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jahresbericht 2007 - Institut für Kernchemie - Johannes Gutenberg ...

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Absolute Frequency Measurements on the 2S → 3S Transition of 7 Li and 6 Li ∗<br />

R. M. Sánchez Alarcón 1 , Z. Andjelkovic 2 , C. Geppert 1 , J. Krämer 2 , J. Kluge 1 , M. Nothhelfer 2 , D.<br />

Tiedemann 2 , D. F. A Winters 1 , M. Zakova 2 , and W. Nörtershäuser 1,2<br />

1 GSI mbH, Atomphysik, Planckstr. 1, D-64291 Darmstadt, Germany; 2 <strong>Institut</strong> für <strong>Kernchemie</strong>, <strong>Johannes</strong><br />

<strong>Gutenberg</strong>-Universität Mainz, Fritz-Strassmann-Weg 2, D-55128 Mainz, Germany<br />

Laser spectroscopy plays an important role in the determination<br />

of ground state properties of atomic nuclei. Recently<br />

this has been again demonstrated by the determination<br />

of the nuclear charge radii of the light halo nuclei 11 Li<br />

[1] and 6,8 He [2]. These have been possible thanks to the<br />

combination of both, the high resolution of 10 −5 achieved<br />

in the laser spectroscopic isotope shift (IS) measurements<br />

and a similar accuracy in atomic theory calculations on the<br />

two- and three-electron systems [3]. In the lithium chain,<br />

we could provide very accurate numbers for the changes<br />

in charge radii between the isotopes. However, absolute<br />

charge radius determinations are limited in accuracy by the<br />

uncertainty of the reference 6,7 Li charge radii, whereas for<br />

the helium isotopes the situation is slightly better because<br />

the charge radius of 4 He is known with higher accuracy. In<br />

principle, laser spectroscopy could also be used for a determination<br />

of the absolute charge radius as it has been shown<br />

in hydrogen [4], provided that the atomic structure calculations<br />

of the absolute transition energies can be improved<br />

by about an order of magnitude. The calculation of absolute<br />

transition energies is still a challenge because of the<br />

higher-order mass-independent QED terms, which cancel<br />

in isotope shift calculations - since they are mass independent<br />

- but contribute fully to the transition energy. Two<br />

groups are working on this problem now and try to clearly<br />

improve the situation. On the experimental side, transition<br />

frequency measurements on these systems are needed with<br />

an accuracy of better than about 1 MHz, which is a relative<br />

accuracy of a few times 10 −10 . The recent development<br />

of the femto-second frequency comb-device, which links<br />

optical and rf frequencies, allows us to determine the transition<br />

frequency with the required accuracy.<br />

Therefore, we have measured the 2S → 3S two-photon<br />

transition frequencies of the stable lithium isotopes 6,7 Li<br />

applying the setup that has been used previously to measure<br />

the lithium IS [5] with a laser system that has been adapted<br />

for this task. The main modification was that the Titanium-<br />

Sapphire (Ti:Sa) laser, which drives the two-photon transition,<br />

was phase-locked to a femto-second frequency comb<br />

[6] instead of being referenced to an iodine line as previously.<br />

Changing the repetition rate of the comb allowed<br />

us to sweep the Ti:Sa laser frequency across the resonance<br />

line, as it is shown in Fig. 1a. The absolute transition frequency<br />

has to be taken as the center of gravity (cg) of the<br />

hyperfine components.<br />

Systematics effects, like AC Stark shifts (see Fig. 1b)<br />

∗ Work supported by HGF under contract VH-NG-148 and by BMBF<br />

under contracts 06MZ215/TP6 and 06TU263I.<br />

Counts (1/s)<br />

10 5 3s F = 2<br />

F = 1<br />

10 4<br />

10 3<br />

10 2<br />

(a)<br />

F = 2 F = 2<br />

F = 1 F = 1<br />

F = 2<br />

F = 1<br />

10 1<br />

0 800 1600 2400 3200<br />

Relative Frequency (MHz)<br />

2s<br />

7 Li Frequency cg (MHz)<br />

224<br />

223<br />

(b)<br />

222<br />

Data<br />

= A + B·P cg Ti:Sa<br />

Upper and lower<br />

95% confidence limit<br />

221<br />

A = 220.84(7) MHz<br />

B = 0.062(3) MHz/mW<br />

220<br />

0 10 20 30 40 50<br />

Ti:Sa Power behind Cavity (mW)<br />

Figure 1: (a) Line shape of the 2S → 3S atomic transition<br />

in 7 Li. (b) An AC Stark shift measurement with extrapolation<br />

to zero laser intensity.<br />

were studied experimentally. Particularly it was noticed<br />

that recorded spectra at high power showed an asymmetry<br />

in the line profile that can clearly be observed in Fig. 2a.<br />

To understand the profile, simulations were performed that<br />

included the lithium atoms crossing through a Gaussian<br />

laser field distribution with intensity fluctuations such as<br />

they were typical during the experiment. The calculated<br />

points shown in Fig. 2 were then fitted with a Lorentzian<br />

line profile and the residuals, plotted underneath the peak<br />

structure, show a very similar behavior for the fitting of the<br />

real as well as of the simulated peaks.<br />

Laser-ions (1/s)<br />

Residuals (1/s)<br />

80000<br />

60000<br />

40000<br />

20000<br />

(a)<br />

0<br />

8000<br />

4000<br />

-4000 0<br />

-8000<br />

90 100 110 120 400 410 420 430<br />

Relative Frequency (MHz)<br />

Laser-ion Population<br />

Residuals<br />

(b)<br />

2.0x10 -3<br />

1.5x10 -3<br />

1.0x10 -3<br />

5.0x10 -4<br />

0.0<br />

1x10 -4<br />

0<br />

-1x10 -4<br />

2.5x10 -3 -30 -20 -10 0 10<br />

Frequency (MHz)<br />

20 30<br />

Figure 2: (a) Line profile in the real transition. (b) A simulation<br />

reproduces the observed asymmetry quite well.<br />

Final analysis is still ongoing but we expect to improve<br />

the accuracy in the transition frequency by about an order<br />

of magnitude. Once theory will make the required<br />

progress, the absolute field shift contribution in the transition<br />

and therefore the total nuclear charge radius could be<br />

extracted by pure optical means.<br />

References<br />

[1] R. Sánchez et al., PRL 96, 033002 (2006).<br />

[2] P. Müller et al., PRL 99, 252501 (<strong>2007</strong>).<br />

[3] G. W. F. Drake et al. Lect. Notes Phys. 745, 131 (2008).<br />

[4] T. Udem et al. PRL 79, 2646 (1997).<br />

[5] G. Ewald et al., PRL 93, 113002 (2004).<br />

[6] http://www.menlosystems.com/fc1500.html<br />

- A4 -

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