Cooling

Author:

Minty Michiko G.,Zimmermann Frank

Abstract

AbstractMany applications of particle accelerators require beam cooling, which refers to a reduction of the beam phase space volume or an increase in the beam density via dissipative forces. In electron and positron storage rings cooling naturally occurs due to synchrotron radiation, and special synchrotron-radiation damping rings for the production of low-emittance beams are an integral part of electron-positron linear colliders. For other types of particles different cooling techniques are available. Electron cooling and stochastic cooling of hadron beams are used to accumulate beams of rare particles (such as antiprotons), to combat emittance growth (e.g., due to scattering on an internal target), or to produce beams of high quality for certain experiments. Laser cooling is employed to cool ion beams down to extremely small temperatures. Here the laser is used to induce transitions between the ion electronic states and the cooling exploits the Dopper frequency shift. Electron beams of unprecedentedly small emittance may be obtained by a different type of laser cooling, where the laser beam acts like a wiggler magnet. Finally, designs of a future muon collider rely on the principle of ionization cooling. Reference [1] gives a brief review of the principal ideas and the history of beam cooling in storage rings; a theoretical dicussion and a few practical examples can be found in [2].

Publisher

Springer Berlin Heidelberg

Reference55 articles.

1. D. Möhl: Physica Scripta T22, 21 (1998)

2. D.V. Pestrikov: Beam Cooling. In: Beam Measurements. Proc. US-CERNJapan-Russian School on Beam Measurement, Montreux, Switzerland, 1998, ed. by S.I. Kurokawa, S.Y. Lee, E. Perevedentsev, S. Turner (World Scientific, 2000 )

3. G.I. Budker: Atomnaja Energia 22, 346 (1967)

4. J. Bosser: Electron Cooling. In: Proc. 4th Advanced Accelerator Physics Course, CERN Accelerator School, CERN 92–01, 1992

5. S.P. Moller: Cooling Techniques. In: Proc. CERN Acc. School, Jyvaeskylae 1992, CERN-94–01, 1994

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