TY - JOUR
T1 - Extremely cold positrons accumulated electronically in ultrahigh vacuum
AU - Haarsma, L. H.
AU - Abdullah, K.
AU - Gabrielse, G.
PY - 1995
Y1 - 1995
N2 - Many cold positrons in ultrahigh vacuum are required to produce cold antihydrogen, to cool highly stripped ions, and for ultracold plasma studies. Up to 3.5×104 such positrons have now been accumulated into the ultrahigh vacuum of a 4.2 K Penning trap, at a rate exceeding 103/h. Both the accumulation rate (per high energy positron incident at the trap) and the number accumulated are much larger than ever before realized at low temperatures in high vacuum. The cooling of high energy positrons (from 22Na decay) in a tungsten crystal near the trap, together with purely electronic trapping and damping, is the key to the efficient accumulation and to projected improvements.
AB - Many cold positrons in ultrahigh vacuum are required to produce cold antihydrogen, to cool highly stripped ions, and for ultracold plasma studies. Up to 3.5×104 such positrons have now been accumulated into the ultrahigh vacuum of a 4.2 K Penning trap, at a rate exceeding 103/h. Both the accumulation rate (per high energy positron incident at the trap) and the number accumulated are much larger than ever before realized at low temperatures in high vacuum. The cooling of high energy positrons (from 22Na decay) in a tungsten crystal near the trap, together with purely electronic trapping and damping, is the key to the efficient accumulation and to projected improvements.
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U2 - 10.1103/PhysRevLett.75.806
DO - 10.1103/PhysRevLett.75.806
M3 - Article
C2 - 10060123
AN - SCOPUS:11944255984
SN - 0031-9007
VL - 75
SP - 806
EP - 809
JO - Physical review letters
JF - Physical review letters
IS - 5
ER -