Laser measurements of the density shifts of resonance lines in antiprotonic helium atoms and stringent constraint on the antiproton charge and mass

Citation
Ha. Torii et al., Laser measurements of the density shifts of resonance lines in antiprotonic helium atoms and stringent constraint on the antiproton charge and mass, PHYS REV A, 59(1), 1999, pp. 223-229
Citations number
37
Categorie Soggetti
Physics
Journal title
PHYSICAL REVIEW A
ISSN journal
10502947 → ACNP
Volume
59
Issue
1
Year of publication
1999
Pages
223 - 229
Database
ISI
SICI code
1050-2947(199901)59:1<223:LMOTDS>2.0.ZU;2-Y
Abstract
We have performed laser spectroscopy of metastable antiprotonic helium atom s ((p) over bar He+) formed in helium media of 0.2-8.0 bars at 5.8-6.3 K an d have observed a density dependence of the resonance vacuum wavelengths fo r the known transitions (n,l) = (39,35)-->(38,34) and (37,34)-->(36,33). Th ey showed Linear redshifts of 0.61 +/- 0.01 GHz and 0.22 +/- 0.02 GHz per 1 g/l, respectively. With the shift parameters above, the transition vacuum wavelengths were extrapolated to zero-density limits, yielding lambda(0) = 597.2570 +/- 0.0003 nm and lambda(0) = 470.7220 +/- 0.0006 nm, respectively . These values, with a 0.5-ppm precision, were compared with the result of recent theoretical calculations on the energy of the Coulombic three-body s ystem, including relativistic corrections and the Lamb shift. The agreement between our experimental values and the calculations has become as good as 2x10(-6). This excellent agreement in turn provides a precise value of the antiproton Rydberg constant that surpasses the currently known precision a nd sets a severe constraint on the antiproton charge (-Q((p) over bar)) and the mass (M-(p over bar)) that both \Q(p) - Q((p) over bar)\/e and \M-p - M-(p over bar)\/M-p be less than 5 x 10(-7), when a more precisely known co nstraint on the charge-to-mass ratio is combined. Thus we have opened a pos sibility of determining fundamental constants of the antiproton. [S1050-294 7(99)04501-1].