Ultrafast spectroscopy with attosecond resolution has enabled the real time observation of ultrafast electron dynamics in atoms, molecules and solids. These experiments employ attosecond pulses or pulse trains and explore dynamical processes in a pump–probe scheme that is selectively sensitive to electronic state of matter via photoelectron or XUV absorption spectroscopy or that includes changes of the ionic state detected via photo-ion mass spectrometry. Here, we demonstrate how the implementation of combined photo-ion and absorption spectroscopy with attosecond resolution enables tracking the complex multidimensional excitation and decay cascade of an Auger auto-ionization process of a few femtoseconds in highly excited krypton. In tandem with theory, our study reveals the role of intermediate electronic states in the formation of multiply charged ions. Amplitude tuning of a dressing laser field addresses different groups of decay channels and allows exerting temporal and quantitative control over the ionization dynamics in rare gas atoms.
In the last decade, time-resolved spectroscopy with attosecond resolution1,2,3,4,5,6,7,8,9,10,11,12,13 has revolutionized our understanding of electron dynamics by capturing ultrafast processes in atoms, molecules and solids in real time. While the first photoelectron studies with attosecond resolution could, for example, track a few-femtosecond Auger process14, meanwhile ultrafast metrology became so advanced that unexpected delays in photoemission from atoms were discovered4,15, most recently down to sub-attosecond precision5. Attosecond time-resolved mass spectroscopy16,17 provided the first time-domain observation of field-induced tunnel ionization manifesting itself in a step-like rise in the ion yield. More recently, attosecond transient absorption detection could launch and detect valence electron wavepackets in atoms11, examine their interference with continuum states13 and enabled studying tunnel ionization in solids18.
Photoelectron detection techniques generally suffer from electron backgrounds produced by strong laser fields or secondary electrons that do not carry any information about the dynamics under inspection. The detection of the correspondingly produced ions, however, is background-free. Nevertheless, both methods require the release of photoelectrons and thus are suitable only for the study of ionizing events. Transient absorption spectroscopy (TAS) in contrast is not limited to phenomena liberating electrons and is the method of choice for investigating bound–bound transitions19,20. Instead of measuring the yield of generated charge carriers, TAS measures the spectrally resolved absorption of an attosecond extreme ultraviolet (XUV) pulse in a medium that has been coherently excited by an XUV pulse or dressed by an intense, time-delayed near-infrared (NIR) few-cycle laser pulse. This method typically provides a higher resolution in energy (ΔE/E ~ 10−3) than ion or electron detection (ΔE/E ~ 10−2 at best). However, it generally lacks the dynamic range to simultaneously detect the characteristic absorption signals of different co-existing ionic charge states due to insufficient spectral bandwidth or due to the absorption cross-sections and abundances of the different ionization states that typically vary by several orders of magnitude. TAS experiments have been successful in recording auto-ionizing state lifetimes in xenon12 and other species21. However, even a detailed theoretical investigation could not explain whether the interrogating ultrashort and intense NIR laser pulse couples the auto-ionizing states to neighboring resonances or to which extent excited electrons are promoted into the ionization continuum by the laser field22. In contrast, the ion detection that enabled the first observation of tunneling electrons in neon and xenon could track the change in ion yield of different charge states. However, mass spectroscopic studies to this date cannot resolve individual shake up satellites16.
To overcome the limitations of single observable experiments and in order to draw a complete picture of the co-evolving excitation/ionization dynamics, in this article we demonstrate the benefit of combining ion spectroscopy and transient absorption with attosecond temporal resolution. Merging these detection methods provides complementary insight into the excitation/decay mechanism as the transient absorption maps the initiating resonant excitation and the ion detection sensitively records the subsequent branching into intermediate and final states. The combination of transient absorption with ion spectroscopy compensates the limits in the simultaneous detection of several ionic states that absorption spectroscopy typically brings along. The prerequisite is that the pump–probe experiment can be performed twice under identical experimental conditions except for differing target densities optimized for the two detection methods. Adjusting the laser electric field amplitude allows selectively addressing different intermediate states of the auto-ionization cascades that follow the XUV excitation resulting in different apparent lifetimes. With that, the experimentalist obtains control of the temporal evolution and the absolute yield of the ionization dynamics by accessing different level groups in the cascade with different NIR intensities. The accompanying absorption measurement enables the determination of the instrument response function, the lifetimes of resonantly excited states involved in the process and proves that the overall conditions of the experiment (resonant excitation and ionization) remain unchanged for a large range of NIR intensities.
To explore the decay dynamics of highly excited krypton (see Fig. 1a), a phase-stabilized Ti:Sapphire few-cycle laser14,16,17 is used to produce isolated attosecond pulses (cp. Supplementary Fig. 1) via high harmonic generation in a pump–probe scheme united with a reflectron-type ion spectrometer and an XUV grating spectrometer (see Fig. 1b and Supplementary Note 1 for details). Figure 1c shows the transmission spectrum without (violet) and with (green) krypton gas sample with the NIR pulse preceding the XUV pulse by 150 fs. For the same time delay, Fig. 1d depicts the corresponding ion spectrum with singly, doubly and triply charged krypton ions. For the time-resolved studies, we measured the krypton transmission and ion spectrum scanning the arrival time difference between XUV and laser pulse.
Merging ultrafast absorption and ion mass spectroscopy
Figure 2a shows the spectrally resolved change in absorbance (optical density OD = −log10(I t (Δt)/I0), with I0 as incident XUV spectrum) as function of the XUV/NIR time delay, while Fig. 2b depicts the isotope-resolved Kr3+ ion yield change. The absorbance starts to transiently decrease at XUV/NIR pulse synchrony while the Kr3+ ion yield shortly rises, however, with a slightly retarded response with respect to the absorption change.
Ionization dynamics in krypton
To reveal further details of the ionization dynamics, Fig. 3 presents the absorbance ΔOD at 91.23 eV (corresponding to the 3d5/25p resonance23) relative to the OD measured at Δt = −30 fs and the Kr3+ ion yield added up over the four most abundant krypton isotopes for two different NIR intensities: Fig. 3a for low NIR intensity of (8.6 ± 1) × 1013 W cm−2 and Fig. 3b for high NIR intensity of (2.9 ± 0.5) × 1014 W cm−2. For both cases, the absorbance decreases on a quick (<10 fs) time scale before it recovers almost to its original value. The time constant of the fast ΔOD decrease reflects the instrument response and the NIR pulse duration. A least squares fit gives an instrument response function24 of 1.8 ± 0.4 fs and hence a duration of 4.5 ± 1 fs for the Gaussian-shaped NIR pulse while the exponential recovery of the absorbance after pulse overlap yields a 6.8 ± 1.5 fs and a 7.7 ± 2.2 fs auto-ionization state lifetime of the 3d−1np levels for low and high NIR intensity, respectively. These lifetime results agree well with the previously reported value of 7.9 ± 0.2 fs25. Potential NIR intensity-dependent effects like the ac Stark shift or resonant coupling to neighboring states resulting in a broadening or even splitting of the resonances could be excluded by careful investigation of the resonance center positions and line shapes for all recorded time delays. This and the comparison to the literature values confirm that the initial Auger decay is virtually unaffected by different NIR laser field intensities. Recovery of the Kr3+ yield shows a strong dependence on the intensity of the applied NIR laser field: the number of Kr3+ ions increases when the XUV and the NIR pulses start to overlap, but not as quickly as the absorption changes at the 3d−1np resonances. This is because at pulse overlap, a significant part of the Kr3+ ions result from a cascaded Auger decay following the resonant 3d−1np excitation. Hence, the Kr3+ ion yield rise time does not only depend on the NIR pulse duration but also on the lifetimes of the resonantly excited 3d−1np states. Taking into account the instrument response function and the 3d−1np lifetime for the increase of the Kr3+ ion yield curve, a least squares fit yields a time constant of 9.3 ± 3.7 fs for the tail of the Kr3+ ion count rate that corresponds to the effective lifetime of the intermediate state of the Auger cascade (here: INIR = (8.6 ± 1) × 1013 W cm−2). This value differs from the previously reported value of 20 ± 4 fs17: our presented study is to our knowledge the first one that systematically investigates the ionization dynamics in krypton for different NIR intensities. As the lowest NIR intensity is twice as high as previously17, different auto-ionization paths in the de-excitation of the Kr+ ions become visible and may lead to a different apparent/effective decay time. In practice, we here observe an effective lifetime for the 3d−1np→4s–2np→4s−14p−1/4p−34d cascades that arise from a large number of individual but not resolved fine-structure transitions. This is confirmed by our multiconfiguration Dirac–Fock calculations using the GRASP26 and RATIP27 codes and by taking the average of all the individual lifetimes, weighted by their relative decay probabilities. This theoretical approach is for the first time applied to reveal effective lifetimes of different potential group cascades (see Supplementary Note 5 for details).
Control of krypton ionization dynamics
Figure 4 shows for three different NIR intensities that the observed decay time increases for higher NIR intensities due to a second set of decay channels (3d−1np → 4s−14p–1np/4p−34dnp → 4p−2). This second set (indicated by B in Fig. 1a) has a much longer effective lifetime as it was already speculated17: A double exponential decay fit gives rise to a second decay time of 60 ± 28 fs, if we apply 9.3 fs as the first decay time that has been found for the lowest intensity. At higher NIR intensity, channel B results in an increase of the amplitude ratio B/A. Amplitude A corresponds to the Auger cascade emerging at low NIR intensities. The results of our theoretical calculations of the effective lifetimes with 6 fs for the 4s−2np levels and 49 fs for the 4s−14p−1np/4p−34dnp levels agree very well with the measurements.
There occurs a transient drop in the Kr3+ ion production shortly before pulse overlap (approximately at −5 fs) that depends on the NIR intensity but appears independent of the carrier envelope phase (strongest dip at high NIR intensities, best visible in Fig. 3b). This dip has been observed previously17, and its origin is not yet understood. It could result from a transient population transfer28 but may arise also as a Fano-type resonance29 that is embedded into the Kr2+ continuum.
While a control of the end configuration in the dissociative ionization process of deuterium by tuning the carrier envelope phase has been already demonstrated30, we have shown here that combined attosecond transient absorption and mass spectrometry allows the observation and control of the XUV-induced ionization dynamics in rare gas atoms. The study reveals the role of intermediate electronic and ionic states and highlights how laser-induced state coupling can be used to control the post-excitation decay dynamics. The experiment simultaneously determines the instrument response function, the effective lifetimes of the resonantly excited states and confirms that the initiating resonant excitation is not affected by the dressing laser field amplitude while the evolution of the post-excitation decay can be dynamically and quantitatively manipulated.
The data that support the findings of this study are available from the corresponding author upon request.
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The authors warmly acknowledge Hartmut Schröder and Martin Schultze for instrumental support and discussions, as well as Marinus Mayerbacher’s and Alexander Späh’s contributions to the vacuum setup. B.B. wants to thank the Alexander von Humboldt foundation and the Carl Zeiss foundation for financial support. N.M.K. acknowledges hospitality and financial support from DIPC (San Sebastian/Donostia) and from the theory group in cooperation with the SQS work package of European XFEL (Hamburg). R.K. acknowledges a Consolidator Grant from the European Research Council (ERC-2014-CoG AEDMOS). S.O.S. gratefully acknowledges funding by the German Federal Ministry of Education and Research (BMBF) under Contract No. 05K16SJA. This work was supported by the Max Planck Society, the Deutsche Forschungsgemeinschaft Cluster of Excellence: Munich Centre for Advanced Photonics (http://www.munich-photonics.de).