Numéro |
J. Phys. IV France
Volume 133, June 2006
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Page(s) | 49 - 55 | |
DOI | https://doi.org/10.1051/jp4:2006133011 | |
Publié en ligne | 16 juin 2006 |
J.-C. Gauthier, et al.
J. Phys. IV France 133 (2006) 49-55
DOI: 10.1051/jp4:2006133011
Advances of dense plasma physics with particle accelerators
D.H.H. Hoffmann1, 2, A. Blazevic1, O.N. Rosmej1, P. Spiller1, N.A. Tahir1, K. Weyrich1, T. Dafni2, M. Kuster2, M. Roth2, S. Udrea2, D. Varentsov2, J. Jacoby3, Zioutas4, 5 and B.Yu. Sharkov61 Gesellschaft für Schwerionenforschung, GSI-Darmstadt, Plasmaphysik, Planckstr. 1, 64291 Darmstadt, Germany
2 Institut für Kernphysik, Technische Universität Darmstadt, Schloßgartenstr. 9, 64289 Darmstadt, Germany
3 Universität Frankfurt, Institut für Angewandte Physik, 6000 Frankfurt, Germany
4 European Organization for Nuclear Research (CERN), Geneve, Switzerland
5 University of Patras, Department of Physics, 26500 Patras, Greece
6 Institut for Theoretical and Experimental Physics ITEP, Moscow 117259, Russia
Abstract
High intensity particle beams from accelerators induce high energy
density states in bulk matter. The SIS-18 heavy ion synchrotron at GSI now
routinely delivers intense Uranium beams that deposit about 1 kJ/g of
specific energy in solid matter, e.g. solid lead. Due to the specific nature
of the ion-matter interaction a volume of matter is heated uniformly with
low gradients of temperature and pressure in the initial phase, depending on
the pulse structure of the beam with respect to space and time. The new
accelerator complex FAIR (Facility for Antiproton and ion Research) at GSI
as well as beams from the CERN large hadron collider (LHC) will vastly
extend the accessible parameter range for high energy density states. One
special piece of accelerator equipment a superconducting high field dipole
magnet, developed for the LHC at CERN is now serving as a key instrument to
diagnose the dense plasma of the sun interior plasma, thus providing an
extremely interesting combination of accelerator physics, plasma physics and
astro-particle physics.
© EDP Sciences 2006