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Frank Schmidt

Publications -  6
Citations -  27

Frank Schmidt is an academic researcher. The author has contributed to research in topics: Space charge & Thermal emittance. The author has an hindex of 3, co-authored 6 publications receiving 24 citations.

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Improved Methods for the Measurement and Simulation of the CERN SPS Non-linear Optics

TL;DR: In this article, detailed measurements of the SPS non-linear chromaticity and detuning with amplitude have been performed for the two optics configurations presently available for LHC type beams, and the measurement results are used to fit systematic multipole components to the main magnets of the sPS MADX model as a basis for the nonlinear machine model that can be used for beam dynamics simulations.

JACoW : Code bench-marking for long-term tracking and adaptive algorithms

TL;DR: In this paper, the main types of frozen space charge and PIC codes are tested in the framework of the GSI bench-marking suite, in particular the subclass of purely frozen and the adaptive frozen modes both part of MAD-X in comparison with the purely frozen MICROMAP code.

Space Charge Studies with High Intensity Single Bunch Beams in the CERN SPS

TL;DR: In this paper, a detailed study of the dependence of losses, transverse emittance blow-up and transverse beam tail creation as function of the working point is presented for a high brightness single bunch beam with a vertical space charge tune spread of about 0.2 on the 26 GeV injection plateau.

Space Charge effects and mitigation in the CERN PS Booster, in view of the Upgrade

TL;DR: In this article, the authors describe the studies (measure-ments and simulations) that have been carried out to con- firm that the PSB can indeed perform as needed in terms of beam brightness for the future HL-LHC runs.

Machine Development Studies in the CERN PS Booster, in 2016

TL;DR: In this paper, the authors present the outstanding studies performed in 2016 in preparation of the PS Booster upgrade, within the LHC Injector Upgrade project (LIU), to provide twice higher brightness and intensity to the High-Luminosity LHC.