EGAS41 - Swansea University
EGAS41 - Swansea University
EGAS41 - Swansea University
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41 st EGAS CP 15 Gdańsk 2009<br />
Nonresonant corrections for the optical resonance frequency<br />
measurements in hydrogen atom<br />
L. Labzowsky 1,2 , G. Schedrin 1 , D. Solovyev 1 , E. Chernovskaya 1,∗ ,<br />
G. Plunien 3 , S. Karshenboim 4,5<br />
1 V.A. Fock Institute of Physics, St. Petersburg State <strong>University</strong>, 198904, Uljanovskaya 1,<br />
Petrodvorets, St. Petersburg, Russia<br />
2 Petersburg Nuclear Physics Institute, 188350, Gatchina, St. Petersburg, Russia<br />
3 Institut für Theoretische Physik, Technische Universität Dresden, Mommsenstrasse 13,<br />
D-01062, Dresden, Germany<br />
4 D.I. Mendeleev Institute for Metrology, St. Petersburg, 190005, Russia<br />
5 Max-Planck Institut für Quantenoptik, Garching, 85748, Germany<br />
∗ Corresponding author: jkfizfak@rambler.ru<br />
The deviation of the natural spectral line profile from the Lorentz shape for the optical<br />
resonant frequency measurements is considered. This deviation leads to an asymmetry,<br />
which is mainly due to nonresonant correction to the resonant Lorentz profile. The nonresonant<br />
corrections are studied for the different types of the atomic resonant experiments<br />
[1,2]. The most accurate recent optical resonance experiments [3,4] are analyzed, i.e. the<br />
two-photon 1s–2s resonance excitation of the hydrogen atom with the delayed decay in<br />
the external electric field. The description of the nonresonant correction in the latter case<br />
requires the employment of QED with different in- and out-Hamiltonians.<br />
The nonresonant corrections for this experiment are investigated and found to be<br />
about 10 −5 Hz, while the recent experimental uncertainty is 34 Hz and in the near feature<br />
is expected to be few Hz. The projected 1s–2s resonance excitation experiment with the<br />
three-photon ionization detection (which is now in progress) is also considered.<br />
References<br />
[1] L.N. Labzowsky, D.A. Solovyev, G. Plunien, G. Soff, Phys. Rev. Lett. 87, 143003<br />
(2001); Can. J. Phys. 80, 1187 (2002); Phys. Rev. A 65, 05 02 (2002)<br />
[2] L. Labzowsky, G. Schedrin, D. Solovyev, G. Plunien, Phys. Rev. Lett. 98, 203003<br />
(2007)<br />
[3] A. Huber, B. Gross, M. Weitz, T.W. Hänsch, Phys. Rev. A 59 , 1844 (1999)<br />
M.Niering, R. Holzwarth, J. Reichert, P. Pokasov, Th. Udem, M.Weitz, T.W. Hänsch,<br />
P. Lemond, G. Semtarelli, M. Abgrall, P. Lourent, C. Salomon, A. Clairon, Phys. Rev.<br />
Lett. 84, 5496 (2000)<br />
[4] M. Fischer, N. Kolachevsky, M. Zimmermann, R. Holzwarth, Th. Udem, T.W. Hänsch,<br />
M. Abgrall, J. Grunert, I. Maksimovic, S. Bize, H. Marion, F. Pereira Dos Santos, P.<br />
Lemonde, G. Santarelli, P. Laurent, A. Clairon, C. Salomon, M. Haas, U.D. Jentschura,<br />
C.H. Keitel, Phys. Rev. Lett. 92, 230802 (2004)<br />
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