COOL2023 - List of Authors (Hall, C.C.)

Paper	Title	Page
TUPPM1R3	Numerical Study of the Wiggler-Based Microbunching Amplifier for EIC	26
	A.A. Zholents ANL, Lemont, Illinois, USA C.C. Hall RadiaSoft LLC, Boulder, Colorado, USA
	Funding: Supported by the Director, Office of Science, Office of Basic Energy Sciences, of the U.S. Department of Energy under Contract No. DE-AC02- 06CH11357. Coherent electron cooling* using a plasma-cascade amplifier (PCA) can provide significantly faster cooling of hadrons than the conventional microwave stochastic cooling due to a wide bandwidth of a pickup, a kicker, and an amplifier. The PCA creates unstable plasma oscillations by modulating the plasma frequency by varying the transverse beam size along the beam line. An alternative approach to the amplifier studied in this work is to modulate the plasma frequency by a sequence of wiggler magnets separated by weak chicanes. We present a new derivation of the amplifier spectral gain function following the initial analysis presented in . Numerical simulations of the gain function were also done using electron beam parameters projected for the Electron Ion Collider. The numerical results consistently show higher gains than those obtained using the analytical gain function. V. Litvinenko, Ya. Derbenev, Phys. Rev. Lett., 102, (2009)114801. V. Litvinenko et al., Phys. Rev. Accel. Beams, 24, (2021)014402. * G. Stupakov, A. Zholents, COOL2021
	Slides TUPPM1R3 [3.136 MB]
DOI •	reference for this paper ※ doi:10.18429/JACoW-COOL2023-TUPPM1R3
About •	Received ※ 28 September 2023 — Revised ※ 11 October 2023 — Accepted ※ 13 October 2023 — Issued ※ 02 December 2023
Cite •	reference for this paper using ※ BibTeX, ※ LaTeX, ※ Text/Word, ※ RIS, ※ EndNote (xml)

Paper

Title

Page

Numerical Study of the Wiggler-Based Microbunching Amplifier for EIC

26

A.A. Zholents
ANL, Lemont, Illinois, USA
C.C. Hall
RadiaSoft LLC, Boulder, Colorado, USA

Funding: Supported by the Director, Office of Science, Office of Basic Energy Sciences, of the U.S. Department of Energy under Contract No. DE-AC02- 06CH11357.
Coherent electron cooling* using a plasma-cascade amplifier (PCA)** can provide significantly faster cooling of hadrons than the conventional microwave stochastic cooling due to a wide bandwidth of a pickup, a kicker, and an amplifier. The PCA creates unstable plasma oscillations by modulating the plasma frequency by varying the transverse beam size along the beam line. An alternative approach to the amplifier studied in this work is to modulate the plasma frequency by a sequence of wiggler magnets separated by weak chicanes. We present a new derivation of the amplifier spectral gain function following the initial analysis presented in ***. Numerical simulations of the gain function were also done using electron beam parameters projected for the Electron Ion Collider. The numerical results consistently show higher gains than those obtained using the analytical gain function.
* V. Litvinenko, Ya. Derbenev, Phys. Rev. Lett., 102, (2009)114801.
** V. Litvinenko et al., Phys. Rev. Accel. Beams, 24, (2021)014402.
*** G. Stupakov, A. Zholents, COOL2021

Slides TUPPM1R3 [3.136 MB]

DOI •

reference for this paper ※ doi:10.18429/JACoW-COOL2023-TUPPM1R3

About •

Received ※ 28 September 2023 — Revised ※ 11 October 2023 — Accepted ※ 13 October 2023 — Issued ※ 02 December 2023

Cite •

reference for this paper using ※ BibTeX, ※ LaTeX, ※ Text/Word, ※ RIS, ※ EndNote (xml)