Emittance Growth in the NLCTA First Chicane | Zendy

Yipeng Sun | Zendy; C. Adolphsen | Zendy

AI Assistant Blog Pricing

Home ZAIA Blog

Open Access

Emittance Growth in the NLCTA First Chicane

Author(s) -

Yipeng Sun,

C. Adolphsen

Publication year - 2011

Publication title -

osti oai (u.s. department of energy office of scientific and technical information)

Language(s) - English

Resource type - Reports

DOI - 10.2172/1022482

Subject(s) - thermal emittance , physics , magnet , dipole , collider , optics , beam (structure) , nuclear physics , quantum mechanics

In this paper, the emittance growth in the NLCTA (Next Linear Collider Test Accelerator) first chicane region is evaluated by simulation studies. It is demonstrated that the higher order fields of the chicane dipole magnet and the dipole corrector magnet (which is attached on the quadrupoles) are the main contributions for the emittance growth, especially for the case with a large initial emittance ({gamma}{epsilon}{sub 0} = 5 {micro}m for instance). These simulation results agree with the experimental observations

The content you want is available to Zendy users.

Already have an account? Click here to sign in.

Having issues? You can contact us here

Accelerating Research