Accumulation of Positrons from a LINAC Based Source |
S. Nianga, M. Charltonb, J.J. Choic, M. Chungd, P. Cladée, P. Cominia, P. Crivellif, P.P. Crépine, O. Dalkarovg, P. Debua, L. Doddb, A. Douillete, h, P. Froehlichi, J. Gafrillerj, S. Guellatie, J. Heinriche, P.A. Hervieuxk, L. Hilicoe, h, A. Hussonl, P. Indelicatoe, G. Jankaf, S. Jonselli, J.P. Karre, h, B.H. Kimc, E-S Kimm, S.K. Kimc, A. Kleyheegj, Y. Kon, T. Kosinskio, N. Kurodap, B. Latacza, H. Leec, J. Leen, A.M.M. Leitea, E. Limm, L. Liszkaya, T. Louvradouxe, D. Lunneyl, K. Lévéquek, G. Manfredik, B. Mansouliéa, M. Matusiako, G. Mornacchij, V.V. Nesvizhevskyq, F. Neze, R. Niship, S. Nourbakshj, K.H. Parkc, N. Paule, P. Péreza, B. Radicsf, C. Regenfusf, S. Reynaude, J.Y. Rousséa, A. Rubbiaf, J. Rzadkiewiczo, Y. Sacquina, F. Schmidt-Kalerr, M. Staszczako, B. Tuchminga, B. Vallagea, D.P. van der Werfb, A. Voroning, A. Welkerj, S. Wolfr, D. Wonc, S. Wronkao, Y. Yamazakis, K.H. Yood, C.J. Bakerb
aIRFU, CEA, Université Paris-Saclay, F-91191 Gif-sur-Yvette, France bDepartment of Physics, College of Science, Swansea University, Swansea SA2 8PP, United Kingdom cDepartment of Physics and Astronomy, Seoul National University, 1 Gwanak-Ro, Gwanak-gu, Seoul 08826, Korea dDepartment of Physics, Ulsan National Institute of Science and Technology (UNIST), 50, UNIST-gil, Ulsan 44919, Republic of Korea eLaboratoire Kastler Brossel, Sorbonne Université, CNRS, ENS-PSL Research University, Collège de France, Campus Pierre et Marie Curie, 4, pl. Jussieu, F-75005 Paris, France fInstitute for Particle Physics and Astrophysics, ETH Zurich, 8093 Zurich, Switzerland gP.N. Lebedev Physical Institute, 53 Leninsky Prospect, 119991 Moscow, Russia hUniversité d'Evry-Val d'Essonne, Université Paris-Saclay, Boulevard François Mitterand, F-91000 Evry, France iDepartment of Physics, Stockholm University, SE-10691 Stockholm, Sweden jCERN, 1211 Geneva 23, Switzerland kUniversité de Strasbourg, CNRS, Institut de Physique et Chimie des Matériaux de Strasbourg, UMR 7504, F-67000 Strasbourg, France lCSNSM-IN2P3-CNRS, Université de Paris Sud, Orsay, France mDepartment of Accelerator Science, Korea University Sejong Campus, Sejong-ro 2511, 30019 Sejong, Republic of Korea nCenter for Underground Physics, Institute for Basic Science, 70 Yuseong-daero 1689-gil, Yuseong-gu, Daejeon 34047, Korea oNational Centre for Nuclear Research (NCBJ), A. Soltana 7, 05-400 Otwock, Swierk, Poland pInstitute of Physics, University of Tokyo, 3-8-1 Komaba, Meguro, Tokyo 153-8902, Japan qInstitut Max von Laue - Paul Langevin (ILL), 71 av. des Martyrs, Grenoble, France, F-38042 rQUANTUM, Institut für Physik, Johannes Gutenberg Universität, D-55128 Mainz, Germany sUlmer Fundamental Symmetries Laboratory, RIKEN, 2-1 Hirosawa, Wako, 351-0198, Saitama, Japan |
Full Text PDF |
The GBAR experiment aims to measure the gravitational acceleration of antihydrogen H̅. It will use H̅+ ions formed by the interaction of antiprotons with a dense positronium cloud, which will require about 1010 positrons to produce one H̅+. We present the first results on the positron accumulation, reaching 3.8±0.4×108 e+ collected in 560 s. |
DOI:10.12693/APhysPolA.137.164 topics: positron plasma, positron accumulation, antimatter, Penning-Malmberg trap, Greaves-Surko trap, GBAR |