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Fast cooling of antiproton and radioactive ion beams in future storage rings at GSI

Key issues of the new accelerator facility proposed for GSI are production, fast cooling, and accumulation of intense secondary beams, antiprotons and rare isotopes (RI). Single primary bunches of 2×1013 protons at 29GeV and 1×1012 U28+-ions at 1GeV/u shall be delivered from the new, fast-ramped 100...

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Published in:Nuclear instruments & methods in physics research. Section A, Accelerators, spectrometers, detectors and associated equipment Accelerators, spectrometers, detectors and associated equipment, 2004-10, Vol.532 (1-2), p.97-104
Main Authors: Franzke, B., Beller, P., Beckert, K., Dolinskii, A., Hülsmann, P., Nolden, F., Peschke, C., Steck, M.
Format: Article
Language:English
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Summary:Key issues of the new accelerator facility proposed for GSI are production, fast cooling, and accumulation of intense secondary beams, antiprotons and rare isotopes (RI). Single primary bunches of 2×1013 protons at 29GeV and 1×1012 U28+-ions at 1GeV/u shall be delivered from the new, fast-ramped 100Tm-synchrotron SIS100. A large acceptance, reversible polarity collector ring is foreseen for fast RF debunching followed by fast stochastic pre-cooling in all phase planes. The envisaged total pre-cooling times are 4–5s for antiprotons at 3GeV and 0.5–1s for fully stripped RI at 740MeV/u. A separate accumulator ring RESR is provided for stochastic accumulation of antiprotons. The RI beams are transferred to a new experimental storage Ring NESR, where electron cooling (EC) is applied simultaneously to internal target and electron–ion collision experiments. For experiments with antiprotons, a special 50Tm storage ring HESR shall be equipped with internal target and EC up to 15GeV, optionally also with stochastic beam halo cooling. A maximum luminosity of 2×1032cm−2s−1 and an energy resolution of about 100keV at lower luminosity are main objectives of the HESR concept. Basic issues for the design of the storage ring complex are discussed.
ISSN:0168-9002
1872-9576
DOI:10.1016/j.nima.2004.06.100