APS » Journals » Phys. Rev. ST Accel. Beams » Volume 4 » Issue 12
< Previous article | Next article >

Phys. Rev. ST Accel. Beams 4, 124401 (2001)

Intrabeam scattering in electron storage rings

Kiyoshi Kubo and Katsunobu Oide

Download: PDF (104 kB) or gzip'ed PS (97 kB) Export: BibTeX or EndNote (RIS)

(Some reference links may require a separate subscription.)

  1. A. Piwinski, in Proceedings of the 9th International Conference on High Energy Accelerators, Stanford, CA, 1974 (National Technical Information Service, Springfield, VA, 1975), p. 405.
  2. J. Bjorken and S. K. Mtingwa, Part. Accel. 13, 115 (1983) [INSPEC][CAS][SPIRES].
  3. J. L. Duff, in Proceedings of the CERN Accelerator School: Second Advanced Accelerator Physics Course, Berlin, 1987 (CERN, Geneva,1989), p. 573.
  4. K. Kubo, in Proceedings of the 18th International Conference on High Energy Accelerators, Tsukuba, 2001 (Report No. ID TU-02, 2001).
  5. K. Bane et al., in Proceedings of the 2001 Particle Accelerator Conference, Chicago (unpublished).
  6. C. Steier et al., in Proceedings of the 2001 Particle Accelerator Conference, Chicago (unpublished).
  7. A computer code, sad (strategic accelerator design), was developed at KEK; For example, see K Hirata, in Proceedings of the 2nd International Committee for Future Accelerator Beam Dynamics Workshop, Lugano, 1988, edited by E. Keil and J. Hagel (CERN Report No. 88-04, 1988).
  8. For example, James D. Bjorken and Sideny D. Drell, Relativistic Quantum Mechanics (McGraw-Hill, New York,1964).
  9. T. Toyomasu, Part. Accel. 40, 161 (1993) (relativistic effects are considered in this reference) [CAS][SPIRES].
  10. From some equations in Ref. [[2]], this factor appears to be qiξj+qjξi+qiΔj+qjΔi+2qiqj. But this difference has no significance because the odd terms of ξ vanish after the integration.
  11. Here we use σδ instead of ση  =  sqrt[2] σδ, which is used in Ref. [[2]]. In this reference the equation Γunbunch  =  \(2π\)3β3γ3εxεzσησs appears, where εx and εz are the horizontal and vertical emittances and σs is the bunch length. It should be Γunbunch  =  (2π)3β3γ3εxεzσδσs. The difference is by a factor of sqrt[2].
  12. R. T. Farouki and E. E. Salpeter, Astrophys. J. 427, 676 (1994) [SPIN][INSPEC][ADS].
  13. T. Raubenheimer, SLAC Report No. SLAC-387, 1991, Sec. 2.3.1.
  14. T. Raubenheimer, Part. Accel. 45, 111 (1994) [INSPEC][CAS][SPIRES].
  15. K. Ohmi, K. Hirata, and K. Oide, Phys. Rev. E 49, 751 (1994) [SPIN][INSPEC][CAS][SPIRES][MEDLINE].