Rosenzweig 1999 0165
Rosenzweig 1999 0165
Rosenzweig 1999 0165
q f ∂Az
z
1 RF FORCE-DERIVED EMITTANCE ∆pz = ∫ dz , with ζ = z − ct. (2)
In a high gradient rf photoinjector, the necessity of using c z i ∂ζ
violent longitudinal acceleration also implies the existence
of large transverse forces. These forces are time-dependent,
The first term in Eq. 1 vanishes because it is a perfect
and may be nonlinear or non-axisymmetric as well. All of
differential, and the transverse components of the vector
these attributes can give rise to transverse emittance
potential vanish at the cathode, and outside of the cavity.
growth. Time dependent monopole[1] and dipole[2] fields
Thus we have the relation
can cause correlations between the beam’s transverse and
longitudinal phase spaces, which, while not contributing
∂ ( ∆p⊥ ) r
to the so-called slice emittance (the transverse emittance of = ∇ ⊥ ( ∆pz ). (3)
a narrow longitudinal slice of the beam), can increase the ∂ζ
total projected transverse emittance. We shall discuss the
relationship between these emittance contributions and the We consider a multipole standing wave field with a
Panofsky-Wenzel theorem, as well as observations sinusoidal dependence of the phase on distance away from
verifying the conclusions we reach from this analysis. the power coupler,
Nonlinear fields have typically been considered in the
( )
∞
context of the axisymmetric, non-synchronous spatial Ez = E0 sin ωt − κ y y + θ 0 cos(kz ) ∑ an r n cos(nφ ) (4)
harmonics of the rf field. In this paper, we examine the n=0
contribution to synchronous rf multipole fields to the
emittance, and analytically estimate the amplitude of these The asymmetry term inside of the sine function is the
multipoles for rf structure types of interest. We compare phase asymmetry due to power flow (finite Q effect), and
the analytical estimates with experimental evidence and the series expansion is the multipole content of the mode
computer simulations. fields. The vector potential associated with Eq. 4 is
( )
2 PANOFSKY-WENZEL THEOREM E0 ∞
Az = cos ωt − κ y y + θ 0 cos(kz ) ∑ an r n cos(nφ ). (5)
As cavities are designed first and foremost to accelerate, it k n=0
( )
eE0 Lg
∆pz = cos kζ − κ y y pz ( y)c ≅ eE0 Lg (1 + a1 y / k ). (10)
2c
eE0 Lg ( ∆φ )2 ( )
2
κ yy If one measures this asymmetry, then one can determine
≅ 1− − , ∆φ = k∆ζ . (6) a1 , and the expected emittance growth due to dipole kicks
2c 2 2
can be estimated. This was done on a 1.5 cell gun
obtained from BNL at UCLA[4], with a view of the
The transient power flow wave number can be estimated momentum spectrometer shown in Fig. 1. Here the
as κ y ≅ k / Q , where Q is the unloaded quality factor, particles at larger y (actually at large x in the gun, as the
which is of order 10 4 . Thus for reasonable beam size focusing solenoid provides a nearly 90 degree rotation) are
parameters, the effect of the power flow can be neglected. seen to have a smaller momentum in the spectrometer.
4 MULTIPOLE FIELDS
2 σ y ( kσ z ) .
eE0 2
= 13
20
2
(7)
2 me c
2043
Proceedings of the 1999 Particle Accelerator Conference, New York, 1999
the outer wall, but are supported by four rods (the cross- the emittance is ε n, y ≅ 2.3 × 10 −8 m-rad, which is almost
sections of two are shown in Fig. 2). The cell-to cell two orders of magnitude smaller than the expected
coupling in this device is obtained through the annular emittance due to monopole rf and space-charge effects.
region between the disks and the outer wall, and can be On the other hand, for the proposed X-band PWT
very strong, leading to excellent mode separation. The photoinjector[6] under study by a DULY/UCLA/LLNL
external coupling is through the outer wall, and is so far collaboration, the rods must expand by a factor of 50%
from the axis that it does not give rise to significant relative to the disk size in order to provide adequate
dipole components of the field. In fact, the rods, which are cooling water flow. In this case Eq. 11 gives
relatively close the axis, give rise to a dominant octupole a4 a0 ≅ 0.15 cm −4 , while the beam, for 1 nC operation
field perturbation. (as in S-band), is smaller by a factor of 3 in all
We have examined this perturbation both analytically dimensions. In this case, the expected octupole
and through field simulations. The rods effect lasts for the contribution to the normalized emittance is
entire structure, just as the dipole component, and so the ε n, y ≅ 2.1 × 10 −7 m-rad. This is now significant, as it is
normalized emittance in such a long device may be roughly 20% of the design monopole emittance. In
impacted more severely than in a short gun. All of the addition, it implies that it would be unwise to raise the
higher multipole components which have a strong effect charge Q significantly in this device, as this would result
on the beam will have a speed-of-light phase velocity, and octupole-induced emittance scaling[8] as Q 5 / 3 .
thus have a transverse field profile which obeys the
equation ∇ 2⊥ Ez = 0 with solutions as in Eq. 4. The
boundary conditions for the situation with the rods may be
approximated as the field being constant at the rod offset
radius ρ , but dropping to zero in the region of the rods
(which have radius b). Fourier analysis of this rectangular
profile in φ gives the ratio of the octupole to monopole
components of the field,
a4 2 sin( 4b ρ )
≅ 4 (11)
a0 ρ (( 4b ρ ) − π )
x
Figure 3. Calculated contours of constant Ez in S-band
PWT at mid-cell, from GdfidL simulation.
Figure 2. S-band PWT photoinjector cross-section, with 2 _____________________
*
support/cooling rods showing. Work supported by US DoE Contracts DE-FG03-92ER40693 and
DE-FG03-98ER45693.
For the S-band PWT linac, Eq. 11 gives a4 a0 ≅ 10 −3 #
Email: rosenzweig@physics.ucla.edu
+Duly Research.
cm −4 , while the GdfidL 3-D field simulations shown in
Fig. 3 give a4 a0 ≅ 1.3 × 10 −3 cm −4 , which is good
5 REFERENCES
agreement for so rough of a model.
1. K.J.Kim, Nucl. Instr. Methods A 275, 201 (1988)
The effect of the octupole component on the emittance 2. D.T.Palmer, et al., Proc. PAC’97, 2687 (IEEE,1998)
in this device can be estimated as 3. W. K. H. Panofsky and W. A. Wenzel, Rev. Sci. Inst. 27, 967
(1956).
4. J.B. Rosenzweig, et al., NIM A 341, 379 (1994).
3
ε n, y = γ f a4σ 4y σ z , (12) 5.
6.
J. Haimson, private communication.
J.B. Rosenzweig, et al., Proc. PAC’97, 1968 (IEEE, 1998)
14
7. D. Yu, et al., Proc. PAC’97, 2806 (IEEE, 1998)
8. J.B. Rosenzweig and E. Colby, Advanced Accel. Concepts, 724
where we have written it as proportional to the final (AIP Conf. Proc. 335, 1995).
energy γ f me c 2 to emphasize that the emittance is linearly
dependent on the length of the structure. For the 20 MeV
S-band PWT photoinjector at UCLA, σ z = 0.7 mm,
σ y ≅1.5 mm, and the expected octupole contribution to
2044