Performance Limiting Effects in X-Band Accelerators
- 1. SLAC National Accelerator Laboratory, Menlo Park, CA, 94025 (United States)
Description
Acceleration gradient is a critical parameter for the design of future TeV-scale linear colliders. The major obstacle to higher gradient in room-temperature accelerators is rf breakdown, which is still a very mysterious phenomenon that depends on the geometry and material of the accelerator as well as the input power and operating frequency. Pulsed heating has been associated with breakdown for many years however there have been no experiments that clearly separate field and heating effects on the breakdown rate. Recently, such experiments have been performed at SLAC with both standing-wave and travelling-wave structures. These experiments have demonstrated that pulsed heating is limiting the gradient. Also, a dual-moded cavity has been designed to better distinguish the electric field, magnetic field and pulsed heating effects on breakdown.
Additional details
Identifiers
- DOI
- 10.1063/1.3520328;
Publishing Information
- Journal Title
- AIP Conference Proceedings
- Journal Volume
- 1299
- Journal Issue
- 1
- Journal Page Range
- p. 280-285
- ISSN
- 0094-243X
- CODEN
- APCPCS
Conference
- Title
- 14. advanced accelerator concepts workshop
- Dates
- 13-19 Jun 2010
- Place
- Annapolis, MD (United States)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 42028840
- Subject category
- S43: PARTICLE ACCELERATORS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ACCELERATION; BREAKDOWN; CAVITY RESONATORS; ELECTRIC FIELDS; HEATING; LINEAR COLLIDERS; MAGNETIC FIELDS; PERFORMANCE; RF SYSTEMS; STANDING WAVES; STANFORD LINEAR ACCELERATOR CENTER; TEV RANGE; TRAVELLING WAVES
- Descriptors DEC
- ACCELERATORS; ELECTRONIC EQUIPMENT; ENERGY RANGE; EQUIPMENT; LINEAR ACCELERATORS; NATIONAL ORGANIZATIONS; RESONATORS; US DOE; US ERDA; US ORGANIZATIONS
Optional Information
- Notes
- (c) 2010 American Institute of Physics