Optical stochastic cooling for RHIC

M. Babzien; I. Ben-Zvi; I. Pavlishin; I. V. Pogorelsky; V. E. Yakimenko; A. A. Zholents; M. S. Zolotorev

doi:10.1016/j.nima.2004.06.108

Optical stochastic cooling for RHIC

M. Babzien
, I. Ben-Zvi
, I. Pavlishin
, I. V. Pogorelsky
, V. E. Yakimenko
, A. A. Zholents
, M. S. Zolotorev

Physics and Astronomy

Brookhaven National Laboratory
Lawrence Berkeley National Laboratory

Research output: Contribution to journal › Conference article › peer-review

5 Scopus citations

Abstract

We propose the use of an optical parametric amplifier (OPA), with a ∼ 12-μm 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.

Original language	English
Pages (from-to)	345-347
Number of pages	3
Journal	Nuclear Inst. and Methods in Physics Research, A
Volume	532
Issue number	1-2
DOIs	https://doi.org/10.1016/j.nima.2004.06.108
State	Published - Oct 11 2004
Event	International Worshop on Beam Cooling and Related Topics - Lake Yamanaka, Yamanashi, Japan Duration: May 19 2003 → May 23 2003

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10.1016/j.nima.2004.06.108

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title = "Optical stochastic cooling for RHIC",

abstract = "We propose the use of an optical parametric amplifier (OPA), with a ∼ 12-μm 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.",

author = "M. Babzien and I. Ben-Zvi and I. Pavlishin and Pogorelsky, \{I. V.\} and Yakimenko, \{V. E.\} and Zholents, \{A. A.\} and Zolotorev, \{M. S.\}",

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doi = "10.1016/j.nima.2004.06.108",

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journal = "Nuclear Inst. and Methods in Physics Research, A",

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note = "International Worshop on Beam Cooling and Related Topics ; Conference date: 19-05-2003 Through 23-05-2003",

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TY - JOUR

T1 - Optical stochastic cooling for RHIC

AU - Babzien, M.

AU - Ben-Zvi, I.

AU - Pavlishin, I.

AU - Pogorelsky, I. V.

AU - Yakimenko, V. E.

AU - Zholents, A. A.

AU - Zolotorev, M. S.

PY - 2004/10/11

Y1 - 2004/10/11

N2 - We propose the use of an optical parametric amplifier (OPA), with a ∼ 12-μm 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.

AB - We propose the use of an optical parametric amplifier (OPA), with a ∼ 12-μm 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.

UR - https://www.scopus.com/pages/publications/4644282840

U2 - 10.1016/j.nima.2004.06.108

DO - 10.1016/j.nima.2004.06.108

M3 - Conference article

AN - SCOPUS:4644282840

SN - 0168-9002

VL - 532

SP - 345

EP - 347

JO - Nuclear Inst. and Methods in Physics Research, A

JF - Nuclear Inst. and Methods in Physics Research, A

IS - 1-2

T2 - International Worshop on Beam Cooling and Related Topics

Y2 - 19 May 2003 through 23 May 2003

ER -

Optical stochastic cooling for RHIC

Abstract

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