Space charge effect and the Booster to AGS transfer

Details Space charge effect and the Booster to AGS transfer Space charge effect and the Booster to AGS transfer

Nov 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aipc..448..198z&link_type=abstract

Workshop on space charge physics in high intensity hadron rings. AIP Conference Proceedings, Volume 448, pp. 198-209 (1998).

Physics

Synchrotrons, Beam Dynamics, Collective Effects And Instabilities, Beam Handling, Beam Transport

Scientific paper

For high intensity proton runs, emittance blow-up is often accompanied with nontrivial beam loss. It has been suggested [10] that the largest portion of the Booster to AGS (BTA) transfer loss is located in the AGS end. It was also found that the space charge tune spread, immediately after the bunched beam enters the AGS ring, is large enough for the envelope resonance and emittance blow-up [11]. It was decided, in 1997 high intensity proton run, to raise the BTA transfer kinetic energy from 1.54 GeV to 1.9 GeV. The transfer efficiency was increased, as expected. The beam emittance in the AGS ring did not increase, even the AGS acceptance was enlarged [12], which is probably because of the reduced space charge tune spread.

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