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Neutrinos
Neutrinos play a fundamental role in the latest particle physics theories, such as Grand Unified Theories, theories of supersymmetry, and superstring theory. Their mass yields an important boundary condition for grand unification models. They are the best candidates for dark matter in the universe, and their mass could determine its large scale structure and evolution. Neutrinos probe the interior of collapsing stars, and understanding them may lead to a solution of the solar neutrino problem. In ten chapters written by experts in each of these fields this book gives a comprehensive presentation of our current knowledge of the neutrino, of its role in nuclear particle and astrophysics theories, and of ongoing experimental efforts to learn more about its own nature. Graduate students and researchers in these fields will find this book a reliable advanced text and source of reference.
Theory, Numerics and Applications of Hyperbolic Problems II
The second of two volumes, this edited proceedings book features research presented at the XVI International Conference on Hyperbolic Problems held in Aachen, Germany in summer 2016. It focuses on the theoretical, applied, and computational aspects of hyperbolic partial differential equations (systems of hyperbolic conservation laws, wave equations, etc.) and of related mathematical models (PDEs of mixed type, kinetic equations, nonlocal or/and discrete models) found in the field of applied sciences.
Astronomy, Cosmology and Fundamental Physics
In the development of Fundamental Physics on one side, and of Astronomy/Cosmology on the other side, periods of parallell, relatively independent progress seem to alternate with others of intense interaction and mutual influence. To this latter case belong the very beginnings of Modern Physics, with Galileo and Newton. There is now a widespread feeling that another of such flourishing periods may have started some ten years ago, with the advent of Unified Theories and the introduction of Inflationary Cosmologies. The interaction between the two disciplines has become tighter ever since, spurring studies of e. g. astronomical and particle Dark Matter candidates, Superstrings and Cosmic String...
Particles And Cosmology - International School
Contents:Theory: Electroweak Baryon Number Non-Conservation in Particle Physics and Cosmology (V A Rubakov)Constraints and Model Considerations for a 17 keV Neutrino (R D Peccei)Solar Neutrinos:Measurement of the Solar υe Flux with the Homestake 37Cl Detector (K Lande)SAGE: The Soviet-American Gallium Solar Neutrino Experiment (V N Gavrin)Calorimetric Measurements of an Artificial Netrino Source Activity for the Baksan Gallium-Germanium Neutrino Telescope (I N Belousov et al)The Status of Gallex (R Wink)The Sudbury Neutrino Observatory (D Sinclair)Results from Underground Experiments: Recent Results from IBM (J LoSecco & J Learned)Analysis of Rare Signals at the Baksan Underground Scintilla...
Neutrinos in Cosmology, Astro, Particle and Nuclear Physics
Neutrinos in Cosmology, Astro, Particle and Nuclear Physics
Cosmogonical Processes
Cosmogony deals with no less than the genesis and development of the universe, the solar system and the earth. This book was developed from a symposium in honour of Prof. A.G.W. Cameron of Harvard University on his 60th birthday, and suitably reflects his broad and influential interests. Appropriate to this perspective, a wide variety of topics are reviewed by internationally recognized experts. Beginning with cosmology and the question of dark matter, the spotlight moves to galaxy formation and then evolution. This is followed by the topic of the production of atomic nuclei in supernovae, the clues for nucleosynthesis from isotopic anomalies, and the age of the universe from nuclear chronol...
Stellar Structure and Evolution
This long-awaited second edition of the classical textbook on Stellar Structure and Evolution by Kippenhahn and Weigert is a thoroughly revised version of the original text. Taking into account modern observational constraints as well as additional physical effects such as mass loss and diffusion, Achim Weiss and Rudolf Kippenhahn have succeeded in bringing the book up to the state-of-the-art with respect to both the presentation of stellar physics and the presentation and interpretation of current sophisticated stellar models. The well-received and proven pedagogical approach of the first edition has been retained. The book provides a comprehensive treatment of the physics of the stellar interior and the underlying fundamental processes and parameters. The models developed to explain the stability, dynamics and evolution of the stars are presented and great care is taken to detail the various stages in a star’s life. Just as the first edition, which remained a standard work for more than 20 years after its first publication, the second edition will be of lasting value not only for students but also for active researchers in astronomy and astrophysics.
High Energy Astrophysics
The second workshop on High Energy Astrophysics of the Ma..x-Planck-Society and the Academia Sinica was held at Ringberg Castle near Tegernsee during the week July 12-July 17, 1987. It is the purpose of these workshops to en courage the exchange of ideas between German and Chinese astrophysicists (scientists from other countries are also welcome, of course), and the pleas ant atmosphere and surroundings of Ringberg Castle certainly helped the development of relaxed and stimulating discussions. In addition, we seemed to have picked out the one week of perfect weather during a rainy summer. Thanks are due to Mr. Hormann and his staff for creating a perfect infra structure. The proceedings have...
Neutron Stars: Theory and Observation
Some twenty-three years after the discovery of pulsars and their identification as rotating neutron stars, neutron star physics may be regarded as comingofage. Pul sars and accreting neutron stars have now been studied at every wavelength, from the initial radio observations, through optical, X-, and "{-ray, up to the very recent observations in the TeV region, while theorists have studied in some detail relevant physical processes both outside and inside neutron stars. As a result, comparisonof theory with observation provides a test ofour theoretical ideas in fields as diverse as neutron and nuclear matter, superfluidity and superconductivity, the acceleration of high energy particles, and...
