Synthesis and characterization of attosecond light vortices in the extreme ultraviolet

Abstract

Infrared and visible light beams carrying orbital angular momentum (OAM) are currently thoroughly studied for their extremely broad applicative prospects, among which are quantum information, micromachining and diagnostic tools. Here we extend these prospects, presenting a comprehensive study for the synthesis and full characterization of optical vortices carrying OAM in the extreme ultraviolet (XUV) domain. We confirm the upconversion rules of a femtosecond infrared helically phased beam into its high-order harmonics, showing that each harmonic order carries the total number of OAM units absorbed in the process up to very high orders (57). This allows us to synthesize and characterize helically shaped XUV trains of attosecond pulses. To demonstrate a typical use of these new XUV light beams, we show our ability to generate and control, through photoionization, attosecond electron beams carrying OAM. These breakthroughs pave the route for the study of a series of fundamental phenomena and the development of new ultrafast diagnosis tools using either photonic or electronic vortices.

ARTICLE

Received 13 Apr 2016 | Accepted 13 Jul 2016 | Published 30 Aug 2016

Infrared and visible light beams carrying orbital angular momentum (OAM) are currently thoroughly studied for their extremely broad applicative prospects, among which are quantum information, micromachining and diagnostic tools. Here we extend these prospects, presenting a comprehensive study for the synthesis and full characterization of optical vortices carrying OAM in the extreme ultraviolet (XUV) domain. We conrm the upconversion rules of a femtosecond infrared helically phased beam into its high-order harmonics, showing that each harmonic order carries the total number of OAM units absorbed in the process up to very high orders (57). This allows us to synthesize and characterize helically shaped XUV trains of attosecond pulses. To demonstrate a typical use of these new XUV light beams, we show our ability to generate and control, through photoionization, attosecond electron beams carrying OAM. These breakthroughs pave the route for the study of a series of fundamental phenomena and the development of new ultrafast diagnosis tools using either photonic or electronic vortices.

DOI: 10.1038/ncomms12583 OPEN

Synthesis and characterization of attosecond light vortices in the extreme ultraviolet

R. Gneaux1, A. Camper2, T. Auguste1, O. Gobert1, J. Caillat3, R. Taeb3 & T. Ruchon1

1 LIDYL, CEA, CNRS, Universit Paris-Saclay, CEA Saclay, 91191 Gif-sur-Yvette, France. 2 Department of Physics, Ohio State University, Columbus, Ohio 43210, USA. 3 Sorbonne Universits, Laboratoire de Chimie PhysiqueMatire et Rayonnement (UMR7614), UPMC Univ Paris 06, 11 rue Pierre et Marie Curie, 75005 Paris, France. Correspondence and requests for materials should be addressed to T.R. (email: mailto:[email protected]

Web End [email protected] ).

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Like massive particles may carry two types of angular momenta, namely spin and orbital angular momenta (SAM and OAM, respectively), the massless photon can be

assigned two such characteristics1. It was recognized earlier that SAM is associated with the circular polarization of light beams, but only 20 years ago was the OAM of light associated with beams with a tilted wavefront2. The unique properties of twisted light beams and their large availability in the infrared and visible spectral regions lead to the emergence of countless applications, from quantum information3 to microscopy4, nanoparticle manipulation5 or ne structuring of materials using pulsed lasers6. In the extreme ultraviolet (XUV) spectral range, technological applications using OAM beams were anticipated7,8, building on predictions of specic light matter interactions9,10. However, because of the lack of sources, most of these predictions could not be confronted to the experiment. Here we rst demonstrate a route based on high harmonic generation to synthesize and characterize helically shaped XUV trains of attosecond pulses. Using this photon source, we also report the experimental synthesis of electronic vortices with attosecond time structure. These breakthroughs pave the route for the study of a series of fundamental phenomena and the development of new ultrafast diagnosis tools using either photonic or electronic vortices or springs11,12, for instance, the observation of new kinds of dichroisms7,8 or the visualization of dislocation strain elds in bulk material13.

The most common implementation of macroscopic beams carrying OAM, typically produced using spiral staircase phase plates, displays a helical phase front, with a phase singularity associated with zero intensity along the axis5. At the photon level, the twisted wavefront of the beam translates into a quantized momentum, with its component along the beam axis taking discrete c values, where c is a positive or negative integer. Laguerre-Gaussian modes (LG) are eigensolutions of the paraxial wave equation and form a natural set for these helically phased beams. Lately, motivated by theoretical predictions, the development of sources of XUV beams carrying OAM was undertaken on both quasi-continuous synchrotron installations14, and on femtosecond free electron lasers15,16. High-harmonic generation (HHG)-based XUV sources constitute a table top, ultrashort and largely tunable alternative to those large-scale instruments. They show unrivalled stability specications, especially useful for pumpprobe experiments targeting attosecond temporal resolution17. They are based on the upconversion of a high-intensity femtosecond visibleinfrared laser beam into the XUV range through highly nonlinear interaction with a gas. When driving HHG with helically phased light beams, momentum conservation predicts a multiplicative rule for OAM transfer11, similar to what is known in low-order nonlinear processes5. The OAM of the harmonic order q is then given by the quantum number cq qc1,

where c1 is the OAM of the driving eld. Two groups measured the helicity of such a harmonic beam: rst, Zrch et al.18 unexpectedly observed, on a single harmonic, that cq c1.

It was argued that this disagreement with theory, which was suggesting violation of momentum conservation, was due to parametric instabilities preventing higher-order vortices from propagating towards the detector19. Later, Gariepy et al.20 succeeded, through ne interferometric measurements performed on three harmonics, in demonstrating the expected multiplicative rule. Therefore, OAMHHG holds the potential for producing XUV pulses of attosecond duration carrying OAM. The shape of such a broad comb of phase-locked helically phased harmonics has been theoretically described11. Such attosecond light springs, as they were dubbed12, could in turn be a unique source to tailor attosecond electron springs through photoionization. Currently,

twisted electron beams, primarily generated through tailoring Gaussian electron beams in the quasi-static regime21,22, are actively studied for future applications in elds covering spectroscopy of diluted and condensed matter23, microscopy and particle physics24.

In the present work, we report on the synthesis of attosecond XUV light springs. First, we show that the multiplicative OAM transfer rule for HHG is valid in our experimental conditions without relying on any diffractive or interferometric technique. Importantly, this approach is directly scalable to an arbitrary spectral range. We then present the results of a two-colour ionization experiment in which we are able to characterize the attosecond structure of the generated light spring, which is in turn used to generate attosecond helically shaped electron beams.

ResultsLink between OAM and divergence in HHG. Twisted attosecond XUV pulses hold great promises for a variety of applications. However, as raised up in ref. 20, a critical point is the characterization of OAM on a broad wavelength range. For instance, the study of helical dichroism in solids is envisioned close to transition-metal K-edges7, which lie at very short wavelengths. In much the same way, the extremely short time resolutions attainable using HHG-based sources are only reached when using a broad spectrum covering a large number of harmonics. In the visibleinfrared range, the characterization is usually done directly using diffractive optical elements or interference schemes5. These approaches were transferred to the XUV domain in the aforementioned lines of work18,20, requiring the resolution of fringes with extremely low spacing because of the short wavelength. These procedures clearly get ever more difcult to implement as the wavelength gets shorter. Here, for our broad harmonic comb, we use a different approach to measure the OAM of the harmonic eld, which does not rely on interferometric measurements. It is based on another signature of the OAM value: the ring-shaped intensity radial proles associated with the vortices phase singularity. In particular, it can be shown that the multiplicative law, cq q c1, is the only one

that yields a single ring with a constant diameter proportional to

1

j j

p over the whole spectrum. Indeed, unlike what is stated in

the Supplementary Information of ref. 18, the enlargement of the rings diameter because of the increase in the OAM is exactly compensated for by the smaller diffraction observed at shorter wavelengths. This statement is supported by both a simple analytical model (see Supplementary Notes 1 and 2) and the results of numerical simulations of HHG25 illustrated in Fig. 1. The simulations were carried out in a similar way as in ref. 11 but taking into account all aspects of a real experiment, including the propagation of the infrared beam towards the gas target (see Methods for more details). As shown in Fig. 1a, the harmonics at focus have a ring-shaped intensity as well as a spiral-shaped phase running q times 2p along the ring. When propagated to the far eld, the harmonic proles show one intense central ring (insets of Fig. 1b), suggesting that the generation is dominated by the emission of a single LG mode. Note that extra faint rings appear around it. They result from both the nonlinearity of the process and an interplay between two different contributions to HHG, associated with distinct electron quantum trajectories at the single atom level (so-called short and long), as explained in ref. 26.

The diameter of the harmonic rings for two different values of c1 is plotted in Fig. 1b. As expected, the diameter is mostly constant apart from a jump around H25, which is precisely where the short and long trajectory contributions are merging. This leads to interferences and a modulation of the spatial prole of the harmonics, similarly to what is observed with Gaussian

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a

b

Intensity (a.u.)

0 1

Phase (rad) 0

8

6

4

2

Ring diameter (mm)

2

100

y(m)

0

100

100 0 100 x (m)

13

15 17 19 21 23 25 27 29 31 33 35

Energy (photon units)

Figure 1 | Calculation of high-order harmonic proles generated with a driving laser carrying OAM. (a) Intensity and phase transverse proles of harmonic 15 close to focus when the driving laser carries c1 1. We observe a well-dened ring-shaped distribution for the intensity (top panel) and a

phase prole linearly increasing by 15 c1 2p along a circle centred on the beam axis (bottom panel). (b) Diameter of the harmonic rings in the far eld

for c1 1 (red circles) and c1 2 (blue triangles), which present a constant diameter proportional to

1

j j

p . Insets: corresponding intensity proles for a

selection of harmonics.

driving beams27. The scaling of the divergence is however very different from the usual Gaussian case, for which the harmonic divergence noticeably changes with harmonic order28. When doubling the OAM carried by the driving eld c1, the harmonic diameter increases by a factor of 1:4 2

p , consistent with the

predicted

a

Gas jet

SP

MCP

L

D

p scaling law.

Generation of attosecond light vortices. The numerical results reported in Fig. 1 were tested experimentally on the LUCA laser facility at CEA Saclay using the experimental set-up described in Fig. 2a. A spiral phase plate (SPP) is inserted to imprint a spiral staircase phase prole on this incoming beam, which is either one, two or three times 2p per round. Focusing such a phase-shaped beam leads to a distribution of light about the focal point very close to a LG mode carrying, respectively, c1 1, 2 or

3 units of OAM, the sign being determined by the orientation of the phase mask29. This is illustrated by the intensity prole reported in Fig. 2b and accurately measured in Supplementary Note 3. XUV harmonic spectra obtained using an infrared driving eld with c1 1, 2 or 3 are displayed in Fig. 2c. For each

harmonic order and all OAM values of c1, we observe a clear ring shape pinched in the horizontal dimension by the dispersion of the grating. The divergence of the harmonics, seen in the vertical dimension, appears to be constant throughout the whole spectrum, as predicted.

We measured the average ring diameters to be 1.010.02,1.330.04 and 1.610.01 mm for c1 1, 2 and 3, respectively, in

agreement within 5% with the anticipated

1

j j

MBES

Grating

1

j j

TM

b

200

1

y(m)

Intensity

(a.u.)

0

0

SPP

200

TS

Optional

200 x (m)

0 200

c

1

1

1

0

0

1

Spatial dimension (mm)

1

1

0

0

1

1

1

0

0

1

1

20 25 30 35 40

1

0

1

Photon energy (eV)

Intensity (a.u.)

p dependency. We

note that we observe only one ring. This is probably because of the selection through phase matching of only the short quantum trajectory. Interestingly, we also note that the harmonics are mostly constituted of one single LG mode. The evidence here is that they show a single ring pattern both at focus (where their shape necessarily mimics that of the driving infrared) and in the far eld, where they were measured. The diameter of the rings being constant throughout the spectrum, the momentum is conserved and the OAM is multiplied by the harmonic order. Here the highest value is obtained when using c1 3, for which

c19 57. We also carried out this experiment in Neon, allowing

0 1

Figure 2 | Experimental observation of HHG spectra carrying OAM.(a) Experimental set-up. It has two operation modes, corresponding to the imaging of HHG light spectra and to the characterization of EWP. The close to Gaussian Ti:Sapphire laser beam is passed through a SPP and used to generate harmonics. They can be either directly imaged using a photon spectrometer or focused inside a MBES, where an extra infrared beam can be added with a delay controlled by a translation stage (TS), allowing to perform RABBIT measurements (Methods). (b) Intensity prole of the laser beam at focus close to the HHG gas inlet. (c) Normalized intensity of harmonic orders 15th to 27th generated in argon and observed in the far eld, using c1 1 (top row), c1 2 (middle row) and c1 3 (bottom row).

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a b

1 1,600

6

4

2

0

2

4

6

0

Intensity (a.u.)

Delay (fs)

Group delay (as)

1,500

1,400

1,300

1,200

1,100

1

0.8

0.6

0.4

Intensity (a.u.)

11 13 15 17 19 21 23

10 12 14 16 18 20 22 Energy (photon units)

Energy (photon units)

c

x (m)

50

50

50

502

1

0

y(m)

Intensity (a.u.)

0

2

Intensity (a.u.)

0

2

Figure 3 | Attosecond electronic beams carrying OAM. (a) Two-colour XUV infrared two-photon photoionization spectrogram of argon for a driving

eld with c1 1. The main lines correspond to odd harmonics, while the weaker oscillating ones, showing a double periodicity of T 1.33 and 2.7 fs, are SBs.

The collection efciency of our spectrometer limits the number of measurable SBs even if the harmonic cutoff lies higher. (b) Delay-averaged spectrum in log scale (red) and group delay of the photoionized EWP (blue circles, the light blue strip about the curve represents the numerical analysis error bar at 3s).

(c) Spatiotemporal shape of the photoelectrons emitted in the forward direction using the intensity proles from Fig. 2c, the group delays from b, and assuming a at cross-section for argon in this energy range. The 3D surface is a contour at 80% of the maximum intensity. The black and white back panel is a projection of this intensity in the t 2 fs plane. (d) Temporal cuts at three different azimuthal angles in the electron beam y 0 (red), 40 (dashed

blue) and 60 (green).

us to reach an OAM c41 41 with c1 1 while keeping a clean

spatial prole (see Supplementary Fig. 3). Combined with the spectral phase locking inherent to the HHG process, this opens a way of synthesizing attosecond light pulses carrying extremely high mean values of OAM. In the next section, we demonstrate that the harmonics generated with a helically phased infrared beam are phase-locked and use the resulting attosecond light spring to shape electron wave packets (EWP) through photoionization.

Attosecond electron vortices. Since the early days of attophysics it has been recognized that attosecond XUV pulses could tailor EWP through photoionization17,30. Applications of such attosecond EWP were proposed, for instance, as a quantum stroboscope31, or as tools to localize EWP in space and time around atoms and molecules32. In the present context, we propose to increase the tailoring knobs by transferring the OAM carried by the harmonics on photoionized electrons, resulting into electron bursts carrying OAM. We demonstrate the synthesis of such helically shaped electron beams through an interferometric measurement based on the well-established XUVinfrared cross-correlation technique called RABBIT33 (reconstruction of attosecond beating by interference of two-photon transitions), in which synchronized XUV harmonics and infrared beams ionize a target gas. Thus, an electron can be promoted to a given nal state called sideband (SB) through two quantum paths involving the absorption of one photon coming

from consecutive harmonic orders and the absorption/emission of one infrared photon. The resulting quantum interference leads to oscillations of the SB yield as a function of the XUV/infrared delay at twice the infrared laser period and its phase is the sum of the total relative phase of the harmonic orders involved plus that of the two-photon dipole transitions at play, denoted by Djq.

Most importantly, for the interference to be observed, a constant phase relation between the XUV and infrared elds across the gas jet is required. Using a twisted XUV beam (see Supplementary Note 4), this condition is met with a dressing infrared beam carrying the OAM c1, but not with a standard

Gaussian dressing beam (see Methods).

Our experimental test is based on a MachZehnder interferometer sketched in Fig. 2a. Scanning the XUVinfrared delay, we observe the expected 2o oscillations of the SBs intensity (Fig. 3a). We also see some o oscillations, which are due to a modulation of HHG by the second infrared eld but do not hinder the 2o SB analysis33. As in standard RABBIT measurements, the phase of the 2o oscillation is directly linked to the group delay (GDCDjq/2o, with o 2p/l) of the EWP

generated at the atomic level by the harmonic comb. This GD exhibits a linear dependence, with an increase of Dte 1039 as

between consecutive odd harmonic orders, which is consistent with the reported values using a Gaussian beam with the same driving wavelength and peak intensity33. The presence of the 2o oscillations demonstrates that the azimuthally spinning infrared intensity is matched with the XUV light spring on the subcycle

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timescale. As explained in the Methods section, this is again consistent with momentum conservation. Supplementary Fig. 5 shows that, if we dress the harmonics with a Gaussian infrared beam, the oscillations wash out as expected. The RABBIT trace also demonstrates the spectral phase-locking of the high harmonic orders, thus conrming the attosecond light spring structure of the XUV bursts generated with a helically phased infrared beam.

DiscussionThe two sets of measurements reported above, that is, the spatial intensity prole of the harmonics and their GD nally provides us with all data needed to reconstruct the full spatiotemporal shape of the emitted attosecond electron beam. We hereafter focus in the case of photoelectrons with linear momentum along the propagation axis, which directly reproduce the spring structure of the XUV beam. As lately predicted11,12, owing to the low GD over our spectral range, we get two intertwined spring-like structures (Fig. 3c). The helical shape is a direct consequence of the ionizing XUV light structure, while the presence of two spirals is reminiscent of the generation of odd harmonics only. A cut in the spatial domain displays a double lobe structure, while the temporal prole shows a train of attosecond pulses lasting B200 as (Fig. 3d). An interesting characteristic of this structure is that it leads to an identical attosecond pulse train when observed at different azimuthal positions, only delayed by 7.4 as.degree 1 (half a period of the infrared driving laser (1,330 as) in 180 degrees). Turning back to light springs, as shown in ref. 11, the corkscrew structure still holds in the case of single attosecond pulses. We believe that this property makes such pulses powerful tools for transient absorption spectroscopy experiments, which require tunable pumpprobe delays on the attosecond timescale. Here one may angularly map the attosecond time delay in a single shot, getting rid of any stability requirement. The dynamical range for the delay scan is here 1.33 fs, that is, the infrared laser half optical cycle, which could easily be increased up to several femtoseconds by increasing the driving eld wavelength.

In conclusion, we reported on the synthesis and full characterization of attosecond XUV pulses and electron beams, both carrying OAM. The experimental evidence for the transfer of OAM is obtained over an extremely broad spectral range down into the XUV region. This divergence-based analysis method can easily be generalized to arbitrarily large spectral bandwidths. The attosecond structure of the generated XUV pulse train was determined through a photoionization-based cross-correlation technique. First, it conrms the conservation of the standard photoionization selection rules when using helically phased XUV light beams. Second, it opens the route to the manipulation of attosecond electron beams carrying OAM, which will use the large panel of attosecond tools developed in the past 15 years, may it be through high harmonics spectroscopy or XUVinfrared pumpprobe experiments. In particular, helical dichroisms were predicted in the XUV spectral range and still remain to be observed. Multicolour HHG using such tailored beams could also provide all-in-one pumpprobe schemes, taking advantage of the spatial encoding of the delay in the azimuthal coordinate of these beams. Finally, the accurate characterization of these new light beams will pave the way to the study of the controversial coupling between SAM and OAM in matter during photoionization.

Methods

Theoretical details. In this paragraph we provide details about the simulation of HHG using a driving laser carrying an OAM. For the infrared beam, we accounted for the full experimental set-up sketched in Fig. 2a. To this end, the beamwas propagated through the different optical elements, by means of the HuygensFresnel integral, up to the gas jet entrance. We consider a spatially and

temporally incident Gaussian beam of 6.25 mm waist and 50 fs duration (full width at half maximum, FWHM). It is propagated through a SPP and focused by a 1 m focal length lens, in the middle of a 500 mm wide (FWHM) Lorentzian argon jet.

The wavelength l is 800 nm and the phase plate here imposes a c1 2p phase shift

along a circle centred on the beam axis (c1 1 here). The equivalent Gaussian

beam waist at focus w0 is 40 mm, leading to an equivalent Rayleigh range zR of6.5 mm. The maximum gas pressure is 10 mbar and the laser peak intensity at focus is 1.5 1014 W cm 2. This is the starting point for HHG calculations. The

structure of the LG mode, which does not possess the cylindrical symmetry of a Gaussian beam, required performing four-dimensional (three-dimensional (3D) in space time) simulations. In brief, the coupled propagation equations for the

driving laser and harmonic elds are numerically solved on a 3D spatial grid, in the paraxial and slowly varying envelope approximations, using a standard nite-difference method. Calculations are performed in a frame moving at the group velocity of the laser pulse, that is, the speed of light in vacuum here. Both electron and atomic dispersions are taken into account. We rst computed the driving eld at a given time t in the pulse envelope and position z along the propagation axis. This eld is then used for calculating the space- and time-dependent ionization yields and dipole strengths. Ionization rates are modelled using Ammosov DeloneKranov tunneling formula34, while dipoles are computed in the strong eld approximation, following the model described in ref. 35. Once these two terms are obtained, the equation of propagation for the harmonic eld is solved. The calculation is repeated for each t and z. The SPP inducing the OAM is modelled by j x; y

1 tan 1 yx, where x and y are the coordinates in the plane perpendicular

to the propagation axis. The results of the calculations are reported in Fig. 1.

As expected, HHG occurs along the peak intensity ring of the generating infrared beam. The FWHM of the prole obtained by a cut along a radius of this ring (hereafter called the thickness of the ring) is a fraction of the thickness of the ring of the driving eld, a consequence of the high nonlinearity of HHG. As for the spatial phase, a typical example is given in Fig. 1 by the 15th harmonic order (H15), showing a spiral running 15 times 2p along the ring. This implies that the H15 photons carry 15 times the OAM of the fundamental frequency photons. This behaviour is consistent with the multiplicative law of perturbative nonlinear optics, and was observed here for all computed harmonic orders, from H11 to H33. Finally, to mimic the experiment, we simulate the propagation of the XUV beam towards an observation plane located 80 cm downstream the gas cell. When reaching the detector the harmonic beam still displays a ring shape, suggesting that generation at focus is dominated by the emission of a single LG mode. The ring diameter increases by a factor of 1:4 2

p when doubling the helicity of the phase. This may be guessed from analytical considerations presented in Supplementary Note 1, which show, under reasonable hypotheses, that the divergence of harmonics goes like

p .

1

j j

Experimental details. The experimental set-up is sketched in Fig. 2a. The experiments were performed using the LUCA laser server at CEA Saclay, which delivers 30 mJ, 50 fs, 800 nm pulses at 20 Hz. The laser Transverse Electromagnetic Mode TEM00 was converted using a 16-level SPP manufactured by SILIOS

Technologies. For RABBIT measurements, the laser is split into two uneven parts using a mirror with a 8 mm hole. The main (outer) part of the beam is focused by a 1 m focal length lens (L) into a gas jet provided by a piezoelectric driven valve (Attotech). We could verify that even after reection off a drilled mirror, the infrared focus kept a donut shape and so did the harmonics, with again a constant divergence. A diaphragm (D) removes the remaining infrared beam, while the harmonics are focused by a 0.5 m focal length toroidal mirror into the sensitive region of a 1 m long magnetic bottle electron spectrometer time of ight (MBES). A SiO2 plate serves as further attenuation of the infrared beam. An extra plain weak infrared beam (4 mm diameter, energy of 70 mJ) may be superimposed and synchronized with the XUV beam in the MBES with a delay controlled by a piezoelectric transducer. Focus imaging in the sensitive region of the electron spectrometer reveals a thick donut prole for the dressing beam, ensuring a homogeneous dressing of the XUV. For intensity measurements, the drilled mirrors are replaced by plain mirrors and the lens has a 2 m focal length. The harmonics are collected downstream the MBES on a photon spectrometer made of a variable line spacing Hitachi grating (001-0437) and a micro channel plate coupled to a phosphor screen. In order to reveal the 2D spatial prole of the harmonics while spectrally resolving them, the MCP are placed 8 cm before the at eld of the grating. The phosphor screen is imaged with a Basler A102f CCD camera. The observation distance from the source to the MCP is 115 cm. We could generate harmonics in argon gas with c1 1, 2 and 3 (Fig. 1) and neon gas with

cq 1 up to H41 (Supplementary Fig. 3). In all cases, we observed a constant ring

diameter over the whole XUV spectral range, conrming the general validity of our rst measurements in argon. The maximum value of OAM obtained was c19 57

using c1 3 in argon.

RABBIT with a beam carrying an OAM. The theory of quantum interferometry used to characterize attosecond XUV pulses usually consider at wavefronts for both the XUV and dressing infrared beam. Here we anticipate the wavefront of the XUV to be tilted. To be more specic, we assume that the spatial phase of the q-th harmonic within the beam is Fq(R,y) cqy, where the (R,y) polar coordinates

refer to the beam axis (R 0). The measured SB intensity is an average of the

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contributions of all emitted electrons in the interaction region. If we write the intensity coming from one point in this region, neglecting the contributions of the so-called atomic phase, we get for the 2o oscillating component33:

SBq1 o; R; y

cos 2ot0 jq2 jq Fq2 R; y

Fq R; y

2FIR R; y

h i

cos 2ot0 jq2 jq q2 q 21

h i;

where o is the angular frequency of the driving laser and jq the spectral phase of the q-th harmonic order. For the intensity to keep oscillating after integration over y, which is the operation mode of our detector, the y-dependent term must vanish, giving cq2 cq 2c1. In particular, if dressing with c1 1, this condition is only

met when having cq qc1. The observation of SBs in this case is therefore another

measurement of the multiplicative rule for OAM transfer. Supplementary Fig. 5 shows that the 2o oscillation component disappears when using c1 0, for which

the y-dependent term does not cancel. The RABBIT33 analysis of the SBs oscillations was carried out under the assumption of fully coherent light36.

Data availability. The data that support the ndings of this study are available from the corresponding author (T.R.) upon request.

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Acknowledgements

We are particularly grateful to Vincent Gruson, Pascal Salires, Fabien Qur and Bertrand Carr for stimulating discussions and fruitful suggestions. T.R. acknowledges Antonio Zelaquett Khoury (Univ. Fed. Fluminense, Brazil) for inviting him and introducing him to this topic. This work was supported by the French Agence Nationale de la Recherche (ANR) through XSTASE project (ANR-14-CE32-0010). A.C. acknowledges support of the US Department of Energy, Ofce of Science,Ofce of Basic Energy Sciences under contract DE-FG02-04ER15614.

Author contributions

R.G., A.C. and T.R. conceived, built and carried out the experiment and analysed the data. O.G. developed the laser system and the mode-ltering stage. T.A. did the HHG simulation. J.C. and R.T. did the RABBIT simulations. All authors contributed to the writing of the manuscript.

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How to cite this article: Gneaux, R. et al. Synthesis and characterization of attosecond light vortices in the extreme ultraviolet. Nat. Commun. 7:12583 doi: 10.1038/ncomms12583 (2016).

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