2012/02/07 by C. M. Ginsburg, Camille Ginsburg, Ginsburg, Camille +2
Engineering · Physics and Astronomy · #Accelerator Physics (physics.acc-ph) #FOS: Physical sciences #Particle Accelerators and Free-Electron Lasers #Particle accelerators and beam dynamics #Superconducting Materials and Applications #physics.acc-ph
paper · pdf · doi:10.48550/arxiv.1202.1533
8 pp. Presented at 10th Workshop on Shielding Aspects of Accelerators, Targets and Irradiation Facilities (SATIF-10), CERN, Geneva, Switzerland, 2-4 June, 2010
arxiv created 2012/02/07 · openalex publication_date 2012/02/07 · arxiv updated 2012/02/09 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/01
A semi-empirical method that allows us to predict intensity of generated field emission in superconducting RF cavities is described. Spatial, angular and energy distributions of the generated radiation are calculated with the FISHPACT code. The Monte Carlo code MARS15 is used for modeling the radiation transport in matter. A comparison with dose rate measurements performed in the Fermilab Vertical Test Facility for ILC-type cavities with accelerating gradients up to 35 MV/m is presented as well.