Development of high current Bi and Au beams for the synchrotron operation at the GSI accelerator facility
Creators
- 1. LINAC Group, GSI Helmholtzzentrum fuer Schwerionenforschung GmbH, Darmstadt (Germany)
Description
In this work, the latest results of developing high current ion beams of Au and Bi at GSI facility are described. The difficulties in the production of required charge state in vacuum arc discharge ion sources using the pure materials in the cathodes are discussed. As a possible solution, admix of a small amount of more refractory metal to the cathode material is considered. As a significant result, a dramatic improvement in the production of high charge state Bi ions using the mixed Bi-Cu cathodes (with 8%-15% of Cu admixed) compared to pure Bi cathodes is presented. The preliminary results of investigation of the material structure of Bi-Cu cathodes are discussed. As a next step, it is planned to test the composition of Au with Pd, Zr, and Fe as cathode materials.
Additional details
Identifiers
- DOI
- 10.1063/1.3670743;
Publishing Information
- Journal Title
- Review of Scientific Instruments
- Journal Volume
- 83
- Journal Issue
- 2
- Journal Page Range
- p. 02A505-02A505.4
- ISSN
- 0034-6748
- CODEN
- RSINAK
Conference
- Title
- 14. international conference on ion sources
- Acronym
- ICIS 2011
- Dates
- 12-16 Sep 2011
- Place
- Giardini-Naxos, Sicily (Italy)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 44023079
- Subject category
- S43: PARTICLE ACCELERATORS; S75: CONDENSED MATTER PHYSICS, SUPERCONDUCTIVITY AND SUPERFLUIDITY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ACCELERATOR FACILITIES; BISMUTH IONS; CATHODES; CHARGE STATES; ELECTRIC ARCS; GOLD IONS; ION BEAMS; ION SOURCES; REFRACTORY METALS; SYNCHROTRONS
- Descriptors DEC
- ACCELERATORS; BEAMS; CHARGED PARTICLES; CURRENTS; CYCLIC ACCELERATORS; ELECTRIC CURRENTS; ELECTRIC DISCHARGES; ELECTRODES; ELEMENTS; IONS; METALS
Optional Information
- Notes
- (c) 2012 American Institute of Physics