45 th ICFA Beam Dynamic Workshop June 8–12, 2009, Cornell University, Ithaca New York Modeling Cyclotron Resonances in ECLOUD Jim Crittenden Cornell Laboratory.

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Presentation transcript:

45 th ICFA Beam Dynamic Workshop June 8–12, 2009, Cornell University, Ithaca New York Modeling Cyclotron Resonances in ECLOUD Jim Crittenden Cornell Laboratory for Accelerator-Based Sciences and Education CTA09 CesrTA Electron Cloud R&D Program for Linear Collider Damping Rings 25 June 2009 CTA09 Cornell University, June 2009

25 June 2009 Modeling Cyclotron Resonances in ECLOUD / J.A.Crittenden 2/14 June 2009 CesrTA Measurements See talk by Joe Calvey, CTA09 4 ns, 2 GeV TiN, Collector 1 Al, Collector 1 TiN, Collector 9 Al, Collector 9

25 June 2009 Modeling Cyclotron Resonances in ECLOUD / J.A.Crittenden 3/14 45 e + bunches, 4-ns spacing, 0.9 mA/bunch Resonance more clear with cylindrical vacuum chamber. Slight offset from n= inch cylindrical v.c.  p.e./e +  100% reflectivity  max = 2.0 E peak = 310 eV I b = 1.44e10 e + /bunch (0.9 mA)

25 June 2009 Modeling Cyclotron Resonances in ECLOUD / J.A.Crittenden 4/14 Azimuthal Distribution on Vacuum Chamber Wall Compare n = 0.5 with n = 1.0 Peaks at top and bottom of chamber more spread out on resonance. Corresponds to bigger effect for collector 1 than collector 9. The RFA covers radians (+-36 degrees). n=0.5 n=1.0 Azimuthal Angle (radians)

25 June 2009 Modeling Cyclotron Resonances in ECLOUD / J.A.Crittenden 5/14 Angle of Incidence on Vacuum Chamber Wall Compare n = 0.5 with n = 1.0 Angles of incidence on wall more glancing on resonance. Consequences for RFA acceptance. More secondary yield in any case. n=0.5 n=1.0

25 June 2009 Modeling Cyclotron Resonances in ECLOUD / J.A.Crittenden 6/14 Kinetic Energy Distribution on Vacuum Chamber Wall Compare n=0.5 with n=1.0 Higher energies on resonance. n=0.5 n=1.0

25 June 2009 Modeling Cyclotron Resonances in ECLOUD / J.A.Crittenden 7/14 Population of SEY Curve Compare n=0.5 with n=1.0 n=0.5 n=1.0 Higher yields on resonance. Higher energies and more grazing angles. ECLOUD SEY model sets cos  < 0.2 to cos  = 0.2 for yield calculation (78 degrees).

25 June 2009 Modeling Cyclotron Resonances in ECLOUD / J.A.Crittenden 8/14 ECLOUD Magnetic Field Scan Choose azimuthal bins corresponding to the chicane RFA collectors. ECLOUD sees the resonances! NB: The RFA transparency has been accounted for, but no correction has been made for either angles of incidence or cyclotron radius.

25 June 2009 Modeling Cyclotron Resonances in ECLOUD / J.A.Crittenden 9/14 What about the TiN minima? Thanks to Mauro for these SEY curves. Since the peak energy is so high, the resonant enhancement of the energy will not suffice to produce the reduction in yield necessary to produce the minima. So I investigated the ECLOUD option to independently set the yield at low energy. I scanned through values 0.6, 0.8, 1.0,1.2 and found that a value of 1.0 produces maxima for Al and minima for TiN most clearly. Other values may do so as well. F. Le Pimpec, R. Kirby, F. King and M. Pivi Nucl. Instr. and Meth. NIM A 551 (2005)

25 June 2009 Modeling Cyclotron Resonances in ECLOUD / J.A.Crittenden 10/14 Scan over n=1 for Al and TiN with d (0)=1.0 ECLOUD can produce maxima for Al and minima for TiN for the same value of the yield at low energy d (0)=1.0 Al: d peak = 2.0 E peak = 310 eVTiN: d peak = 0.95 E peak = 500 eV

25 June 2009 Modeling Cyclotron Resonances in ECLOUD / J.A.Crittenden 11/14 ECLOUD Secondary Yield Distribution for TiN The SEY curve for TiN results in a low yield region being populated by the resonant energy enhancement. Off resonanceOn resonance

25 June 2009 Modeling Cyclotron Resonances in ECLOUD / J.A.Crittenden 12/14 Scan n=1,2,3,4 for Al and TiN with d (0)=1.0 Sum of 17 Collectors ECLOUD can produce maxima for Al and minima for TiN for the same value of the yield at low energy d (0)=1.0 Al: d peak = 2.0 E peak = 310 eVTiN: d peak = 0.95 E peak = 500 eV

25 June 2009 Modeling Cyclotron Resonances in ECLOUD / J.A.Crittenden 13/14 Scan n=1,2,3,4 for Al and TiN with d (0)=1.0 Collectors 1 and 9 Collectors 1 and 9 show the resonances less clearly. Al: d peak = 2.0 E peak = 310 eVTiN: d peak = 0.95 E peak = 500 eV

25 June 2009 Modeling Cyclotron Resonances in ECLOUD / J.A.Crittenden 14/14 Conclusions The cyclotron resonances provide a means of mapping out the energy dependence of the secondary yield without varying the bunch current. Much work remains to be done.