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Accelerator text-books do not have to be rewritten. We haven't found a 'Super'-structure with lower surface fields than acc. gradients (yet) ... – PowerPoint PPT presentation

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Title: Stop the


1
Stop the bruits de couloirs!
  • The quest for a better acc. structure
  • quasi-optical?
  • The résumé in the beginning
  • Physics still holds.
  • Accelerator text-books do not have to be
    rewritten.
  • We havent found a Super-structure with lower
    surface fields than acc. gradients (yet).
  • but the numbers are quite OK for PETS (low r/Q)

In the following, I often normalize to the
frequency (or wavelength). This allows easy
scaling. For comparison, a standard CLIC
structure has iris aperture a/l of 0.2, and a
normalized period length p/l of 1/3. A typical
value for r/Q for the standard structure 25
kW/m, or 250 W/l. A typical ratio surface field
to acc. gradient is 2.5.
2
Bad transit time factor
  • Parameters for this example
  • Shape sphere, centered on axis.
  • f 27.361 GHz, l 10.957 mm
  • b 10.207 mm, b/l 0.932
  • a 8 mm, a/l 0.73
  • p 14 mm, p/l 1.278
  • vg -34.55 c Dj 460
  • r/Q 533.4 W/m 5.845 W/l

gradient 0.132 surface field 0.291
3
strange field maximum under iris!
  • Parameters for this example
  • Shape sphere, centered on axis.
  • f 30.868 GHz, l 9.712 mm
  • b 10.207 mm, b/l 1.051
  • a 8 mm, a/l 0.824
  • p 14 mm, p/l 1.441
  • vg -3.09 c Dj 518
  • r/Q 403.3 W/m 3.917 W/l

gradient 0.093 surface field 0.312
4
Quasi-optical, high vg
  • Parameters for this example
  • Shape sphere, centered on axis.
  • f 43.652 GHz, l 6.868 mm
  • b 10.207 mm, b/l 1.486
  • a 8 mm, a/l 1.165
  • p 14 mm, p/l 2.038
  • vg 67.78 c Dj 733
  • r/Q 27.8 W/m 0.191 W/l

gradient 0.035 surface field 0.63
5
example with moderate aperture 0.65
  • Parameters for this example
  • Shape ellipsoids, centered on axis.
  • f 29.981 GHz, l 10 mm
  • b 9.41 mm, b/l 0.941
  • a 6.5 mm, a/l 0.65
  • p 6.666 mm, p/l 0.6666
  • vg -4.412 c Dj 240
  • r/Q 679.3 W/m 6.793 W/l

gradient 0.159 surface field 0.55
This is similar to the case which fascinated
me.In opposite direction one gets (wrongly)
14.1 kW/m !
6
Inverse problem
  • Different approach
  • Distribute Hertzian dipoles on the axis, spaced
    by the period, and properly phased, but in free
    space.
  • The vector potential has only a z-component and
    can be given analytically.
  • Calculate Er and Ez, and determine a possible
    slope for a metallic wall, i.e. rwall(z) -
    Ez/Er.
  • Choose a starting point and try to integrate to
    get a periodic solution for rwall(z).
  • This is not perfect, but see what I got.
  • Parameters
  • Shape special, from numerical integration.
  • f 30.358 GHz, l 9.875 mm
  • b 10.64 mm, b/l 1.077
  • a 7.679 mm, a/l 0.699
  • p 13.333 mm, p/l 1.35
  • vg 5.556 c Dj 486
  • r/Q 447 W/m 4.414 W/l

gradient 0.122 surface field 0.44
7
Yet another approach ...
  • Start from Maxwells equations, for round,
    periodical solutions. Formulation with space
    harmonics

(normalized to f c e0 m0 l 1, so k0
w 2 p)
8
Space harmonic expansion
  • Like in round waveguides (but not quite ...), we
    can separate r- and z-dependence. The field
    vector (Er, Ej, Ez) looks like

where n runs over the space harmonics and p is
the period. Note that only the space harmonic
zero has net interaction with the beam.
But ... a short period p requires kz 2p n
/ p to be larger than k0. With the separation
condition k02 kr2 kz2 , this requires
imaginary kr. This leads to modified Bessel
functions ...
Remark When separating Maxwells equations for a
round waveguide, you get something similar below
cutoff, but there you require a real kr, so you
you get an imaginary kz, whereas here you require
a real kz, so you get an imaginary kr.
9
Space harmonic expansion radial dependence of
fields
This example is for p 4/3 Note space
harmonic 0 has a constant axial and a linearily
growing radial field! It is similar to a radial
cutoff Space harmonics 1 and 2 have a real kr
10
Can it be done?
  • This describes exactly the fields which are
    required to accelerate particles in round
    periodic structures.
  • It is in closed form, and has only parameters
    a(n) and the period p.
  • The question is
  • playing with a few amplitudes a(n), keeping of
    course a(0) to a maximum
  • can we synthesize a contour, i.e. find a line in
    r-z-plane where
  • 1. we have local linear polarization, i.e. field
    vector does not rotate (Er and Ez are in phase)
  • 2. the tangential E-field vanishes.

Will this lead to structures which are better
than what we have today?
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