarks and gluons is then presented. A lot of space is devoted to the processes used experimentally to unravel the structure of hadrons and to probe quantum chromodynamics, with particular focus on lepton scattering. Following the treatment of two-nucleon systems and few-body nuclei, which have mass numbers below five, the authors discuss the properties of many-body nuclei, and also extend the treatment of lepton scattering to include the weak interactions of leptons with nucleons and nuclei. The last group of chapters is dedicated to relativistic heavy-ion physics and nuclear and particle astrophysics. A brief perspective on physics beyond the Standard Model is also provided.
The volume includes approximately 120 exercises and is completed by two appendices collecting values of important constants, useful equations and a brief summary of quantum theory.
By Gerard M Crawley and Eoin O’Sullivan
Imperial College Press
This book is designed as a “how to” guide to writing grant proposals for competitive peer review. Nowadays researchers are often required to apply to funding agencies to secure a budget for their work, but being a good researcher does not necessarily imply being able to write a successful grant proposal. Typically, the additional skills and insights needed are learnt through experience.
This timely book aims to guide researchers through the whole process, from conceiving the initial research idea, defining a project and drafting a proposal, through to the review process and responding to reviewers’ comments. Drawing on their own experience as reviewers in a number of different countries, the authors provide many important tips to help researchers communicate both the quality of their research and their ability to carry it out and manage a grant. The authors illustrate their guidelines with the help of many examples of both successful and unsuccessful grant applications, and emphasise key messages with quotes from reviewers.
The book also contains valuable advice for primary investigators on how to set up their research budget, manage people and lead their project. Two appendices at the end of the volume provide website addresses and references, as well as an outline of how to organise a grant competition.
Aimed primarily at early career researchers applying for their first grant, the book will also be beneficial to more experienced scientists, to the administrators of universities and institutions that support their researchers during the submission process, and to the staff of recently established funding organisations, who may have little experience in organising peer-review competitions.
This 235 page book is dedicated to the ITER tokamak, the deuterium–tritium fusion reactor under construction in France, which aims to investigate the feasibility of fusion power. The book provides a concise overview of the state-of-the-art plasma physics involved in nuclear-fusion processes. Definitely not an introductory book – not even for a plasma-physics graduate student – it would be useful as a reference text for experts. Across 10 chapters, the authors describe the physics learned from previous tokamak projects around the world and the application of that experience to ITER.
After an introduction to the ITER project, the conventional magneto-hydrodynamic description of plasma physics is discussed, with strong emphasis on the geometry of the divertor (located at the bottom of the vacuum vessel to extract heat and reduce contamination of the plasma from impurities). Chapter 3 deals with the problem of alpha-particle distribution, which is a source of Alfven and cyclotron instabilities. Edge localised mode (ELM) instabilities associated with the divertor’s magnetic separatrix are also discussed. Conditions of turbulent transport are assumed throughout, so chapter 4 provides a general review of our (mainly experimental) knowledge of the topic. Chapters 5 and 6 are specific to the ITER design because they describe the ELM instabilities in the ITER tokamak and the solutions adopted for their control. Concluding the part dedicated to the fusion-reactor transient phase, steady-state operations and plasma diagnostics techniques are described in chapters 7 and 8, respectively.
The tokamak’s complex magnetic field is able to confine charged particles in the fusion plasma but not neutral particles. Neutron bombardment of surfaces can be viewed as an inconvenience, making it necessary to ensure the walls are radiation hard, or an advantage, turning the surfaces into a breeding blanket to generate further tritium fuel. Radiation hardness of the tokamak walls is discussed in chapter 9, while chapter 10 explains how ITER will transmute a lithium blanket into tritium via bombardment with fusion neutrons. The IFMIF (International Fusion Materials Irradiation Facility) project, conceived for fusion-material tests and still in its final design phase, is also briefly presented. The book closes with some predictions about the expectations to be fulfilled by ITER, before proceeding to the design of DEMO – a future tokamak for electrical-energy production.
In summary, ITER Physics is a book for expert scientists who are looking for a compact overview of the latest advances in tokamak physics. I appreciated the exhaustive set of references at the end of each chapter, since it provides a way to go deeper into concepts not exhaustively explained in the book. Plasma-fusion physics is complex, not only because it is a many-body problem but also because our knowledge in this field is limited, as the authors stress. I would have appreciated more graphic material in some parts: in order to fully understand how a fusion reactor works, one has to think in 3D, so schematics are always helpful.
By Gregory V Vereshchagin and Alexey G Aksenov
Cambridge University Press
This book provides an overview of relativistic kinetic theory, from its theoretical foundations to its applications, passing through the various numerical methods used when analytical solutions of complex equations cannot be obtained.
Kinematic theory (KT) was born in the 19th century and aims to derive the properties of macroscopic matter from the properties of its constituent microscopic particles. The formulation of KT within special relativity was completed in the 1960s.
Relativistic KT has traditional applications in astrophysics and cosmology, two fields that tend to rely on observations rather than experiments. But it is now becoming more accessible to direct tests due to recent progress in ultra-intense lasers and inertial fusion, generating growing interest in KT in recent years.
The book has three parts. The first deals with the fundamental equations and methods of the theory, starting with the evolution of the basic concept of KT from nonrelativistic to special and general relativistic frameworks. The second part gives an introduction to computational physics and describes the main numerical methods used in relativistic KT. In the third part, a range of applications of relativistic KT are presented, including wave dispersion and thermalisation of relativistic plasma, kinetics of self-gravitating systems, cosmological structure formation, and neutrino emission during gravitational collapse.
Written by two experts in the field, the book is intended for students who are already familiar with both special and general relativity and with quantum electrodynamics.
Have you ever thought that batteries capable of providing energy over very long periods could be made with radioisotopes? Did you know that the bacterium deinococcus radiodurans can survive enormous radiation doses and, thanks to its ability to chemically alter highly radioactive waste, it could be potentially employed to clean up radioactively contaminated areas? And do you believe that cockroaches have an extremely high radiation tolerance? Apparently, the latter is a myth. These are a few of the curiosities contained in this “all that you always wanted to know about radioactivity” book from Grupen and Rodgers. It gives a comprehensive overview of the world of radioactivity and radiation, from its history to its risks for humans.
The book begins by laying the groundwork with essential, but quite detailed (similar to a school textbook), information about the structure of matter, how radiation is generated, how it interacts with matter and how it can be measured. In the following chapters, the book explores the substantial benefits of radioactivity through its many applications (not only positive, but also negative and sometimes questionable) and the possible risks associated with its use. The authors deal mainly with ionising radiation; however, in view of the public debate about other kinds of radiation (such as mobile-phone and microwave signals), they include a brief chapter on non-ionising radiation. Also interesting are the final sections, provided as appendices, which summarise the main technologies of radiation detectors as well as the fundamental principles of radiation protection. In the latter, the rationale behind current international rules and regulations, put in place to avoid excessive radiation exposure for radiation workers and the general public, is clearly explained.
This extensive topic is covered using easily understood terms and only elementary mathematics is employed to describe the essentials of complex nuclear-physics phenomena. This makes for pleasant reading intended for the general public interested in radioactivity and radiation, but also for science enthusiasts and inquisitive minds. As a bonus, the book is illustrated with eye-catching cartoons, most of them drawn by one of the authors.
The book emphasises that radiation is everywhere and that almost everything around us is radioactive to some degree: there is natural radioactivity in our homes, in the food that we eat and the air that we breathe. Radiation from the natural environment does not present a hazard; however, radiation levels higher than the naturally occurring background can be harmful to both people and the environment. These artificially increased radiation levels are mainly due to the nuclear industry and have therefore risen substantially since the beginning of the civil-nuclear age in the 1950s. This approach helps readers to put things in perspective and allows them to compare the numbers and specific measurement quantities that are used in the radiation-protection arena. These quantities are the same used by the media, for instance, to address the general public when a radiation incident occurs.
Not only will this book enrich the reader’s knowledge about radioactivity and radiation, it will also provide them with tools to better understand many of the related scientific issues. Such comprehension is crucial for anyone who is willing to develop their own point of view and be active in public debates on the topic.
When developing technologies involving the use of nuclear material or ionisation radiation, a number of safety issues and potential risks have to be addressed. The author of this book, a certified health physicist and an expert in radiation protection, discusses these emerging topics related to radiation-generating technologies and associated hazards.
The book opens with a brief overview of modern radiation-protection challenges, before delving into specific areas. First, the author discusses the nuclear-fuel cycle, analysing its steps and related issues such as reactors, new technologies for uranium enrichment and waste disposal. In the following section, he deals with nuclear accidents and radiological emergencies – making specific reference to the well-known disasters of Three Mile Island, Chernobyl and Fukushima Daiichi – and with the risk of terrorist events involving sabotage or the use of improvised nuclear weapons and devices.
Today, nuclear material is also largely employed for medical imaging and therapies, thus a part of the book is devoted to these technologies and to the consequent increase of public radiation exposure. Finally, the last section focuses on regulatory issues, limitations and challenges.
Meant for upper-level undergraduate and graduate students of health-physics and engineering courses, the book would also be a useful reference for scientists and professionals working in radiation protection, fuel-cycle technology and nuclear medicine. More than 300 problems with solutions accompany the text and many appendices provide background information.
This review volume is motivated by the 2014 observation of a high-energy neutrino flux of extraterrestrial origin by the IceCube experiment at the South Pole. The energy of the events recorded ranges from 30 to 2000 TeV, with the latter marking the highest-energy neutrino interaction ever observed. The study of neutrinos originating from violent astrophysical sources enhances our knowledge not only of cosmological phenomena but also of neutrinos themselves.
This book gives an overview of the current status of research in the field and of existing and future neutrino observatories. The first group of chapters present the physics of potential sources of high-energy neutrinos, including gamma-ray bursts, active galactic nuclei, star-forming galaxies and sources in the Milky Way. A chapter is then dedicated to the measurements performed by IceCube, the results of which are discussed in terms of energy spectrum, flavour-ratio and arrival-direction isotropy. Following this, the results of two deep-sea neutrino experiments, ANTARES and Baikal, are presented.
After a brief discussion of other research topics in which the study of high-energy astrophysical neutrinos can play an important role, such as the quest for dark matter, the book examines the next generation of cosmic neutrino detectors. In particular, the future KM3NeT experiment, which will consist of a network of underwater telescopes located in the Mediterranean Sea, and IceCube-Gen2, characterised by unprecedented sensitivity and higher angular resolution compared to IceCube, are described.
Finally, a review of present and in-planning experiments aiming at detecting radio emissions from high-energy neutrino interactions concludes the volume.
There is always great excitement among the academic community when a new book by renowned scientists is published. Written by leading experts in particle physics, this book by Luciano Maiani and Omar Benhar, with contributions from the late Nicola Cabibbo, does not disappoint in this regard. Former CERN Director-General Maiani co-proposed the GIM mechanism, which is required to suppress flavour-changing neutral currents at the tree level and assumed the existence of a fourth quark that was discovered in 1974 at SLAC and BNL, while Cabibbo proposed a solution to the puzzle of electroweak decays of strange particles, which was later extended to give rise to the Cabibbo–Kobayashi–Maskawa mixing matrix. Omar Benhar, an INFN research director and professor at the University of Rome “La Sapienza”, is expert in the theory of many-particle systems, the structure of compact stars and electroweak interactions of nuclei.
Their book is the third volume of a series dedicated to relativistic quantum mechanics, gauge theories and electroweak interactions, based on material taught to graduate students at the University of Rome over a period of several decades. Given that gauge theories are the basis of interactions between elementary particles, it is not surprising that there are many books about gauge theories already out there – among the best are those written by Paul Frampton, J R Aitchison and Anthony Hey, Chris Quigg, Ta-Pei Cheng and Ling-Fong Li. One might therefore think that it is hard to add something new to the field, but this book introduces the reader in a concise and elegant manner to a modern account of the fundamentals of renormalisation in quantum field theories and to the concepts underlying gauge theories.
Containing more than 300 pages organised in 20 chapters and several appendices, the book focuses mainly on quantum electrodynamics (QED), which – despite its simplicity and limitations – serves as the mould of a gauge theory and at the same time it has a high predictive power and numerous applications. The first part of this treatise deals with the quantisation of QED via the path-integral method, from basic to advanced concepts, followed by a brief discussion on the renormalisation of QED and some of its applications, such as bremsstrahlung, the Lamb shift, and the electron anomalous magnetic moment. The prediction of the latter is considered one of the great achievements of QED.
In the second part of the book, the authors cover the renormalisation group equations of QED and introduce the quantisation of non-Abelian gauge theories, finishing with a proof of the asymptotic freedom of quantum chromodynamics. Afterwards, the concept of the running coupling constant is used to introduce a few ideas about grand unification. The final chapters are devoted to concepts related to the Standard Model of particle physics, such as the Higgs mechanism and the electroweak corrections to the muon anomalous magnetic moment. Finally, a few useful formulas and calculations are provided in several appendices.
Throughout the book the authors not only present the mathematical framework and cover basic and advanced concepts of the field, but also introduce several physical applications. The most recent discoveries in the field of particle physics are discussed. This is a book targeted at advanced students accustomed to mental challenges. A minor flaw is the lack of problems at the end of the chapters, which would offer students the possibility to apply the acquired knowledge, although the authors do encourage readers to complete a few demonstrations. This text will be very helpful for students and teachers interested in a treatment of the fundamentals of gauge theories via a concise and modern approach in the constantly changing world of particle physics.
By César Augusto Zen Vasconcellos (ed.)
World Scientific
In 1915 Albert Einstein presented to the Royal Prussian Academy of Sciences his theory of general relativity (GR), which represented a breakthrough in modern physics and became the foundation of our understanding of the universe at large. A century later, this elegant theory is still the basis of the current description of gravitation and a number of predictions derived from it have been confirmed in observations and experiments – most recently with the direct detection of gravitational waves.
This book celebrates the centenary of GR with a collection of 11 essays by different experts, which offer an overview of the theory and its numerous astrophysical and cosmological implications. After an introduction to GR, the Tolman–Oppenheimer–Volkoff equations describing the structure of relativistic compact stars are derived and their extension to deformed compact stellar objects presented. The book then moves to the so-called pc-GR theory, in which GR is algebraically extended to pseudo-complex co-ordinates in an attempt to get around singularities. Other topics covered are strange matter, in particular a conjecture that pulsar-like compact stars may be made of a condensed three-flavour quark state, and the use of a particular solution of the GR equations to construct multiple non-spherical cosmic structures.
Keeping the book contemporary, it also gives an overview of the most recent experimental results in particle physics and cosmology. Several contributions are devoted to the search for physics beyond the Standard Model at CERN, studies of cosmic objects and phenomena through gamma-ray lenses and, finally, to the recent detection of gravitational waves by the LIGO experiment.
By Gerard Auger and Eric Plagnol (eds)
World Scientific
In 2016, the first direct detection of gravitational waves – produced more than a billion years ago during the coalescence of two black holes of stellar origin – by the two detectors of the LIGO experiment was a tremendous milestone in the history of science. This timely book provides an overview of the field, presenting the basics of the theory and the main detection techniques.
The discovery of gravitational radiation is extraordinarily important, not only for confirming the key predictions of Einstein’s general relativity, but also for its implications. A new window on the universe is opening up, with more experiments – already built or in the planning stage – joining the effort to perform precise measurements of gravitational waves.
The book, composed of eight chapters, collects the contributions of many experts in the field. It first introduces the theoretical basics needed to follow the discussion on gravitational waves, so that no prior knowledge of general relativity is required. A long chapter dedicated to the sources of such radiation accessible to present and future observations follows. A section is then devoted to the principles of gravitational-wave detection and to the description of present and future Earth- and space-based detectors. Finally, an alternative detection technique based on cold atom interferometry is presented.
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