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

Title: Theory and Observations of Microbunching Instability in Electron Machines

Technical Report ·
DOI:https://doi.org/10.2172/813151· OSTI ID:813151

For not very short bunches, the coherent synchrotron radiation (CSR) is usually suppressed by the shielding effect of the conducting walls of the vacuum chamber. However an initial density fluctuation in the beam with a characteristic length much shorter than the bunch length can radiate coherently. If the radiation-reaction force drives growth of the initial fluctuation, one can expect an instability which leads to micro-bunching of the beam and increased coherent radiation at short wavelengths. It has recently been realized that such an instability can play an important role in electron/positron rings where it often manifests itself as a bursting of radiation in the range of hundreds of gigahertz or terahertz. This instability can also be a source of an undesirable emittance growth in bunch compressors used in the next generation short-wavelength FELs. In this paper, we review progress in theoretical studies and numerical simulations of the microbunching instability and show connection of the theory to recent observations in electron machines.

Research Organization:
SLAC National Accelerator Lab., Menlo Park, CA (United States)
Sponsoring Organization:
USDOE Office of Science (US)
DOE Contract Number:
AC03-76SF00515
OSTI ID:
813151
Report Number(s):
SLAC-PUB-9880; TRN: US0303710
Resource Relation:
Other Information: PBD: 27 May 2003
Country of Publication:
United States
Language:
English

Similar Records

Microbunching Instability due to Bunch Compression
Journal Article · Tue Dec 13 00:00:00 EST 2005 · ICFA Beam Dynamics Newsletter · OSTI ID:813151

Microbunch Instability Theory and Simulations
Technical Report · Wed Jan 26 00:00:00 EST 2005 · OSTI ID:813151

The contribution of microbunching instability to solar flare emission in the GHz to THz range of frequencies
Journal Article · Sun Aug 10 00:00:00 EDT 2014 · Astrophysical Journal · OSTI ID:813151