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EGAS41 - Swansea University

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41 st EGAS CP 114 Gdańsk 2009<br />

XUV frequency comb spectroscopy<br />

D.Z. Kandula, C. Gohle, T.J. Pinkert, A. Renault,<br />

W. Ubachs, K.S.E. Eikema ∗<br />

LCVU, Vrije Universiteit Amsterdam, De Boelelaan 1081, 1081HV Amsterdam,<br />

The Netherlands<br />

∗ Corresponding author: kjeld@few.vu.nl,<br />

Precision spectroscopy in the extreme ultraviolet on helium atoms and ions is very interesting<br />

as it could provide more stringent tests of quantum electrodynamics than currently<br />

possible with hydrogen. One problem is that spectroscopy in this region typically requires<br />

amplification and harmonic upconversion of visible light sources, which can introduce difficult<br />

to control systematic errors as a result of so-called frequency-chirping effects [1,2].<br />

This issue can be overcome using a combination of amplification and harmonic upconversion<br />

of a frequency comb laser. With this technique a pair of phase-locked extreme<br />

ultraviolet pulses is generated and used to excite the 1s 2 1 S 0 −1s5p 1 P 1 transition in helium.<br />

Viewed in the frequency domain, the spectrum of the pulses in the XUV resembles<br />

again a frequency comb, but now in the form of a cosine-modulated spectrum. Viewed in<br />

the time-domain, excitation with phase-locked pulses is in fact a form of Ramsey excitation<br />

(see e.g. [3,4]).<br />

The setup consists of a Ti:Sapphire frequency comb as a source of phase controlled<br />

pulses at 773 nm. A dedicated parametric amplifier is used to amplify two subsequent<br />

pulses from the comb laser to a few mJ per pulse. The 15th harmonic is used to excite<br />

the 1s 2 1s5p transition in atomic helium at 51.56 nm. The excited atoms are ionized with<br />

an infrared laser pulse at 1064 nm and detected in a time of flight spectrometer. By<br />

changing the delay between the pulses (i.e. the repetition rate of the frequency comb<br />

laser) in one-attosecond steps, we scan the cosine-shaped comb over the transition.<br />

To achieve an accuracy in the MHz range, a careful analysis is required of phase shifts<br />

and wave front deformation in the amplification and the harmonic upconversion process,<br />

as it shifts the positions of the modes in the XUV. This is achieved with an interferometric<br />

measuring technique which has a single-laser shot accuracy of 10 mrad [5]. Many other<br />

systematic effects have been investigated in detail, which should allow an initial target<br />

accuracy of 10 MHz for the ground state of helium (which is 5 times the current best<br />

value [1,2])<br />

References<br />

[1] K.S.E. Eikema et al., Phys. Rev. A55, 1866-1883 (1997)<br />

[2] S.D. Bergeson et al., Phys. Rev. Lett. 80, 3475 (1998)<br />

[3] S. Witte et al., Science 307, 400-403 (2005)<br />

[4] S. Cavalieri et al., Phys. Rev. Lett. 89, 133002 (2002)<br />

[5] D.Z. Kandula et al., Optics Express 16, 7071-7082 (2008)<br />

174

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