Bini Simone
TUPR02
Advancements in X-band technology at the TEX facility at INFN-LNF
1421
In anticipation of the Eupraxia@SPARC_LAB project at the INFN Frascati National Laboratories, an intensive testing and validation activity for the X-band RF system has commenced at the TEX test facility. The Eupraxia@SPARC_LAB project entails the development of a Free-Electron Laser (FEL) radiation source with a 1 GeV Linac based on plasma acceleration and an X-band radiofrequency (RF) booster. The booster is composed of 16 high-gradient accelerating structures working at 11.994GHz. All radiofrequency components comprising the basic module of the booster, from the power source to the structure, must undergo testing at nominal parameters and power levels to verify their reliability. For this reason, since 2021, several experimental runs have been conducted to test various components in X-band technology at the TEX facility. This paper presents the results obtained thus far from the different experimental runs, and it also outlines the future upgrade of the facility, which will enhance testing capabilities and the future prospects of the facility itself.
  • F. Cardelli, A. Gallo, A. Liedl, A. Falone, B. Serenellini, B. Buonomo, C. Marta, C. Taruggi, C. Di Giulio, D. Alesini, E. Di Pasquale, G. Catuscelli, G. Luminati, G. Latini, L. Piersanti, L. Spallino, M. Bellaveglia, S. Cantarella, S. Bini, S. Pioli
    Istituto Nazionale di Fisica Nucleare
Paper: TUPR02
DOI: reference for this paper: 10.18429/JACoW-IPAC2024-TUPR02
About:  Received: 15 May 2024 — Revised: 21 May 2024 — Accepted: 21 May 2024 — Issue date: 01 Jul 2024
Cite: reference for this paper using: BibTeX, LaTeX, Text/Word, RIS, EndNote
TUPR10
Preliminary results on X-Band structures for the Eupraxia@SPARC_LAB project
1436
The Eupraxia@SPARC_LAB project involves the development of a 1 GeV normal conducting Linac with an S-band injector followed by an X-band booster. To achieve the final energy, the booster consists of 16 traveling wave accelerating structures operating at 11.994 GHz with a minimum working gradient of 60 MV/m. An intensive design activity, prototyping, and testing of these structures is underway at INFN-LNF. This paper comprehensively presents all the work conducted in the design and prototyping, along with preliminary test results obtained from the first RF prototype of the Eupraxia@SPARC_LAB X-band accelerating structure.
  • F. Cardelli, A. Gallo, A. Iungo, A. Liedl, B. Serenellini, D. Alesini, E. Di Pasquale, G. Di Raddo, G. Latini, L. Piersanti, L. Faillace, M. Bellaveglia, R. Di Raddo, S. Cantarella, S. Bini, S. Pioli, V. Lollo
    Istituto Nazionale di Fisica Nucleare
  • L. Giuliano
    Sapienza University of Rome
  • M. Diomede
    Deutsches Elektronen-Synchrotron
Paper: TUPR10
DOI: reference for this paper: 10.18429/JACoW-IPAC2024-TUPR10
About:  Received: 15 May 2024 — Revised: 21 May 2024 — Accepted: 21 May 2024 — Issue date: 01 Jul 2024
Cite: reference for this paper using: BibTeX, LaTeX, Text/Word, RIS, EndNote
WEPR17
DAFNE operation strategy for the observation of the kaonic deuterium
2504
DAFNE, the Frascati F-factory the collider where the Crab-Waist collision scheme has been implemented and successfully tested, is presently working for a physics program in the field of exotic atoms. The present scientific program foresees the study and the characterization of the never observed before kaonic deuterium. Providing a suitable data sample for such measurement requires the collider to provide the highest flux of k- meson and the lowest possible background shower on the detector. The operation strategy, and the collider setup in terms of collisions and beam dynamics are presented and discussed.
  • C. Milardi, A. Gallo, A. Stecchi, A. Vannozzi, A. Ciarma, A. Liedl, A. Michelotti, A. Stella, A. De Santis, B. Buonomo, C. Di Giulio, D. Quartullo, D. Alesini, E. Di Pasquale, G. Di Pirro, G. Franzini, L. Foggetta, L. Piersanti, M. Boscolo, M. Zobov, M. Behtouei, R. Gargana, R. Ricci, S. Cantarella, S. Bilanishvili, S. Incremona, S. Bini, S. Spampinati, U. Rotundo
    Istituto Nazionale di Fisica Nucleare
  • O. Etisken
    Kirikkale University
  • S. Ozdemir
    Ege University
Paper: WEPR17
DOI: reference for this paper: 10.18429/JACoW-IPAC2024-WEPR17
About:  Received: 15 May 2024 — Revised: 20 May 2024 — Accepted: 23 May 2024 — Issue date: 01 Jul 2024
Cite: reference for this paper using: BibTeX, LaTeX, Text/Word, RIS, EndNote
THPS01
STAR High-Energy Linac status: complete installation acceptance tests
3718
The installation of the STAR High-Energy Linac, the energy upgrade of the Southern European Thomson Back-Scattering Source for Applied Research (STAR) project at the University of Calabria, was conducted by INFN by the end of 2023. This paper presents the testing procedures aimed at confirming the consistency, completeness, and quality of the STAR accelerator upgrade installation (electron beam energy boost from 65 MeV up to 150 MeV). We illustrate the installation and testing of the electrical, hydraulic and related automation and auxiliary systems. We will discuss the high-power commissioning of the two C-band RF power stations and testing of the low-level C-band RF system and control system configuration based on EPICS. Finally, we will describe the layout and testing of the vacuum system, the characterization and commissioning of the magnets with related power supplies and the assessment of the installed diagnostics devices. The linac commissioning as well as electron beam measurements are planned for Summer 2024, due to pending radioprotection authorizations.
  • L. Faillace, A. Esposito, A. Bacci, A. Gallo, A. Vannozzi, A. Ghigo, A. Stella, B. Serenellini, D. Giannotti, D. Alesini, F. Cardelli, F. Chiarelli, F. Broggi, G. Catuscelli, G. Luminati, G. Scarselletta, I. Drebot, J. Beltrano, L. Piersanti, L. Serafini, L. Pellegrino, M. Rossetti Conti, M. Bellaveglia, R. Magnanimi, S. Samsam, S. Vescovi, S. Bini, S. Tocci
    Istituto Nazionale di Fisica Nucleare
  • A. Bravin
    European Synchrotron Radiation Facility
  • A. Puppin, F. Prelz
    Universita' degli Studi di Milano & INFN
  • E. Tassi, R. Agostino, R. Barberi, V. Formoso
    Università della Calabria
  • E. Puppin
    Politecnico/Milano
  • G. D'Auria
    Elettra-Sincrotrone Trieste S.C.p.A.
  • V. Petrillo
    Universita' degli Studi di Milano
Paper: THPS01
DOI: reference for this paper: 10.18429/JACoW-IPAC2024-THPS01
About:  Received: 15 May 2024 — Revised: 20 May 2024 — Accepted: 23 May 2024 — Issue date: 01 Jul 2024
Cite: reference for this paper using: BibTeX, LaTeX, Text/Word, RIS, EndNote