Distribution of Heating from Untrapped HOM Radiation in the LCLS-II Cryomodules
Author(s) -
K. Bane,
C. Nantista,
C. Adolphsen,
T. Raubenheimer,
A. Saini,
N. Solyak,
Vyacheslav Yakovlev
Publication year - 2015
Publication title -
physics procedia
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.26
H-Index - 61
ISSN - 1875-3892
DOI - 10.1016/j.phpro.2015.11.057
Subject(s) - terahertz radiation , beam (structure) , physics , nuclear engineering , range (aeronautics) , power (physics) , radiation , materials science , ceramic , optics , optoelectronics , engineering physics , quantum mechanics , composite material , engineering
The superconducting cavities in the CW linacs of LCLS-II will operate at 2 K, where cooling is very expensive. One source of heat is presented by the higher order mode (HOM) power deposited by the beam. Due to the very short bunch length, especially in the L3 region, the LCLS-II beam spectrum extends into the terahertz range. Ceramic absorbers, at 70 K between cryomodules, are meant to absorb much of this power. In this report we perform two kinds of calculations to estimate the effectiveness of the absorbers and the fractional power that remains to be removed at 2 K
Accelerating Research
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom
Address
John Eccles HouseRobert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom