Spatial Distribution of Cold Antihydrogen Formation
Author(s) -
N. Madsen,
Michele Amoretti,
C. Amsler,
G. Bonomi,
P. D. Bowe,
C. Carraro,
C. L. Cesar,
M. Charlton,
M. Doser,
A. Fontana,
M. Fujiwara,
R. Funakoshi,
P. Genova,
J. S. Hangst,
R. Hayano,
L. V. Jo̸rgensen,
A. Kellerbauer,
V. Lagomarsino,
R. Landua,
E. Lodi–Rizzini,
M. Macrı́,
D. Mitchard,
P. Montagna,
H.S. Pruys,
C. Regenfus,
A. Rotondi,
G. Testera,
A. Variola,
L. Venturelli,
D. P. van der Werf,
Y. Yamazaki,
N. Zurlo
Publication year - 2005
Publication title -
physical review letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 3.688
H-Index - 673
eISSN - 1079-7114
pISSN - 0031-9007
DOI - 10.1103/physrevlett.94.033403
Subject(s) - antihydrogen , spatial distribution , nuclear physics , distribution (mathematics) , physics , antimatter , positron , geography , remote sensing , electron , mathematical analysis , mathematics
Antihydrogen is formed when antiprotons are mixed with cold positrons in a nested Penning trap. We present experimental evidence, obtained using our antihydrogen annihilation detector, that the spatial distribution of the emerging antihydrogen atoms is independent of the positron temperature and axially enhanced. This indicates that antihydrogen is formed before the antiprotons are in thermal equilibrium with the positron plasma. This result has important implications for the trapping and spectroscopy of antihydrogen.
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