## Abstract

Detections of the pulse durations and arrival timings of relativistic electron beams are important issues in accelerator physics. Electro-optic diagnostics on the Coulomb fields of electron beams have the advantages of single shot and non-destructive characteristics. We present a study of introducing the electro-optic spatial decoding technique to laser wakefield acceleration. By placing an electro-optic crystal very close to a gas target, we discovered that the Coulomb field of the electron beam possessed a spherical wavefront and was inconsistent with the previously widely used model. The field structure was demonstrated by experimental measurement, analytic calculations and simulations. A temporal mapping relationship with generality was derived in a geometry where the signals had spherical wavefronts. This study could be helpful for the applications of electro-optic diagnostics in laser plasma acceleration experiments.

## Introduction

With the advantages of high acceleration gradient ($\sim GV/cm$) and ultra-short temporal structure ($\sim fs$), laser wakefield acceleration (LWFA)^{1} has been investigated intensively in the past decade^{2,3,4,5,6,7,8,9,10,11}. Applications of the laser wakefield accelerated electron beams and LWFA based secondary x-ray sources^{12,13,14,15,16} for pump-probe studies have been proposed^{17,18}. Concerning applications, temporal information of the electron beam could be important because it has an impact on the resolution of the experiment. Previous studies on electron temporal diagnostics were performed by detecting and analyzing the coherent transition radiation (CTR) produced by electron beams^{19,20,21}. Although electron pulse durations of 50 fs to 1.7 fs (rms) have been demonstrated, such measurements either lacked single-shot capability because of low conversion efficiency from electron to terahertz (THz) radiation, or sacrificed electron beam quality by inserting a metal radiator in the beam path. On the other hand, none of these experiments have shown electron arrival timing results which are essential for determining the temporal fluctuation of the electron beams.

Electro-optic (EO) sampling is a widely used technique in conventional accelerators^{22,23,24,25,26,27,28,29,30,31,32,33,34}. When placing an EO crystal close to the electron beam path, the Coulomb fields of electrons residing in the THz range propagate through the crystal and act as a DC bias inducing the Pockels effect. By the incidence of a probe laser through the EO crystal at similar timing, the electron Coulomb field is converted to birefringence. In this way, the electron temporal information can be detected non-destructively in a single shot. The maximum phase retardation is achieved as ${\mathrm{\Gamma}}_{max}={n}_{0}^{3}{r}_{41}{E}_{THz}{\omega}_{0}d/c$ when setting the [−1,1,0] axis of the crystal parallel to the Coulomb field polarization direction, where *n*_{0} is the refractive index of probe laser in EO crystal, *r*_{41} is the EO coefficient, *ω*_{0} is the probe laser frequency, *d* is the crystal thickness and *c* is the speed of light. Methods such as electro-optic spectral decoding (EOSD)^{23} and electro-optic temporal decoding (EOTD)^{24} have been invented to measure the electron pulse duration down to <100 fs^{25,26}.

For the measurement of the electron arrival timing jitter, a spatial decoding method has been introduced from THz studies^{27}. It has a simple set-up where the probe beam is incident on the crystal with an angle relative to the electron beam path^{28,29,30,31,32,33} so that the temporal profile of the electron Coulomb field is transversely recorded on the probe pulse. Usually a cross-polarizer set-up is used to pick out the polarization rotated signal. A measured signal down to 82 fs (rms) has been demonstrated in a conventional accelerator^{30}. Also, this diagnostic served well as a simple electron beam timing monitor detecting the arrival time of the signal peak^{28,29,30,31,32}. Previously, a model has been widely used by considering the Coulomb field compressed in a narrow cone perpendicular to the electron moving direction. The wavefront of the Coulomb field signal has an incident angle of *θ*_{
s
}= 0 to the EO crystal surface. In such a geometry, a linear temporal mapping relationship *c*Δ*τ* = Δ*ξ* tan *θ*_{
p
} was utilized to deduce the timing information from the measured EO signal^{28,30,33,35}, where Δ*τ* is the timing difference, Δ*ξ* denotes the observed displacement on the CCD and *θ*_{
p
} is the relative angle between probe laser and electron beams. Up to now, non-destructive single-shot EO spatial decoding diagnostics and the corresponding temporal mapping relationship in LWFA have not yet been investigated.

In this paper, we introduced the EO spatial decoding diagnostics to LWFA. By placing the EO crystal very close to the electron source, the measured temporal mapping relationship was found to be inconsistent with that used in previous work. Analytical calculations and simulations revealed that the inconsistency was due to the spherical structure of the Coulomb field when a relativistic electron beam was very close to the source. A general nonlinear temporal mapping relationship was derived in a geometry where the signals had spherical wavefronts. We believe this work could be helpful for applications of the EO spatial decoding method in laser plasma acceleration experiments.

## Results

### EO diagnostics set-up

A 10 TW, 40 fs (FWHM) drive laser was focused by an F/20 off-axis-parabola mirror to a 3 mm conical Helium gas jet to generate relativistic electrons (see Methods for details). To perform EO sampling, a 50 *μ*m thick, (110) cut GaP crystal was utilized with the [−1, 1, 0] optical axis perpendicular to the propagation direction drive laser. The 40 fs (FWHM) probe laser was incident through the EO crystal to perform spatial decoding. The relative angle between probe laser and drive laser was set to be *θ*_{
p
} = 44°. We noted that, different from conventional accelerators, there is always a residual intense drive laser together with the electron bunch on the beam path as shown in Fig. 1.

The EO crystal could be damaged by the strong irradiance of the transmitted drive laser pulse. The damage threshold of the GaP crystal by a femtosecond laser has been measured to be ∼ 4.3 mJ/cm^{2} ^{36}. Since the electric field of the electron beam has an opening angle of 2/*γ*^{33}, the fields get broader and weaker with larger transverse distance. The EO crystal should be placed very close to the drive laser axis. In the experiment, the detection point of the probe laser (probe center) on the EO crystal was set at a distance of 1.5 mm from the laser axis. Considering a 400 mJ laser pulse and F/20 light cone, the GaP crystal should be placed at least 2 m away from the target to avoid damage. However, even when we put the EO crystal 1.5 m away from the target, the EO signals were barely observed in the experiment. The reasons include: (1) Laser wakefield accelerated electron bunches always have energy spreads magnitudes broader than that from conventional accelerators. For large propagation distance, the electron bunch durations will be elongated because of the propagation time lag between electrons with different energies. The peak currents will drop drastically; (2) Existing divergences of several mrad level result in an electron spot size of ∼ cm at large propagation distance. The charge densities could drop by several orders of magnitude; (3) Due to pointing fluctuation, the electron beam could arrive at positions with transverse distance so large to the EO crystal that the field strength is too weak to be detected.

A solution was found by placing the EO crystal very close to the target. As shown in Fig. 1, the crystal was at a position 2.2 mm downstream of the target exit. With similar transverse displacement, the crystal could reside at a position outside of the light cone of the transmitted drive laser. Also, at such a distance, the electric field weakening resulting from the electron beam divergence and energy spread is negligible. Figure 2 shows the typical experimental results of EO signals and corresponding electron energy spectra signals. To check the source of the EO signal, we took data in three different cases: (i) without gas; (ii) with gas but no electron beams were observed; (iii) electron beams were generated. Data in case (i) was used as background. As for case (ii), we found that when the gas densities were relatively low, no electron beams were observed, which suggested that the wakefield strengths were below the self-injection threshold^{3}. Simultaneously, no EO signals were observed, as illustrated in Fig. 2(a) and (c). For case (iii), when electron signals appeared at a slightly higher density (${n}_{e}>2.0\phantom{\rule{.25em}{0ex}}\times \phantom{\rule{.25em}{0ex}}{10}^{19}$ cm^{−3}), EO signals were also observed, as shown in Fig. 2(b). The corresponding electron energy spectrum is shown in Fig. 2(d). This comparison demonstrated that the EO signals were generated by the electric field accompanying the electron beams.

### Measurement of temporal mapping relationship

The typical EO signal profiles showed a curved structure, as illustrated in Fig. 2(b), which means that the upper and lower parts of the signal in the vertical direction have a slight arrival time difference on the EO crystal. This suggested that the wavefront of the Coulomb field is not completely a plane wave. To verify the Coulomb field propagation direction, we checked the signal displacement dependence on various probe laser delay settings at a plasma density of 3.5 × 10^{19} cm^{−3} where electron beams with relatively stable timings were generated. The electron beams had pointing fluctuations residing in ±10 mrad and divergences of (${4.6}_{-1.1}^{+1.6}$, ${5.1}_{-1.0}^{+1.8}$) mrad (FWHM) in the horizontal and vertical directions. Since the EO crystal was placed 2.2 mm away from the plasma exit, the detection of the temporal mapping relationship was barely affected by such small fluctuations.

The EO signals were taken at four different probe delays: 3.2 mm, 3.5 mm, 3.8 mm, 4.1 mm (relative value), as shown in Fig. 3(a–d), respectively. To eliminate shot by shot fluctuations, statistics on the peak positions of 20 consecutive EO signals at each probe delay were made, as shown in Fig. 3(e). The mean positions are denoted by black dots and standard deviations are denoted by error bars. From this measurement, we can deduce the temporal mapping relationship between the signal displacement *ξ* and timing variation *cτ* by linear fitting, as illustrated by the red dashed line in Fig. 3(e). The fitted relationship was *ξ* = 0.58*cτ* − *ξ*_{1}, where *ξ*_{1} represents a relative initial value. Thus, the measured temporal mapping relationship can be written as *c*Δ*τ* = 1.72Δ*ξ*. To our surprise, the slope 0.58 of the fitted red dashed line was much smaller than 1/tan *θ*_{
p
} ≈ 1.04 based on *c*Δ*τ* = Δ*ξ* tan *θ*_{
p
}, as illustrated by the blue dashed line set with the same beginning point in Fig. 3(e). This measurement is somehow inconsistent with the previous assumption that the Coulomb field of the relativistic electron beam is compressed as a narrow cone perpendicular to the electron path and propagates along the electron moving direction^{22,23,24,25,26,28,29,30,31,32,33}. The smaller slope of the plot implied that the relative angle between the probe laser and Coulomb field wavefront propagation direction is much larger than *θ*_{
p
}.

### Calculation of the Liénard–Wiechert potential

To understand the physics of how the Coulomb field evolves, we calculated the Liénard–Wiechert potential of a single electron with an energy of 30 MeV. The calculation scheme is shown in Fig. 4(a). The electron emitted from “0” position propagates along the *x* direction with a velocity of *βc*, while the plane *x* = 0 denotes the boundary between the plasma and vacuum. The electric field can be calculated as^{37}

where *ε*_{0} is the vacuum permittivity, “*ret*” means the field is calculated at a retarded time, *R* is the retarded source to observer distance, $\overrightarrow{n}=\overrightarrow{R}/R$ and *γ* = 1/(1 − *β*^{2})^{1/2}. Assuming that at time t, the electron is at position A (*βct*, 0). The electric field at point C(X, Y) was generated at an earlier time when the electron was at position B. We have $|\overrightarrow{BC}|\phantom{\rule{thinmathspace}{0ex}}=R$ and $|\overrightarrow{BA}|\phantom{\rule{thinmathspace}{0ex}}=\beta R$. The retarded source to observer distance *R* can be calculated by the equation (*βR* + Δ*x*)^{2} + Δ*y*^{2} = *R*^{2}(*R* > 0), where Δ*x* = *X* − *βct* and Δ*y* = *Y*. Thus, we get: $R(X,\phantom{\rule{thinmathspace}{0ex}}Y,\phantom{\rule{thinmathspace}{0ex}}t)=\beta \mathrm{\Delta}x{\gamma}^{2}+\sqrt{(\beta \mathrm{\Delta}x{\gamma}^{2}{)}^{2}+{\gamma}^{2}(\mathrm{\Delta}{x}^{2}+\mathrm{\Delta}{y}^{2})}$.

The electric fields are shielded when the electron is inside the plasma. That is, when the source position B(*βct* − *βR*,0) is on the left side of the Y axis, the field strength at observer point C should be 0. Thus, the transverse electric field distribution of the whole space at a certain time *t* can be written as:

where *sgn* is the sign function with values of *sgn*(*x*) = (1, x > 0; 0, x = 0; −1, x < 0) and *θ* is defined by sin $\theta =\phantom{\rule{thinmathspace}{0ex}}|\overrightarrow{\mathrm{\Delta}\mathrm{y}}|/R$. The calculated results of Eq. (2) are shown in Fig. 4(b–d).

When observing the overall electric field at a large angle and a small longitudinal distance, the difference of propagation distances between the field and the electron is so small that the front boundary of the Coulomb field is “attached” to the electron. The Coulomb field of the electron distributed along the spherical boundary with center at (0, 0), as shown in Fig. 4(b). This corresponds to the case in our experiment where the longitudinal distance between source and the crystal is 2.2 mm and the observation angle is 1.5 mm/2.2 mm ∼ 680 mrad. However, if the electric field is detected at a small angle 1 m away (1 mm/1 m = 1 mrad), as illustrated in Fig. 4(c), the curvature is negligible. Since the electron velocity is smaller than c, the field boundary is in front of the electron after propagating for certain distances. When the detection point is further away, as shown in Fig. 4(d), the boundary of the field is far from the electron. The Coulomb field is symmetrically confined as a cone perpendicular to the electron path. Figure 4(d) corresponds to previous work in conventional accelerators, where the EO crystals were placed several mm aside from the beam path while the electron beams had propagated hundreds of meters away from the cathode. In such cases, the electron beams can be considered as propagating in a free space. In our calculation, the electron suddenly appeared with the energy of 30 MeV, thus the rising edge looks like a cut-off. In a realistic case, the electron has an acceleration process inside the plasma and the rising edge of the field should be gentle. But still, the Coulomb field should be confined along the hemisphere with radius of *ct* at small propagation distances, where *t* is the electron propagation time.

### Simulations of the Coulomb field

To qualitatively study the propagation of the Coulomb field of electron beam and confirm the elaborated physics process in Fig. 4, we performed simulations using the code REMP^{38} (see Methods for details). We note that to understand the physics of how the spherical wavefront Coulomb field appears, it is unnecessary to repeat a specific electron parameter in the experiment. Thus, we focus on investigating the evolution of the electric field accompanying the electron bunches when they are propagating out of the plasma (first simulation) and passing by the EO crystal at 2.2 mm away from the source (second simulation).

First, we considered the laser pulse interaction with a supersonic jet modeled as a plasma slab. The laser pulse propagated through the plasma producing several bunches of relativistic electrons. (see Methods for details.) The relativistic electrons escaping from the plasma were accompanied by their Coulomb field with a characteristic spherical distribution, as shown in Fig. 5(a). When electron bunches were in the plasma, the Coulomb fields were completely shielded. Therefore the Coulomb field distribution of emitted electrons evolves as it had been created at the plasma-vacuum interface due to the loss of quasi-neutrality. When the electron bunches propagated further away, the Coulomb fields expanded as spherical waves, as illustrated in Fig. 5(b). The observation of the spherical-wavefront Coulomb field in the simulation justifies our calculation of the Liénard–Wiechert potential above.

For comparison and further confirmation of the physics model, we performed a second simulation of an isolated electron bunch detaching from a neutralizing background (see Methods for details). In this simulation, we investigated on the Coulomb field shape when the electron beam passed by the EO crystal. Figure 5(c–e) show the electric field patterns when a 30 MeV electron beam passes by the EO crystal. We observed that the Coulomb field wavefront distributed as a spherical shape along an imagined light front with a radius of *ct* (*t* is the electron propagation time) centered at the electron emitting point. In a small area shown in Fig. 5(e), the signal could be considered as a plane wave with an incident angle of *θ*_{
s
} ≈ tan^{−1}(1.5 mm/2.2 mm) = 34.3°. The relative angle between the probe laser and the signal wavefront propagation direction is larger than *θ*_{
p
}. This is the reason why the measured slope of the temporal mapping relationship in Fig. 3(e) is much smaller than 1/tan *θ*_{
p
}.

### Nonlinear temporal mapping relationship

Since the spherical shape of the Coulomb field wavefront cannot be neglected at large observation angles, a new temporal mapping relationship should be derived for the application of EO spatial decoding diagnostics in laser plasma acceleration experiments. The calculation geometry of spherical signal wavefronts is illustrated in Fig. 6(a). We consider two signal lines S1 and S2 in the Coulomb signal field with a time delay of Δ*τ*. The probe laser collides with the first signal line S1 at time *t*_{
A
} (point A on Y axis) and second signal line S2 at time *t*_{
B
} (point B on Y axis) on the crystal front surface. The distance between the source position to the crystal front surface is *L*. The cross points of signal lines S1 and S2 with the crystal front surface have displacement functions of: *y*_{s1}(*t*) = $\sqrt{{c}^{2}{t}^{2}-{L}^{2}}$ and *y*_{s2}(*t*) = $\sqrt{{c}^{2}{(t-\mathrm{\Delta}\tau )}^{2}-{L}^{2}}$, respectively. The probe laser and crystal front surface have a cross point at *y*_{
p
}(*t*) = *y*_{p0} − *ct*/sin *θ*_{
p
}, where *y*_{p0} is the initial probe position that originates from the probe laser delay settings.

At time *t*_{
A
}, we set *y*_{0} = *y*_{s1}(*t*_{
A
}) = *y*_{
p
}(*t*_{
A
}) and define the signal incident angle to be *θ*_{s0} = tan^{−1}(*y*_{0}/*L*) (In the experiment, *y*_{0} was choosen to be at the center of the probe laser spot by setting a suitable probe delay). Thus, we have the initial probe position *y*_{p0} = *L* tan *θ*_{s0} + *ct*_{
A
}/sin *θ*_{
p
}, and the timing *t*_{
A
} is determined by *ct*_{
A
} = *L*/cos *θ*_{s0}.

At time *t*_{
B
} (${t}_{B}>{t}_{A}$), the colliding position of the probe laser with the second signal line S2 can be determined by *y*_{
p
}(*t*_{
B
}) = *y*_{s2}(*t*_{
B
}), that is: $\phantom{\rule{thinmathspace}{0ex}}{y}_{p0}-\frac{c{t}_{B}}{\mathrm{sin}\phantom{\rule{thinmathspace}{0ex}}{\theta}_{p}}=\sqrt{{c}^{2}{({t}_{B}-\mathrm{\Delta}\tau )}^{2}-{L}^{2}}$. We observe the signal displacement Δ*ξ* by projection of the displacement of the two cross points (distance between A and B) to the CCD chip:

Based on the discussions above, we have the equation determining the temporal mapping relationship as:

Eq. (4) has solutions: $c\mathrm{\Delta}\tau =\mathrm{\Delta}\xi \phantom{\rule{.25em}{0ex}}\mathrm{tan}\phantom{\rule{.10em}{0ex}}{\theta}_{p}+\frac{L}{\mathrm{cos}\phantom{\rule{.10em}{0ex}}{\theta}_{s0}}\pm \frac{L}{\mathrm{cos}\phantom{\rule{.10em}{0ex}}{\theta}_{s0}}\sqrt{1-\frac{2\phantom{\rule{.25em}{0ex}}\mathrm{sin}\phantom{\rule{.10em}{0ex}}{\theta}_{s0}\phantom{\rule{.25em}{0ex}}\mathrm{cos}\phantom{\rule{.10em}{0ex}}{\theta}_{s0}}{\mathrm{cos}\phantom{\rule{.10em}{0ex}}{\theta}_{p}}\frac{\mathrm{\Delta}\xi}{L}+\frac{{\mathrm{cos}}^{2}{\theta}_{s0}}{{\mathrm{cos}}^{2}{\theta}_{p}}\frac{\mathrm{\Delta}{\xi}^{2}}{{L}^{2}}}$. When we observe zero displacement on the CCD: Δ*ξ* → 0, the timing difference should be zero: *c*Δ*τ* → 0. We choose the “–” solution:

This is the nonlinear temporal mapping relationship in the geometry of spherical-wavefront signal. If we invesitigate on a small time scale such as the case in LWFA, where $\mathrm{\Delta}\xi \ll L$, we can expand the Eq. (5) as $c\mathrm{\Delta}\tau =(1+\frac{\mathrm{sin}\phantom{\rule{thinmathspace}{0ex}}{\theta}_{s0}}{\mathrm{sin}\phantom{\rule{thinmathspace}{0ex}}{\theta}_{p}})\mathrm{tan}\phantom{\rule{thinmathspace}{0ex}}{\theta}_{p}\mathrm{\Delta}\xi -\frac{\mathrm{cos}\phantom{\rule{thinmathspace}{0ex}}{\theta}_{s0}}{{\mathrm{cos}}^{2}{\theta}_{p}}\frac{\mathrm{\Delta}{\xi}^{2}}{2L}$. Ignoring the higher order term, we get a linear equation showing the case of an obliquely incident plane wave signal:

By setting *y*_{0} = 1.5 mm, L = 2.2 mm, Eq. (5) and Eq. (6) are plotted out in Fig. 6(b) as the black curve and red line, respectively. We see that, for a measurement with large timing difference, the plane wave assumption has larger timing delay than the realistic value and the data should be fitted with a nonlinear relationship based on the spherical-wavefront field. Yet, for small timing gap in the Coulomb field, the plane wave assumption could be applicable because the difference of the calculated values between both cases is very small. As shown in Fig. 3(e), the measured temporal mapping relationship fitted well with a linear fitting. The average signal incident angle can be calculated from Eq. (6) to be $\overline{{\theta}_{s}}=33.1$° according to the fitted relationship in Fig. 3(e), which is in correspondence with the experimental set up of *θ*_{s0} = tan^{−1}(1.5 mm/2.2 mm) = 34.3°. This correspondence demonstrates that the Coulomb field has a spherical wavefront structure and the derived temporal mapping relationship denoted by Eq. (6) is applicable in the large observation angle set-up for detecting the temporal information of electron beams from LWFA. Furthermore, we find that, if *θ*_{s0} = 0 and $\mathrm{\Delta}\xi \ll L$, Eq. (6) returns to *c*Δ*τ* = Δ*ξ*tan*θ*_{
p
}, which corresponds to the case of a conventional accelerator where the EO crystal is placed far away from the source and the observation angle is very small.

## Discussion

The electric field of the electron beam can be roughly estimated as a convolution *E*_{
THz
} = (*E* * *Q*)(*r*, *t*)^{33}, where *E*(*t*) = $\frac{e}{4\pi {\epsilon}_{0}}\frac{\gamma r}{({r}^{2}+{\gamma}^{2}{v}^{2}{t}^{2}{)}^{3/2}}$ is the radial electric field of a single electron at distance *r*, *Q*(*t*) = $\frac{1}{\sqrt{2\pi {\sigma}^{2}}}\mathrm{exp}(\phantom{\rule{-0.25em}{0ex}}-\phantom{\rule{-0.25em}{0ex}}{t}^{2}/2{\sigma}^{2})$ is the electron beam temporal distribution assuming a Gaussian distribution and *v* is the electron velocity. It is related to the electron energy and three dimensional charge density. Assuming an electron beam has infinitesimal transverse size with a pulse duration of 20 fs (rms) and charge of 20 pC (i.e.1 kA), the Coulomb field temporal profiles of various electron energies at transverse distance r = 1.5 mm are calculated and plotted in Fig. 7(a). We see that the electric field becomes weaker and broader with lower electron energy since the the field is compressed with the ratio of ∝ 1/*γ*^{37}. The peak electric field strengths of 30 MeV, 10 MeV, and 1 MeV electron beams are 1.0 × 10^{6} V/m, 3.7 × 10^{5} V/m and 5.3 × 10^{4} V/m, respectively. Since the detected signal ${I}_{sig}\propto {\mathrm{sin}}^{2}(\mathrm{\Gamma}\mathrm{/2)}\propto {E}_{T\phantom{\rule{.25em}{0ex}}Hz}^{2}$ in the cross-polarization set-up^{33}, where Γ ∝ *E*_{
THz
} is the phase retardation, the signal intensity of the 30 MeV electron beam should be 7 times and 356 times larger than 10 MeV and 1 MeV ones, respectively. In the experiment, when quasi-monoenergetic electron beams with a peak energy around 30 MeV (as shown in Fig. 2(d)) are generated (average charge of 17 pC), the EO signals have an average peak intensity of ∼ 30000 counts on the 16 bit CCD, while the background was at level of 1600. Based on the calculation, the signal from a 10 MeV electron beam is just above the detection threshold and the signal from a 1 MeV beam is undetectable, assuming the same current of 1 kA.

We want to clarify that the CTR emission did not affect our EO measurement. CTR in the THz range could be generated when the electrons pass the plasma vacuum boundary. However, since the underdense gas profile is much more gentle than a solid metal surface, the intensity of CTR should be rather weak. The CTR emission is concentrated at an angle of 1/*γ* aside from the forward direction^{39}. For higher energy electron beams, the CTR emission direction is very close to the laser direction so that it cannot be detected in our experimental set-up with an observation angle of 34.3°. For CTR generated by hot electrons, experimental measurement has been made by J. van Tilborg *et al*.^{19}, where similar plasma densities were used and nC electron beams with Maxwellian energy distribution were generated. According to the experimental set-up and results therein, the THz field strength could be roughly estimated to be <5 × 10^{4} V/m at the detection point in our experiment. The CTR field strength should be at a similar level or smaller than the Coulomb field of a 1 kA, 1 MeV electron beam and much lower than the detection threshold.

Using the measured temporal mapping relationship illustrated in Fig. 3(e), we found that the durations of the EO signals in Fig. 3 resided between 110 fs–150 fs (rms). A typical signal profile with duration of 115 fs (rms) is plotted out in Fig. 7(b). Figure 7(c) shows the corresponding electron energy spectrum. The observed EO signal durations were much larger than the plasma wakewave timescale (∼ 20 fs). One of the main reasons is that the electron beams generated in our experiment had relatively low energies. As shown in Fig. 7(a), the Coulomb fields of 30 MeV and 10 MeV electrons expand to 70 fs and 188 fs (rms), respectively. The measured EO signal duration illustrated in Fig. 7(b) is in correspondence with the simultaneously detected electron energy spectrum in Fig. 7(c) where a low energy tail existed. Other effects such as: crystal absorption, phase mismatch because of the difference between THz phase velocity and probe laser group velocity and smearing caused by multi bunches will also limit the resolution of the measurement^{33}. A better resolution can be achieved by measuring electron beams with higher energies since the Coulomb fields at the detection position could possess temporal distributions similar to those of the electron bunches. The directly observable pulse duration using a GaP crystal has been calculated to be >50 fs (RMS) with 450 MeV electron bunches in previous numerical studies^{33,40}. Although direct observation of several femtosecond pulse duration is difficult, such a set-up can still serve well as an electron bunch timing monitor even for electron beams with relatively lower energies since the peak position of the field is not affected^{30,31}. On the other hand, the observed broadened signal also demonstrated that the main contributions to the EO signals came from the Coulomb fields of the electron beams. The CTR emissions from electron beams should possess the original electron pulse duration and propagate in the form of electro-magnetic waves. If CTR contributed considerably to the signal, the observed signal should be on a level of several tens of femtoseconds^{19}.

In summary, the EO spatial decoding diagnostic was introduced to LWFA. By placing the EO crystal very close to the electron source, we found the measured temporal mapping relationship was different from that used in previous work. Analytic calculations and simulations demonstrated that the Coulomb fields of the electron beams have spherical wavefronts due to the shielding of the plasma. A general nonlinear temporal mapping relationship was derived in a geometry where the signals had spherical wavefronts. This study could be helpful for applications of the EO spatial decoding method in laser plasma acceleration experiments.

## Methods

### Laser system and electron generation

The experiment was performed on the JLITE-X Ti: Sapphire laser system at Kansai Photon Science Institute, National Institutes for Quantum and Radiological Science and Technology (QST), Kyoto, Japan. In the experiment, the 10 TW laser pulses with pulse durations of 40 fs (FWHM) were focused using an F/20 off-axis-parabolic (OAP) mirror and incident on a 3 mm supersonic conical Helium gas jet to generate relativistic electron beams. The focal spot has a 1/*e*^{2} radius of *w*_{0} = 21 *μ*m. The resultant laser peak intensity was I = 1.6 × 10^{18} W/cm^{2}, corresponding to a normalized vector potential ${a}_{0}\sim 0.87$, where *a*_{0} = 8.6 × 10^{−10}*λ*[*μ*m] I^{1/2} [W/cm^{2}]. LWFA in our experiment was performed with a moderate power laser in the case where *a*_{0} < 1. Collimated electron beams were generated when the plasma density was > 2 × 10^{19} cm^{−3}. The neutral gas densities have been measured by a Mach-Zehnder interferometer.

### Simulations

We performed two-dimensional simulations using the PIC code REMP in two modes. Firstly, we considered the laser pulse interaction with a supersonic jet modeled as a plasma slab with a bell-shaped longitudinal profile of electron density. The maximum density at the center of the plasma slab was set to be *n*_{
e
} = 1.7 × 10^{19} cm^{−3}. The maximum-to-periphery density ratio was 3. The laser pulse with the energy of 0.5 J had a Gaussian spatial profile both in longitudinal and transverse directions with a corresponding FWHM width of 15 *λ* and 26 *λ* respectively, where *λ* = 800 nm is the laser wavelength. Its focal plane was set at the depth about 1000 *λ* inside the density slab. The total length of the plasma slab was 2444 *λ*. The simulation was performed within a window moving at the speed of light along the laser axis with a size of 512 *λ* × 1024 *λ*. The simulation resolution was *λ*/32 × *λ*/16. The total number of quasiparticles was 1.6 × 10 ^{9}. The laser pulse propagated through the plasma producing several relativistic electron bunches with energies > 50 MeV. The electron bunches escaping from the plasma were accompanied by their Coulomb field with a characteristic spherical distribution.

For the second mode, we performed a simulation of an isolated electron bunch detaching from a neutralizing background. The electron bunch with a quasiparticle number of 10^{5} was emitted from the left boundary. Electrons were set at rest when born and gradually accelerated to 30 MeV within 100 *μ*m. A moving window with a size of 1.5 mm × 4 mm was utilized. The spatial resolutions were Δ*x* = Δ*y* = 1/16 *μ*m. A Gaussian spatial distribution was assumed with an initial transverse and longitudinal bunch size of *σ*_{
x
} = 50 *μ*m and *σ*_{
y
} = 20 *μ*m, respectively. Divergence in terms of *p*_{
y
}/*p*_{
x
} was set to be 1%. The EO crystal was modeled as a rectangular area with an assumed dielectric constant of *ε* = 9. The imaginary part in the refractive index was assumed to be zero. The EO crystal was placed at the same position as in the experiment.

## Additional information

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## Acknowledgements

We acknowledge Prof. A. Zigler, Prof. P. Bolton and Dr. A. Pirozhikov for fruitful discussions, and Prof. Hosokai, Dr. Sano for encouragement. This work was funded by the ImPACT Program of the Council for Science, Technology and Innovation (Cabinet Office, Government of Japan). S.V.B. acknowledges support by the project High Field Initiative (CZ.02.1.01/0.0/0.0/15 003/0000449) from the European Regional Development Fund.

## Author information

### Affiliations

#### Kansai Photon Science Institute, National Institutes for Quantum and Radiological Science and Technology (QST), 8-1-7 Umemidai, Kizugawa-city, Kyoto, 619-0215, Japan

- K. Huang
- , T. Esirkepov
- , J. K. Koga
- , H. Kotaki
- , M. Mori
- , Y. Hayashi
- , N. Nakanii
- , S. V. Bulanov
- & M. Kando

#### Institute of Physics ASCR, v.v.i. (FZU), ELI BEAMLINES, Za Radnicí 835, Dolní Břežany, 252241, Czech Republic

- S. V. Bulanov

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### Contributions

K.H., M.K., H.K., M.M., Y.H. and N.N. performed the experiment. T.E. performed the simulation. K.H., T.E. and M.K. conducted the theoretical calculations. K.H., M.K., T.E., J.K.K., N.N. and S.V.B. discussed the physics models. K.H., M.K. and J.K.K. wrote the paper. M.K. conceived the research. All authors reviewed the manuscript.

### Competing Interests

The authors declare no competing interests.

### Corresponding author

Correspondence to K. Huang.

## About this article

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### DOI

https://doi.org/10.1038/s41598-018-21242-y

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