Recent results in analysis and simulation of beam halo
Creators
- 1. AOT-1, MS H817 Los Alamos National Laboratory, Los Alamos, New Mexico 87544 (United States)
Description
Understanding and predicting beam halo is a major issue for accelerator driven transmutation technologies. If strict beam loss requirements are not met, the resulting radioactivation can reduce the availability of the accelerator facility and may lead to the necessity for time-consuming remote maintenance. Recently there has been much activity related to the core-halo model of halo evolution [1-5]. In this paper we will discuss the core-halo model in the context of constant focusing channels and periodic focusing channels. We will present numerical results based on this model and we will show comparisons with results from large scale particle simulations run on a massively parallel computer. We will also present results from direct Vlasov simulations
Additional details
Identifiers
- DOI
- 10.1063/1.49173;
Publishing Information
- Journal Title
- AIP Conference Proceedings
- Journal Volume
- 346
- Journal Issue
- 1
- Journal Page Range
- p. 383-389
- ISSN
- 0094-243X
- CODEN
- APCPCS
Conference
- Title
- International conference on accelerator-driven transmutation technologies and applications
- Dates
- 25-29 Jul 1994
- Place
- Las Vegas, NV (United States)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 40034107
- Subject category
- S43: PARTICLE ACCELERATORS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ACCELERATOR DRIVEN TRANSMUTATION; ACCELERATOR FACILITIES; BEAM EMITTANCE; BEAM PRODUCTION; BOLTZMANN-VLASOV EQUATION; COMPARATIVE EVALUATIONS; COMPUTERIZED SIMULATION; FOCUSING; MAINTENANCE; PARTICLE BEAMS; PARTICLE LOSSES; PERIODICITY; RADIOACTIVATION
- Descriptors DEC
- BEAMS; DIFFERENTIAL EQUATIONS; EQUATIONS; EVALUATION; LOSSES; PARTIAL DIFFERENTIAL EQUATIONS; SIMULATION; TRANSMUTATION; VARIATIONS
Optional Information
- Notes
- (c) 1995 American Institute of Physics.