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STUDIES OF ENERGY RECOVERY LINACS AT ... - CASA

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tics could not be loaded. Because the quadrupoles were running at strengths<br />

(Emax/Einj) = 51 times smaller than in standard CEBAF operations, scanning the<br />

quadrupole by tens of Gauss has a negligible effect on the emittance measurement<br />

- despite not producing compensatory optics. An expression for the relative change<br />

in the beta functions due to a focusing error is given by [42]<br />

δβ<br />

βo<br />

= ∓ βi<br />

f<br />

47<br />

sin(2∆ψ) (2.15)<br />

where βi is the initial, unperturbed beta function, ∆ψ is the phase advance for a<br />

single revolution in the machine starting from the location of βi, f is the focal length<br />

of the focusing error and the upper (lower) sign applies to the horizontal (vertical)<br />

plane. To first order the betatron phase advances can be determined from the model<br />

optics and are 60 ◦ and 145 ◦ for the vertical and horizontal planes, respectively.<br />

Assuming a focusing error of 150 G (the extent to which each quadrupole was<br />

scanned) gives<br />

δβ<br />

βo<br />

δβ<br />

βo<br />

= −βi<br />

= βi<br />

<br />

<br />

150<br />

sin(2 · 145<br />

33.365 · 1020<br />

◦ ) βi(0.004) (2.16)<br />

<br />

<br />

150<br />

sin(2 · 60<br />

33.365 · 1020<br />

◦ ) βi(0.004) (2.17)<br />

where Eq. (2.16) corresponds to the horizontal plane and Eq. (2.17) corresponds<br />

to the vertical plane. For the first pass beam with an initial unperturbed beta<br />

function of 100 m, the result of the focusing perturbation caused by not producing<br />

compensating optics leads to a contribution of 40 cm to the beta function on the<br />

second pass. Because the beta functions are on the order of 35 m, the contribution<br />

is approximately 1% and can safely be ignored.<br />

Other sources of error include errors in the magnet-to-harp distance, magnet<br />

power supplies, quadrupole excitation calibration, and beam energy. However, the

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