Non-linear beam dynamics in an RFQ under 3D space charge and image charge effects

1993 ◽  
Vol 106 (11) ◽  
pp. 1531-1535 ◽  
Author(s):  
Y. Oguri ◽  
M. Okamura ◽  
T. Hattori ◽  
O. Takeda ◽  
K. Satoh
2014 ◽  
Vol 38 (3) ◽  
pp. 037005 ◽  
Author(s):  
Chao Li ◽  
Zhi-Lei Zhang ◽  
Xin Qi ◽  
Xian-Bo Xu ◽  
Yuan He ◽  
...  

2019 ◽  
Vol 37 (01) ◽  
pp. 38-48
Author(s):  
B. Nayak ◽  
S. Krishnagopal

AbstractHigh-intensity electron linacs have severe space-charge effects that lead to the production of beam halo which degrade the beam quality. For a given charge per bunch, hollow beams have a weaker nonlinear space-charge force. In this paper, we have investigated the possibility of using hollow beam to control halo growth in linacs. We simulate the dynamics of such a beam in a 17 MeV radio frequency linac using ASTRA beam dynamics code and show that it experiences a smaller emittance growth as well as reduced beam halo. The results suggest that using a hollow beam, high charge per bunch could be propagated and accelerated in a radio frequency linac.


2007 ◽  
Vol 22 (22) ◽  
pp. 4000-4005 ◽  
Author(s):  
S. B. VAN DER GEER ◽  
O. J. LUITEN ◽  
M. J. DE LOOS

Because uniformly filled ellipsoidal ‘waterbag’ bunches have linear self-fields in all dimensions, they do not suffer from space-charge induced brightness degradation. This in turn allows very efficient longitudinal compression of high-brightness bunches at sub or mildly relativistic energies, a parameter regime inaccessible up to now due to detrimental effects of non-linear space-charge forces. To demonstrate the feasibility of this approach, we investigate ballistic bunching of 1 MeV, 100 pC waterbag electron bunches, created in a half-cell rf-photogun, by means of a two-cell booster-compressor. Detailed GPT simulations of this table-top set-up are presented, including realistic fields, 3D space-charge effects, path-length differences and image charges at the cathode. It is shown that with a single 10MW S-band klystron and fields of 100 MV/m, 2kA peak current is attainable with a pulse duration of only 30 fs at a transverse normalized emittance of 1.5 μm.


Instruments ◽  
2021 ◽  
Vol 5 (1) ◽  
pp. 9
Author(s):  
Sandro Palestini

The subject of space charge in ionization detectors is reviewed, showing how the observations and the formalism used to describe the effects have evolved, starting with applications to calorimeters and reaching recent, large time-projection chambers. General scaling laws, and different ways to present and model the effects are presented. The relations between space-charge effects and the boundary conditions imposed on the side faces of the detector are discussed, together with a design solution that mitigates some of the effects. The implications of the relative size of drift length and transverse detector size are illustrated. Calibration methods are briefly discussed.


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