Journal article
Radio frequency and DC high voltage breakdown of high pressure helium, argon, and xenon
Journal of instrumentation, Vol.15(4), pp.P04022-P04022
04/01/2020
DOI: 10.1088/1748-0221/15/04/P04022
Abstract
Motivated by the possibility of guiding daughter ions from double beta decay events to single-ion sensors for barium tagging, the NEXT collaboration is developing a program of R&D to test radio frequency (RF) carpets for ion transport in high pressure xenon gas. This would require carpet functionality in regimes at higher pressures than have been previously reported, implying correspondingly larger electrode voltages than in existing systems. This mode of operation appears plausible for contemporary RF-carpet geometries due to the higher predicted breakdown strength of high pressure xenon relative to low pressure helium, the working medium in most existing RF carpet devices. In this paper we present the first measurements of the high voltage dielectric strength of xenon gas at high pressure and at the relevant RF frequencies for ion transport (in the 10MHz range), as well as new DC and RF measurements of the dielectric strengths of high pressure argon and helium gases at small gap sizes. We find breakdown voltages that are compatible with stable RF carpet operation given the gas, pressure, voltage, materials and geometry of interest.
Details
- Title: Subtitle
- Radio frequency and DC high voltage breakdown of high pressure helium, argon, and xenon
- Creators
- K. Woodruff - The University of Texas at ArlingtonJ. Baeza-Rubio - The University of Texas at ArlingtonD. Huerta - The University of Texas at ArlingtonB. J. P. Jones - The University of Texas at ArlingtonA. D. McDonald - The University of Texas at ArlingtonL. Norman - The University of Texas at ArlingtonD. R. Nygren - The University of Texas at ArlingtonC. Adams - Harvard UniversityV. Alvarez - Instituto de Física CorpuscularL. Arazi - Ben-Gurion University of the NegevI. J. Arnquist - Pacific Northwest National LaboratoryC. D. R. Azevedo - University of AveiroK. Bailey - Argonne National LaboratoryF. Ballester - Instituto de Instrumentación para Imagen MolecularJ. M. Benlloch-Rodriguez - Instituto de Física CorpuscularF. I. G. M. Borges - University of CoimbraN. K. Byrnes - The University of Texas at ArlingtonS. Carcei - Universitat de ValènciaJ. V. Carrion - Instituto de Física CorpuscularS. Cebrian - Universidad de ZaragozaE. Church - Pacific Northwest National LaboratoryC. A. N. Conde - University of CoimbraT. Contreras - Harvard UniversityA. A. Denisenko - The University of Texas at ArlingtonG. Diaz - Donostia International Physics CenterJ. Diaz - Instituto de Física CorpuscularM. Diesburg - Fermi National Accelerator LaboratoryJ. Escada - University of CoimbraR. Esteve - Instituto de Instrumentación para Imagen MolecularR. Felkai - Instituto de Física CorpuscularA. F. M. Fernandes - University of CoimbraL. M. P. Fernandes - University of CoimbraP. Ferrario - IkerbasqueA. L. Ferreira - University of AveiroF. W. Foss - The University of Texas at ArlingtonE. D. C. Freitas - University of CoimbraJ. Generowicz - Donostia International Physics CenterA. Goldschmidt - Lawrence Berkeley National LaboratoryD. Gonzalez-Diaz - Universidade de Santiago de CompostelaJ. J. Gomez-Cadenas - IkerbasqueS. Ghosh - Harvard UniversityR. Guenette - Harvard UniversityR. M. Gutierrez - Universidad Antonio NariñoJ. Haefner - Harvard UniversityK. Hafidi - Argonne National LaboratoryJ. Hauptman - Iowa State UniversityC. A. O. Henriques - University of CoimbraJ. A. Hernando Morata - Universidade de Santiago de CompostelaP. Herrero - Donostia International Physics CenterV. Herrero - Instituto de Instrumentación para Imagen MolecularS. Johnston - Argonne National LaboratoryM. Kekic - Instituto de Física CorpuscularL. Labarga - Universidad Autónoma de MadridA. Laing - The University of Texas at ArlingtonP. Lebrun - Fermi National Accelerator LaboratoryN. Lopez-March - Instituto de Física CorpuscularM. Losada - Universidad Antonio NariñoR. D. P. Mano - University of CoimbraJ. Martin-Albo - Harvard UniversityA. Martinez - Donostia International Physics CenterG. Martinez-Lema - Instituto de Física CorpuscularF. Monrabal - Donostia International Physics CenterC. M. B. Monteiro - University of CoimbraF. J. Mora - Instituto de Instrumentación para Imagen MolecularJ. Munoz Vidal - Donostia Int Phys Ctr DIPC, Paseo Manuel Lardizabal 4, E-20018 Donostia San Sebastian, SpainP. Novella - Instituto de Física CorpuscularB. Palmeiro - Instituto de Física CorpuscularA. Para - Fermi National Accelerator LaboratoryJ. Perez - Instituto de Física CorpuscularM. Querol - Instituto de Física CorpuscularJ. Renner - Instituto de Física CorpuscularJ. Repond - Argonne National LaboratoryS. Riordan - Argonne National LaboratoryL. Ripoll - Universitat de GironaY. Rodriguez Garcia - Univ Antonio Narino, Ctr Invest Ciencias Basicas & Aplicadas, Carretera 3 Este 47 A-15, Bogota, ColombiaJ. Rodriguez - Instituto de Instrumentación para Imagen MolecularL. Rogers - The University of Texas at ArlingtonB. Romeo - Donostia International Physics CenterC. Romo-Luque - Instituto de Física CorpuscularF. P. Santos - University of CoimbraJ. M. F. dos Santos - University of CoimbraA. Simon - Ben-Gurion University of the NegevC. Sofka - Texas A&M UniversityM. Sorel - Instituto de Física CorpuscularT. Stiegler - Texas A&M UniversityP. Thapa - The University of Texas at ArlingtonJ. F. Toledo - Instituto de Instrumentación para Imagen MolecularJ. Torrent - Donostia International Physics CenterA. Uson - Instituto de Física CorpuscularJ. F. C. A. Veloso - University of AveiroR. Webb - Texas A&M UniversityR. Weiss-Babai - Ben-Gurion University of the NegevJ. T. White - Texas A&M UniversityN. Yahlali - Instituto de Física Corpuscular
- Resource Type
- Journal article
- Publication Details
- Journal of instrumentation, Vol.15(4), pp.P04022-P04022
- DOI
- 10.1088/1748-0221/15/04/P04022
- ISSN
- 1748-0221
- eISSN
- 1748-0221
- Publisher
- Iop Publishing Ltd
- Number of pages
- 15
- Language
- English
- Date published
- 04/01/2020
- Academic Unit
- Physics and Astronomy
- Record Identifier
- 9984627324402771
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