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Space Charge in Isochronous Regime (IR) E. Pozdeyev, BNL* *work partly done at Michigan State University in 2001-2003 (experiments and simulations) together.

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Presentation on theme: "Space Charge in Isochronous Regime (IR) E. Pozdeyev, BNL* *work partly done at Michigan State University in 2001-2003 (experiments and simulations) together."— Presentation transcript:

1 Space Charge in Isochronous Regime (IR) E. Pozdeyev, BNL* *work partly done at Michigan State University in 2001-2003 (experiments and simulations) together with J.A. Rodriguez

2 08/27/08E. Pozdeyev, HB082 Isochronous regime Several types of machines operate / run into IR: –rings for precise nuclear mass spectrometry –some isochronous-optics light sources. –hadron synchrotrons during transition crossing –cyclotrons (FFAG?) Studies of beam dynamics of intense beams around transition have been conducted and documented (including text books, K. Ng) Effect of space charge (SC) on transverse motion and coupling of radial and longitudinal motion must be included in consideration in IR (usually omitted)

3 08/27/08E. Pozdeyev, HB083 Longitudinal impedance at short λ -Long wavelength approximation (includes image charges) -Short wavelength approximation (no image charges) SC impedance peaks at short wavelength: λ m ~2.5 

4 08/27/08E. Pozdeyev, HB084 Transverse SC field Linear charge density modulation => Energy modulation => Radius modulation => Radial electric field x z ErEr ErEr The radial field comes from the snaky shape and can come from image charges. (We neglect images assuming flat vacuum chamber (like in a cyclotron).) The radial field due to snaky shape EzEz Field from a slice ErEr

5 08/27/08E. Pozdeyev, HB085 Dispersion function and slip factor Steady state solution Exactly at the transition If there is dispersion function error, the slip factor is Negative Mass instability below γ tr ?! Sure…

6 08/27/08E. Pozdeyev, HB086 Growth rate with SC in Isoch. Reg. The growth rate for the microwave instability:

7 08/27/08E. Pozdeyev, HB087 BeamH2+H2+ Energy10-30 keV x, y 1.14, 1.11  p – 1/  2 1.7e-4 T 5  sec C6.6 m N turns 100 I peak 0-25  A FFC Small Isochronous Ring (SIR), Circa end of 2003

8 08/27/08E. Pozdeyev, HB088 Beam dynamics simulations in SIR X Z Turn CYCO simulations ( N p =3  10 5 ) Bunch breaks up within a few turns throughout the bunch Contour plot of bunch charge density in median plane for turns 0 to 75 J.A. Rodriguez Ph.D. dissertation, MSU I peak =10 A

9 08/27/08E. Pozdeyev, HB089 Experimental results: Longitudinal beam dynamics Measured longitudinal bunch profile Turn# 10 (fixed), Current increases Vertical axis: peak current measured by Faraday Cup Horizontal axis: arrival time to the Faraday Cup (equivalent to Z)

10 08/27/08E. Pozdeyev, HB0810 Comparison Experiments to Simulations # of clusters as a function of # of turns for 5, 10 and 20 A Simulations Experiments J.A. Rodriguez, Ph.D. dissertation, MSU Simulations included only SC and image charges on the vacuum chamber

11 08/27/08E. Pozdeyev, HB0811 Experimental Results: Scaling with Beam Current I = 5 μA I = 9.9 μAI = 19.9 μA J.A. Rodriguez Ph.D. dissertation, MSU Growth rate depends linearly on the beam current!!! Not as sqrt(I)!!! I 0 (μA)  /  (turn) + SC  (turn) NO SC 5-0.0114.951.3 9.9-0.0232.536.2 19.9-0.0451.326.5

12 08/27/08E. Pozdeyev, HB0812 Simulation results: Dependence on Emittance Simulations: number of clusters vs. turn # for different beam emittance J.A. Rodriguez Ph.D. dissertation, MSU

13 08/27/08E. Pozdeyev, HB0813 Experimental Results: Scaling with Bunch Length T BUNCH = 600 ns T BUNCH = 300 ns T BUNCH = 150 ns J.A. Rodriguez, Ph.D. dissertation, MSU Breakup happens throughout the bunch (no roll-up from the ends as thought by some). Size of clusters and number per unit length does not depend on current.

14 08/27/08E. Pozdeyev, HB0814 7.1  - + E1E1 E2E2 E 2 > E 1 y0y0 Experimental results: Transverse beam dynamics I=20 A, E=17 keV, T=1 sec Energy spread grows from 0 to 5% in 10-20 turns

15 08/27/08E. Pozdeyev, HB0815 Conclusions Effect of space charge (SC) on transverse motion and coupling of radial and longitudinal motion can play a crucial role at IR (usually omitted) This can drive Negative Mass Instability at and below γ tr Simulation results (CYCO) and experimental data (SIR) agree remarkably well They show that –the instability causes very fast beam fragmentation and energy spread growth –the growth rate is proportional to the beam current and inversely proportional to the beam emittance Landau damping most likely exist through modification of the dispersion function non-coherently

16 08/27/08E. Pozdeyev, HB0816 Acknowledgements Special thanks: J.A. Rodriguez, F. Marti, R.C. York J. Bierwagen, D. Cole, D. Devereaux, R. Fontus, S. Hitchcock, D. Lawton, D. Pedtke, D. Sanderson, J. Wagner, A. Zeller, R. Zink Personnel of the NSCL machine, welding, electronic shops, assembly group, computer department, designers and detailers.


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