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Transverse Space-Charge Effects in Circular Accelerators

Transverse Space-Charge Effects in Circular Accelerators
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Release: 1968
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The particles in an accelerator interact with one another by electromagnetic forces and are held together by external focusing forces. Such a many-body system has a large number of transverse modes of oscillation (plasma oscillations) that can be excited at characteristic frequencies by errors in the external guide field. In Part I we examine one mode of oscillation in detail, namely the quadrupole mode that is excited in uniformly charged beams by gradient errors. We derive self-consistent equations of motion for the beam envelope and solve these equations for the case in which the space-charge force is much less than the external focusing force, i.e., for strong-focusing synchrotrons. We find that the resonance intensity is shifted from the value predicted by the usual transverse incoherent space-charge limit; moreover, because the space-charge force depends on the shape and size of the beam, the beam growth in always limited. For gradient errors of the magnitude normally present in strong-focusing synchrotrons, the increase in beam size is small provided the beam parameters are properly chosen; otherwise the growth may be large. Thus gradient errors need not impose a limit on the number of particles that can be accelerated. In Part II we examine the other modes of collective oscillation that are excited by machine imperfections. For simplicity we consider only one-dimensional beams that are confined by harmonic potentials, and only small-amplitude oscillations. The linearized Vlasov and Poisson equations are used to find the twofold infinity of normal modes and eigenfrequencies for the stationary distribution that has uniform charge density in real space. In practice, only the low-order modes (the dipole, quadrupole, sextupole, and one or two additional modes) will be serious, and the resonant conditions for these modes are located on a tune diagram. These results, which are valid for all beam intensities, are compared with the known eigenfrequencies for the stationary distribution that has uniform particle density in phase space, and are extrapolated to the Gaussian distribution observed in the Brookhaven AGS.


Space Charge Limits in the AGS Booster

Space Charge Limits in the AGS Booster
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Release: 1987
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Space charge effects are expected to be strong in the AGS booster. The beam intensity may be high enough to cause upsilon-shifts due to space charge of the order of .delta.upsilon approx. .5. In this paper, space charge effects are studied through the use of a tracking program. At each element of the lattice the particles receive a kick which is proportional to the electric field E(subscript x), E/sub y/ produced by the beam and to the length of the element. The beam growth can be studied using the tracking program to track a sample of the particles and to use the growth found in the tracking to find the charge in the beam shape and in the beam size. The techniques used and the assumptions made in studying beam growth are described in the following sections. Using the results found for the beam growth, one can find the space charge limit which is defined as the beam intensity that causes the beam to grow where it reaches the available aperture limits of the accelerator. Space charge limit results are found for the AGS Booster. For a beam of fixed dimensions, which is not growing, the tracking program allows one to compute various effects, some of which are difficult to compute by analytical means. One can compute the space charge upsilon-shift as a function of the particle momentum and as a function of the particle betatron oscillation amplitude. One can also study the effects due to resonances which are excited by magnetic field imperfections or by the field of the beam itself. This study would include the important effect due to the change in the upsilon-values because of changes in the betatron oscillation amplitude. The case of two dimensional motion could also be studied.


Proposal of a Beam Study in the AGS Booster

Proposal of a Beam Study in the AGS Booster
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Total Pages: 17
Release: 1991
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IN order to achieve the design luminosity, the Superconducting Super Collider (SSC) parameter choices emphasize the preservation of the transverse emittance requiring in the collider a normalized transverse emittance of 1 [pi].mm.mrad. A stringent accelerator chain emittance budget must be maintained to achieve the final value. Budgeted emittance specifications for the Low Energy Booster (LEB) include 0.4 [pi].mm.mrad at injection and ≤ 0.6 [pi].mm.mrad at extraction. The space-charge tune shift is expected to be more than 0.5 when the rms normalized emittance of 0.4 [pi].mm.mrad at injection and the total number of particles is 1.1 × 1012 with 1 × 101° particles per bunch. Therefore, it is necessary to cope with a large tune shift and avoid emittance deterioration. We have been studying the beam emittance evolution in the LEB by a multi-particle simulation code with space-charge effects. As reported in the several papers we have obtained from the simulation some new insights into the effects which seem to explain qualitatively a cause of the emittance growth. Even quantitatively, we believe that the simulation can predict the emittance growth as a function of time quite accurately because the code includes most details of the physics processes, such as the adiabatic bunching process and acceleration in the fully 6-D phase space treatment, transverse as well as longitudinal space-charge calculations in a self-consistent manner, and intensity decrease due to particle loss. The purpose of this study is to determine quantitatively the emittance deterioration due to space-charge effects, not to find the maximum current an accelerator could accommodate. Since the charge distribution itself may not remain the same, an accurate measurement of the beam profile is an essential factor of the beam study.


Energy Research Abstracts

Energy Research Abstracts
Author:
Publisher:
Total Pages: 782
Release: 1995
Genre: Power resources
ISBN:

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Space Charge Dominated Beams and Applications of High Brightness Beams

Space Charge Dominated Beams and Applications of High Brightness Beams
Author: S. Y. Lee
Publisher: Springer
Total Pages: 552
Release: 1996
Genre: Science
ISBN:

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Proceedings of the October 1995 workshop on space charge dominated beams, which took a close look at major breakthroughs of the past few years. The workshop results are organized in sections on topics of general interest; experiments with space charge dominated beams and halo formation; statistical