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Space charge effect and the Booster to AGS transfer

 

作者: S. Y. Zhang,  

 

期刊: AIP Conference Proceedings  (AIP Available online 1998)
卷期: Volume 448, issue 1  

页码: 198-209

 

ISSN:0094-243X

 

年代: 1998

 

DOI:10.1063/1.56773

 

出版商: AIP

 

数据来源: AIP

 

摘要:

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. ©1998 American Institute of Physics.

 

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