Published June 1, 2011
| Version v1
Journal article
Production And Characterization Of Tungsten-Based Positron Moderators
- 1. Instituto de Fisica, Universidad Nacional Autonoma de Mexico, Apartado Postal 20-364 01000, Mexico DF (Mexico)
Description
Experiments of interest in Atomic Physics require production of well-defined low-energy positron beams through a moderation process of high-energy positrons, which can be produced by either the use of a radioactive source or by accelerator based pair production process. Tungsten is one of the most commonly used moderator materials because of its reasonable efficiency, high work function and relatively low cost. In this work we present different methods to produce tungsten-based candidate moderators in a variety of shapes. We also present results from characterizing these candidate moderators by ion beam analysis and microscopy techniques.
Additional details
Identifiers
- DOI
- 10.1063/1.3586155;
Publishing Information
- Journal Title
- AIP Conference Proceedings
- Journal Volume
- 1336
- Journal Issue
- 1
- Journal Page Range
- p. 524-527
- ISSN
- 0094-243X
- CODEN
- APCPCS
Conference
- Title
- 21. International Conference on the Application of Accelerators in Research and Industry
- Acronym
- CAARI 2010
- Dates
- 8-13 Aug 2010
- Place
- Fort Worth, TX (United States)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 42104911
- Subject category
- S43: PARTICLE ACCELERATORS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ACCELERATORS; ATOMIC PHYSICS; EFFICIENCY; ION BEAMS; MODERATORS; NANOSTRUCTURES; PAIR PRODUCTION; POSITRON BEAMS; POSITRONS; RADIATION SOURCES; TUNGSTEN; WORK FUNCTIONS
- Descriptors DEC
- ANTILEPTONS; ANTIMATTER; ANTIPARTICLES; BEAMS; ELEMENTARY PARTICLES; ELEMENTS; FERMIONS; FUNCTIONS; INTERACTIONS; LEPTON BEAMS; LEPTONS; MATTER; METALS; PARTICLE BEAMS; PARTICLE PRODUCTION; PHYSICS; REFRACTORY METALS; TRANSITION ELEMENTS
Optional Information
- Notes
- (c) 2011 American Institute of Physics