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Dramatic progress has been made in all branches of physics since the National Research Council's 1986 decadal survey of the field. The Physics in a New Era series explores these advances and looks ahead to future goals. The series includes assessments of the major subfields and reports on several smaller subfields, and preparation has begun on an overview volume on the unity of physics, its relationships to other fields, and its contributions to national needs. Nuclear Physics is the latest volume of the series. The book describes current activity in understanding nuclear structure and symmetries, the behavior of matter at extreme densities, the role of nuclear physics in astrophysics and cosmology, and the instrumentation and facilities used by the field. It makes recommendations on the resources needed for experimental and theoretical advances in the coming decade.
Hardbound. In cosmology the neutrinos determine the expansion rate of the early universe. They probably constitute part of hot dark matter and are essential for supernova explosions. In spite of great efforts, the missing solar neutrinos are not completely understood. Various solar neutrino experiments seem to give different results about the missing solar neutrinos. However each of these experiments, such as the C1 detector, GALLEX, SAGE and KAMIOKANDE, measure slightly different quantities. Only GALLEX and SAGE look exactly for the same neutrinos and seem to be in agreement with each other.This volume of review articles looks in depth at the latest research results and presents a state-of-art view of this fast exanding field. All the chapters are written by leading experts active in the field today.
This volume provides up-to-date information on selected topics in nuclear physics and their future prospects. Topics discussed include nuclear astrophysics; synthesis of very heavy elements; physics with exotic nuclei; heavy ion collisions; spin-isospin excitation. This volume contains 47 papers by invited speakers and nine summaries by chairpersons.
Neutrinos play a key role in many areas of particle physics, nuclear physics and astrophysics. The recent discovery of neutrino oscillation has given the first hint of new physics beyond the standard model. Clearly, it is extremely important to study further the oscillation and other fundamental properties of neutrinos. It is also important to improve our knowledge of neutrino-nucleus reactions, which are crucial for understanding a large class of astrophysical phenomena. These and many other interesting questions can be investigated at stopped pion neutrino facilities like the one planned for the Spallation Neutron Source at the Oak Ridge National Laboratory. The purpose of the Carolina Symposium was twofold: (1) to explore and exchange ideas on the latest developments in general frontiers of neutrino physics and related fields; (2) to address specific issues pertaining to the above-mentioned stopped pion neutrino facility. Among the topics covered in the proceedings are: cosmology and neutrino; standard model tests with neutrinos; neutrino oscillation, experiments and theories; dark matter search; double beta-decay; rare events detection techniques; the solar neutrino problem; supernova explosion; nucleosynthesis; and the ORLaND project.
The scientific program of these important proceedings was arranged to cover most of the field of neutrino physics. In light of the rapid growth of interest stimulated by new interesting results from the field, more than half of the papers presented here are related to the neutrino mass and oscillations, including atmospheric and solar neutrino studies. Neutrino mass and oscillations could imply the existence of a mass scale many orders of magnitudes higher than presented in current physics and will probably guide scientists beyond the standard model of particle physics.
This is the proceedings of the symposium on Frontiers of Nuclear Structure Physics which was held from March 2-5, 1994, in honor of Akito Arima. Nuclear structure physics is approaching a new era owing to various recent developments such as radioactive nuclear beams, multiple gamma-ray detectors, massive parallel computers, etc. In the near future RHIC, CEBAF and other facilities will further extend the horizons of the field and this meeting offered a look at these exciting possibilities ahead. Topics discussed included (i) new trends in shell model, (ii) electroweak interactions in nuclei, (iii) unstable nuclei, (iv) Interacting Boson Model, (v) proton-neutron degrees of freedom in nuclear collectivity, (vi) quarks in hadrons and nuclei, (vii) nuclear astrophysics, (viii) nuclear and atomic clusters.
The 14th RCNP OSAKA International Symposium on Nuclear Reaction Dynamics of Nucleon-Hadron Many Body System was held in Osaka from December 6 to 9, 1995. The symposium covered current topics from Nucleon Spins and Mesons in Nuclei to Quark Lepton Nuclear Physics. Thus it included the field of hadron/nuclear physics from sub-GeV to multi-GeV energy region, as well as recent activities and development at RCNP. It was also intended to be a kind of winter school for young researchers/graduate students.This proceedings consists of the invited talks and lectures presented by leading physicists in the field and short oral presentations.
Vols. 1, 6, 8-9, 11, 13- consist of Proceedings of the International School of Nuclear Physics.
This is the proceedings of the International Symposium on Origin of Matter and Evolution of Galaxies which was held near Tokyo, Japan, in November 2003. The meeting brought together many scientists from vast fields — nuclear physics, particle physics, cosmic-ray physics, cosmology, astronomy, geophysics, and others — to promote discussion and collaboration.The proceedings have been selected for coverage in:• Index to Scientific & Technical Proceedings® (ISTP® / ISI Proceedings)• Index to Scientific & Technical Proceedings (ISTP CDROM version / ISI Proceedings)• CC Proceedings — Engineering & Physical Sciences