Hostname: page-component-68c7f8b79f-m4fzj Total loading time: 0 Render date: 2026-01-18T01:45:16.224Z Has data issue: false hasContentIssue false

Modelling of a variable length gas cell target for laser wakefield acceleration

Published online by Cambridge University Press:  22 October 2025

Runfeng Luo*
Affiliation:
The John Adams Institute, Imperial College London , London, UK
Greg Christian
Affiliation:
The John Adams Institute, Imperial College London , London, UK
Michael Backhouse
Affiliation:
The John Adams Institute, Imperial College London , London, UK
Nelson Lopes
Affiliation:
GoLP/Instituto de Plasmas e Fusão Nuclear, Instituto Superior Técnico , Lisboa, Portugal
Saleh Alatabi
Affiliation:
The John Adams Institute, Imperial College London , London, UK
Michael Bloom
Affiliation:
The John Adams Institute, Imperial College London , London, UK
Matthias Maier
Affiliation:
Department of Mathematics, Texas A&M University , College Station, Texas, USA
Zulfikar Najmudin
Affiliation:
The John Adams Institute, Imperial College London , London, UK
*
Correspondence to: R. Luo, The John Adams Institute, Imperial College London, London SW7 2BZ, UK. Email: runfeng.luo18@imperial.ac.uk

Abstract

We present time-dependent two-dimensional (2D) and three-dimensional (3D) fluid simulations of a gas cell with a variable length of 0–5 cm, designed for laser wakefield acceleration. The cell employs an output nozzle producing extended density ramps, which can facilitate the production of high-quality electron beams. In both geometries, the simulations demonstrate uniform density inside the cell. In the 3D case, the mean density inside the cell reaches a density nonuniformity below $1\%$ after 100 ms. The density equilibrium time, $\tau$, scales with the ratio of cell volume-to-outlet area, a relationship that is not captured by the 2D simulations showing five times shorter equilibrium time. We present a method to determine $\tau$ from fluid simulations, allowing the estimation of the minimum delay required to enable a uniform target density. Such uniformity prevents uncontrolled electron injection from density ripples, which has direct implications for optimizing beam quality and reproducibility in wakefield acceleration.

Information

Type
Research Article
Creative Commons
Creative Common License - CCCreative Common License - BY
This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (https://creativecommons.org/licenses/by/4.0), which permits unrestricted re-use, distribution and reproduction, provided the original article is properly cited.
Copyright
© The Author(s), 2025. Published by Cambridge University Press in association with Chinese Laser Press

1 Introduction

Conventional radiofrequency (RF) cavity-based accelerators are typically limited to $100\kern0.22em {\mathrm{MV\ m}}^{-1}$ , constrained by cavity wall breakdown under strong fields[ Reference Döbert and Park 1 , Reference Senes, Argyropoulos, Tecker and Wuensch 2 ]. Laser wakefield acceleration (LWFA) is a compact alternative for accelerating electrons in a plasma wave driven by a high-intensity laser[ Reference Tajima and Dawson 3 ]. For the densities required, the plasma is usually produced from ionization of an initially gaseous target. One method to make a suitable plasma is to use a capillary discharge, in which an electrical discharge flows through a gas-filled capillary[ Reference Spence, Butler and Hooker 4 , Reference Karsch, Osterhoff, Popp, Rowlands-Rees, Major, Fuchs, Marx, Hörlein, Schmid, Veisz, Becker, Schramm, Hidding, Pretzler, Habs, Grüner, Krausz and Hooker 5 ]. Thermal balance with the capillary walls produces a plasma density channel that can serve to guide the laser over long lengths[ Reference Butler, Spence and Hooker 6 ]. Wakefield acceleration in capillary wave-guides has produced acceleration of electrons to 8 GeV over 20 cm of plasma[ Reference Gonsalves, Nakamura, Daniels, Benedetti, Pieronek, Raadt, Steinke, Bin, Bulanov, Tilborg, Geddes, Schroeder, Tóth, Esarey, Swanson, Fan-Chiang, Bagdasarov, Bobrova, Gasilov, Korn, Sasorov and Leemans 7 ]. However, capillary wave-guides are susceptible to laser-induced damage, particularly at high repetition rates. Gas jets can produce targets ranging in density from ${10}^{23}$ to ${10}^{26}\ {\mathrm{m}}^{-3}$ [ Reference Hansen, Haberberger, Katz, Mastrosimone, Follett and Froula 8 ]. Supersonic jets[ Reference Semushin and Malka 9 ] enable the accelerator to be operated far from the gas jet nozzle, reducing damage issues. An alternative way to generate wave-guides is through the hydrodynamic expansion of optical field-ionized (HOFI) plasmas[ Reference Lemos, Grismayer, Cardoso, Geada, Figueira and Dias 10 Reference Shalloo, Arran, Corner, Holloway, Jonnerby, Walczak, Milchberg and Hooker 12 ]. This method has recently been used to accelerate electrons to 10 GeV in a 30 cm plasma formed in a gas jet target[ Reference Picksley, Stackhouse, Benedetti, Nakamura, Tsai, Li, Miao, Shrock, Rockafellow, Milchberg, Schroeder, van Tilborg, Esarey, Geddes and Gonsalves 13 ].

However, gas jets operate at significantly higher backing pressures, resulting in greater gas flow. This increased flow places a higher strain on the load of vacuum pumps and limits the system’s repetition rate. The flow can suffer from stability issues due to turbulence. For a helium gas jet with a nozzle throat diameter of 1 mm and atomic density of $1\times {10}^{25}\ {\mathrm{m}}^{-3}$ , the Reynolds number is approximately equal to $3400$ assuming a flow speed of $1000\kern0.22em {\mathrm{ms}}^{-1}$ , which is in the transitional regime where turbulence begins to develop. It has been shown that small-scale density ripples over a distance of just a few plasma wave wavelengths can induce unwanted electron self-injection[ Reference Kuschel, Schwab, Yeung, Hollatz, Seidel, Ziegler, Sävert, Kaluza and Zepf 14 ], which leads to poor electron beam quality[ Reference Bohlen, Wood, Brüammer, Grüaner, Lindstrøm, Meisel, Staufer, D’Arcy, Põder and Osterhoff 15 ].

Gas cells are enclosed structures that confine a gas flow to produce a gaseous target[ Reference Kononenko, Lopes, Cole, Kamperidis, Mangles, Najmudin, Osterhoff, Poder, Rusby, Symes, Warwick, Wood and Palmer 16 Reference Drobniak, Baynard, Beck, Demailly, Douillet, Gonnin, Iaquaniello, Kane, Kazamias, Kubytskyi, Lenivenko, Lericheux, Lucas, Mercier, Peinaud, Pittman, Serhal and Cassou 19 ]. Gas cells can accommodate HOFI channels[ Reference Mewes, Boyle, Pousa, Shalloo, Osterhoff, Arran, Corner, Walczak, Hooker and Thévenet 20 ], but can also be used for self-guided LWFA[ Reference Osterhoff, Popp, Major, Marx, Rowlands-Rees, Fuchs, Geissler, Hörlein, Hidding, Becker, Peralta, Schramm, Grüner, Habs, Krausz, Hooker and Karsch 21 ]. This is where the non-linear response of the high-intensity laser pulses enables them to be guided far beyond the length over which they would be normally diffracted[ Reference Thomas, Najmudin, Mangles, Murphy, Dangor, Kamperidis, Lancaster, Mori, Norreys, Rozmus and Krushelnick 22 ]. Gas cells are typically filled at a lower inlet pressure and have smaller exits for laser entry and exit. As such, the flow rates to reach the required densities are much slower and less prone to turbulence. Kuschel et al. [ Reference Kuschel, Schwab, Yeung, Hollatz, Seidel, Ziegler, Sävert, Kaluza and Zepf 14 ] investigated the dependence of the wavelength of the relativistic plasma wave, ${\lambda}_\mathrm{p}\equiv 2\pi c/{\omega}_\mathrm{p}$ , along a fixed-length gas cell. They reported a gradient of ${\partial}_z{\lambda}_\mathrm{p}=0.25\%$ in gas cells, compared to ${\partial}_z{\lambda}_\mathrm{p}=3\%$ in gas jets. Their findings indicated that density ripples in gas jets caused strong structuring of the electron beam due to self-injection, whereas gas cells produced nearly unstructured beams with no uncontrolled injection.

Another advantage of gas cells is their ability to offer a tunable plasma length. By incorporating a piston, the plasma length in a gas cell can be precisely and rapidly adjusted, ranging from many centimetres down to a few hundred micrometres. This adjustability makes the gas cell suitable for operation across a wide range of densities, particularly as the distance required to reach maximum electron energy scales inversely with density. In addition, this variable length allows for precise control of the acceleration distance over which electrons are accelerated. This enables the acceleration dynamics to be accurately determined and optimized[ Reference Põder, Wood, Lopes, Cole, Alatabi, Backhouse, Foster, Hughes, Kamperidis, Kononenko, Mangles, Palmer, Rusby, Sahai, Sarri, Symes, Warwick and Najmudin 23 ].

However, care must be taken at the laser exit outlet of the gas cell. Sharp density transitions at this outlet can lead to unwanted degradation of beam emittance[ Reference Backhouse 24 ]. By using suitably engineered density ramps[ Reference Schroeder, Esarey, Benedetti and Leemans 25 Reference Zhao, An, Xu, Li, Hildebrand, Hogan, Yakimenko, Joshi and Mori 27 ], it is possible to reduce the beam divergence and thus better preserve beam emittance. Being able to control the divergence of the beams produced during LWFA is particularly important for many applications, such as staged acceleration[ Reference Steinke, Tilborg, Benedetti, Geddes, Schroeder, Daniels, Swanson, Gonsalves, Nakamura, Matlis, Shaw, Esarey and Leemans 28 ] or injection into undulators to produce radiation[ Reference Schlenvoigt, Haupt, Debus, Budde, Jäckel, Pfotenhauer, Schwoerer, Rohwer, Gallacher, Brunetti, Shanks, Wiggins and Jaroszynski 29 Reference Wang, Feng, Ke, Yu, Xu, Qi, Chen, Qin, Zhang, Fang, Liu, Jiang, Wang, Wang, Yang, Wu, Leng, Liu, Li and Xu 31 ].

In this paper, we present simulations of a tunable-length gas cell to investigate the density uniformity and the time taken to reach equilibrium in the target. Understanding the evolution of the target density is critical for optimizing the LWFA process, as the uniformity and shape of the density profile are crucial in producing high-quality electron beams. Furthermore, an accurate estimation of the time to reach equilibrium provides insight into the density evolution. This is particularly important for the target design for high-repetition-rate LWFA operation, as high-density uniformity is crucial for beam stability. We also explore the use of an outlet designed as a converging–diverging nozzle. This generates longer exit density ramps that can be used to avoid rapid spread of the electron beam at the plasma exit[ Reference Backhouse 24 ]. Since these regions are often difficult to diagnose experimentally, high-fidelity density profile calculations will enable more accurate predictions of LWFA performance by providing precise inputs for particle-in-cell (PIC) simulations.

2 Computational fluid dynamics

To model the gas flow within the cell, computational fluid dynamics (CFD) simulations can be employed. However, CFD solvers face challenges when simulating vacuum conditions and extreme density variations[ Reference Liu, Zhou, Shyy and Xu 32 ]. These abrupt density transitions can cause numerical oscillations, necessitating fine-tuning of ad hoc parameters to achieve a stable solution. Such artificial parameter tuning becomes questionable for supersonic and transonic flows due to the lack of pointwise stability[ Reference Maier and Kronbichler 33 ]. Two-dimensional (2D) CFD simulations have been performed for a gas cell designed for density down-ramp injection[ Reference Kononenko, Lopes, Cole, Kamperidis, Mangles, Najmudin, Osterhoff, Poder, Rusby, Symes, Warwick, Wood and Palmer 16 ]. Extending these simulations to three dimensions is challenging, as the added geometrical complexity often leads to severe stability issues and substantially increased computational cost. Attempts have been made to simulate the gas cell using quasi-three-dimensional ( $r$ - $z$ ) geometries[ Reference Audet, Lee, Maynard, Dufrénoy, Maitrallain, Bougeard, Monot and Cros 17 ], or using three-dimensional (3D) geometries with a reduced volume, focusing on the outlet[ Reference Drobniak, Baynard, Beck, Demailly, Douillet, Gonnin, Iaquaniello, Kane, Kazamias, Kubytskyi, Lenivenko, Lericheux, Lucas, Mercier, Peinaud, Pittman, Serhal and Cassou 19 ]. However, performing a full 3D simulation that accurately captures the complete spatial and physical complexity of the gas cell system remains a substantial computational challenge.

For the simulations presented here, we use the code Ryujin, an open-source finite-element solver for conservation equations such as the compressible Navier–Stokes and Euler equations of gas dynamics[ Reference Maier and Kronbichler 33 , Reference Guermond, Kronbichler, Maier, Popov and Tomas 34 ]. The code uses a convex limiting technique[ Reference Guermond, Nazarov, Popov and Tomas 35 ] that guarantees admissibility in each time step by ensuring that the computed update maintains an invariant-domain property in each collocation point. Concretely, for the compressible Euler equations positivity of the density, positivity of the internal energy and a local minimum principle on the specific entropy are enforced[ Reference Guermond, Nazarov, Popov and Tomas 35 ]. This limiting strategy guarantees robustness even under extreme shock conditions and for complex geometries, making Ryujin particularly suitable for modelling scenarios with significant density variation, sharp transitions and real-life geometries, such as gas cells for LWFA. The method is guaranteed to be stable without the use of any ad hoc tuning parameters[ Reference Maier and Kronbichler 33 , Reference Guermond, Nazarov, Popov and Tomas 35 ]. Owing to its convex limiting feature, Ryujin remains robust when simulating complex geometries, unlike other CFD methods that may experience divergence of physical quantities.

Ryujin’s convex limiting algorithm blends an intermediate, robust and viscous low-order update with a high-order update while maintaining the invariant-domain property. The intermediate low-order update is designed in such a way that it ensures that all thermodynamical constraints and entropy inequalities are maintained[ Reference Guermond and Popov 36 ]. Ryujin accurately captures extreme density transitions, such as those occurring near vacuum boundaries, and is inherently stable against the divergence of physical quantities such as temperature, a difficulty that often arises in other fluid simulations, particularly within complex 3D geometries. For further details about the underlying theory and implementation we refer the reader to Refs. [Reference Maier and Kronbichler33,Reference Guermond, Nazarov, Popov and Tomas35,Reference Guermond and Popov36].

3 Simulation setup

The computational work is based on a gas cell designed for use as a wakefield accelerator utilizing controlled ionization injection[ Reference Bohlen, Wood, Brüammer, Grüaner, Lindstrøm, Meisel, Staufer, D’Arcy, Põder and Osterhoff 15 , Reference Rowlands-Rees, Kamperidis, Kneip, Gonsalves, Mangles, Gallacher, Brunetti, Ibbotson, Murphy, Foster, Streeter, Budde, Norreys, Jaroszynski, Krushelnick, Najmudin and Hooker 37 Reference Pak, Marsh, Martins, Lu, Mori and Joshi 39 ]. It was optimized to produce low-divergence ( $<$ mrad) and low-emittance ( $<$ mm mrad) beams.

The cell is filled with helium gas, doped with a few percent of nitrogen by mass. The nitrogen K-shell electrons, which have a high ionization threshold ( ${a}_0>1$ ), ionize only near the peak laser intensity[ Reference Bohlen, Wood, Brüammer, Grüaner, Lindstrøm, Meisel, Staufer, D’Arcy, Põder and Osterhoff 15 , Reference Rowlands-Rees, Kamperidis, Kneip, Gonsalves, Mangles, Gallacher, Brunetti, Ibbotson, Murphy, Foster, Streeter, Budde, Norreys, Jaroszynski, Krushelnick, Najmudin and Hooker 37 Reference Pak, Marsh, Martins, Lu, Mori and Joshi 39 ]. Here, ${a}_0$ represents the normalized laser vector potential. Electrons ionized near this peak intensity can be generated with the optimal phase within the plasma bubble to remain trapped and accelerated[ Reference Chen, Esarey, Schroeder, Geddes and Leemans 40 ]. By adjusting the laser focus, the timing of the injection can be controlled to generate high-quality electron beams[ Reference Wang, Feng, Zhu, Li, He, Li, Tan, Ma and Chen 41 ].

The gas cell provides a helium atomic density ranging from ${10}^{23}$ to ${10}^{25}\;{\mathrm{m}}^{-3}$ , doped with a few percent of nitrogen by mass. To simplify the fluid simulations, and considering the low concentrations of nitrogen in the cell, our simulations assumed that the gas was pure helium.

A cone with a $400\;\mu \mathrm{m}$ diameter hole serves as the aperture through which the laser enters the cell. The dimensions of the cone were selected as a compromise between achieving a higher operating density and minimizing laser-induced damage to the outlet. As shown in Figure 1, the cone is mounted on a piston that allows the aperture position to be adjusted along the laser beam axis while maintaining the gas cell seal, providing control over the target length. The cell is 5.9 cm in length with a volume of $38\kern0.22em {\mathrm{cm}}^3$ . The piston is oriented towards the laser entrance to facilitate rapid downstream access for applications such as staged acceleration.

Figure 1 A computer-aided design (CAD) rendering of the cell geometry along with a zoomed-in view of the nozzle at the laser exit.

To introduce the density down-ramp, the exit aperture is shaped into a converging–diverging nozzle, approximating de Laval nozzles that are used for accelerating fluids to supersonic speed[ Reference Deshpande, Vidwans, Mahale, Joshi and Jagtap 42 ]. The resulting longer ramps would help collimate the naturally divergent electron beams produced by LWFA. Figure 1 includes a detailed view of the converging–diverging nozzle. The converging section began with a diameter of 1.9 mm and was extended 0.8 mm in length. The throat section measured 1.0 mm in diameter and 0.1 mm in length. The diverging section extended 1.7 mm, widening to a final diameter of 1.6 mm.

Ryujin defines the initial conditions on either side of the inlet interface using two sets of primitive states. A primitive state refers to a set of physical parameters that describe the fluid at a given point, including density, thermal velocity and pressure. In this study, we simulated pure helium with an inlet pressure of 100 mbar. The density was determined using the ideal gas law, assuming a temperature of 300 K. The velocity of the primitive state corresponds to the mean thermal velocity of gas particles as derived from the Boltzmann distribution. The initial vacuum pressure was assumed to be ${10}^{-5}\ \mathrm{mbar}$ .

The Knudsen number, $\mathrm{Kn}$ , is the ratio of the molecular mean free path to the physical scale in the system. It characterizes the type of the flow. For $Kn<0.01$ , the continuum flow assumption is valid, and the no-slip boundary condition applies. For $0.01< \mathrm{Kn}<0.1$ , the velocity slip at the wall becomes important, and the slip boundary conditions should be used[ Reference Zhang, Shan, Zhao and Guo 43 ]. The Knudsen number for helium at 300 K and 100 mbar, with the nozzle throat as the smallest length scale at 0.1 mm, is approximately $0.0138$ . This value indicates that the gas flow in the cell is within the slip-flow regime and, consequently, for these simulations, the wall conditions were set to slip.

4 Simulation results

To evaluate the capability of Ryujin, we first conducted 2D trial simulations using a simplified geometry without the piston. Figure 2(a) shows transverse slices of the density distribution at 5 and 50 ms after gas release. At 5 ms, the system had not yet reached equilibrium, and a higher density was found near the inlet. By 50 ms, the density had stabilized and become uniform. As shown in Figure 2(b), the density plateaued at $4.91\times {10}^{25}\ {\mathrm{m}}^{-3}$ after 50 ms. An exponential fit to the mean density reveals a characteristic time of 16 ms.

Figure 2 Helium atomic density distribution and uniformity for the 2D cell without a piston. (a) Transverse slices of the density distribution at 5 and 50 ms. (b) Mean helium atomic density in the gas cell as a function of time after gas release. (c) Temporal evolution of density uniformity (standard deviation) in the gas cell.

Figure 3 presents the results of the 2D simulation, including the trombone, as implemented in the variable length gas cell. The distance from the trombone to the outlet was set to 9 mm. Figure 3(a) shows transverse slices of the density distribution at 5 and 50 ms after gas release, which also illustrate the cell geometry. The cell comprised an inlet at the bottom and a piston inside. The outlet on the piston was neglected, as this area was significantly smaller compared to the nozzle size. The right-hand wall served as the outlet. At 5 ms, the flow is again quite nonuniform, but the mean density is observed to have stabilized at $4.24\times {10}^{25}\ {\mathrm{m}}^{-3}$ after 40 ms, as shown in Figure 3(b). The density evolution indicated a characteristic time of 9.3 ms. The density inhomogeneity in the LWFA region, defined as a cylindrical volume within the cell with a radius twice that of the outlet and centred along the laser direction, decreased to below $1\%$ after 15 ms, as shown in Figure 3(c). However, the density inhomogeneity across the entire cell remains above 15%, at 50 ms. As illustrated in Figure 3(a), density gradients persist in the top left-hand corner even after the mean density throughout the cell has stabilized. The complex geometry of the cell obstructs fluid flow to the corners, thereby leading to persistent nonuniformities in the density distribution. In addition, the presence of the piston results in a reduced characteristic time, attributed to the smaller effective volume compared to configurations without the piston.

Figure 3 Helium atomic density distribution and uniformity for the 2D cell geometry with a piston. (a) Transverse slices of the density distribution at 5 and 50 ms. (b) Mean helium atomic density in the gas cell as a function of time after gas release. (c) Temporal evolution of density uniformity (standard deviation) in the LWFA region.

While 2D simulations provide useful insights into general flow behaviour, they inherently lack the ability to capture the full spatial complexity of gas dynamics within the cell. Transitioning to 3D simulation is crucial for further investigation of the density equilibrium time and the density inhomogeneities caused by the cell’s geometry and outlet configuration, but the complex geometry increases the computational difficulty. The 3D finite-element mesh requires particular consideration. Currently, Ryujin only accepts quadrilateral and hexahedral mesh elements. While tetrahedral meshing offers greater flexibility for handling complex geometries, it is prone to numerical diffusion, particularly when modelling shocks and sharp density transitions[ Reference Kotrasova and Michalcova 44 ]. By contrast, the hexahedral mesh provides higher accuracy, but generating a fine mesh for complex geometries is challenging. For simplification, the cylindrical piston was replaced by a hexagonal-shaped rod inside the cell. In addition, the cones defining the converging–diverging nozzles were approximated using polygons, while squares were used to represent the outlet, reducing computational time. A 3D finite-element mesh generator, known as Gmsh[ Reference Geuzaine and Remacle 45 ], was used to generate the Ryujin inputs. It features the ability to force the mesh elements to be hexahedral, and 3D volume meshes were created as a compromise between the mesh quality and the computation time. The simulations were performed on the Imperial HPC system with eight Icelake CPU cores[ 46 ]. It took a day to compute 300 ms for the 3D simulations, compared to a few hours for the 2D simulations. The 3D mesh resolution resulted in about 35,000 collocation points, which amounted to 175,000 total spatial degrees of freedom.

Figure 4 presents the gas cell geometry used for the 3D simulation. Figure 5(a) displays transverse slices of the density distribution at 5 and 300 ms after gas release. As observed in 2D simulations, the density within the cell becomes uniform upon reaching equilibrium. The mean density inside the cell was projected to plateau at $5.02\times {10}^{24}\ {\mathrm{m}}^{-3}$ , as shown in Figure 5(b). The characteristic time for the density increase was 56 ms, and the density nonuniformity within the cell decreased below $1\%$ after 100 ms, as depicted in Figure 5(c). Figure 5(c) also compares the density nonuniformity in both the entire cell and the LWFA region. The LWFA region exhibited smaller final density spread. After the initial fluctuation, the density spread plateaued at 1% beyond 40 ms.

Figure 4 Visualization of the 3D cell geometry in Gmsh.

Figure 5 Helium atomic density distribution and uniformity for the 3D cell geometry. (a) Transverse slices of the density distribution at 5 and 300 ms. (b) Mean helium atomic density in the entire cell and in the LWFA region as a function of time after gas release. (c) Temporal evolution of density uniformity (standard deviation) in the entire cell and the LWFA region.

The characteristic time scale, $\tau$ , represents the exponential time constant for density stabilization. Achieving uniformity within 1% requires approximately two to three characteristic time periods. This time determines the minimum laser delay necessary to ensure a uniform density. The characteristic time can be estimated as the ratio of the fluid mass contained within the cell to the mass flow rate exiting through the nozzle, given by the following[ Reference Golijanek-Jedrzejczyk, Świsulski, Hanus, Zych and Petryka 47 ]:

(1) $$\begin{align}\tau =\frac{V}{C_\mathrm{d}{A}_\mathrm{out}}\sqrt{\frac{\rho_0}{2\Delta P}},\end{align}$$

where ${\rho}_0$ is the mass density and $\Delta P$ is the pressure difference between the cell and the vacuum. The volume of the cell and the area of the outlet are denoted by $V$ and ${A}_\mathrm{out}$ , respectively. When the inlet size is significantly larger than the outlet, the gas fills the cell on a timescale that is much shorter than the density equilibrium time. Although the initial filling dynamics of an empty gas cell are strongly governed by the inlet area, the outlet size ultimately determines the rate at which the system approaches density equilibrium. Here, ${C}_\mathrm{d}$ is the discharge coefficient, which is close to unity for a nozzle[ Reference Woodward 48 ].

Table 1 summarizes the equilibrium times obtained from the simulations, alongside the values predicted by Equation (1), assuming the outlet size of 1 mm, equivalent to the throat size. Equation (1) accurately predicts the equilibrium time in 3D simulations, with deviations at the percent level.

Table 1 Comparison of the equilibrium time obtained from simulations ( ${\tau}_\mathrm{sim}$ ) with the theoretical value ( ${\tau}_\mathrm{theory}$ ) predicted by Equation (1), along with the percentage difference between them.

In the 2D simulations, the case with the piston exhibited a shorter equilibrium time compared to the case without the piston, as expected from theoretical predictions, due to the smaller effective cell volume. However, in the 2D case, the concept of volume becomes ambiguous. The 2D model effectively assumes the cell extends infinitely in the direction perpendicular to the simulation plane, such that the influence of the third dimension is negligible. As a result, the volume-to-outlet area ratio reduces to the ratio of the cell’s cross-sectional area to the outlet length. Equation (1) can then be reformulated as follows:

(2) $$\begin{align}{\tau}_{3\mathrm{d}}={\tau}_{2\mathrm{d}}\frac{2{L}_\mathrm{cell}}{\pi {r}_\mathrm{out}},\end{align}$$

where ${L}_\mathrm{cell}$ is the length of the cell in the direction perpendicular to the plane of the 2D simulation. Based on this relation, Figure 5(b) is expected to show a characteristic time 40 times larger than in Figure 3(b). A longer equilibrium time was observed in the 3D case as compared to the 2D case. However, the predicted time for the 2D case was almost an order of magnitude lower than the computational results. This discrepancy arises from the complex internal geometry of the gas cell, which the simplified model does not fully account for. As shown in Figure 3(b), the upper section of the gas cell is connected to the inlet only via a narrow path around the piston tip, which restricts gas flow and leads to a prolonged equilibrium time. By contrast, in the 3D case the gas flow from the inlet is less obstructed, resulting in a shorter equilibrium time that differs by only $1.5\%$ from the theoretical prediction. The 3D fluid simulation, combined with the theoretical model, provides an accurate estimation of the density equilibrium time for the gas cell target. This capability is readily extendable to arbitrary gas cell targets and even other types of LWFA targets, thereby aiding target design by providing reliable equilibrium time estimates. Owing to the convex limiting feature, Ryujin remains robust when simulating complex geometries, which broadens the applicability of Ryujin to a wide range of wakefield targets.

The cell studied here exhibits a characteristic recovery time of approximately 56 ms, with density equilibrium established between 100 and 200 ms. This corresponds to a maximum repetition rate of 5–10 Hz. The transverse cross-section of the cell is about 3 cm by 2 cm. If reduced to 1 cm by 1 cm or less, the repetition rate could increase by a factor of 6–10. The outlet area can also be increased, albeit at the cost of a shorter density ramp length. Such a cell would be well-suited for high-repetition-rate LWFA.

To investigate the density down-ramp, we conducted a 2D convergence study of the density profile using a reduced geometry consisting of only the outlet nozzle. Figure 6 compares the on-axis density profile along the down-ramp for different mesh resolutions, characterized by the element size factor. This factor represents the element size relative to the characteristic Gmsh size, which is heuristically determined as a fraction of the geometry’s bounding box size and further refined based on the smallest geometric features. All the simulations with varying element sizes produced the same uniform density within the gas cell and a consistent down-ramp profile for 0.25 cm $<x<$ 0.75 cm. This indicates that the mesh resolution does not significantly influence the density plateau or the ramp scale-length. However, for a coarse mesh an artificial thickness is assigned to the density bump that forms at the location where the shockwaves, generated by discontinuities in the nozzle, rejoin. The inset in Figure 6 reveals that the density profile begins to converge at an element size of 0.06. While this does not alter the gas flow within the cell, a fine mesh resolution is necessary to accurately capture the key features of the supersonic flows emerging from the nozzles. The peak density of the bump is orders of magnitude lower than the plateau density, as shown in Figure 6. Hence, this feature is not expected to significantly influence the dynamics of the wakefield accelerator.

Figure 6 Convergence scan of the density down-ramp profile using 2D simulations.

To characterize the length of the density down-ramp, an analytical function of

(3) $$\begin{align}\rho ={\rho}_0{\left({e}^{-x/\lambda }+1\right)}^{-1}\end{align}$$

was fitted to the on-axis density lineout for the fluid simulation with an element size of 0.06. Here, ${\rho}_0$ is the plateau density, while $\lambda$ represents the scale-length of the ramp. For a circular outlet, the scale-length $\lambda$ is approximately $R/2$ , where $R$ is the outlet radius. In the case of a nozzle that is a tailored nozzle with a throat radius of 0.5 mm, the ramp scale-length was found to be extended to 0.32 mm[ Reference Backhouse 24 ]. The converging–diverging nozzle geometry, combined with the large aperture size, contributes to an extended scale-length. Such extended ramps could be beneficial in reducing electron beam divergence from the LWFA[ Reference Backhouse 24 ]. However, obtaining experimental measurements of density profiles near the gas outlets are usually obscured by the metallic and opaque nozzle structure. This makes it difficult to have accurate measurements of this region where critical dynamics take place. Hence, integrating the results from these fluid simulations with PIC simulations provides a powerful approach to investigate density down-ramps and their role in generating low-divergence electron beams. This is vital for practical applications such as wakefield-based free-electron lasers[ Reference Wang, Feng, Ke, Yu, Xu, Qi, Chen, Qin, Zhang, Fang, Liu, Jiang, Wang, Wang, Yang, Wu, Leng, Liu, Li and Xu 31 ].

5 Conclusions

We performed hydrodynamics simulations of a variable length gas cell. For both 2D and 3D simulations, the standard deviation of the density fell below 1%, indicating high-density uniformity for a cell target. This would help to reduce uncontrolled self-injection due to density ripples on the scale of the plasma wave wavelength, demonstrating that a gas cell target offers finer density control as compared to a gas jet. Our results show that 2D simulations underestimate the true equilibrium time by a factor of five times. This highlights the importance of 3D simulations for accurately determining the equilibrium time of the cell, a task for which the Ryujin simulations are well-suited. The simulation is adaptable to arbitrary LWFA targets, and the code enables robust studies of gas dynamics in complex targets, free from stability issues. The 3D simulation shows a characteristic time of 56 ms for a gas cell with a volume of $38\kern0.22em {\mathrm{cm}}^3$ , and predicts that the density variation inside the cell drops below $1\%$ after 100 ms. Such a cell would thus be unsuitable for use in pulsed mode for high-repetition-rate LWFA. However, our modelling and Equation (1) indicate that the design of a smaller cell volume would have smaller equilibrium times. Ryujin simulations, combined with Equation (1), can be used to design a gas cell target appropriate for LWFA operation at 10 Hz.

Acknowledgements

The authors acknowledge funding from STFC (ST/J002062/1, ST/P002021/1, ST/V001639/1), and support from the Imperial College Research Computing Service.

References

Döbert, S. and Park, M., Proc. LINAC 2004, 513 (2004).Google Scholar
Senes, E., Argyropoulos, T., Tecker, F., and Wuensch, W., Phys. Rev. Accel. Beams 21, 102001 (2018).Google Scholar
Tajima, T. and Dawson, J. M., Phys. Rev. Lett. 43, 267 (1979).Google Scholar
Spence, D. J., Butler, A., and Hooker, S. M., J. Opt. Soc. Am. B 20, 138 (2003).Google Scholar
Karsch, S., Osterhoff, J., Popp, A., Rowlands-Rees, T. P., Major, Z., Fuchs, M., Marx, B., Hörlein, R., Schmid, K., Veisz, L., Becker, S., Schramm, U., Hidding, B., Pretzler, G., Habs, D., Grüner, F., Krausz, F., and Hooker, S. M., New J. Phys. 9, 415 (2007).Google Scholar
Butler, A., Spence, D. J., and Hooker, S. M., Phys. Rev. Lett. 89, 185003 (2002).Google Scholar
Gonsalves, A. J., Nakamura, K., Daniels, J., Benedetti, C., Pieronek, C., Raadt, T. C. D., Steinke, S., Bin, J. H., Bulanov, S. S., Tilborg, J. V., Geddes, C. G., Schroeder, C. B., Tóth, C., Esarey, E., Swanson, K., Fan-Chiang, L., Bagdasarov, G., Bobrova, N., Gasilov, V., Korn, G., Sasorov, P., and Leemans, W. P., Phys. Rev. Lett. 122, 084801 (2019).Google Scholar
Hansen, A. M., Haberberger, D., Katz, J., Mastrosimone, D., Follett, R. K., and Froula, D. H., Rev. Sci. Instrum. 89, 10C103 (2018).Google Scholar
Semushin, S. and Malka, V., Rev. Sci. Instrum. 72, 2961 (2001).Google Scholar
Lemos, N., Grismayer, T., Cardoso, L., Geada, J., Figueira, G., and Dias, J. M., Phys. Plasmas 20, 103109 (2013).Google Scholar
Lemos, N., Grismayer, T., Cardoso, L., Figueira, G., Issac, R., Jaroszynski, D. A., and Dias, J. M., Phys. Plasmas 20, 063102 (2013).Google Scholar
Shalloo, R. J., Arran, C., Corner, L., Holloway, J., Jonnerby, J., Walczak, R., Milchberg, H. M., and Hooker, S. M., Phys. Rev. E 97, 053203 (2018).Google Scholar
Picksley, A., Stackhouse, J., Benedetti, C., Nakamura, K., Tsai, H. E., Li, R., Miao, B., Shrock, J. E., Rockafellow, E., Milchberg, H. M., Schroeder, C. B., van Tilborg, J., Esarey, E., Geddes, C. G. R., and Gonsalves, A. J., Phys. Rev. Lett. 133, 255001 (2024).Google Scholar
Kuschel, S., Schwab, M. B., Yeung, M., Hollatz, D., Seidel, A., Ziegler, W., Sävert, A., Kaluza, M. C., and Zepf, M., Phys. Rev. Lett. 121, 154801 (2018).Google Scholar
Bohlen, S., Wood, J. C., Brüammer, T., Grüaner, F., Lindstrøm, C. A., Meisel, M., Staufer, T., D’Arcy, R., Põder, K., and Osterhoff, J., Phys. Rev. Accel. Beams 25, 031301 (2022).Google Scholar
Kononenko, O., Lopes, N. C., Cole, J. M., Kamperidis, C., Mangles, S. P., Najmudin, Z., Osterhoff, J., Poder, K., Rusby, D., Symes, D. R., Warwick, J., Wood, J. C., and Palmer, C. A., Nucl. Instrum. Methods Phys. Res. Sect. A 829, 125 (2016).Google Scholar
Audet, T. L., Lee, P., Maynard, G., Dufrénoy, S. D., Maitrallain, A., Bougeard, M., Monot, P., and Cros, B., Nucl. Instrum. Methods Phys. Res. Sect. A 909, 383 (2018).Google Scholar
Aniculaesei, C., Kim, H. T., Yoo, B. J., Oh, K. H., and Nam, C. H., Rev. Sci. Instrum. 89, 025110 (2018).Google Scholar
Drobniak, P., Baynard, E., Beck, A., Demailly, J., Douillet, D., Gonnin, A., Iaquaniello, G., Kane, G., Kazamias, S., Kubytskyi, V., Lenivenko, M., Lericheux, N., Lucas, B., Mercier, B., Peinaud, Y., Pittman, M., Serhal, J., and Cassou, K., Rev. Sci. Instrum. 96, 033304 (2025).Google Scholar
Mewes, S. M., Boyle, G. J., Pousa, A. F., Shalloo, R. J., Osterhoff, J., Arran, C., Corner, L., Walczak, R., Hooker, S. M., and Thévenet, M., Phys. Rev. Res. 5, 033112 (2023).Google Scholar
Osterhoff, J., Popp, A., Major, Z., Marx, B., Rowlands-Rees, T. P., Fuchs, M., Geissler, M., Hörlein, R., Hidding, B., Becker, S., Peralta, E. A., Schramm, U., Grüner, F., Habs, D., Krausz, F., Hooker, S. M., and Karsch, S., Phys. Rev. Lett. 101, 085002 (2008).Google Scholar
Thomas, A. G. R., Najmudin, Z., Mangles, S. P. D., Murphy, C. D., Dangor, A. E., Kamperidis, C., Lancaster, K. L., Mori, W. B., Norreys, P. A., Rozmus, W., and Krushelnick, K., Phys. Rev. Lett. 98, 095004 (2007).Google Scholar
Põder, K., Wood, J. C., Lopes, N. C., Cole, J. M., Alatabi, S., Backhouse, M. P., Foster, P. S., Hughes, A. J., Kamperidis, C., Kononenko, O., Mangles, S. P. D., Palmer, C. A. J., Rusby, D., Sahai, A., Sarri, G., Symes, D. R., Warwick, J. R., and Najmudin, Z., Phys. Rev. Lett. 132, 195001 (2024).Google Scholar
Backhouse, M., “Measurement and optimisation of beam quality from laser wakefield accelerators”, Ph.D. thesis (Imperial College London, 2022).Google Scholar
Schroeder, C. B., Esarey, E., Benedetti, C., and Leemans, W. P., Phys. Plasmas 20, 080701 (2013).Google Scholar
Litos, M. D., Ariniello, R., Doss, C. E., Hunt-Stone, K., and Cary, J. R., Philos. Trans. R. Soc. A Math. Phys. Eng. Sci. 377, 20180181 (2019).Google Scholar
Zhao, Y., An, W., Xu, X., Li, F., Hildebrand, L., Hogan, M. J., Yakimenko, V., Joshi, C., and Mori, W. B., Phys. Rev. Accel. Beams 23, 011302 (2020).Google Scholar
Steinke, S., Tilborg, J. V., Benedetti, C., Geddes, C. G., Schroeder, C. B., Daniels, J., Swanson, K. K., Gonsalves, A. J., Nakamura, K., Matlis, N. H., Shaw, B. H., Esarey, E., and Leemans, W. P., Nature 530, 190 (2016).Google Scholar
Schlenvoigt, H. P., Haupt, K., Debus, A., Budde, F., Jäckel, O., Pfotenhauer, S., Schwoerer, H., Rohwer, E., Gallacher, J. G., Brunetti, E., Shanks, R. P., Wiggins, S. M., and Jaroszynski, D. A., Nat. Phys. 4, 130 (2008).Google Scholar
Fuchs, M., Weingartner, R., Popp, A., Major, Z., Becker, S., Osterhoff, J., Cortrie, I., Zeitler, B., Hörlein, R., Tsakiris, G. D., Schramm, U., Rowlands-Rees, T. P., Hooker, S. M., Habs, D., Krausz, F., Karsch, S., and Grüner, F., Nat. Phys. 5, 826 (2009).Google Scholar
Wang, W., Feng, K., Ke, L., Yu, C., Xu, Y., Qi, R., Chen, Y., Qin, Z., Zhang, Z., Fang, M., Liu, J., Jiang, K., Wang, H., Wang, C., Yang, X., Wu, F., Leng, Y., Liu, J. S., Li, R., and Xu, Z., Nature 595, 516 (2021).Google Scholar
Liu, C., Zhou, G., Shyy, W., and Xu, K., Shock Waves 29, 1083 (2019).Google Scholar
Maier, M. and Kronbichler, M., ACM Trans. Parallel Comput. 8, 16 (2021).Google Scholar
Guermond, J.-L., Kronbichler, M., Maier, M., Popov, B., and Tomas, I., Comput. Methods Appl. Mech. Eng. 389, 114250 (2022).Google Scholar
Guermond, J.-L., Nazarov, M., Popov, B., and Tomas, I., SIAM J. Sci. Comput. 40, A3211 (2018).Google Scholar
Guermond, J.-L. and Popov, B., SIAM J. Numer. Anal. 54, 2466 (2016).Google Scholar
Rowlands-Rees, T. P., Kamperidis, C., Kneip, S., Gonsalves, A. J., Mangles, S. P. D., Gallacher, J. G., Brunetti, E., Ibbotson, T., Murphy, C. D., Foster, P. S., Streeter, M. J. V., Budde, F., Norreys, P. A., Jaroszynski, D. A., Krushelnick, K., Najmudin, Z., and Hooker, S. M., Phys. Rev. Lett. 100, 105005 (2008).Google Scholar
McGuffey, C., Thomas, A. G. R., Schumaker, W., Matsuoka, T., Chvykov, V., Dollar, F. J., Kalintchenko, G., Yanovsky, V., Maksimchuk, A., Krushelnick, K., Bychenkov, V. Y., Glazyrin, I. V., and Karpeev, A. V., Phys. Rev. Lett. 104, 025004 (2010).Google Scholar
Pak, A., Marsh, K. A., Martins, S. F., Lu, W., Mori, W. B., and Joshi, C., Phys. Rev. Lett. 104, 025003 (2010).Google Scholar
Chen, M., Esarey, E., Schroeder, C. B., Geddes, C. G., and Leemans, W. P., Phys. Plasmas 19, 033101 (2012).Google Scholar
Wang, J., Feng, J., Zhu, C., Li, Y., He, Y., Li, D., Tan, J., Ma, J., and Chen, L., Plasma Phys. Control. Fusion 60, 034004 (2018).Google Scholar
Deshpande, N. D., Vidwans, S. S., Mahale, P. R., Joshi, R. S., and Jagtap, K. R., in 4th IRF International Conference (2014), p. 61.Google Scholar
Zhang, L., Shan, B., Zhao, Y., and Guo, Z., Int. J. Heat Mass Transf. 139, 144 (2019).Google Scholar
Kotrasova, K. and Michalcova, V., MATEC Web Conf. 310, 00039 (2020).Google Scholar
Geuzaine, J. and Remacle, C., Int. J. Numer. Meth. Eng. 79, 1309 (2009)Google Scholar
Golijanek-Jedrzejczyk, A., Świsulski, D., Hanus, R., Zych, M., and Petryka, L., Flow Meas. Instrum. 62, 84 (2018).Google Scholar
Woodward, J., Reference Module in Chemistry, Molecular Sciences and Chemical Engineering (Elsevier, 2014).Google Scholar
Figure 0

Figure 1 A computer-aided design (CAD) rendering of the cell geometry along with a zoomed-in view of the nozzle at the laser exit.

Figure 1

Figure 2 Helium atomic density distribution and uniformity for the 2D cell without a piston. (a) Transverse slices of the density distribution at 5 and 50 ms. (b) Mean helium atomic density in the gas cell as a function of time after gas release. (c) Temporal evolution of density uniformity (standard deviation) in the gas cell.

Figure 2

Figure 3 Helium atomic density distribution and uniformity for the 2D cell geometry with a piston. (a) Transverse slices of the density distribution at 5 and 50 ms. (b) Mean helium atomic density in the gas cell as a function of time after gas release. (c) Temporal evolution of density uniformity (standard deviation) in the LWFA region.

Figure 3

Figure 4 Visualization of the 3D cell geometry in Gmsh.

Figure 4

Figure 5 Helium atomic density distribution and uniformity for the 3D cell geometry. (a) Transverse slices of the density distribution at 5 and 300 ms. (b) Mean helium atomic density in the entire cell and in the LWFA region as a function of time after gas release. (c) Temporal evolution of density uniformity (standard deviation) in the entire cell and the LWFA region.

Figure 5

Table 1 Comparison of the equilibrium time obtained from simulations (${\tau}_\mathrm{sim}$) with the theoretical value (${\tau}_\mathrm{theory}$) predicted by Equation (1), along with the percentage difference between them.

Figure 6

Figure 6 Convergence scan of the density down-ramp profile using 2D simulations.