Transit-time method of optical stochastic cooling
Author(s) -
M. Zolotorev,
A. Zholents
Publication year - 1994
Publication title -
physical review. e, statistical physics, plasmas, fluids, and related interdisciplinary topics
Language(s) - English
Resource type - Journals
eISSN - 1095-3787
pISSN - 1063-651X
DOI - 10.1103/physreve.50.3087
Subject(s) - transit time , electron , water cooling , laser cooling , transit (satellite) , ion , physics , computational physics , nuclear engineering , statistical physics , atomic physics , mechanics , materials science , nuclear physics , optics , thermodynamics , quantum mechanics , engineering , laser , public transport , transport engineering
In Ref. [1] the utilization of a broadband optical amplifier was proposed for the stochastic cooling process in order to enhance the ultimate possibilities of the conventional microwave stochastic cooling technique [2]. It was shown that the radiation of a particle in a quadrupole wiggler can be amplified and applied back to the same particle in a dipole wiggler, producing therein an energy kick in proportion to the particle's transverse position in the quadrupole wiggler. It was also shown that this scheme is capable of providing damping for both transverse and longitudinal oscillations, but that cooling takes place only in the case of a small beam exnittance & 10 m. We show how to avoid this limitation by using a difFerent approach.
Accelerating Research
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom
Address
John Eccles HouseRobert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom