Cooling by spontaneous decay of highly excited antihydrogen atoms in magnetic traps.
An efficient cooling mechanism of magnetically trapped, highly excited antihydrogen (H) atoms is presented. This cooling, in addition to the expected evaporative cooling, results in trapping of a large number of H atoms in the ground state. It is found that the final fraction of trapped atoms is insensitive to the initial distribution of H magnetic quantum numbers. Expressions are derived for the cooling efficiency, demonstrating that magnetic quadrupole (cusp) traps provide stronger cooling than higher order magnetic multipoles. The final temperature of H confined in a cusp trap is shown to depend as approximately 2.2T(n0)n(0)(-2/3) on the initial Rydberg level n0 and temperature T(n0).
Pohl
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T
ITAMP, Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge Massachusetts 02138, USA.
Sadeghpour
H R
HR
Nagata
Y
Y
Yamazaki
Y
Y