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This volume documents an important event in the World Year of Physics 2005 and a continuation of the traditional international summer schools that have taken place in Romania regularly since 1964. On one hand, the study of exotic nuclei seeks answers about the structure and interaction of unique finite quantum mechanical many-body systems. On the other, it provides data that have an impact on the understanding of the origin of the elements in the Universe. The contributions, written by outstanding professors from prestigious research centers over the world, provide the reader with both comprehensive reviews and the most recent results in the field. Large experimental facilities are discussed together with future research projects. The book offers insights into how experiments in terrestrial nuclear physics laboratories may be combined with observations in outer space to enlarge our basic knowledge. Sample Chapter(s). Chapter 1: Research on Neutron Clusters (1,195 KB). Contents: Exotic Nuclei: Research on Neutron Clusters (F M Marques); Neutron Transfer Studied with a Radioactive Beam of 24 Ne, Using TIARA at SPIRAL (W Catford et al.); Rare Isotopes INvestigations at GSI (RISING) Using Relativistic Ion Beams (J Jolie et al.); Mass Formula from Normal to Hypernuclei (C Samanta); Exotic Nuclear Structures: Exotic Phenomena in Medium Mass Nuclei (A Petrovici); NUSTAR at FAIR. Nuclear Structure Research at GSI and the Future (G Muenzenberg); From Super-Radiance to Continuum Shell Model (V Zelevinski); New Methods for the Exact Solution of the Nuclear Eigenvalue Problem Beyond Mean Field Approaches (N Lo Iudice et al.); Q-Phonon Approach for Low-Lying 1 - Two-Phonon States in Spherical Nuclei (V V Voronov et al.); Analytic Description of the Phase Transition from Octupole Deformation to Octupole Vibrations (D Bonatsos et al.); Three-Body Models in Nuclear Physics (P Descouvemont); Properties of Low-Lying States: Shape Parameters and Proton-Neutron Symmetry (V Werner); Shell Model Nuclear Level Densities (M Horoi); Exotic Decays, Clusters and Superheavy Nuclei: Nuclear Structure and Double Beta Decay (J Suhonen); Systematics of Proton Emission (D S Delion et al.); Synthesis of Superheavy Elements at SHIP (S Hofmann et al.); Synthesis of Heaviest Elements Using a Gas-Filled Recoil Separator at RIKEN (K Morita); Fission Valleys and Heavy Ion Decay Modes (D N Poenaru et al.); Dynamics of Mass Asymmetry in Dinuclear Systems (W Scheid et al.); Exotic Matter in Nuclei and Stars. Neutrinos: Clusters of Matter and Antimatter: A Mechanism for Cold Compression (W Greiner); BRAHMS Experiment Quest for Early Universe Phases of Hadronic Matter (Z Majka); Strange Matter in Core-Collapse Supernova (J Horvath); Neutrino Astrophysics: Gamma Ray Bursts (G C McLaughlin); Neutrino Emission from Neutron Stars (D G Yakovlev et al.); New Achievements in Neutrino Properties (S Stoica); High Energy Cosmic Rays: The Origin of Cosmic Rays (P Biermann); The Mystery of the Highest Energies in the Universe (H Rebel); The Cosmic Ray Experiment KASCADE-GRANDE (I M Brancus et al.); Prospects for the Detection of High-Energy Cosmic Rays Using Radio Techniques (Ad van den Berg); Nucleosynthesis and Nuclear Physics for Astrophysics: Explosive Nucleosynthesis: Supernovae, Classical Novae, and X-Ray Bursts (J Jose); Experimental Approach to Nuclear Reactions of Astrophysical Interest Involving Radioactive Nuclei (C Angulo); Background Studies at the LUNA Underground Accelerator Facility (Zs Fulop); Thoughts about Two of the Important Reactions in Nuclear Astrophysics (L Buchmann); Recent Experimental Studies of Nuclear Astrophysics Using Intermediate-Energy Exotic Beams (T Motobayashi); An Indirect Method Using ANCs in Nuclear Astrophysics (R E Tribble et al.); Recent Applications of the Trojan-Horse Method in Nuclear Astrophysics (C Spitaleri); Nuclear Astrophysics Experiments at CIAE (W Liu et al.); Global Reaction Models Relevant to the p Process (S V Harissopoulos); Large Facilities: TRIUMF OCo Canada's National Laboratory for Particle and Nuclear Physics (L Buchmann); Status of the AGATA Project (E Farnea); Research at ISOLDE and the Path to Eurisol (P A Butler); and other papers. Readership: Academics, Universities and research centres in physics. Undergraduate and graduate students, taking nuclear physics classes, research professionals in nuclear physics and astrophysics."
The book represents the proceedings of the 23rd edition of the Carpathian Summer School of Physics and was held in the Carpathian Mountains resort of Sinaia, Romania. It provides the reader with comprehensive reviews on topics in exotic nuclei, nuclear and particle astrophysics, cosmic rays and neutrino physics. Lectures at graduate student level on basic topics and most recent results in the field are presented in articles written by outstanding researchers from over the world. It treats phenomena from the smallest to largest scales in the Universe, from nuclei to stars. On one hand, the study of exotic nuclei is seeking answers about the structure and interaction of unique finite quantum mechanical many-body systems. On another hand, it provides data that have impact on the understanding of the origin of the elements in the Universe. Particular emphasis is given to the physics of neutrinos. The High Energy cosmic rays give access to phenomena we cannot reproduce on Earth and places we will never want to visit, but seek to understand. The book collects articles that offer insights on how experiments in the terrestrial nuclear physics laboratories can be combined with observations of the outer space to enlarge our basic knowledge.
This volume documents an important event in the World Year of Physics 2005 and a continuation of the traditional international summer schools that have taken place in Romania regularly since 1964. On one hand, the study of exotic nuclei seeks answers about the structure and interaction of unique finite quantum mechanical many-body systems. On the other, it provides data that have an impact on the understanding of the origin of the elements in the Universe.The contributions, written by outstanding professors from prestigious research centers over the world, provide the reader with both comprehensive reviews and the most recent results in the field. Large experimental facilities are discussed together with future research projects. The book offers insights into how experiments in terrestrial nuclear physics laboratories may be combined with observations in outer space to enlarge our basic knowledge.
The conferences in the Carpathians are called by tradition ‘schools’, but are a combination of a school and a conference with invited talks and communications. This was the 24th Carpathian summer school in physics, a tradition since 1964, and the 4th with the current title. Its main objectives are:To educate new generations of specialists in the field of nuclear structure and reactions, of nuclear astrophysics and astroparticles. -To help disseminate and discuss the latest developments in the fields of interest among the participants, to facilitate interactions across field boundaries. -The mixed character school-conference is meant to facilitate the contacts between generations of scientists. -To create conditions of direct contacts between best specialists in the above fields and the local researchers, in particular from Romania.
Nuclear physics is an exciting, broadly faceted field. It spans a wide range of topics, reaching from nuclear structure physics to high-energy physics, astrophysics and medical physics (heavy ion tumor therapy). New developments are presented in this volume and the status of research is reviewed. A major focus is put on nuclear structure physics, dealing with superheavy elements and with various forms of exotic nuclei: strange nuclei, very neutron rich nuclei, nuclei of antimatter. Also quantum electrodynamics of strong fields is addressed, which is linked to the occurrence of giant nuclear systems in, e.g., U+U collisions. At high energies nuclear physics joins with elementary particle physics. Various chapters address the theory of elementary matter at high densities and temperature, in particular the quark gluon plasma which is predicted by quantum chromodynamics (QCD) to occur in high-energy heavy ion collisions. In the field of nuclear astrophysics, the properties of neutron stars and quark stars are discussed. A topic which transcends nuclear physics is discussed in two chapters: The proposed pseudo-complex extension of Einstein's General Relativity leads to the prediction that there are no black holes and that big bang cosmology has to be revised. Finally, the interdisciplinary nature of this volume is further accentuated by chapters on protein folding and on magnetoreception in birds and many other animals.
This memorial volume is dedicated to physicist Gerald E Brown (1926-2013) or 'Gerry' as he was known to his many students, postdocs, colleagues and friends. As written by one of the contributors to this book, 'Gerry was an inspiring father figure for generations of theoretical nuclear physicists and a great human being'.This book covers a wide range of topics in nuclear physics, including nuclear structure, two- and three-body nuclear forces, strangeness nuclear physics, chiral symmetry, hadrons in dense medium, hidden local symmetry, heavy quark symmetry, cosmic neutrinos, nuclear double-beta decay, neutron stars, gravitational waves, renormalization group methods, exotic nuclei, electron ion collider (EIC), and much more. Most of the authors are Gerry's former students and collaborators.We hope readers will find this book very interesting not only for its physics content but also for the window it gives into Gerry's personal legacy and humanity. This book has vivid recollections of Gerry at Stony Brook, Princeton and Copenhagen, together with his humor and his very special intuitive way of thinking.
This volume presents the state-of-the-art in selected topics across modern nuclear physics, covering fields of central importance to research and illustrating their connection to many different areas of physics. It describes recent progress in the study of superheavy and exotic nuclei, which is pushing our knowledge to ever heavier elements and neutron-richer isotopes. Extending nuclear physics to systems that are many times denser than even the core of an atomic nucleus, one enters the realm of the physics of neutron stars and possibly quark stars, a topic that is intensively investigated with many ground-based and outer-space research missions as well as numerous theoretical works. By colliding two nuclei at very high ultra-relativistic energies one can create a fireball of extremely hot matter, reminiscent of the universe very shortly after the big bang, leading to a phase of melted hadrons and free quarks and gluons, the so-called quark-gluon plasma. These studies tie up with effects of crucial importance in other fields. During the collision of heavy ions, electric fields of extreme strength are produced, potentially destabilizing the vacuum of the atomic physics system, subsequently leading to the decay of the vacuum state and the emission of positrons. In neutron stars the ultra-dense matter might support extremely high magnetic fields, far beyond anything that can be produced in the laboratory, significantly affecting the stellar properties. At very high densities general relativity predicts the stellar collapse to a black hole. However, a number of current theoretical activities, modifying Einstein’s theory, point to possible alternative scenarios, where this collapse might be avoided. These and related topics are addressed in this book in a series of highly readable chapters. In addition, the book includes fundamental analyses of the practicalities involved in transiting to an electricity supply mainly based on renewable energies, investigating this scenario less from an engineering and more from a physics point of view. While the topics comprise a large scope of activities, the contributions also show an extensive overlap in the methodology and in the analytical and numerical tools involved in tackling these diverse research fields that are the forefront of modern science.
Nuclear astrophysics as it stands today is a fascinating science. Even though, compared to other scientific fields, it is a young discipline which has developed only in this century, it has answered many questions concerning the under standing of our cosmos. One of these great achievements was the concept of nucleosynthesis, the creation of the elements in the early universe in interstellar matter and in stars. Nuclear astrophysics has continued, to solve many riddles of the evolution of the myriads of stars in our cosmos. This review volume attempts to provide an overview of the current status of nuclear astrophysics. Special emphasis is given to the interdisciplinary nature of the field: astronomy, nuclear physics, astrophysics and particle physics are equally involved. One basic effort of nuclear astrophysics is the collection of ob servational facts with astronomical methods. Laboratory studies of the nuclear processes involved in various astrophysical scenarios have provided fundamen tal information serving both as input for and test of astrophysical models. The theoretical understanding of nuclear reaction mechanisms is necessary, for example, to extrapolate the experimentally determined reaction rates to the thermonuclear energy range, which is relevant for the nuclear processes in our cosmos. Astrophysical models and calculations allow us to simulate how nuclear processes contribute to driving the evolution of stars, interstellar matter and the whole universe. Finally, elementary particle physics also plays an important role in the field of nuclear astrophysics, for instance through weak interaction processes involving neutrinos.
The Carpathian Summer School of Physics 2016 was organized in Sinaia, Romania, as the 27th edition of a tradition that began in 1964. For this two-week, mixed format school-conference, more than 100 students and lecturers gathered to discuss topics pertaining to nuclear physics, nuclear astrophysics, and astroparticle physics, as well as applications of small accelerators. The subject matter ranged from the minute energies of individual nuclear reactions in stars to the gigantic energy releases in supernovae; from sub-nucleonic sizes to the size of the whole universe; from small electrostatic accelerators to new radioactive ion beam facilities; and to the most powerful lasers to be used for nuclear physics.