On the symmetry of cylindrical implosions driven by a rotating beam of fast ions
- 1. Institut fuer Theoretische Physik, Universitaet Frankfurt, D-60054 Frankfurt (Germany)
- 2. TU Darmstadt, Institut fuer Kernphysik, Schlossgartenstrasse 9, D-64289 Darmstadt (Germany)
- 3. Gesellschaft fuer Schwerionenforschung, Planckstrasse 1, D-64291 Darmstadt (Germany)
Description
Cylindrical implosions driven by intense beams of heavy ions are one of the promising ways to create high energy density states in matter. To ensure the needed azimuthal symmetry of the beam energy deposition, it was proposed [Sharkov et al., Nucl. Instrum. Methods Phys. Res. A 464, 1 (2001)] to rotate the ion beam around the target axis. Combining analytical calculations with two-dimensional hydrodynamic simulations, a lower limit is established on the frequency ν of the beam rotation dictated by the target hydrodynamics. This limit is shown to be directly proportional to the desired radial convergence ratio Cr for stepwise beam power profiles, and to Cr1/2 for smooth pulses. With a smooth pulse, 6-10 beam revolutions per pulse should be sufficient to reach Cr≅30, while a stepwise pulse requires ≅100 revolutions. Also, the upper bound on the asymmetry of the elliptical focal spot of a rotating ion beam is calculated
Additional details
Identifiers
- DOI
- 10.1063/1.1650352;
Publishing Information
- Journal Title
- Physics of Plasmas
- Journal Volume
- 11
- Journal Issue
- 4
- Journal Page Range
- p. 1577-1588
- ISSN
- 1070-664X
- CODEN
- PHPAEN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 35106068
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- BEAM DYNAMICS; HEAVY IONS; HYDRODYNAMICS; IMPLOSIONS; INERTIAL CONFINEMENT; ION BEAMS; PLASMA SIMULATION; TWO-DIMENSIONAL CALCULATIONS
- Descriptors DEC
- BEAMS; CHARGED PARTICLES; CONFINEMENT; DYNAMICS; FLUID MECHANICS; IONS; MECHANICS; PLASMA CONFINEMENT; SIMULATION
Optional Information
- Notes
- (c) 2004 American Institute of Physics.