Title of article
Optical stochastic cooling for RHIC
Author/Authors
Babzien، نويسنده , , M. and Ben-Zvi، نويسنده , , I. and Pavlishin، نويسنده , , I. and Pogorelsky، نويسنده , , I.V. and Yakimenko، نويسنده , , V.E. and Zholents، نويسنده , , A.A and Zolotorev، نويسنده , , M.S.، نويسنده ,
Pages
3
From page
345
To page
347
Abstract
We propose the use of an optical parametric amplifier (OPA), with a ∼ 12 - μ m on wavelength for optical stochastic cooling (Phys. Rev. Lett. 71 (1993) 4146; Phys. Rev. E 50 (1994) 3087) of gold ions in the relativistic heavy ion collider. The use of infrared wavelengths in comparison with the visible ensures a higher efficiency interaction of heavy ions withlight in the kicker undulator. The transition to longer wavelength also relaxes the requirements for stability of the path length during ion-beam transport between pickup and kicker.
Journal title
Astroparticle Physics
Record number
2024567
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