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2 - CERN Accelerator School

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The solution of the system is<br />

Scattering through thin foil -<br />

VI<br />

This can be solved exactly, or by assuming that the<br />

relative emittance growth is small, then<br />

emittance growth is now only half<br />

π<br />

Δε<br />

rms = θ 2β<br />

rms 0<br />

4<br />

1, β1<br />

Twiss<br />

⎡<br />

⎤<br />

⎢ π θ 2 ⎥<br />

β = β ⎢1−<br />

rms<br />

1 0<br />

⎥<br />

⎢ 4 ε ⎥<br />

⎢⎣<br />

rms ⎥⎦<br />

NB: NB: the the emittance<br />

growth is now only half<br />

of of the the previous estimate!<br />

Downstream of of the the foil foil the the transfer line<br />

line<br />

should be be matched using the the new new Twiss<br />

parameters α1, α1, β1<br />

Massimo Giovannozzi CAS - 2-14 14 October 2005 11<br />

A<br />

β1<br />

β<br />

0<br />

2<br />

1<br />

2<br />

=<br />

−<br />

A<br />

2<br />

0<br />

A<br />

A<br />

A<br />

2<br />

0<br />

2<br />

0<br />

2<br />

1<br />

2<br />

=<br />

2β<br />

0<br />

θ<br />

2<br />

rms

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