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This proceedings contains contributions dealing with the radiative properties of dense plasmas, including radiative transport, opacity, atomic processes, spectroscopy, line-shapes and hydrodynamic behavior. Laser-produced plasmas are a primary focus . The latest experimental and theoretical developments are presented and discussed. New results are reported for plasma opacity modeling, plasma-dependent atomic processes, absorption spectroscopy of laser-produced plasmas, statistical treatments of spectral line clusters, and ultra-short pulse laser-plasma spectroscopy.
This work will be of interest to a wide range of academics. It provides a comprehensive round-up of the proceedings and papers delivered at the 2006 Conference on High Energy Density Laboratory Astrophysics, held at Rice University in Houston, Texas, USA. The contributions come from scientists interested in this emerging field. They discuss the progress in topics covering everything from stellar evolution and envelopes, to opacities, radiation transport and x-ray photoionized plasmas.
These are the proceedings of international conference on Numerical As trophysics 1998 (NAP98), held at National Olympic Memorial Youth Cen ter, in Tokyo, Japan in the period of March 10 - 13, 1998, and hosted by the National Astronomical Observatory, Japan (NAOJ). In the last decade numerical simulations have grown up as a major tool for astrophysics. Numerical simulations give us invaluable informa tion on complex systems and physical processes under extreme conditions which can be neither realized by experiments nor directly observed. Super computers and special purpose computers may work as very large telescopes and special purpose telescopes for theoretical astrophysics, respectively. Nu merical astrophysics ranks with other tool-oriented astronomy such as ra dio astronomy, infrared astronomy, ultraviolet astronomy, X-ray astronomy, and ')'-ray astronomy. This conference, NAP98, was planned to explore recent advances in astrophysics aided by numerical simulations. The subjects of the confer ence included the large-scale structure formation, galaxy formation and evolution, star and planets formation, accretion disks, jets, gravitational wave emission, and plasma physics. NAP98 had also sessions on numerical methods and computer science. The conference was attended by 184 sci entists from 21 countries. We enjoyed excellent talks, posters, videos, and discussions: there are 40 oral presentations, 96 posters and 16 video pre sentations. We hope that these proceedings and accompanying CD-ROM replay the friendly but inspiring atmosphere of the conference.
Neutrino '96 is indispensable for students and researchers of neutrino physics. It contains up-to-date reviews and discussions on topics such as Solar Neutrino Physics, Neutrino Oscillations, Intrinsic Neutrino Properties, and Neutrino Cosmology and Astronomy.
There is general agreement among astrophysicists that most of the matter in the universe is dark, but a wide divergence of views about what this dark matter is. This volume addresses the problem of detecting and identifying dark matter candidates from axions to black holes. Although theoretical issues are considered, the focus of the book is on observational and experimental techniques, current results and future prospects.
Proceedings of the 6th International Workshop on Application of Lasers in Atomic Nuclei Research, LASER 2004, held in Poznan, Poland, 24-27 May, 2004 Blaszczak, Zdzislaw; Marinova, Krassimira; Markov, Boris (Eds.) 2006, ISBN: 3-540-30925-X This volume contains papers presented at the 6th International Workshop on Application of Lasers in Atomic Nuclei Research, LASER 2004, held in Poznan, Poland, 24-27 May, 2004. It should be of interest to researchers and PhD students working or interested in recent results in the nuclear structure investigation by laser spectroscopy and the new generation of experimental laser spectroscopy methods.
Gravitational wave detection is certainly one of the most challenging goals for today's physics. For three decades detectors have improved in sensitivity in order to confirm the existence of these waves, which are predicted by general relativity and other theories of gravitation. Besides testing these theories themselves the detection of gravitational waves will open a new window to observe the Universe — gravitational astronomy — which will be responsible for a great number of the new discoveries in physics, astrophysics and cosmology, and major technological advances in the next millennium. The last generation of detectors is under study now, and it will probably consist of several antennas sensitive to all directions, forming an “omnidirectional gravitational radiation observatory”. This book is a compilation of the papers presented at a recent workshop for this kind of observatory. It includes original works from some of the most active physicists in the field, both experimentalists and theorists, and the present status of the different detectors around the world.
These books presents a wide spectrum of research and development activities in the field of High Pressure Science and Technology. These book provide comprehensive and interdisciplinary descriptions of recent research accomplishments in the biological, chemical, Earth, materrals, physical, physiological and related sciences.