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Title: Transverse Microwave Convective Instability at Transition Crossing

Abstract

An analytical model of transverse convective instability of a bunch at transition crossing is presented for the microwave case, when the wake is sufficiently short compared with the bunch length. The space charge is assumed to be strong, as it typically is for the low and medium energy synchrotrons. A simple formula for the intensity threshold is obtained and its prediction is compared with available CERN PS data; without a single fitting parameter, a good agreement is demonstrated.

Authors:
ORCiD logo [1]
  1. Fermilab
Publication Date:
Research Org.:
Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
Sponsoring Org.:
USDOE Office of Science (SC), High Energy Physics (HEP) (SC-25)
OSTI Identifier:
1573829
Report Number(s):
arXiv:1908.02916; FERMILAB-PUB-19-394-AD-APC
oai:inspirehep.net:1748620
DOE Contract Number:  
AC02-07CH11359
Resource Type:
Journal Article
Journal Name:
TBD
Additional Journal Information:
Journal Name: TBD
Country of Publication:
United States
Language:
English
Subject:
43 PARTICLE ACCELERATORS

Citation Formats

Burov, Alexey. Transverse Microwave Convective Instability at Transition Crossing. United States: N. p., 2019. Web.
Burov, Alexey. Transverse Microwave Convective Instability at Transition Crossing. United States.
Burov, Alexey. Wed . "Transverse Microwave Convective Instability at Transition Crossing". United States. https://www.osti.gov/servlets/purl/1573829.
@article{osti_1573829,
title = {Transverse Microwave Convective Instability at Transition Crossing},
author = {Burov, Alexey},
abstractNote = {An analytical model of transverse convective instability of a bunch at transition crossing is presented for the microwave case, when the wake is sufficiently short compared with the bunch length. The space charge is assumed to be strong, as it typically is for the low and medium energy synchrotrons. A simple formula for the intensity threshold is obtained and its prediction is compared with available CERN PS data; without a single fitting parameter, a good agreement is demonstrated.},
doi = {},
journal = {TBD},
number = ,
volume = ,
place = {United States},
year = {2019},
month = {8}
}