% IMPORTANT: The following is UTF-8 encoded. This means that in the presence % of non-ASCII characters, it will not work with BibTeX 0.99 or older. % Instead, you should use an up-to-date BibTeX implementation like “bibtex8” or % “biber”. @INPROCEEDINGS{Peetermans:607655, author = {Peetermans, Karel and Lemery, Francois and Hillert, Wolfgang and Decking, Winni and Floettmann, Klaus and Trebushinin, Andrei and Wernsmann, Juna and Golubeva, Nina and Lockmann, Nils and Steffen, Bernd and Czwalinna, Marie Kristin and Dohlus, Martin and Zagorodnov, Igor and Richards, Jonah and Giesteira, Filipe and Wohlenberg, Torsten and Mueller, Lukas and Kalendar, Vahit and Thoden, Daniel and Mueller, Lucy and Wichmann, Riko and Walker, Stuart and Guetg, Marc and Liu, Shan and Tomin, Sergey and Qin, Weilun and Long, Tianyun and Bielawski, Serge and Krasilnikov, Mikhail and Geloni, Gianluca and Serkez, Svitozar and Lipka, Dirk and Novokshonov, Artem and Kube, Gero and Hartl, Ingmar and Negodin, Evgeny and Scholz, Matthias}, title = {{STERN}: {S}uperradiant {TH}z {R}adiation {G}eneration at {XFEL}}, school = {DESY}, reportid = {PUBDB-2024-01984}, year = {2024}, abstract = {In order to exploit the full scientific potential of high-energy XFELs (electron energy > 10 GeV), it is necessary to provide adequate pump sources to enable pump-probe science. Users of the European XFEL have requested a THz pump source matching the machine repetition rate (10 Hz burst mode with up to 2700 bunches per burst). In addition, they have demanded a spectral range spanning 0.1-30 THz with a tunable bandwidth to investigate broad and narrow resonances in matter. The EuXFEL $R\&D$ project, STERN, is exploring beam-based radiation generation methods using Cherenkov waveguides and diffraction radiation to satisfy these user requirements. This presentation will provide an overview of radiation generation from Cherenkov waveguides and diffraction sources, including theory, simulation and previous experimental results. We will cover a technical overview of our experimental area including the lattice and vacuum design. We furthermore discuss the collection and transport of the generated THz radiation. Finally, we will mention plans for THz diagnostics to characterize the generated radiation.}, month = {Mar}, date = {2024-03-18}, organization = {DPG spring meeting - Berlin24, Berlin (Germany), 18 Mar 2024 - 22 Mar 2024}, cin = {MXL / FS-LA}, cid = {I:(DE-H253)MXL-20160301 / I:(DE-H253)FS-LA-20130416}, pnm = {621 - Accelerator Research and Development (POF4-621) / 6G13 - Accelerator of European XFEL (POF4-6G13)}, pid = {G:(DE-HGF)POF4-621 / G:(DE-HGF)POF4-6G13}, experiment = {EXP:(DE-H253)XFEL-Exp-20150101 / EXP:(DE-H253)REGAE-20150101}, typ = {PUB:(DE-HGF)6}, url = {https://bib-pubdb1.desy.de/record/607655}, }