skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Coherent wiggler radiation impedance at the storage ring cooler for the EIC project

Technical Report ·
DOI:https://doi.org/10.2172/1888293· OSTI ID:1888293
 [1];  [1];  [2]
  1. Brookhaven National Lab. (BNL), Upton, NY (United States)
  2. KEK, High Energy Accelerator Organization, Tsukuba (Japan)

The Electron Ion Collider project is presently under design at Brookhaven National Laboratory. One of the options how to achieve an electron-proton high-luminosity of 1034 cm–2 s–1 range, is the storage ring cooler concept, which is based on employing a significant amount of the damping wigglers. One of the main concerns, in achieving the required beam parameters, is the collective effects, especially the coherent synchrotron radiation impedance produced by the damping wigglers and its effect on the longitudinal beam dynamics. Low energy of the electrons, Eo=149.6 MeV, small vacuum chamber aperture, b=15 mm, small bending radius and a big number of poles make the coherent synchrotron radiation simulations for the damping wiggler with D. Zhou’s CSRZ code, pretty challenging. The obtained numerical results have been compare with a theoretical approach of Stupakov and Zhou. The strong narrow-band impedance, due to a presence of the periodic poles and the vacuum chamber, have been identified and classified. To suppress or detune the high-Q resonance peaks, a design of the damping wiggler with a varied period of length is presented and discussed.

Research Organization:
Brookhaven National Laboratory (BNL), Upton, NY (United States)
Sponsoring Organization:
USDOE Office of Science (SC), Nuclear Physics (NP)
DOE Contract Number:
SC0012704
OSTI ID:
1888293
Report Number(s):
EIC-ADD-TN-34; BNL-223400-2022-TECH; TRN: US2308986
Country of Publication:
United States
Language:
English

Similar Records

Microwave instability threshold from coherent wiggler radiation impedance in storage rings
Journal Article · Wed May 17 00:00:00 EDT 2023 · Physical Review Accelerators and Beams · OSTI ID:1888293

New wiggler beam line for SSRL
Conference · Sun Aug 01 00:00:00 EDT 1982 · OSTI ID:1888293

Impact of the Wiggler Coherent Synchrotron Radiation Impedance on the Beam Instability
Technical Report · Tue May 27 00:00:00 EDT 2003 · OSTI ID:1888293

Related Subjects