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The proceedings of the 4th Italy-Japan Symposium on Heavy Ion Physics cover the following fields of nuclear physics: heavy ion nuclear reactions; nuclei under extreme conditions; nuclear astrophysics; photon detectors and physics; technology of RI beams and experimental instrumentation; application of RI beams.
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Some countries have moved beyond the design and operation of nuclear electricity generating systems to confronting the issue of nuclear waste disposal, whole others are still committed to further nuclear facility construction. Volume 24 chronicles these key developments and examines nuclear reactor accidents at Chernobyl, Bhopal, and TMI. The text also analyzes current international knowledge of neutron interactions; deterministic methods based on mean values for assessing radiation distributions; practical applications of the TIBERE models to explicit computation of leakage terms in realistic reactor geometry; and a technique to deal with the issues of finance, risk assessment, and public perception.
Nuclear engineering. --- Nuclear physics. --- Nuclear Physics, Heavy Ions, Hadrons. --- Heavy ions. --- Ions --- Atomic nuclei --- Atoms, Nuclei of --- Nucleus of the atom --- Physics --- Atomic power engineering --- Engineering --- Nuclear physics --- Nuclear energy
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Chemistry --- Elements --- chemical structure --- Acid base equilibrium --- chemical reactions --- Ions --- Chemistry, Inorganic.
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This volume presents a comprehensive collection of state-of-the-art advances in the field of solid state ionic materials and the design, fabrication and performance of devices that use them, such as lithium batteries, gas sensors, fuel cells, supercapacitors and electrochromic displays. These electrochemical devices are becoming pervasive in our technologically driven lifestyles.The book includes research activities being carried out in the new millennium, through special keynote addresses, as well as invited and contributed papers, related to experimental and theoretical modeling in solid sta
Solid state electronics --- Semiconductors --- Ions --- Intermediates (Chemistry) --- Matter --- Physics --- Solution (Chemistry) --- Electrolysis --- Electrons --- Properties
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Acrylic resins. --- Aqueous solutions. --- Ion exchange resins. --- Lead (metal) --- Metal ions.
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Hollow cathodes. --- Ions. --- Double layer. --- Plasmas (physics) --- Electric propulsion. --- Ion engines.
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An expert and illuminating review of the leading models of nuclear structure: effective field theories based on quantum chromodynamics; ab initio models based on Monte Carlo methods employing effective nucleon-nucleon interactions; diagonalization and the Monto Carlo shell model; non-relativistic and relativistic mean-field theory and its extensions; and symmetry-dictated approaches. Theoretical advances in major areas of nuclear structure are discussed: nuclei far from stability and radioactive ion beams; gamma ray spectroscopy; nuclear astrophysics and electroweak interactions in nuclei; electron scattering; nuclear superconductivity; superheavy elements. The interdisciplinary aspects of the many-body problem are also discussed. Recent experimental data are examined in light of state-of-the-art calculations. Recent advances in several broad areas of theoretical structure are covered, making the book ideal as a supplementary textbook.
Nuclear reactions --- Many-body problem --- Réactions nucléaires --- Problème des N corps --- Congresses. --- Congrès --- Nuclear physics. --- Heavy ions. --- Mathematical physics. --- Observations, Astronomical. --- Astronomy—Observations. --- Nuclear Physics, Heavy Ions, Hadrons. --- Theoretical, Mathematical and Computational Physics. --- Astronomy, Observations and Techniques. --- Astronomical observations --- Observations, Astronomical --- Physical mathematics --- Physics --- Ions --- Atomic nuclei --- Atoms, Nuclei of --- Nucleus of the atom --- Mathematics
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This textbook is intended as an introduction to the physics of solar and stellar coronae, emphasizing kinetic plasma processes. It is addressed to observational astronomers, graduate students, and advanced undergraduates without a ba- ground in plasma physics. Coronal physics is today a vast field with many different aims and goals. So- ing out the really important aspects of an observed phenomenon and using the physics best suited for the case is a formidable problem. There are already several excellent books, oriented toward the interests of astrophysicists, that deal with the magnetohydrodynamics of stellar atmospheres, radiation transport, and radiation theory. In kinetic processes, the different particle velocities play an important role. This is the case when particle collisions can be neglected, for example in very brief phenomena – such as one period of a high-frequency wave – or in effects produced by energetic particles with very long collision times. Some of the most persistent problems of solar physics, like coronal heating, shock waves, flare energy release, and particle acceleration, are likely to be at least partially related to such p- cesses. Study of the Sun is not regarded here as an end in itself, but as the source of information for more general stellar applications. Our understanding of stellar processes relies heavily, in turn, on our understanding of solar processes. Thus an introduction to what is happening in hot, dilute coronae necessarily starts with the plasma physics of our nearest star.
Stars --- Plasma astrophysics. --- Plasma dynamics. --- Particle beams. --- Corona. --- Sun --- Planetology. --- Nuclear physics. --- Plasma Physics. --- Astrophysics and Astroparticles. --- Nuclear Physics, Heavy Ions, Hadrons. --- Atomic nuclei --- Atoms, Nuclei of --- Nucleus of the atom --- Physics --- Planetary sciences --- Planetology --- Plasma (Ionized gases). --- Astrophysics. --- Heavy ions. --- Ions --- Astronomical physics --- Astronomy --- Cosmic physics --- Gaseous discharge --- Gaseous plasma --- Magnetoplasma --- Ionized gases
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For the first half of the 20th Century, low-energy nuclear physics was one of the dominant foci of all of science. Then accelerators prospered and energies rose, leading to an increase of interest in the GeV regime and beyond. The three articles comprising this end-of-century Advances in Nuclear Physics present a fitting and masterful summary of the energy regimes through which nuclear physics has developed and promises to develop in future. One article describes new information about fundamental symmetries found with kV neutrons. Another reviews our progress in understanding nucleon-nucleus scattering up to 1 GeV. The third analyzes dilepton production as a probe for quark-gluon plasmas generated in relativistic heavy-ion collisions.
Nuclear physics. --- Physics. --- Nuclear Physics, Heavy Ions, Hadrons. --- Atomic, Molecular, Optical and Plasma Physics. --- Heavy ions. --- Atoms. --- Natural philosophy --- Philosophy, Natural --- Physical sciences --- Dynamics --- Chemistry, Physical and theoretical --- Matter --- Stereochemistry --- Ions --- Atomic nuclei --- Atoms, Nuclei of --- Nucleus of the atom --- Physics --- Constitution
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Prominent progress in science is inevitably associated with controversies. Thus, young researchers, in particular, have to learn how to persevere during the period of controversy and struggle for acceptance. Unfortunately, the skills needed are not taught in textbooks or monographs, which mostly describe the consensus of contemporary experts. This book, which is based on my own experiences as a scientist, describes the history of the progress made in auroral science and magnetospheric physics by providing examples of ideas, controversies, struggles, acceptance, and success in some instances. Although no general methodology (if any exists) is mentioned, I hope that the reader will learn about the history of progress in auroral science and examples (right or wrong) of dealing with the controversies.
Auroras. --- Physical geography. --- Nuclear physics. --- Astrophysics and Astroparticles. --- Geophysics/Geodesy. --- Atmospheric Sciences. --- Nuclear Physics, Heavy Ions, Hadrons. --- Atomic nuclei --- Atoms, Nuclei of --- Nucleus of the atom --- Physics --- Geography --- Astrophysics. --- Geophysics. --- Atmospheric sciences. --- Heavy ions. --- Ions --- Atmospheric sciences --- Earth sciences --- Atmosphere --- Geological physics --- Terrestrial physics --- Astronomical physics --- Astronomy --- Cosmic physics --- Aurora australis --- Aurora borealis --- Northern lights --- Polar lights --- Atmospheric physics
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