Two-dimensional axisymmetric Child-Langmuir scaling law
- 1. Applied Science and Technology, University of California, Berkeley, California 94720 (United States)
- 2. Nuclear Engineering, University of California, Berkeley, California 94720 (United States)
Description
The classical one-dimensional (1D) Child-Langmuir law was previously extended to two dimensions by numerical calculation in planar geometries. By considering an axisymmetric cylindrical system with axial emission from a circular cathode of radius r, outer drift tube radius R>r, and gap length L, we further examine the space charge limit in two dimensions. Simulations were done with no applied magnetic field as well as with a large (100 T) longitudinal magnetic field to restrict motion of particles to 1D. The ratio of the observed current density limit JCL2 to the theoretical 1D value JCL1 is found to be a monotonically decreasing function of the ratio of emission radius to gap separation r/L. This result is in agreement with the planar results, where the emission area is proportional to the cathode width W. The drift tube in axisymmetric systems is shown to have a small but measurable effect on the space charge limit. Strong beam edge effects are observed with J(r)/J(0) approaching 3.5. Two-dimensional axisymmetric electrostatic particle-in-cell simulations were used to produce these results.
Additional details
Identifiers
- DOI
- 10.1063/1.3243474;
Publishing Information
- Journal Title
- Physics of Plasmas
- Journal Volume
- 16
- Journal Issue
- 10
- Journal Page Range
- p. 103102-103102.6
- ISSN
- 1070-664X
- CODEN
- PHPAEN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 41021650
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- AXIAL SYMMETRY; CATHODES; CURRENT DENSITY; EMISSION; PLASMA SIMULATION; SCALING LAWS; SPACE CHARGE; TWO-DIMENSIONAL CALCULATIONS
- Descriptors DEC
- ELECTRODES; SIMULATION; SYMMETRY
Optional Information
- Notes
- (c) 2009 American Institute of Physics