Optical properties of relativistic plasma mirrors

Abstract

The advent of ultrahigh-power femtosecond lasers creates a need for an entirely new class of optical components based on plasmas. The most promising of these are known as plasma mirrors, formed when an intense femtosecond laser ionizes a solid surface. These mirrors specularly reflect the main part of a laser pulse and can be used as active optical elements to manipulate its temporal and spatial properties. Unfortunately, the considerable pressures exerted by the laser can deform the mirror surface, unfavourably affecting the reflected beam and complicating, or even preventing, the use of plasma mirrors at ultrahigh intensities. Here we derive a simple analytical model of the basic physics involved in laser-induced deformation of a plasma mirror. We validate this model numerically and experimentally, and use it to show how such deformation might be mitigated by appropriate control of the laser phase.

Introduction

Ultrafast laser technology now makes it possible to study the interaction of femtosecond laser pulses with plasmas in an extreme regime, where the motion of electrons in the laser field is relativistic1. With several facilities aiming at peak powers beyond a PetaWatt, the study of new regimes of quantum electrodynamics should thus become feasible in the near future2. The rapid growth in the number of high-power ultrashort lasers is also driven by the perspective of societal and scientific applications, such as compact laser-driven particle accelerators3,4,5.

These laser developments and their prospects call for new types of optical elements, which can be used to manipulate and tailor ultrahigh-power laser beams at very high intensities I, both in the temporal and spatial domains. As soon as I1013 W cm−2, any medium gets strongly ionized by the field, making conventional optics inappropriate: in this regime, optical components will inevitably consist of a plasma medium. Easy to use and versatile, plasma mirrors (PMs) have a major role to play as high-intensity optical components6, and constitute simple testbeds for models of relativistic laser–plasma interaction.

PMs are already routinely used at moderate light intensities (1014−1016 W cm2) as ultrafast optical switches, to enhance the temporal contrast of femtosecond lasers6,7,8,9. As I1016 W cm−2, the nonlinear response of PMs to the laser field results in subcycle temporal modulations of the reflected field, associated to high-order harmonic generation (HHG) in its spectrum10,11. These harmonics, generated through different mechanisms, are associated in the time domain to attosecond pulses12,13. Beyond ~1018 W cm−2, a key HHG mechanism is the relativistic oscillating mirror (ROM) where the laser-driven oscillation of the plasma surface induces a periodic Doppler effect on the reflected field11,14,15,16,17, which can result in harmonic orders of several thousands18. PMs thus hold great promise for the generation of intense attosecond pulses of light19,20, which would break down a major barrier in attosecond science, opening the way to potential ground-breaking applications such as pump-probe experiments on electron dynamics in matter21.

In addition to these temporal effects, the initial solid target on which the PM is created can be geometrically shaped to also spatially manipulate the reflected beam. At moderate intensities, elliptical PMs have thus recently allowed extremely tight focusing of a high-power laser beam22. In the relativistic regime, curved PMs have been proposed as a way to focus the very high generated harmonic orders to a spot size w<<λL (where λL is the laser wavelength)17,23. Combined with their attosecond temporal bunching, this is a promising path to boost the peak intensity of ultrashort lasers, which might help approaching the Schwinger limit24 Is=2.25 × 1029 W cm−2, where the light field starts inducing electron-positron pair creation from vacuum25,26.

In these high-intensity applications, the laser field exerts such a high pressure on the plasma (typically 5 Gbar for I≈1019 W cm−2) that it induces a significant motion of the PM surface, even during a femtosecond laser pulse. Any spatial variation of the intensity on target, as generally occurs at or around focus, then leads to a deformation of the PM surface—typically a curvature—which can affect the spatial27,28,29 and spectral30 properties of the reflected beam. Beyond its fundamental interest, understanding and controlling this intrinsic dynamics of PMs is crucial for any of the previous applications. In particular, it determines the divergence of attosecond beams produced from PMs, which is a key parameter for future experiments.

In this article, we elucidate the physics of the light-induced curvature of PMs, with an analytical model of the surface dynamics and its consequences on the reflected light. Despite its simplicity, it captures the essential aspects of this process, and disentangles the influences of electron and ion dynamics in the femtosecond regime. Owing to their small wavelengths, high-order harmonics generated on PM are strongly affected, and thus constitute sensitive probes of its curvature. We present some of the most exhaustive measurements of the ROM harmonic properties performed to date, which we use to validate this model experimentally. Controlling the spatial properties of these harmonics is crucial for future applications in attosecond science. We finally demonstrate that such a control can be achieved very simply by using the spatial phase of the driving laser.

Results

Model of laser-induced PM curvature

Properly describing the PM surface motion requires taking into account both the plasma electron and ion dynamics. The response time of electrons to the laser field is much smaller than the optical period, while ions react on a longer timescale because of their larger mass. Akin to the Born–Oppenheimer approximation in molecular physics, this makes it possible to model the system in the following three steps: (i) we first describe the quasi-instantaneous response of electrons to the laser field, considering a given ion background (Fig. 1a); (ii) we then calculate the slow ion motion, resulting from the combined actions of the laser field and of the charge separation fields it induces (Fig. 1b) and (iii) finally, the influence of the slow dynamics on the fast one is included to determine the surface motion over the entire laser pulse (Fig. 1c). The derivations of all formulas and their validation by particle-in-cell (PIC) simulations are provided in the online Supplementary Information.

Figure 1: Laser-induced curvature of a relativistic PM.
figure1

(a) Spatial map of the plasma electron density ne(x,y) at the maximum of a laser pulse with a gaussian focus, from a 2D PIC simulation (aL=8, L=λL/8, θ=45°) performed with fixed ions. (b) Same spatial map, now for the plasma ion density ni(x,y) (charge state of the ions Z=1) at the maximum of the laser pulse, from a 2D PIC simulation with moving ions in the same interaction conditions as in a. (c) Temporal evolution of the electron density ne(x,t) at the centre y=0 of the laser focal spot, with moving ions. A logarithmic scale is used in all cases, and densities are expressed in units of nc. In a and b, the dashed curves show the predictions of the model (equation (1) in a, equation (2) in b). The results of the total model for xT(t)=xi(t)+xe(t), which combines electron and ion dynamics, are shown by the black dots in c. In d, this model is used to disentangle the contributions of the electron dynamics and ion dynamics to the total surface displacement by plotting the following: (i) the electron surface displacement when no ion motion occurs, calculated using equation (1) with a fixed value n0=nccos2θ, (ii) the ion surface displacement xi, calculated using Equation (2), and (iii) the total displacement xT=xi+xe, where is now the electron surface displacement calculated when ion motion is taken into account, by using n0=n(xi) in equation (1). Panels e and f sketch the electron (red) and ion (blue) density profiles, at two different times of the laser pulse, and define the different quantities used in the model. All surface displacements are calculated with respect to the reference position xe=xi=0, where the laser field reflects at the very beginning of the laser pulse, at low intensity. For an angle of incidence θ, this is the point where n=nccos2θ, which also corresponds to the value of n0 in equation (1) at the beginning of the interaction.

Qualitatively, the plasma electrons respond to the laser field as a spring, being alternatively pushed inside, and pulled outside the ion background in each optical period17. When pulled outwards, they form relativistic electron jets (red arrow in Fig. 1a) that are responsible for the ROM attosecond pulse emission. When pushed inwards, a high-density spike is formed at the sharp surface of the electron distribution (white arrow in Fig. 1a), at a position xe(t) (Fig. 1e,f). A detailed analysis of PIC simulations (see Supplementary Note 1) shows that the position of the outgoing electron jet responsible for the emission of an attosecond pulse in each laser cycle is tied to the position of the high-density spike formed in this compression phase, and thus follows the same evolution as the laser intensity changes in time or space. We therefore concentrate on the value of xe(t), which can be easily determined by the balance between the pushing force exerted by the laser field, and the restoring force exerted by the ion background. In the relativistic regime, this balance leads to the following expression for the maximum inward excursion xe of electrons in a given optical period:

where θ is the angle of incidence of the laser on the PM and nc is the critical plasma density at the laser frequency. n0 is the ion charge density at the ion-vacuum boundary (Fig. 1e,f), that is, the density from which the laser field starts pushing electrons inside the ion background. For this derivation, the ion density gradient at the PM surface has been assumed to be exponential beyond n0, with a scale length L, that is, n(x)exp(x/L) for n>n0 (Fig. 1e,f). L is a crucial parameter of the interaction, which in particular strongly affects the HHG efficiency11,31,32. xe increases for larger values of L in equation (1) because the laser field can more easily push electrons inside a smoother ion background.

The electron boundary displacement xe also increases with , the amplitude of the normalized vector potential of the incident laser field: the higher this amplitude, the further electrons get pushed inside the target. For a focused laser pulse, the field envelop is a function of both time and space, aL(y,t). The spatial envelop results in an overall spatial curvature—a denting—of the plasma electron density surface. This laser-cycle-averaged curvature is clearly observed on a spatial map of electron density at t0 corresponding to the laser pulse maximum (Fig. 1a). It is very well reproduced by the curve xe[aL(y,t0)] deduced from equation (1) and can be attributed to the spatially inhomogenous ponderomotive force exerted by the laser field.

As for the temporal evolution xe(t) associated to the laser pulse temporal envelop, the prediction of equation (1) is shown as a red dashed line in Fig. 1d, in the case of a fixed ion background: electrons move back to their initial position in the falling edge of the laser pulse, owing to their immediate response to the field aL(t) (equation (1)) and the restoring force from the ion background. However, this temporal evolution will be affected when ion motion is taken into account, because n0 then becomes a slow function of time in equation (1). The second step of our model aims at determining n0(t).

The charge separation induced by the laser field between the electron and ion populations leads to a quasi-electrostatic field in the plasma, which peaks around xe and tends to accelerate the ion population located around this position33. This acceleration expels the ions from this location, which results in an erosion of the ion density gradient in time. The position xi of the ion-vacuum boundary thus drifts inwards during the laser pulse, and the density n0=n(xi) increases in time (Fig. 1e,f).

The so-called hole-boring velocity υp=dxi/dt of the ion surface can be calculated by writing a momentum flux balance34,35,36,37,38. The reflection of the laser beam corresponds to a change in momentum of the field, which is compensated by an opposite change in momentum of the plasma particles. To determine how the light momentum is shared between electrons and ions, we use the same approach as developed independently in ref. 39, that is, we also write the energy flux balance, assuming that the absorbed laser intensity (1−R)I (where R is the plasma reflection coefficient for the laser) is entirely carried away by electrons. The combination of these two balances leads to:

with Π0=(RZmecos θ/2AMp)1/2, where Z and A are, respectively, the average charge state and mass number of the ions, Mp is the proton mass and me is the electron mass. The prediction of this equation for xi(y,t0) at the laser pulse maximum t0 is shown as a blue line in Fig. 1b, and fits well the surface of the superimposed ion density map obtained from a PIC simulation with mobile ions. The derivation of equation (2) shows that this curvature of the ion surface is induced by the spatially inhomogenous laser radiation pressure on the PM.

The temporal evolution xi(t) is represented in Fig. 1d by the blue line. As opposed to xe, the ion boundary displacement xi does not return to its initial value at the end of the pulse. This is because xi depends on the time integral of aL (see equation (2) where aL corresponds to the envelop of the laser field), indicating that it is the cumulated action of the laser field over time that is responsible for the ion dynamics. This results in a progressive change in the ion profile, which in turn affects the electrons dynamics. This coupling is included in our model in a very simple way.

Owing to the erosion of the ion density profile, the laser field now starts pushing the electrons inside the ion background directly from xi(t), instead of xi=0 initially. Consequently, the position of the electron boundary xT(t) when ion motion is taken into account is now given by xT(t)=xi(t)+xe(t) (see Fig. 1f). In this equation, the value of xe(t) is also affected by ion motion because the restoring force induced by the ions initially located between x=0 and xi(t) is suppressed. As explained before, this second effect is accounted for simply by using n0=n(xi(t)) in equation (1).

The temporal evolution of the electron boundary resulting from these coupled dynamics is illustrated in Fig. 1c. An excellent agreement is obtained between the PIC simulation and the prediction of the full model (black dots). An extensive parametric study of the surface dynamics, using hundreds of PIC simulations, confirms the excellent accuracy (≤5%) of this model over a broad range of physical conditions (see Supplementary Note 2).

Figure 1d uses our model to highlight the relative contributions of ion and electron dynamics in the case of the simulation of Fig. 1c. Despite the brevity of the pulse, the influence of ion motion on the position xT of the electron boundary becomes significant in the second part of the pulse (beyond t≈10 TL). Its main effect is to prevent the electron boundary from moving back to its initial position in the falling edge of the laser pulse, which has observable consequences in experiments, as we will see later. As expected intuitively, the influence of ion dynamics on the total PM surface motion is predicted to become more and more significant as the laser pulse duration increases (Fig. 2).

Figure 2: Influence of ion motion on the plasma surface displacement.
figure2

This colour map shows the relative change in the plasma electron boundary displacement at the peak t0 of the pulse, δx/xT=(xTxeFI)/xT, when ion motion is taken into account (xT=xi+xe(n0(t))) and when ions are considered as fixed (xeFI, equation (1) with a constant n0), as predicted by our model. This is plotted as a function of aL and pulse duration for a typical value of the density gradient (L=λL/10). The white dot corresponds to the interaction conditions of the experiment performed with UHI100.

The laser-induced denting of the PM leads to a curvature of the wavefronts of the reflected light beam, which tends to focus this beam—including the harmonics generated on reflection—in front of the surface27,29. This is clearly observed in Fig. 3 on the attosecond pulse train generated by the ROM mechanism, which is focused at a distance zn from the surface, with a magnification ratio γn=wf/wn<1. This focusing of the beam naturally tends to increase its divergence. Assuming a Gaussian intensity profile of width wn for the nth harmonic in the source plane, this divergence is given by (see Supplementary Note 3):

Figure 3: Focusing of ROM harmonics by a curved PM in a 2D PIC simulation.
figure3

The laser-induced curvature of the PM surface tends to focus the reflected light in front of the PM. Higher harmonic orders are more affected by this curvature owing to their smaller wavelengths. The right panel shows a spatial map of the plasma electron density ne at the maximum of the laser pulse in dark purple scale. A zoom on the surface is shown in the left panel, which also defines the denting parameter δT. The multicolour map shows the intensity I(y′,t) of the train of attosecond pulses obtained by filtering ROM harmonics from order 4–8 at three different times during its propagation away from the PM. Focusing of this train at a distance znfpcos θ from the PM surface is observed, where fp is the focal length of the curved PM (here zn≈25 λL. that is, 20 μm for λL=800 nm).

Ψn is the PM dimensionless focusing parameter for the nth harmonic, which characterizes the effect of the PM curvature on all spatial properties of the reflected beam:

with λn=λL/n the harmonic wavelength. Here δT is defined as (Fig. 3, left), that is, it is the difference between the surface position at the centre of the focal spot y=0, and its position at (with wL the half spatial width at 1/e of the laser field amplitude). In equation (3), is the divergence that would be obtained in the absence of surface curvature, that is, imposed by diffraction from the source plane. It can be expressed as a function of laser divergence .

In equation (3), each term of corresponds to a different physical limit. If Ψn<<1 (for example, δT<<λn or wn<<wL), surface curvature has a negligible effect on the spatial properties, which are determined only by the beam diffraction from the source plane. On the opposite, if Ψn>>1, the focusing induced by the PM imposes the beam divergence, leading to . Ψn is in principle a function of time. However, our model shows that after a fast transient of less than five laser periods only, δT and hence Ψn weakly vary in time (black dots in Fig. 1d). As a first approximation, we therefore neglect its temporal variation in our study of the spatial properties of the reflected beam.

This model for the reflected beam properties has been successfully compared with a series of two-dimensional (2D) PIC simulations (see Supplementary Note 4). In the interaction conditions corresponding to the present state of the art of femtosecond lasers (aL10, LλL/5), it predicts δT≈0.1λL (80 nm for λL=800 nm) and Ψn≈0.6n typically. The effect of surface curvature thus already becomes significant for harmonic orders n3. We now turn to an experimental investigation of the spatial properties of such harmonics, to validate the model, and show what insight it provides on HHG, and more generally on the physics of PMs.

Experimental study

The experiment was performed on the UHI100 laser of IRAMIS (CEA, France), which delivers 25 fs pulses with a peak power of up to 100 TW and an ultrahigh temporal contrast (see Methods section). This beam was focused in p-polarization to a spot size of 4 μm on a silica target, reaching an estimated peak intensity of 6.7 × 1019 W cm−2 (aL=5.6), thus producing a relativistic PM. The density gradient scale length L at the PM surface was varied by using a small controlled prepulse, intense enough to create a plasma (I=1016 W cm−2) at an adjustable delay τ (0≤τ≤2 ps) before the main pulse. The value of L was determined experimentally using time-resolved interferometry32,40.

Under these conditions, high-order harmonics are produced in the reflected beam by the ROM mechanism6,18, and two diagnostics were used to characterize the spatial properties of the resulting harmonic beam in the far field (see Fig. 4a,b and Methods section). The spectrally resolved divergence, extracted from images such as shown in Fig. 4a, is presented in Fig. 4c,d as a function of harmonic order and of the density gradient L at the PM surface. The full lines show the results of the model. The only two unknowns of the model are the plasma reflectivity R (used only to calculate the ionic contribution to the surface curvature) and the ratio of harmonic and laser source size wn/wL (used to deduce the harmonic divergence from the surface curvature). These are, however, not used as free parameters to fit the data, but are directly extracted from 2D PIC simulations performed in the physical conditions of the experiment (see Methods section). This provides R≈0.7 and wn/wL≈0.5 for the 25th harmonic. Parametric studies (see Supplementary Note 3) show that these values hardly change over a broad range of interaction conditions (aL and L). In addition, we note that R hardly influences the results, since it only affects ion motion and appears in a square root in Equation (2). These curves are in remarkable agreement with the measurements, thus validating the model and showing it can be used to gain insight on the physics involved in this experiment. Note that this agreement was obtained without introducing any additional ‘intrinsic phase’ ϕ, such as the one described by an der Brügge and Pukhov30. Our model actually suggests that this phase is simply given by ϕ=2πxe/λL where xe is the electron denting provided by Equation (1), and is thus implicitly included in our analysis. This expression exactly predicts the scaling of ϕ obtained in ref. 30 for normal incidence, fixed ions, and a step-like plasma surface in the limit of ultra-relativistic intensities.

Figure 4: Measurements of ROM harmonic beams divergence.
figure4

(a,b) Typical raw images obtained with the UHI100 laser. See Methods section for a description of the diagnostic instruments. Image a shows the angularly resolved harmonic spectrum measured in the far field, for a peak intensity of I=3.5 × 1019 W cm−2 (aL=5.6) and an initial density gradient L=λL/20. The apparent decrease of the harmonic divergence with order is mainly an effect of the 2D colour map. Image b displays the full far-field spatial profile of the beam corresponding to the superposition of harmonics 20 to ~35, measured in similar interaction conditions. The shadow of the supporting mesh of the thin Si filter used to select a group of harmonics is clearly observed. From these images, quantitative information on the harmonics spatial properties can be extracted. Panel c thus shows the spectrally resolved divergence (in units of laser divergence θL, with θL=200 mrad in our experiment) as a function of harmonic order, for two values of the density gradient L. The plot in d is the divergence of the 25th harmonic as a function of L. In both panels, the full lines show the results of the model. The divergence that would be imposed by diffraction from the same source size in the absence of the laser-induced PM curvature is shown as the dashed lines in c and d. A fully consistent set of parameters was used for all curves. All experimental data points correspond to a single laser shot. The two shots displayed in panel c correspond to the data points for which the absolute value of the divergence is in best agreement with the model in panel d.

Comparing the measured divergences with those that would be obtained by diffraction from a flat PM for the same source size (black dashed lines in Fig. 4c,d) shows that the harmonic divergence is close to this limit when L is small, but is then very significantly increased by the PM curvature, here by a factor of up to 3, for the typical gradients that optimize the ROM conversion efficiency (L≈0.05–0.1λL)11,31,32. This analysis provides a clear indication of the focusing of the harmonics in front of the PM because of its surface curvature. The measurements of Fig. 4d show that this focusing increases with the gradient scale length L, as expected from the model, since a longer gradient leads to a softer restoring force from the ion background, and hence to a larger surface denting δT.

The laser pulse duration used in this experiment is so short that ion motion has little influence on the PM curvature, and hence on the harmonic divergence (white dot on Fig. 2). According to Fig. 1d, it however significantly changes the temporal dynamics of the surface in the falling edge of the pulse. We now demonstrate that this can lead to observable effects in the experiment by considering the spectral properties of the harmonics.

After a fast initial transient where the denting δT strongly varies, the temporal evolution of the field envelop aL(t) only leads to a weak residual drift of PM surface during the pulse (black dots in Fig. 1d), with typical velocities of the order of 0.01c according to our model. This motion appears as a slow drift on the femtosecond timescale that combines with the fast relativistic oscillation of the plasma surface at the laser frequency responsible for HHG (see Fig. 1c). This results in a Doppler shift on the reflected light, which scales linearly with harmonic order n, and thus gets measurable for large enough values of n.

Since the ion dynamics affects the temporal evolution of the PM surface, it can potentially influence this Doppler effect. This is confirmed by a comparison of PIC simulations performed with fixed (Fig. 5a) and moving ions (Fig. 5b). In the case of fixed ions, the plasma surface moves inwards in the rising part of the pulse, leading to a Doppler redshift, and then moves outwards in the falling part, leading to a Doppler blueshift. If strong enough, this effect leads to harmonics with a double peak structure41, clearly observed in Fig. 5a. In contrast, when ion motion is allowed in the simulation, the irreversible erosion of the ion density gradient prevents the electron boundary from moving back to its initial position when the laser intensity decreases. This naturally suppresses the Doppler blueshift, and only a Doppler redshift is observed, in the interaction conditions considered here.

Figure 5: Doppler shift of high-order harmonics.
figure5

The two images show the angularly resolved spectra of the 9th harmonic, obtained from 2D PIC simulations for aL=8 and L=λ/8, considering either fixed (a) or mobile (b) ions. The curves in the upper panels show line outs of the spectra at the centre of these beams (θy=0). In these interaction conditions, the PM curvature is strong enough to lead to a geometrical mapping of the PM surface onto the propagation angle (sketch in panel c). The centre of the focal spot where the surface recession velocity is the largest and the Doppler redshift the strongest is mapped to the centre of the far-field beam. This explains the shape of the distributions in a and b, where the Doppler shifts are always larger at the centre of the beams.

Turning back to the experiment, Fig. 6a shows a zoom on the spatio-spectral distribution of the 23rd harmonic, measured in a typical shot. It is very similar to the PIC results of Fig. 5b, and only a redshift is observed: according to the previous discussion, this is a signature of ion motion. Figure 6b shows that the Doppler shift at the centre of the beam increases with the density gradient scale length L, which is consistent with the stronger curvature of the PM for larger L. This dependence is quantitatively reproduced by our model, when both ion and electron dynamics are taken into account using the same parameters as in Fig. 4. Thus, although ion dynamics does not affect the spatial properties of harmonics in our experimental conditions, it has a clear signature in the spectral domain, which validates the ionic part of our model.

Figure 6: Measured Doppler shift of an individual harmonic.
figure6

The image in a shows the measured angularly resolved spectrum of the 23rd harmonic, for aL=5.6 and L=0.044 λL. It is a zoom on a measured image such as displayed in Fig. 4a. An angle-dependent Doppler redshift is observed, similar to the PIC simulation with moving ions of Fig. 5b, owing to the position-to-angle mapping resulting from the PM curvature. Panel b shows the measured Doppler shift at the centre of the beam as a function of the density gradient scale length L. The full line shows the results of the model. All experimental data points correspond to a single laser shot.

Discussion

We have presented a simple analytical model for the spatial properties of light beams reflected by relativistic PMs, in excellent agreement with both PIC simulations and experimental results. It provides insight into the respective roles of ion and electron dynamics, and into the spatial and spectral properties of harmonics generated in the reflected beam. Combined with this model, these harmonics now constitute a direct and powerful diagnostic of the femtosecond motion of the PM surface, with spatial resolution within the laser focal spot (Fig. 5c). Measurements schemes such as photonic streaking42 will potentially also provide temporal resolution within the laser pulse envelop.

This model will be instrumental in designing future applications of PMs, in particular for attosecond science. It can for instance be used to determine what laser pulse duration is required to generate isolated ROM attosecond pulses using the lighthouse effect43,44. In this perspective, as well as in most applications where the reflected beam is manipulated or used in the far field, being able to control and minimize the attosecond beam divergence is essential29, which requires mitigating the effect of the laser-induced PM curvature. Figure 7 provides the first experimental demonstration in the relativistic regime of a very simple scheme for such a control45; by using a driving laser beam with a slightly diverging wavefront on target, the effect of the PM curvature on the attosecond beam can be compensated, leading to a divergence close to the one that would be obtained for a flat mirror, reduced by a factor of more than 2 compared with the one obtained at best focus.

Figure 7: Control of the harmonic divergence from a relativistic PM.
figure7

The blue dots in panel a show the divergence of the 25th harmonic measured in our experiment as a function of the distance z between the laser best focus and the target surface. The full line shows the prediction of the model. The two images in b and c show the 2D spatial profiles of the harmonic beam measured at the two focusing positions indicated by the arrows, sketched in d and e. A slightly curved, diverging laser wavefront (z<0; d) compensates the effect of the laser-induced PM curvature, thus reducing the harmonic beam divergence to a value that is imposed by diffraction from the source plane. All experimental data points correspond to a single laser shot.

In other applications, PM will prove useful to focus the reflected beam and boost the peak intensity of the fundamental laser frequency22 or its harmonics17,23. This can be achieved using either curved substrates or the natural light-induced PM curvature described in this work, which typically leads to magnification factors γn=wf/wn≈0.1 for n≥10 in the interaction regime considered here. In either case, the understanding of the laser-induced PM surface dynamics provided by this work will be essential.

Methods

Simulations

We used the codes EUTERPE for one-dimensional (1D) PIC simulations, and CALDER for 2D PIC simulations, to confront our model to simulations. In all simulations, we considered a p-polarized laser pulse of amplitude aL impinging with an angle θ on a plasma density profile that has a maximum density of 200nc, and an initial exponential density gradient of scale length L. The laser field is injected in the simulation box through boundary conditions. In 1D, we account for the oblique incidence by performing all the calculations in the boosted frame. The size of the simulation box is 30 λL, with a mesh size of 6.7 × 10−4λL, the time step is 4 × 10−4 TL, and we used 500 particles per cell. A typical calculation requires 24 h on 1 central processing unit (CPU). In 2D, the simulations parameters are the following: a simulation box of 30 λL × 40 λL, with a mesh size of 2.8 × 10−3λL, a time step 2 × 10−3 TL and 20 macroparticles per cell. A typical calculation requires 24 h on 512 CPUs. All simulation results presented in the main text are from 2D simulations with CALDER. The results of 1D simulations with EUTERPE are presented in the online Supplementary Material (Supplementary Note 2).

Experiment

The experiments are performed using the UHI100 Ti:sapphire laser that delivers 25 fs full width at half maximum pulses centred at 800 nm. The ps pulse contrast is improved to more than 1012 using an antireflection-coated double PM set-up. The high contrast p-polarized laser beam is then aberration corrected using an adaptive optical system and focused on an optically flat target at an incidence angle of 55° using an off-axis parabola. A small fraction of the main beam is picked up for the prepulse and is focused to generate a preplasma. The prepulse focal spot is five times larger than that of the main beam allowing homogenous density gradient all across the HHG source. The controlled delay between the prepulse and the pump beam determines the initial gradient scale length L, which is measured using time-resolved interferometry. The harmonic beam produced by the main laser pulse on the gradient-controlled PM is spectrally dispersed and angularly resolved using a 1,200 lines per mm varied line spacing Extreme Ultraviolet grating (Shimadzu 30-002), and is detected on a 69 × 88 mm2 rectangular microchannel plate (MCP; Fig. 4a). For the 2D spatial diagnostics (Fig. 4b), the reflected beam is spectrally filtered by the combination of two silica plates used at grazing incidence and anti-reflection coated at the laser wavelength, and a high pass 250 nm thick Si filter, and then detected using another MCP. The MCPs are coupled to phosphor screens imaged on 12 bit charge-coupled device cameras.

Fit of experimental data with the model

We extracted the harmonic source size wn from the results of 2D PIC simulations performed in the physical conditions of the experiment and obtained wn/wL=0.72−9.10−3.n for orders n between 5 and 25. For the theoretical curves shown in Fig. 4, wn/wL thus varies from 0.59 for n=15 to 0.5 for n=25. However, the curves are hardly changed if a constant source size of wn/wL=0.5 is used for this entire spectral range. The same values of the source size ratio were used for all gradient scale lengths L, as suggested by PIC simulations.

Additional information

How to cite this article: Vincenti, H. et al. Optical properties of relativistic plasma mirrors. Nat. Commun. 5:3403 doi: 10.1038/ncomms4403 (2014).

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Acknowledgements

We are grateful to E. Lefebvre from CEA/DAM/DPTA for providing us the CALDER code, C. Thaury for fruitful discussions in the early stage of this work and P. Oliveira, F. Réau and O. Tcherbakoff for operating, maintaining and optimizing the UHI100 laser source used for the experiments. The research leading to these results has received funding from ‘Conseil Général de l’Essonne’ through the ASTRE2010 grant, of the Région île de France through SESAME, of the Triangle de la physique through PLASMOPT2, of OSEO through SAPHIR, of the European Research Council (ERC Grant Agreement number 240013) and of Laserlab-ALADIN (Grant number 228334). The numerical simulations were performed by using HPC resources from GENCI-CCRT/CINES (Grant numbers 2012-056057 and 2013-056057).

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H.V. and F.Q. developed the theoretical model. H.V. performed the PIC simulations with some help from G.B.; F.Q., S.K. and S.M. envisioned and designed the experiment; S.M. and S.K. built the experiment and performed the measurements with some help from F.Q.; S.K. led the FDI measurements, with the help of S.M. and did the corresponding data analysis. S.K. and S.M. had comparable overall contributions on the experimental part. S.M. analysed the harmonic data and compared the results with the model, with the help of H.V. All authors participated in the discussions and contributed to the preparation of the manuscript. F.Q. provided overall guidance.

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Correspondence to H. Vincenti or F. Quéré.

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Supplementary Figures 1-16, Supplementary Notes 1-4 and Supplementary References (PDF 1163 kb)

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Vincenti, H., Monchocé, S., Kahaly, S. et al. Optical properties of relativistic plasma mirrors. Nat Commun 5, 3403 (2014). https://doi.org/10.1038/ncomms4403

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