Beam loading in the bubble regime in plasmas with hollow channels

Beam loading in the bubble regime in plasmas with hollow channels

Abstract

Based on the already existing analytical theory of the strongly-nonlinear wakefield (which is called “bubble”) in transversely inhomogeneous plasmas, we study particular behavior of non-loaded (empty) bubbles and bubbles with accelerated bunches. We obtain an analytical expression for the shape of a non-loaded bubble in a general case and verify it with particle-in-cell (PIC) simulations. We derive a method of calculation of the acceleration efficiency for arbitrary accelerated bunches. The influence of flat-top electron bunches on the shape of a bubble is studied. It is also shown that it is possible to achieve acceleration in a homogeneous longitudinal electric field by the adjustment of the longitudinal density profile of the accelerated electron bunch. The predictions of the model are verified by 3D PIC simulations and are in a good agreement with them.

I Introduction

Lately a lot of attention has been given to plasma acceleration methodsEsarey, Schroeder, and Leemans (2009); Kostyukov and Pukhov (2015) in which a driver (an intense laser pulse Tajima and Dawson (1979) or a bunch of charged particles Rosenzweig et al. (1988)) is used to excite a plasma wakefield whose large longitudinal field is used for acceleration. Such methods provide acceleration rates orders of magnitude higher than conventional methods. So far electron bunches with the energy up to at the acceleration distance of have been observed in experiments for laser-wakefield acceleration (LWFA)Leemans et al. (2014), while for plasma-wakefield acceleration (PWFA) the possibility of energy doubling from to at a distance of approximately one meter has been demonstrated Blumenfeld et al. (2007).

One of the most promising regimes of plasma acceleration is the so-called “bubble” or “blow-out” regime in which electrons behind the driver are almost completely expelled and a spherical plasma cavity free of electrons is formed Pukhov and Meyer-ter-Vehn (2002). On its border a thin electron sheath consisting of the expelled electrons is created. The cavity itself travels with a near-luminous velocity through the plasma. The longitudinal electric field in it is uniform in the transversal direction, while the focusing force acting on the accelerated electrons is linear in radius and uniform along the cavity Kostyukov, Pukhov, and Kiselev (2004). In the current paper this cavity will be referred to as a “bubble”. In spite of the fact that this regime provides large acceleration gradients, obtaining electron bunches with low emittance, low energy spread, and high stability is a challenging task Malka et al. (2002). Such properties of electron bunches are important for applications, for example for their use in free electron lasers Jaroszynski et al. (2006). Numerous methods dedicated to the improvement of the bunch quality have been proposed including self-guiding of the laser pulse Clayton et al. (2010), guiding of the pulse in a preformed parabolic channel Leemans et al. (2006, 2014), different types of controlled injection Fubiani et al. (2004); Faure et al. (2006); Chen et al. (2006); Zeng et al. (2015), etc. One of such ways is the use of plasmas with deep (hollow) channels, which is commonly proposed for different types of plasma accelerators Chiou et al. (1995); Schroeder, Whittum, and Wurtele (1999); Kimura et al. (2011); Gessner et al. (2016). The lack of the ion column at the axis for such kind of channels significantly reduces the focusing force acting on the accelerated electrons, while, for the case of LWFA, the parameters of the channel also provide additional freedom for balancing between the laser depletion and dephasing lengths. For instance, the possibility of obtaining electron bunches with the energy of and the energy spread of only 0.3% in the bubble regime in a plasma with a deep channel has been shown in numerical simulations Pukhov et al. (2014).

Due to the complexity of the strongly nonlinear “bubble” regime of the plasma wakefield it is commonly studied using 3D particle-in-cell (PIC) simulations Pukhov (1999). However, its theoretical description is also of considerable interest. Despite the nonlinear nature of the strongly non-linear wakefield, various approaches have led to the creation of phenomenological models of the bubble Kostyukov, Pukhov, and Kiselev (2004); Kostyukov et al. (2009), as well as the development of a similarity theory Gordienko and Pukhov (2005) and an analytical model describing the border of a bubble in homogeneous plasmasLu et al. (2006). Generalization of this theory to the case of plasmas with arbitrary radial inhomogeneity has recently been made in Thomas et al. (2016). A subsequent generalization to arbitrary spatial distribution of electrons inside the sheath at the bubble’s border has shown that the choice of this profile has little effect on the shape of the cavity Golovanov et al. (2016).

The current paper uses the generalized theory to analytically study the blow-out regime for the case of plasmas with channels and to analyze beam loading for this case. The results are obtained for arbitrary plasma profiles. Certain examples of density profiles, namely power-law ones and plasmas with deep channels, are used for illustrative purposes. Power-law profiles are notable as many results for them can be obtained analytically, while plasmas with deep (vacuum) channels are of interest because, as previously mentioned, the transversal focusing force in them is almost completely suppressed Pukhov et al. (2014). In section II we briefly describe the model introduced in Thomas et al. (2016) and simplify the equation for the boundary of the bubble derived in that paper to make further analysis easier. In section III we obtain the shape of a non-loaded bubble (i.e. a bubble without accelerated particles) for an arbitrary plasma profile. This solution is necessary for the further analysis of loaded bubbles. The obtained shapes for the case of a plasma with a vacuum channel are compared to the results of 3D PIC simulations. Section IV is dedicated to the efficiency of the energy transfer from the electromagnetic fields in the bubble to accelerated bunches. We propose the definition of the efficiency and a method of its calculation for arbitrary plasma profiles and arbitrary accelerated electron bunches. Section V then discusses the case of a flat-top accelerated bunch. A threshold value of a charge density for which the efficiency reaches its maximum is calculated. Finally, section VI focuses on the possibility of creating a homogeneous accelerating field by adjusting the profile of a witness electron bunch. Such bunch profiles are found for arbitrary plasma density profiles. The analytical results are also compared to the results of 3D PIC simulations.

Ii General equations

In our model we assume that we have boundless plasma in which a laser pulse or an electron driver propagates along the axis and excites a plasma wakefield in the bubble or blow-out regime. The plasma is non-uniform in the plane perpendicular to the axis with the electron density depending only on the distance from the axis. Axial symmetry is assumed. For simplicity we use dimensionless units in which all charges are normalized to , densities to , time to , coordinates to , momenta and energies to and respectively, and electric and magnetic fields to . Here is the elementary charge, is the electron mass, is the speed of light in vacuum, is a typical plasma density (for example, for the case of a plasma with a hollow channel it may be the density outside the channel), is a typical electron plasma frequency.

In analytical theories of the strongly-nonlinear regime a bubble is commonly described as a cavity completely free of electrons and surrounded by a thin electron sheath. In this case the plasma outside the sheath is considered non-perturbed. For example, such approach is used in Lu et al. (2006), where it has been shown that the bubble boundary (the inner border of the bubble sheath) can be described with a second-order ordinary differential equation (ODE). As shown in Thomas et al. (2016), the bubble boundary for the case of radially-inhomogeneous plasma can be described with a similar equation

(1)

where is the coordinate comoving with the bubble. This equation is derived under the quasistatic approximation, thus all dependencies on time and the longitudinal coordinate are replaced with dependencies on their combination . Under certain conditions—which are discussed below—the coefficients of Eq. (1) are

(2)

These coefficients depend on the radial ion charge density profile via the function

(3)

As opposed to a similar function with the opposite sign introduced in Thomas et al. (2016), the function is always positive, as . The function in the right-hand side of Eq. (1) is determined by electron bunches inside the bubble:

(4)

Here is the longitudinal current density created by electron bunches. As typical velocities of accelerated and driving bunches are close to the speed of light , this current density in the dimensionless units is approximately equal to the electron bunch charge density: . Because , the function is always positive for electron bunches which are considered in this paper. However, for positron or proton bunches the sign is the opposite.

If the coefficients , , and are given by Eq. (2), the longitudinal electric field in the bubble is determined by its boundary according to

(5)

This electric field is accelerating for electrons situated in the rear part of the bubble () and is decelerating in its front part where the driver is located. It is also important that the longitudinal electric field retains the property of being uniform in the transverse direction even for plasmas with channels.

As already mentioned above, the simple expressions for the coefficients (2) and for the longitudinal field (5) are not universal and are valid only if the electron sheath is thin and the bubble is large enough. To be more precise, the conditions and should be fulfilledGolovanov et al. (2016). Here is the thickness of the electron sheath surrounding the bubble. It is assumed to be independent of the longitudinal coordinate in our model. Therefore, Eqs. (2), (5) are not valid in the areas where the bubble local radius is small, i.e. at the front and rear edges of the bubble. Hence, these equations cannot be used to describe the process of the bubble excitation by an electron bunch. However, this process will be out of scope of this paper because the evolution of the bubble boundary behind the driver does not depend on it. This allows us not to consider the properties of the driver at all. This fact also implies that the part of the bubble behind a laser driver is correctly described by Eq. (1) despite it containing no laser-related terms.

So, we assume that we have an arbitrary driver which excites a bubble with a maximum transverse size . For convenience we also assume that the maximum is reached at , so the initial conditions of Eq. (1) are

(6)

We also assume that the driver is fully located in the front part of the bubble (). Therefore, in the rear part of the bubble () the term is determined solely by witness electron bunches.

In its rear part the bubble collapses to the axis due to the Coulomb attraction of the plasma ion column. Hence, we will assume that is monotonous for . This monotonicity might be broken if the source in the right-hand side of Eq. (1) is sufficiently large, i.e. when an accelerated electron bunch has a charge large enough to prevent the collapse of the bubble. If is monotonous, its inverse function exists. Therefore, we can use as a new variable and obtain an equation for from Eq. (1):

(7)

where . Multiplying this equation by and dividing it by we get a total derivative in the left-hand side of the equation:

(8)

Integrating this equation with the initial conditions (6) and returning to the function , we obtain the equation

(9)
(10)

The negative sign before the square root is chosen based on the fact that in the rear part of the bubble. As the function , according to its definition (3), is at least quadratic in the neighborhood of , dividing it by in Eq. (9) does not lead to any singularities. The longitudinal electric field, according to Eq. (5), is

(11)

A similar approach to the derivation of the first-oder equation has been used in Tzoufras et al. (2009) for homogeneous plasmas.

In the most general case Eq. (9) is not an ODE because the function depends on its solution and therefore is also unknown. However, in several special cases this equation can be drastically simplified and solved analytically. These cases are discussed next.

Iii Non-loaded bubble

Let us consider a non-loaded bubble, i.e. a bubble without accelerated electron bunches. In this case , and Eq. (9) can easily be integrated leading to the bubble boundary defined by

(12)

This equation can be used to find the length of the rear part of the bubble by assuming . For specific plasma profiles the boundary of the bubble can be described by special functions. In particular, it is done in Tzoufras et al. (2009) for homogeneous plasmas and in Thomas et al. (2016) for plasmas with power-law channels (i.e. channels with the power-law plasma density profile).

According to Eq. (11), the longitudinal electric field in a non-loaded bubble is

(13)

Due to the fact that the function is monotonous, also has to be monotonous. Therefore, it is impossible to find a plasma profile for which the longitudinal field in a non-loaded bubble is homogeneous (i.e. does not depend on ).

From general formulas (12) and (13) it is also possible to find the longitudinal field in the central part of the bubble, i.e. near . The boundary in the neighborhood of is

(14)

which corresponds to a sphere of a radius . The longitudinal field is zero at , therefore near the center of the bubble it can be approximated with a linear function

(15)

If we consider a channel in plasma, so that , the function is limited () and therefore . So, the gradient of the electric field in the center of a bubble in a plasma channel is limited by the value which is reached for the case of homogeneous plasma.

The influence of power-law channels on the shape of the bubble has been already discussed in Thomas et al. (2016). It has been shown that the increase of the channel width and depth leads to the contraction of the bubble. Here we check if similar behavior is observed for the case of plasma with a vacuum channel for which the ion density is modeled as , where is the radius of the channel and is the Heaviside step function. For this profile the function defined by (3) as well as all the integrals including this function can be analytically calculated. Therefore, determined by Eq. (12) is calculated using a single integral instead of a double integral.

Figure 1: Electron density distributions (a–c) and corresponding longitudinal electric field profiles on the axis of the bubbles (d–f) as observed in PIC simulations for different channel radii , respectively. Analytical solutions for the bubbles’ boundaries and the fields in them calculated using Eqs. (12) and (13), respectively, are shown with the dashed lines. The dotted lines in (b, c, e, f) also show the solution for for comparison. All lengths are normalized to .

The resulting boundaries of non-loaded bubbles for different values of and the corresponding longitudinal fields are shown in Fig. 1 in comparison to the results of PIC simulations carried out using the code Quill. In these simulations we used plasma with a density outside the channel corresponding to a plasma wavelength of . In all three cases an electron bunch with a total charge of , particle energy of , and typical longitudinal and transverse sizes of and , respectively, was used as a driver. From Fig. 1 it is obvious that the length of the bubble and the gradient of the field in it decreases with the increase of a channel radius. The figure also shows good correspondence between the results of the simulations and the predictions of the model both for the bubble boundaries and the longitudinal electric fields in them.

Iv Acceleration efficiency

As we have found the solution for a non-loaded bubble, we may now consider a bubble with an accelerated electron bunch. One of the key points of efficient acceleration is the usage of the largest possible percentage of the energy pumped into the bubble by its driver. Hence, the aim of this section is to describe the efficiency of the energy transfer from the bubble to the accelerated bunch.

Let us assume that a cylindrically symmetric electron bunch with an arbitrary profile is placed inside a bubble of the size , and that its front and trailing edges have the coordinates and , respectively. The boundary of this bubble is described with the function . Let us assume that the bubble boundary reaches zero at , i.e. the whole electron bunch is situated inside the bubble. In this case the points and correspond to certain transverse sizes of the bubble . Consequently, Eq. (9) for the bubble shape for becomes

(16)

One may notice that this equation corresponds to the equation for a non-loaded bubble with a different maximum radius determined by

(17)

As has to be positive (otherwise the radicand would always be negative), we obtain limitations on :

(18)

The case when this inequality does not hold corresponds to electron bunches in which electrons in the trailing edge of the bunch are decelerated instead of being accelerated (an example is given in Sec. V). We will not consider this case here and will assume that all electrons in the bunch are accelerated. Then we can introduce a parameter characterizing the efficiency of the energy transfer from the bubble to the bunch:

(19)

Due to Eq. (18) this parameter can take values from 0 to 1. In order to understand its physical meaning we can make a transformation and, by using Eqs. (4) and (5), obtain

(20)

where is the total power consumed by the accelerated electron bunch as a result of the accelerating force action. Therefore, the introduced efficiency (19) measures the ratio between the power consumed by the accelerated bunch and the maximum possible power for the specified bubble. Alternatively it may be written as

(21)

This expression makes it possible to calculate the acceleration efficiency for any electron bunch.

V Bubble with a flat-top bunch

Let us consider a bubble with the simplest electron bunch profile, i.e. an infinitely long flat-top electron bunch, whose front edge has the longitudinal coordinate . The source for this type of the bunch is , where is the Heaviside step function. For the source is zero, therefore the solution (12) for a non-loaded bubble remains valid. From this solution we can obtain the transversal size of the bubble for the coordinate corresponding to the front edge of the bunch. Then the function in Eq. (9) is , therefore for this equation becomes

(22)

For any point there is a threshold value of for which the radicand is zero at this point:

(23)

It can be shown that is a monotonically increasing function of , therefore there is a global threshold value defined by

(24)

If , the derivative is always negative, which means that is a monotonous function and the bubble boundary reaches the axis . If the value of exceeds the threshold value, there is a certain point where the radicand and, consequently, reach zero, which means that the charge density of the electron bunch becomes sufficiently large to prevent the collapse of the rear part of the bubble; instead, the bubble expands after reaching this point. Due to the fact that the sign of the longitudinal electric field inside the bubble is determined by the sign of , the field changes from accelerating to decelerating beyond this point. Therefore, it is sensible to place the trailing edge of a flat-top accelerated bunch at the point where for this bunch. As a result, the length of a flat-top bunch is limited either by the length of the resulting bubble (if the charge density is less then the threshold value) or by the point where the accelerating field reaches zero and would change to decelerating if we made the bunch any longer.

Knowing these limitations on the flat-top bunch’s length, we can calculate the efficiency which can be reached with the use of a flat-top bunch. To do so we use Eq. (19). If , the bubble boundary reaches , therefore and the expression for the efficiency is

(25)

This expression shows that the efficiency grows linearly from to with the increase of until the charge density reaches the threshold value.

For there is a minimum value of the boundary’s radial coordinate, therefore we should set . The value of can be found from Eq. (22) using the fact that for . The resulting equation for the efficiency is

(26)

With the increase of the value of also increases and therefore the efficiency decreases.

Thus, the efficiency of the energy transfer from the bubble to the accelerated bunch reaches its maximal value of 1 for a flat-top bunch with the threshold charge density (i.e. ) for the specified injection point . For charge densities larger or smaller than the threshold value the efficiency drops below 1. If we use a bunch shorter then optimal for the specified and , then the efficiency becomes even less than the one given by Eqs. (25), (26).

Let us for example consider the case of a power-law plasma profile . The normalization of density is chosen in the way that density is equal to 1 at the point where the bubble reaches its maximum transverse size. Typical boundaries of bubbles with flat-top electron bunches and corresponding electric fields are shown in Fig. 2. This picture shows that the presence of an accelerated bunch leads to the elongation of the bubble compared to the case of a non-loaded bubble (line 1 in Fig. 2). The picture also confirms that there is a predicted threshold value (line 3) which separates bubbles which collapse to from bubbles which continue expanding.

Figure 2: Dependencies of (a) the bubble boundaries and (b) the longitudinal fields on the longitudinal coordinate for different electron bunch charge densities . The dependencies are calculated numerically using Eqs. (1) and (5), respectively. Lines 1–5 show the solutions for the densities from to in increments. The plasma profile used for calculations is parabolic (), the maximum radius of the bubbles , the electron bunch injection coordinate .

The threshold value determined by Eq. (24) is

(27)

This value grows with the increase of the injection coordinate (larger corresponds to smaller ). Therefore, the minimum threshold value is reached for (and thus ) and is equal to

(28)

This minimum value decreases with the increase of the plasma profile exponent . It is also proportional to the square of the bubble size.

The efficiency for this kind of profile can be calculated analytically from Eqs. (25) and (26) and is

(29)

where

(30)

Typical dependencies given by Eq. (29) are shown in Fig. 3 for different plasma profiles and different injection points. It is visible that the threshold value of the charge density is lower for plasmas with deeper channels corresponding to larger values of . One may also notice that the efficiency drops more rapidly with the increase of beyond the threshold for a smaller injection point . It can be explained by the fact that for smaller the transverse velocities of the electrons in the bubble sheath at this point are smaller, and thus the electrons in the sheath are more sensitive to the variations of the charge density of the witness bunch.

Figure 3: Dependencies of the efficiency on the charge density calculated using Eq. (29) for different exponents (, 2, 4 for the solid, dashed, and dotted lines, respectively) for the injection point (a) and (b) . The maximum radius of the bubble .

Vi Uniform accelerating field by the adjustment of the bunch profile

In order not to increase the energy spread of the electrons in the accelerated bunch it is important to accelerate them in a uniform longitudinal field . This field is always uniform in the transverse direction in the scope of our model, therefore we are interested in reaching only the longitudinal homogeneity. As shown in section III, it is impossible to create a homogeneous longitudinal field in a non-loaded bubble. However, the accelerated bunch’s charge influences the shape of the bubble, which may be used to achieve the uniform field. For homogeneous plasma it is done in Tzoufras et al. (2009).

Let us assume that the front edge of the electron bunch has the coordinate which is referred to as the injection point. Then for there are no sources in the right-hand side of Eq. (1) and the solution (12) for a non-loaded bubble is valid, which gives us the transversal size of the bubble at the injection point. The longitudinal field at this point can be found from Eq. (13) and is

(31)

The positive sign of is chosen for convenience.

For we try to find such a profile that the longitudinal field remains constant at the level of . Using Eq. (11) to find the required function and Eq. (5) to find the bubble boundary , we obtain in a parametric form

(32)
(33)

Thus, it has been shown that the electron bunch profile providing homogeneous accelerating field can be found for any plasma profile .

As the length of the accelerated bunch is limited by the length of the bubble, we can find the maximum possible length of the accelerated bunch for any injection point using Eq. (33) and setting :

(34)

Knowing the maximum length of the bunch and the charge density in it, we can also calculate the maximum total charge of the bunch:

(35)

It is worth mentioning that total power consumed by such a bunch and defined by does not depend on the value of the field . Therefore, by choosing the injection point we can balance between a high acceleration rate or a high value of the accelerated charge.

It is also worth mentioning that the average charge density of the bunch with the maximum length is equal to the threshold charge density defined by Eq. (24) for the case of a flat-top bunch. At the same time, the efficiency of the energy transfer (19) for such bunch is also equal to 1.

So, the electron bunch profile providing homogeneous longitudinal electric field in the whole volume of the bunch and leading to the acceleration with the efficiency up to has been found for an arbitrary plasma density profile.

vi.1 Power-law plasma profile

As the first example let us consider plasmas with the power-law density profile . For these plasmas the function determined parametrically by Eqs. (32) and (33) can be found analytically and is

(36)

where

(37)

and can be found from Eq. (31).

Figure 4: Dependencies of the charge density in the accelerated bunches on the longitudinal coordinate calculated using Eq. (36) for different exponents of the power-law density profiles. The injection coordinate , the bubble maximum radius .

The bunch profiles determined by Eq. (36) for plasma profiles with different exponents are shown in Fig. 4. This picture shows that the dependence of the charge density on the longitudinal coordinate for such profiles is almost linear. In the case of homogeneous plasma () the bunch profile is strictly trapezoidal, while for there is a singularity at the trailing edge of the bunch caused by the fact that the plasma density reaches at . This singularity makes it difficult to use the electron bunch with the maximum length, thus further limiting the efficiency of the energy transfer. It is also visible that the total charge in the accelerated bunch is smaller for deeper channels, i.e. larger values of .

Figure 5: Dependencies of (a) the bubbles boundaries and (b) the longitudinal electric fields in them on the longitudinal coordinate calculated numerically using Eqs. (1) and (5), respectively, for different exponents and electron bunches determined by Eq. (36). The solid, dashed, and dotted lines correspond to , , , respectively. The maximum bubble radius , the injection coordinate .

Fig. 5 shows the bubbles corresponding to the profiles in Fig. 4 and the longitudinal electric fields in them. This image demonstrates that the longitudinal field is indeed homogeneous in the region where the bunch is present. It is also seen that the presence of an electron bunch significantly increases the length of the bubble. Figs. 4 and 5 also demonstrate the fact that the total acceleration power is much lower for channels with deeper channels (i.e. with higher values of ), which is also supported by Eq. (35) which for the power-law profiles is written as

(38)

This equation shows that thincreasee product equal to the acceleration power rapidly decreases with the increase of corresponding to the deepening and widening of the channel.

vi.2 Plasma with a vacuum channel

Let us consider plasmas with a vacuum channel for which the plasma density is defined as . In this case the solutions for the electron bunch profiles providing the homogeneous longitudinal electric field can be found only numerically from Eqs. (32) and (33); they are shown in Fig. 6. The shapes of these electron bunches are again very close to trapezoidal like in the previous case of the power-law plasma profiles. They also share the same behavior of having less charge in them for wider channels.

Figure 6: Dependencies of the charge density in the accelerated bunches on the longitudinal coordinate for different channel radii . The dependencies are calculated numerically using Eqs. (32) and (33). The maximum bubble radius , the injection coordinate .

To check if a uniform accelerating field can be generated in plasmas with a channel by using an appropriate electron bunch we carried out 3D PIC simulations. The results of these simulations are shown in Fig. 7. We used plasma with a channel with the density outside the channel. The bubble in this plasma was driven by an electron bunch which had a total charge of and typical longitudinal and transverse sizes of and , respectively. The accelerated bunch had the same typical width while its longitudinal shape was determined from Eqs. (32), (33). The energy of the particles in both bunches was . The comparison of the results of these simulations to the analytical solutions in the scope of our model shows good correspondence between them.

Figure 7: (a) The bubble and (b) the time average longitudinal electric field at the axis of the bubble for an electron bunch with the profile chosen according to Eqs. (32), (33). The channel radius . Analytical solutions calculated using Eqs. (1) and (5) are shown with the dashed lines. All lengths are normalized to .

Vii Conclusions

The equation for the bubble boundary in transversely inhomogeneous plasmas derived in Thomas et al. (2016) is analytically studied. The boundary of a non-loaded bubble is found for an arbitrary plasma profile. The efficiency of the energy transfer from the bubble to an arbitrary accelerated electron bunch is described. When the accelerated bunch is flat-top the threshold value of the bunch charge density which provides maximum efficiency of the acceleration is found. It is also shown that the artificial selection of the electron bunch profile can be used to create homogeneous longitudinal field in the volume of the bunch, which is important for increasing the quality of the accelerated bunch.

The general results are applied to plasmas with power-law profiles and with vacuum channels. It is shown that the increase of the channel size or its depth leads to the contraction of the bubble and to the decrease of the electric field gradient in it. For these plasma profiles the possibility of creating homogeneous accelerating field by the adjustment of the density profile of the electron bunch is demonstrated. The shape of these bunch profiles is proved to be close to trapezoidal.

For the case of a vacuum channel 3D PIC simulations are carried out. They demonstrate good correspondence with the predictions of the model both for non-loaded bubbles and for a bubble with the accelerated bunch providing homogeneous electric field.

Acknowledgements.
This work has been supported by the Russian Science Foundation through Grant No. 16-12-10383.

References

References

  1. E. Esarey, C. B. Schroeder,  and W. P. Leemans, Rev. Mod. Phys. 81, 1229 (2009).
  2. I. Yu. Kostyukov and A. M. Pukhov, Phys.-Usp. 58, 81 (2015).
  3. T. Tajima and J. M. Dawson, Phys. Rev. Lett. 43, 267 (1979).
  4. J. B. Rosenzweig, D. B. Cline, B. Cole, H. Figueroa, W. Gai, R. Konecny, J. Norem, P. Schoessow,  and J. Simpson, Phys. Rev. Lett. 61, 98 (1988).
  5. W. P. Leemans, A. J. Gonsalves, H.-S. Mao, K. Nakamura, C. Benedetti, C. B. Schroeder, Cs. Tóth, J. Daniels, D. E. Mittelberger, S. S. Bulanov, J.-L. Vay, C. G. R. Geddes,  and E. Esarey, Phys. Rev. Lett. 113, 245002 (2014).
  6. I. Blumenfeld, C. E. Clayton, F.-J. Decker, M. J. Hogan, C. Huang, R. Ischebeck, R. Iverson, C. Joshi, T. Katsouleas, N. Kirby, W. Lu, K. A. Marsh, W. B. Mori, P. Muggli, E. Oz, R. H. Siemann, D. Walz,  and M. Zhou, Nature 445, 741 (2007).
  7. A. Pukhov and J. Meyer-ter-Vehn, Appl. Phys. B 74, 355 (2002).
  8. I. Kostyukov, A. Pukhov,  and S. Kiselev, Phys. Plasmas 11, 5256 (2004).
  9. V. Malka, S. Fritzler, E. Lefebvre, M.-M. Aleonard, F. Burgy, J. Chambaret, J.-F. Chemin, K. Krushelnick, G. Malka, S. P. D. Mangles, Z. Najmudin, M. Pittman, J.-P. Rousseau, J.-N. Scheurer, B. Walton,  and A. E. Dangor, Science 298, 1596 (2002).
  10. D. A. Jaroszynski, R. Bingham, E. Brunetti, B. Ersfeld, J. Gallacher, B. van der Geer, R. Issac, S. P. Jamison, D. Jones, M. de Loos, A. Lyachev, V. Pavlov, A. Reitsma, Y. Saveliev, G. Vieux,  and S. M. Wiggins, Phil. Trans. Roy. Soc. A 364, 689 (2006).
  11. C. E. Clayton, J. E. Ralph, F. Albert, R. A. Fonseca, S. H. Glenzer, C. Joshi, W. Lu, K. A. Marsh, S. F. Martins, W. B. Mori, A. Pak, F. S. Tsung, B. B. Pollock, J. S. Ross, L. O. Silva,  and D. H. Froula, Phys. Rev. Lett. 105, 105003 (2010).
  12. W. P. Leemans, B. Nagler, A. J. Gonsalves, Cs. Tóth, K. Nakamura, C. G. R. Geddes, E. Esarey, C. B. Schroeder,  and S. M. Hooker, Nat. Phys. 2, 696 (2006).
  13. G. Fubiani, E. Esarey, C. B. Schroeder,  and W. P. Leemans, Phys. Rev. E 70, 016402 (2004).
  14. J. Faure, C. Rechatin, A. Norlin, A. Lifschitz, Y. Glinec,  and V. Malka, Nature 444, 737 (2006).
  15. M. Chen, Zh.-M. Sheng, Y.-Y. Ma,  and J. Zhang, J. Appl. Phys. 99, 056109 (2006).
  16. M. Zeng, M. Chen, L. L. Yu, W. B. Mori, Z. M. Sheng, B. Hidding, D. A. Jaroszynski,  and J. Zhang, Phys. Rev. Lett. 114, 084801 (2015).
  17. T. C. Chiou, T. Katsouleas, C. Decker, W. B. Mori, J. S. Wurtele, G. Shvets,  and J. J. Su, Phys. Plasmas 2, 310 (1995).
  18. C. Schroeder, D. Whittum,  and J. Wurtele, Phys. Rev. Lett. 82, 1177 (1999).
  19. W. D. Kimura, H. M. Milchberg, P. Muggli, X. Li,  and W. B. Mori, Phys. Rev. ST Accel. Beams 14, 041301 (2011).
  20. S. Gessner, E. Adli, J. M. Allen, W. An, C. I. Clarke, C. E. Clayton, S. Corde, J. P. Delahaye, J. Frederico, S. Z. Green, C. Hast, M. J. Hogan, C. Joshi, C. A. Lindstrøm, N. Lipkowitz, M. Litos, W. Lu, K. A. Marsh, W. B. Mori, B. O’Shea, N. Vafaei-Najafabadi, D. Walz, V. Yakimenko,  and G. Yocky, Nat. Commun. 7, 11785 (2016).
  21. A. Pukhov, O. Jansen, T. Tueckmantel, J. Thomas,  and I. Yu. Kostyukov, Phys. Rev. Lett. 113, 245003 (2014).
  22. A. Pukhov, J. Plasma Phys. 61, 425 (1999).
  23. I. Kostyukov, E. Nerush, A. Pukhov,  and V. Seredov, Phys. Rev. Lett. 103, 175003 (2009).
  24. S. Gordienko and A. Pukhov, Phys. Plasmas 12, 043109 (2005).
  25. W. Lu, C. Huang, M. Zhou, W. B. Mori,  and T. Katsouleas, Phys. Rev. Lett. 96, 165002 (2006).
  26. J. Thomas, I. Yu. Kostyukov, J. Pronold, A. Golovanov,  and A. Pukhov, Phys. Plasmas 23, 053108 (2016).
  27. A. A. Golovanov, I. Yu. Kostyukov, A. M. Pukhov,  and J. Thomas, Quantum Electron. 46, 295 (2016).
  28. M. Tzoufras, W. Lu, F. S. Tsung, C. Huang, W. B. Mori, T. Katsouleas, J. Vieira, R. A. Fonseca,  and L. O. Silva, Phys. Plasmas 16, 056705 (2009).
Comments 0
Request Comment
You are adding the first comment!
How to quickly get a good reply:
  • Give credit where it’s due by listing out the positive aspects of a paper before getting into which changes should be made.
  • Be specific in your critique, and provide supporting evidence with appropriate references to substantiate general statements.
  • Your comment should inspire ideas to flow and help the author improves the paper.

The better we are at sharing our knowledge with each other, the faster we move forward.
""
The feedback must be of minimum 40 characters and the title a minimum of 5 characters
   
Add comment
Cancel
Loading ...
103386
This is a comment super asjknd jkasnjk adsnkj
Upvote
Downvote
""
The feedback must be of minumum 40 characters
The feedback must be of minumum 40 characters
Submit
Cancel

You are asking your first question!
How to quickly get a good answer:
  • Keep your question short and to the point
  • Check for grammar or spelling errors.
  • Phrase it like a question
Test
Test description