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Research Article

Attosecond coherent electron motion in Auger-Meitner decay

Siqi Li https://orcid.org/0000-0002-1262-6292, Taran Driver https://orcid.org/0000-0002-3761-6883, Philipp Rosenberger https://orcid.org/0000-0002-4271-3557, Elio G. Champenois https://orcid.org/0000-0002-3530-8377, Joseph Duris https://orcid.org/0000-0002-9930-1166, Andre Al-Haddad, Vitali Averbukh https://orcid.org/0000-0001-7999-0075, Jonathan C. T. Barnard, Nora Berrah, Christoph Bostedt, Philip H. Bucksbaum https://orcid.org/0000-0003-1258-5571, Ryan N. Coffee https://orcid.org/0000-0002-2619-8823, Louis F. DiMauro https://orcid.org/0000-0002-0171-7033, Li Fang https://orcid.org/0000-0002-8058-8216, Douglas Garratt https://orcid.org/0000-0002-8637-9984, Averell Gatton https://orcid.org/0000-0002-2550-0277, Zhaoheng Guo, Gregor Hartmann, Daniel Haxton, Wolfram Helml https://orcid.org/0000-0003-1537-2993, Zhirong Huang, Aaron C. LaForge https://orcid.org/0000-0002-5758-6917, Andrei Kamalov, Jonas Knurr https://orcid.org/0000-0002-9455-0702, Ming-Fu Lin https://orcid.org/0000-0001-8086-2484, Alberto A. Lutman https://orcid.org/0000-0001-5791-9198, James P. MacArthur, Jon P. Marangos https://orcid.org/0000-0001-7169-6955, Megan Nantel https://orcid.org/0000-0002-9684-3314, Adi Natan https://orcid.org/0000-0002-6594-7794, Razib Obaid https://orcid.org/0000-0002-1759-4752, Jordan T. O’Neal, Niranjan H. Shivaram https://orcid.org/0000-0002-9550-3588, Aviad Schori, Peter Walter https://orcid.org/0000-0001-8839-1154, Anna Li Wang https://orcid.org/0000-0001-7515-0626, Thomas J. A. Wolf https://orcid.org/0000-0002-0641-1279, Zhen Zhang https://orcid.org/0000-0002-9139-2497, Matthias F. Kling https://orcid.org/0000-0002-1710-0775, Agostino Marinelli https://orcid.org/0000-0002-7248-4652 [email protected], and James P. Cryan https://orcid.org/0000-0002-7776-0919 [email protected]
Science6 Jan 2022First ReleaseDOI: 10.1126/science.abj2096

Abstract

In quantum systems, coherent superpositions of electronic states evolve on ultrafast timescales (few femtosecond to attosecond, 1 as = 0.001 fs = 10 18 s), leading to a time dependent charge density. Here we performed time-resolved measurement using attosecond soft x-ray pulses produced by a free-electron laser, to track the evolution of a coherent core-hole excitation in nitric oxide. Using an additional circularly polarized infrared laser pulse we created a clock to time-resolve the electron dynamics, and demonstrated control of the coherent electron motion by tuning the photon energy of the x-ray pulse. Core-excited states offer a fundamental test bed for studying coherent electron dynamics in highly excited and strongly correlated matter.
Interference is a pillar of quantum physics, and a manifestation of one of its most remarkable consequences: the wavelike nature of matter. A quantum system can exist in a superposition of energy states whose relative quantum phases progress in time. This behavior can cause the states to interfere constructively or destructively as the system evolves, causing physical observables (e.g., charge density) to oscillate in time. Such oscillations are known as quantum beats (QBs), and have a period of TQB=h/ΔE, where h is Planck’s constant and ΔE is the energetic separation between the states (15). In order to display a quantum beat, two conditions must be satisfied: First, the quantum system must be prepared in a superposition of two or more different energy states that have a well-defined (or coherent) relationship between their individual quantum phases, which remains stable over the beat period between the relevant phases. Second, the physical observable must be sensitive to the difference between the quantum phases of the energy states forming the coherent superposition.
In this work, we demonstrated the creation and observation of coherent superpositions of core-excited states in molecules using attosecond x-ray pulses. These molecules decayed non-radiatively via the Auger-Meitner (AM) mechanism; a multi-electron process where the core vacancy created by an x-ray pulse is filled by one electron from a valence orbital, and another valence electron is emitted to conserve energy. The AM process is the dominant mechanism for relaxation following x-ray absorption in most biologically relevant molecules, and any molecules composed of light atoms such as carbon, oxygen, and nitrogen.
We demonstrated how coherence in short x-ray pulses is imprinted on excited electronic states following x-ray/matter interaction, and how this coherence affects the attosecond evolution of the excited electronic wavepacket. To this end, we measured the time-dependent AM yield, and found that it was sensitive to the quantum coherence of the electronic wavepacket, as well as the differences in the excited state populations. The coherence of the wavepacket was manifested as femtosecond modulations (or quantum beats) in the time-dependent electron yield. The effect of the wavepacket coherence on the relaxation process could affect a broad class of other ultrafast experiments where the need for high temporal resolution necessitates the use of broad bandwidth X-ray pulses.
Time-resolved measurements of any correlated electron interaction (including AM decay) are challenging due to the extreme timescale (few- to sub-femtosecond) on which electron-electron interactions occur. Previous time-resolved measurements have extracted a single parameter (Γ) to characterize the decay of a core-excited system (69). In the case of short excitation/ionization pulses, Γ corresponds to the lifetime of the core-excited state, but for long pulses the extracted decay constant is altered by interferences with the excitation process (911). Our distinct combination of short excitation pulses and a sufficiently long observation window allowed for a direct time-resolved measurement of the AM emission process. We measured a quantum beat, demonstrating the creation and observation of electronic coherence in a core-excited molecular system. Our technique of mapping coherent electronic motion to the AM decay profile offered a distinctive test-bed for studies of electronic coherence in highly excited and strongly correlated systems.

Measurement

Our experimental setup is shown in Fig. 1a. Isolated soft x-ray attosecond pulses from a free-electron laser (12), tuned near the oxygen 1sπ resonance in nitric oxide (NO) (530–540 eV), irradiated a gas target in the presence of a circularly polarized, 2.3 μm, 5×1012 W/cm 2 laser field. The momentum distribution of the resultant photoelectrons was recorded by a co-axial velocity map imaging spectrometer (c-VMI) (13). Interaction with the x-ray pulse produced electrons from several different photoionization channels: direct ionization of nitrogen K-shell electrons, KLL AM emission resulting from the nitrogen K-shell vacancy, and resonant oxygen AM emission following O 1sπ excitation. These channels are labeled in Fig. 1b, which shows the electron momentum distribution recorded without the 2.3 μm laser field. The 1sπ excitation in nitric oxide corresponds to the promotion of an oxygen 1s electron to the degenerate 2π molecular orbital, which is already partially occupied by an unpaired valence electron. The resonant AM emission following this excitation has a dominant feature corresponding to channels where one of the degenerate 2π electrons participates in the decay, leading to excited cationic states. There is a small contribution from the channel where both 2π electrons participate, resulting in a 2π0 ground configuration of the cation (14).
Fig. 1. Experimental observation of Auger-Meitner emission.
(a) NO gas is ionized by an attosecond XFEL pulse (530–540 eV, central photon energy) in the presence of a 2.3 μm circularly polarized streaking field. The resultant photoelectron momentum distribution is measured by a co-axial velocity map imaging spectrometer (c-VMI) (13). The streaking field maps the instantaneous ionization rate onto the measured photoelectron momentum distribution. (b) Single-color electron momentum spectrum projected along the axis of the c-VMI in the absence of the streaking field. Atomic units denoted here and throughout as ‘a.u.’. We define px to lie along the x-ray polarization axis. (c) Applying an inverse Abel transform to this image, we retrieve the electron kinetic energy distribution (‘arb.’ denotes arbitrary units). In (d) we show the change in the projected momentum distribution as the direction of the streaking laser vector potential (A0, light gray line pointing along 0 fs of the stopwatch face) is varied. The projected momentum distribution is presented as a difference image where the electron momentum shown in panel (b) is used as a background. To observe the temporal evolution of AM emission we monitor the AM yield in a small (15 ) region of the detector (black box shown in the panels of (d), energetic position also shown in pale red in panel (c). The time-dependence of this yield is shown in black dots in panel e (dashed red line shows trace with high frequency noise filter applied, see SM for further details). The AM yield in (e) is plotted as a function of angle between the streaking laser vector potential at the time of ionization and the angle of the detection box, which is shown as a gray shaded area in (d). E shows the direction of rotation of the electric field. The red error bars have a total length of four times the standard error of the mean of the measured electron yield, ±2σx¯.
The circularly polarized laser field maped the temporal profile of the electron emission on to the momentum measured at the detector. When electrons were released from the molecule following interaction with the x-ray pulse, their trajectory was altered by the presence of the infrared laser field, similar to the principle of a time-resolving streak camera (15, 16). This interaction altered (or ‘streaked’) the final electron momentum, which was measured at the detector. In a semi-classical approximation, the final momentum of an ionized electron is given by
pt=p0+eAt0,
(1)
where At0=t0ELtdt is the vector potential of the circularly polarized laser field, ELt, at the time of ionization t0, e is the charge of an electron (1 atomic unit) and p0 is the momentum of the electron in the absence of the infrared laser field. All the quantities are expressed in atomic units.
In our measurement the temporal duration of the circularly polarized ‘streaking’ laser field (100 fs) was much longer than the laser period (TL=7.7 fs). This fact implies that over the timescale of a single laser period the vector potential had nearly constant amplitude (A) but a direction that rotated with constant angular velocity 2π/TL. Thus, Eq. 1 describes how the streaking technique encodes the temporal evolution of the electron emission rate onto the electron momentum spectrum: an electron emitted at ti will experience a momentum shift in the direction of Ati. Because the period TL of the circularly polarized laser is well known, if two photoemission features are found to have momentum shifts that differ by an amount Δθ, this difference implies that the photoemission events were separated by a time Δτ:
Δτ=Δθ2π×TL.
(2)
This mapping of angle-to-time resembles the face of a clock, which has led to the term ‘attoclock’ being used to describe this type of time-resolved measurement (1719).
Our method for extracting the temporal profile of the AM electron yield is illustrated in Figs. 1d and 1e. Figure 1d shows the variation in the differential electron yield for measurements with three different x-ray arrival times, or directions of the streaking laser vector potential,A0. The differential images show the difference between the averaged electron image when the vector potential of the IR laser was chosen to lie along the line labeled A0 on the figure (and labeled as ‘0 fs’ on the clock face) and the averaged electron image where the IR laser has been intentionally mistimed with the x-rays to ensure there was no effect from the streaking field. To extract the time-dependent emission rate of resonant AM electrons we monitored a small angular region on the detector (black wedge in Fig. 1d) and plot this yield as a function of streak angle, or the angle between the observation bin and the streaking laser vector potential, in Fig. 1e. The observation region was chosen to be slightly higher in momentum than the center of the field-free resonant emission spectrum shown in Fig. 1b. The electron yield in this radial bin therefore mapped to the number of electrons released into the continuum at the time the vector potential A0t is pointed in the angular direction of the observation region. The lower momentum limit of this region is 6.4 atomic units and the upper limit extends to include all electrons at higher momenta. Equation 2 can be used to convert the streak angle into a time delay, and this value is used to label the clock face in Fig. 1d and the lower horizontal axis in Fig. 1e.
At the LCLS, the synchronization of the streaking laser and x-ray pulse has a jitter of roughly 500 fs (20), which is orders of magnitude below the required precision for directly timing the AM process. Thus in order to produce the images shown in Fig. 1d we must employ a single-shot diagnostic of the relative arrival time between the x-rays and laser pulse. As described above, in addition to driving resonant excitation near the oxygen K-edge, the attosecond x-ray pulse ionized electrons from the nitrogen K-shell of the NO molecule (see Fig. 1b and 1c). This direct photoionization process produced high energy (120 eV) electrons. The photoionization delay between the arrival of the x-ray pulse and the appearance of these fast photoelectrons in the continuum was negligibly small ( 5 as) compared to the streaking laser period TL of 7.7 fs (2123). Therefore the momentum shift observed for the nitrogen K-shell photoemission feature provided an accurate, single-shot measurement of the direction of the streaking laser vector potential A0 at the time of arrival of the x-ray pulse.
We monitor the AM yield in a small angular region of the detector to avoid introducing artifacts in the extracted time-dependent trace due to angular anisotropy in the AM emission (24). We note that the period of the streaking field was chosen to be longer than the dominant timescale of the AM process. This fact simplifies interpretation of the streaking measurement by limiting the effect of ‘wrapping’, where electrons released into the continuum at time τ and τ+TL experience a similar momentum kick from the streaking field.
The time-dependent electron yield shown in Fig. 1e shows a maximum at τ=0, when A0 was directed along the detection direction, and the the core-excited population (and AM emission rate) was at a maximum. In addition to an exponentially decaying electron emission rate, we observed a revival in the time-dependent emission rate at τ=3.5 fs.

Model

We modeled our measurement according to the theory of attosecond streaking of multiple Fano resonances described by Wickenhauser et al. (25, 26). Our model, illustrated in Fig. 2a, included a ground state which is doubly degenerate and was resonantly coupled to four bound states, one of which ( 2Δ) is also doubly degenerate, and thus is labeled as a single state in the figure. These bound states were also coupled to a single, structure-less continuum, which was dressed by the circularly polarized, 2.3μm streaking laser field. The coupling between the bound and continuum states was the result of electron correlation interactions, and drove the AM decay process. The bound states had excitation energies of 531.5 eV ( 2Σ), 532.6 eV ( 2Δ) and 533.5 eV ( 2Σ+), which represented the core-excitation spectrum of nitric oxide (27). The continuum coupling constant (Γ=170 meV) was consistent with previous x-ray absorption measurements (27). The relative amplitude between transitions to the bound, core-excited states and direct photoionization of valence electrons to the continuum was represented by the Fano parameter, qi (see SM) (28). We choose the value for qi according to the measured absorption spectrum of NO (27).
Fig. 2. Model for Auger-Meitner emission.
(a) presents a schematic representation of the model used for AM emission. Sub-femtosecond x-ray pulses coherently excite four resonances (labeled  2Σ+,2Σ, and a doubly degenerate  2Δ). In addition to the resonant pathway, electrons can be directly ionized by the x-ray pulse, leading to interfering paths from the ground state to the field-dressed continuum (although the direct ionization pathway is a minor channel (14)). (b) shows the calculated photoelectron momentum spectrum for 0.5 fs x-ray pulses centered at 533 eV photon energy in the presence of a 2.3μm laser field. (d) shows the kinetic energy distribution of the continuum electron as a function of time in the absence of the streaking laser field. (e) shows the time-dependent ionization rate for this wavefunction, summed over electron kinetic energy, for a central photon energy of 533 eV (red), 534.5 eV (green), and 536 eV (blue). (f) shows the total population of the core-excited states as a function of time delay for the same photon energies as in (e). (c) shows the time evolution of the electron density of the bound electronic states. The 3D contour is drawn at 20% of the maximum electron density and its transparency represents the overall bound-state population, which decays via AM emission. The blue and red dots in the right most panel show the positions of the nitrogen and oxygen atoms, respectively.
The coherent bandwidth of the exciting x-ray source was 5 eV (12), which was sufficient to span all core-excited bound states in the model. Symmetry constraints do not allow for the coherent population of the  2Σ and  2Σ+ states since the  2Σ and  2Σ+ states each coupled to a different component of the doubly degenerate ground state (14). Moreover, each component of the ground state coupled to a different component of the degenerate  2Δ state (14). Thus the model only included coherence between the  2Σ & one of the  2Δ states and the  2Σ+ & the other  2Δ state, but not the  2Σ &  2Σ+ states. In both simulation and experiment we tune the central wavelength of the x-ray source across the 1s2pπ resonance (red, green and blue shaded curves, bandwidth drawn to scale with energetic separation of core-excited states).
In simulation we could calculate the energy-resolved continuum wavefunction in the absence of the streaking-field, shown in Fig. 2d, demonstrating the build-up of resonant features. The rate of electron emission (integrated over electron kinetic energy) is shown in Fig. 2e), and we clearly observe an oscillatory emission rate. Finally, in Fig. 2f we show the population of each core-excited state as a function of time, which again shows oscillatory behavior. The periodic modulation of the electron emission rate resulted from the coherent population of the two pairs of excited states  2Σ &  2Δ and  2Δ &  2Σ+. Electronic coherence between the pairs of excited states resulted in consecutive minima (maxima) in time-dependent ionization rate, due to destructive (constructive) interference between emission from the core-excited states. Because the core-excited wavepacket consisted of states with different angular momentum projections along the molecular axis, the excited state wavepacket produced an excited electron density which ‘rotated’ around the molecular axis, as shown in Fig. 2c.

Results

We directly modeled our experimental observable by computing the asymptotic (t) momentum distribution of ionized electrons within the Strong-Field Approximation (SFA) (26) (Fig. 2b) and performing the same analysis routine as we applied to the experimental data. The asymmetry parameters describing emission from the oxygen 1s2Σ, O 1s2Δ and O 1s2Σ+ excitations were expected to be different for each of the electronic states (24) and have not previously been measured, meaning the contribution of each channel to emission in the direction of our observation window was not well defined. We fit the simulation to the experimental data using the lower kinetic energy limits of the small detector region defined in Fig. 1e, and the relative contribution from each decay channel at the precise region on the detector, as free parameters. With a separate measurement taken concurrent with the presented data, we determined an error distribution of σ=30  for single-shot vector potential determination. We accounted for this experimental error by convolution of the time-dependent electron yield with a Gaussian kernel of σ=30 . Further details are provided in the SM. We also accounted for the possibility of a small systematic error in t0 determination between experiment and theory, resulting from the finite temporal profile of the reference nitrogen K-shell photoline produced by the attosecond x-ray pulse (12). We identified an offset of 1.7% of the full detector angle.
Figure 3a shows the vector potential-direction dependent electron yield measured at different x-ray excitation energies (black dots) compared with the simulated yield (solid line). The transient revival at τ3.5 fs resulting from electronic coherence in the core-excited state was indicated by the gray arrow and is observed in both experiment and simulation. This feature is a quantum beat, occurring at the moment when the quantum phases of the coherently excited  2Σ and  2Δ excitations re-aligned. This alignment caused constructive interference between the two core-excited states, and an increase in AM emission rate. The feature at 1.3 fs measured at central photon energy 536 eV was possibly due to the temporal build-up of the Fano interference between the resonant and direct excitation channels and has been qualitatively reproduced in further simulation. Analysis of the energetic positions of the Rydberg series converging to the oxygen K-edge (27) was not consistent with the interpretation that this modulation was due to further coherent excitation involving Rydberg states.
Fig. 3. Comparison between model and experimental results for resonant Auger-Meitner emission.
(a) Measurement of time-resolved Auger-Meitner emission from core-excited NO. The left hand panel shows the experimentally measured time-dependent AM yield for various the central XFEL photon energies (black dots). Colored error bars have a total length of four times the standard error of the mean of the measured electron yield, ±2σx¯. This measurement is compared with the results of the model shown in Fig. 2 (solid colored lines). The right hand panel shows total electron yield, which decreases as the central photon energy moves away from the center of the 1sπ resonance (bars). The time-dependent yields change by a factor of 2 between the minimum (normalized to 0) and maximum (normalized to 1) values. The coherent bandwidth of the attosecond XFEL pulse spans 5 eV, as illustrated by a Gaussian curve of equivalent full width at half maximum at each central photon energy. The black line shows the O1sπ feature reported in (27), comprising the  2Σ,  2Δ and  2Σ+ electronic states. The revival at τ3.5 fs, marked by the black vertical arrow, is due to the rephasing (constructive interference) of the AM emission from the core-excited states ( 2Σ and  2Δ) populated by the x-ray pulse. The coherent revival is suppressed as the photon energy moves above the 1sπ resonance and the contribution from the direct photoionization channel increases. The photon energy-dependence of the quantum beat is shown in the zoom-in in panel (b), for experiment (left) and simulation (right). The shaded area represents the streak-angle-dependent yield with corresponding errorbar ±2σx¯ and the solid line shows this electron yield following application of a high-frequency filter along the time axis (see SM for further details). The color of the curves corresponds to the central photon energies shown on the left side of panel (a). (c) Comparison between two different models where core-excited states are populated coherently (deep red) and incoherently (pale red) at 533 eV central photon energy. The experimental measurement is shown in black dots with error bars ±2σx¯. Coherent interaction between the core-excited states is required to account for the measured data.
Figure 3b shows a zoom-in of the revival feature. By tuning the central x-ray photon energy away from the center of the 1s2pπ resonance, we were able to suppress the quantum beat in both experiment (left) and in simulation (right), demonstrating control over the coherent evolution of the core-excited states. The beat was suppressed at higher photon energy due to an increased relative contribution from the direct channel versus the coherently excited resonant decay pathways. In Fig. 3c we compare our measurement, for a central x-ray excitation energy of 533 eV, to our simulation including (deep red) and excluding (pale red) the coherence between the core excited states. As expected, it was only possible to reproduce the revival features by including the coherence between the different core-excited electronic states. The result from incoherent summation of the AM emission from the different core-excited states fails to reproduce the feature at 150 streaking angle.

Conclusion

In conclusion, this work reports the real-time measurement of electronic coherence in the temporal evolution of a core-excited molecule. Electronic coherence imparted a modulation in the time-dependent emission rate of AM electrons, driven by an isolated attosecond soft x-ray pulse from a free electron laser. The AM emission occurred on a few-femtosecond timescale and we time-resolved it using angular streaking. Our measurement provides a testbed for exploring the effect of electronic coherence in the photoexcitation dynamics and subsequent photochemical behavior of molecular systems. The existence of this electronic coherence provides the opportunity to explore inter-atomic site electronic wavepacket coupling, which can reveal interactions between different parts of an extended system (2931). Measuring this coupling can reveal important information on the system’s fundamental physical properties (32, 33). For example, the spectral makeup of the observed modulations provides rich information on the composition of the excited superposition state. This information opens the possibility to observe the evolution and decay of coherent electronic states in real-time, as they evolve and couple to subsequent nuclear motion in the first stages of a photochemical reaction (3437).

Acknowledgments

Funding: S.L., Z. Z., and A.M. acknowledge support from DOE, BES Scientific User Facilities Division Field Work Proposal 100317; J.D. and A. M. were supported by the Laboratory Directed Research and Development Program in support of the Panofsky fellowship. The contributions from T.D., P.H.B., A.K., A.N., J.T.O., T.J.A.W., A.L.W., and J.P.C. were supported by the U.S. Department of Energy (DOE), Office of Science, Office of Basic Energy Sciences (BES), Chemical Sciences, Geosciences, and Biosciences Division (CSGB); E.G.C. was supported by the DOE Laboratory Directed Research and Development program at SLAC National Accelerator Laboratory, under contract DE-AC02-76SF00515. P.R. and M.F.K. acknowledge support by the German Research Foundation via KL-1439/10, and the Fellow program of the Max Planck Society. V.A, J.C.T.B., D.G., J.P.Mar. gratefully acknowledge funding support from UK EPSRC grants No. EP/R019509/1, EP/T006943/1 and No. EP/ I032517/1. N.B., R.O. and A.C.L. acknowledge the Chemical Sciences, Geosciences and Biosciences Division, Office of Basic Energy Sciences, Office of Science, US Department of Energy, grant no. DE-SC0012376. C.B. acknowledges the Swiss National Science Foundation and the National Center of Competence in Research – Molecular Ultrafast Science and Technology NCCR – MUST. L.F.D. and L.F. acknowledge support from NSF Grant No. 1605042 and DOE DE-FG02-04ER15614. W.H. thanks the German BMBF for funding of the project ‘SpeAR_XFEL’ under the contract number 05K19PE1. Use of the Linac Coherent Light Source (LCLS), SLAC National Accelerator Laboratory, is supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences under Contract No. DE-AC02-76SF00515. Author contributions: SL, AM and JPC devised the experimental scheme. S.L., A.M., J.P.C. developed the experimental apparatus. S.L., J.D., J.P.Mac., Z.Z., and A.M. prepared the attosecond X-ray pulses. M-F.L., N.H.S., P.W. prepared the experimental beam-line. All Authors participated in the collection and interpretation of the experimental data. T.D. led the data analysis. S.L., T.D., P.R., and E.G.C. worked on the single-shot ‘streaking’ diagnostic. S.L., T.D., A.M., and J.P.C. prepared an initial version of the manuscript. All authors provided critical feedback in preparing the submitted manuscript. Competing interests: None declared. Data and materials availability: The partially analyzed raw data and the raw data from the calculations is available on the Zenodo repository (38). All (other) data needed to evaluate the conclusions in the paper are present in the paper or the Supplementary Materials.

Supplementary Materials

This PDF file includes:

Materials and Methods
Supplementary Text
Figs. S1 to S8
References (3942)

References and Notes

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Received: 28 April 2021
Accepted: 29 November 2021

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Acknowledgments

Funding: S.L., Z. Z., and A.M. acknowledge support from DOE, BES Scientific User Facilities Division Field Work Proposal 100317; J.D. and A. M. were supported by the Laboratory Directed Research and Development Program in support of the Panofsky fellowship. The contributions from T.D., P.H.B., A.K., A.N., J.T.O., T.J.A.W., A.L.W., and J.P.C. were supported by the U.S. Department of Energy (DOE), Office of Science, Office of Basic Energy Sciences (BES), Chemical Sciences, Geosciences, and Biosciences Division (CSGB); E.G.C. was supported by the DOE Laboratory Directed Research and Development program at SLAC National Accelerator Laboratory, under contract DE-AC02-76SF00515. P.R. and M.F.K. acknowledge support by the German Research Foundation via KL-1439/10, and the Fellow program of the Max Planck Society. V.A, J.C.T.B., D.G., J.P.Mar. gratefully acknowledge funding support from UK EPSRC grants No. EP/R019509/1, EP/T006943/1 and No. EP/ I032517/1. N.B., R.O. and A.C.L. acknowledge the Chemical Sciences, Geosciences and Biosciences Division, Office of Basic Energy Sciences, Office of Science, US Department of Energy, grant no. DE-SC0012376. C.B. acknowledges the Swiss National Science Foundation and the National Center of Competence in Research – Molecular Ultrafast Science and Technology NCCR – MUST. L.F.D. and L.F. acknowledge support from NSF Grant No. 1605042 and DOE DE-FG02-04ER15614. W.H. thanks the German BMBF for funding of the project ‘SpeAR_XFEL’ under the contract number 05K19PE1. Use of the Linac Coherent Light Source (LCLS), SLAC National Accelerator Laboratory, is supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences under Contract No. DE-AC02-76SF00515. Author contributions: SL, AM and JPC devised the experimental scheme. S.L., A.M., J.P.C. developed the experimental apparatus. S.L., J.D., J.P.Mac., Z.Z., and A.M. prepared the attosecond X-ray pulses. M-F.L., N.H.S., P.W. prepared the experimental beam-line. All Authors participated in the collection and interpretation of the experimental data. T.D. led the data analysis. S.L., T.D., P.R., and E.G.C. worked on the single-shot ‘streaking’ diagnostic. S.L., T.D., A.M., and J.P.C. prepared an initial version of the manuscript. All authors provided critical feedback in preparing the submitted manuscript. Competing interests: None declared. Data and materials availability: The partially analyzed raw data and the raw data from the calculations is available on the Zenodo repository (38). All (other) data needed to evaluate the conclusions in the paper are present in the paper or the Supplementary Materials.

Authors

Affiliations

SLAC National Accelerator Laboratory, Menlo Park, CA, USA.
Department of Physics, Stanford University, Stanford, CA, USA.
SLAC National Accelerator Laboratory, Menlo Park, CA, USA.
Stanford PULSE Institute, SLAC National Accelerator Laboratory, Menlo Park, CA, USA.
The Blackett Laboratory, Department of Physics, Imperial College London, London, UK.
SLAC National Accelerator Laboratory, Menlo Park, CA, USA.
Stanford PULSE Institute, SLAC National Accelerator Laboratory, Menlo Park, CA, USA.
Max Planck Institute of Quantum Optics, Garching, Germany.
Physics Department, Ludwig-Maximilians-Universität Munich, Garching, Germany.
Stanford PULSE Institute, SLAC National Accelerator Laboratory, Menlo Park, CA, USA.
SLAC National Accelerator Laboratory, Menlo Park, CA, USA.
Andre Al-Haddad
Paul Scherrer Institute, Villigen, Switzerland.
The Blackett Laboratory, Department of Physics, Imperial College London, London, UK.
Jonathan C. T. Barnard
The Blackett Laboratory, Department of Physics, Imperial College London, London, UK.
Nora Berrah
Physics Department, University of Connecticut, Storrs, CT, USA.
Christoph Bostedt
Paul Scherrer Institute, Villigen, Switzerland.
LUXS Laboratory for Ultrafast X-ray Sciences, École Polytechnique Fédérale de Lausanne, Lausanne, Switzerland.
Department of Physics, Stanford University, Stanford, CA, USA.
Stanford PULSE Institute, SLAC National Accelerator Laboratory, Menlo Park, CA, USA.
Department of Applied Physics, Stanford University, Stanford, CA, USA.
SLAC National Accelerator Laboratory, Menlo Park, CA, USA.
Stanford PULSE Institute, SLAC National Accelerator Laboratory, Menlo Park, CA, USA.
Department of Physics, The Ohio State University, Columbus, OH, USA.
Department of Physics, The Ohio State University, Columbus, OH, USA.
Department of Physics, University of Central Florida, Orlando, FL, USA.
The Blackett Laboratory, Department of Physics, Imperial College London, London, UK.
SLAC National Accelerator Laboratory, Menlo Park, CA, USA.
Zhaoheng Guo
SLAC National Accelerator Laboratory, Menlo Park, CA, USA.
Department of Applied Physics, Stanford University, Stanford, CA, USA.
Gregor Hartmann
Institut für Physik und CINSaT, Universität Kassel, Kassel, Germany.
Daniel Haxton
KLA Corporation, Milpitas, CA, USA.
Department of Physics, TU Dortmund University, Dortmund, Germany.
Zhirong Huang
SLAC National Accelerator Laboratory, Menlo Park, CA, USA.
Department of Physics, Stanford University, Stanford, CA, USA.
Physics Department, University of Connecticut, Storrs, CT, USA.
Andrei Kamalov
SLAC National Accelerator Laboratory, Menlo Park, CA, USA.
Department of Physics, Stanford University, Stanford, CA, USA.
Stanford PULSE Institute, SLAC National Accelerator Laboratory, Menlo Park, CA, USA.
Stanford PULSE Institute, SLAC National Accelerator Laboratory, Menlo Park, CA, USA.
SLAC National Accelerator Laboratory, Menlo Park, CA, USA.
SLAC National Accelerator Laboratory, Menlo Park, CA, USA.
James P. MacArthur
SLAC National Accelerator Laboratory, Menlo Park, CA, USA.
Department of Physics, Stanford University, Stanford, CA, USA.
The Blackett Laboratory, Department of Physics, Imperial College London, London, UK.
SLAC National Accelerator Laboratory, Menlo Park, CA, USA.
Department of Physics, Stanford University, Stanford, CA, USA.
Stanford PULSE Institute, SLAC National Accelerator Laboratory, Menlo Park, CA, USA.
SLAC National Accelerator Laboratory, Menlo Park, CA, USA.
Physics Department, University of Connecticut, Storrs, CT, USA.
Jordan T. O’Neal
Department of Physics, Stanford University, Stanford, CA, USA.
Stanford PULSE Institute, SLAC National Accelerator Laboratory, Menlo Park, CA, USA.
SLAC National Accelerator Laboratory, Menlo Park, CA, USA.
Department of Physics and Astronomy and Purdue Quantum Science and Engineering Institute, Purdue University, West Lafayette, IN, USA.
Aviad Schori
Stanford PULSE Institute, SLAC National Accelerator Laboratory, Menlo Park, CA, USA.
SLAC National Accelerator Laboratory, Menlo Park, CA, USA.
Stanford PULSE Institute, SLAC National Accelerator Laboratory, Menlo Park, CA, USA.
Department of Applied Physics, Stanford University, Stanford, CA, USA.
SLAC National Accelerator Laboratory, Menlo Park, CA, USA.
Stanford PULSE Institute, SLAC National Accelerator Laboratory, Menlo Park, CA, USA.
SLAC National Accelerator Laboratory, Menlo Park, CA, USA.
SLAC National Accelerator Laboratory, Menlo Park, CA, USA.
Stanford PULSE Institute, SLAC National Accelerator Laboratory, Menlo Park, CA, USA.
Max Planck Institute of Quantum Optics, Garching, Germany.
Physics Department, Ludwig-Maximilians-Universität Munich, Garching, Germany.
SLAC National Accelerator Laboratory, Menlo Park, CA, USA.
Stanford PULSE Institute, SLAC National Accelerator Laboratory, Menlo Park, CA, USA.
SLAC National Accelerator Laboratory, Menlo Park, CA, USA.
Stanford PULSE Institute, SLAC National Accelerator Laboratory, Menlo Park, CA, USA.

Funding Information

U.S. Department of Energy: DE-AC02-76SF00515
Neurosciences Foundation: DOE DE-FG02-04ER15614

Notes

These authors contributed equally to this work.
*Corresponding author: Email: [email protected] (A.M.); [email protected] (J.P.C.)

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