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An analytical optimization of plasma density profiles for downramp injection in laser wake-field acceleration

Gaetano Fiore, Paolo Tomassini

Abstract

We propose and detail a multi-step analytical procedure, based on an improved fully relativistic plane model for Laser Wake Field Acceleration, to tailor the initial density of a cold diluted plasma to the laser pulse profile, so as to control and optimize the partial wave-breaking of the plasma wave and maximize the acceleration of small bunches of electrons self-injected by the first wave-breaking at the density down-ramp, at least in the first stages of their acceleration phase. We find an excellent agreement with the results of Particle In Cell simulations obtained with the same input data.

An analytical optimization of plasma density profiles for downramp injection in laser wake-field acceleration

Abstract

We propose and detail a multi-step analytical procedure, based on an improved fully relativistic plane model for Laser Wake Field Acceleration, to tailor the initial density of a cold diluted plasma to the laser pulse profile, so as to control and optimize the partial wave-breaking of the plasma wave and maximize the acceleration of small bunches of electrons self-injected by the first wave-breaking at the density down-ramp, at least in the first stages of their acceleration phase. We find an excellent agreement with the results of Particle In Cell simulations obtained with the same input data.

Paper Structure

This paper contains 18 sections, 2 theorems, 76 equations, 15 figures, 1 table.

Key Result

Proposition 1

$\bar{P}(\xi_0)$ belongs to $\bar{P}_3\bar{P}_0$ if $\xi_0\!-\!\xi_{b}\ll\bar{\xi}_{{ H}}$ and, abbreviating $r(\bar{n})\equiv\tfrac{\bar{h}(\bar{n})}{\sqrt{\bar{h}^2(\bar{n})-{\bf 1}}}-1$,

Figures (15)

  • Figure 1: Schematic illustration of the direct and inverse problems
  • Figure 2: a) As every particle travels slower than light, $\tilde{\xi}(t)=ct\!-\!z(t)$ grows strictly, and $\xi=ct\!-\!z$ can replace $t$ as the independent parameter along its worldline (WL) $\lambda$ in Minkowski space and in its eq. of motion Fio18JPA. $\tilde{\xi}\to\xi_f<\infty$ as $t\to\infty$ implies $\dot z\to c$, see e.g. WL $\lambda'$. While the instants of intersection with the front and the end of a plane EM wave (\ref{['EBfields0']}) (whose support we have painted in pink) depend on the particular WL (we have pinpointed the ones $t_{1i},t_{1f}$ for $\lambda_1$), the corresponding light-like coordinates are the same for all WLs: $\xi_{1i}=\xi_{2i}=0$, $\xi_{1f}=\xi_{2f}=l$: the pulse acts as a "clock" for "time" $\xi$. b) We label the "particles" (i.e. elements) of the electron fluid by their initial positions ${\bm X}$; the hydrodynamic regime (HR) holds as long as their WLs do not intersect, i.e. the maps ${\bm X}\mapsto {\bm x}$ are one-to-one.We denote Eulerian, Lagrangian observables as follows: Eulerian observables${\color{red}{f}}(t,{\bm x})={\color{red}{\check f}}({\color{blue}{\xi}},{\bm x})={\color{magenta}{\tilde{f}}}(t,{\bm X})={\color{magenta}{\hat{f}}}({\color{blue}{\xi}},{\bm X})$Lagrangian observables.
  • Figure 3: a) An initial plasma density of the type (\ref{['n_0bounds']}) with an up-ramp, a down-ramp, and a plateau. b) An essentially short, slowly modulated quasi-monochromatic (SMM) laser pulse.
  • Figure 4: (a) Normalized gaussian pulse of FWHM $l'\!=\!10.5\lambda$, linear polarization, peak amplitude $a_0\!\equiv\!\lambda eE^{ \perp}_{ M}/2\pi mc^2\!=\!2$, as in section III.B of BraEtAl08. We consider $l\!=\!40\lambda$ and cut the tails outside $|\xi\!-\!l/2|\!<\!l/2$. (b) Corresponding solution of (\ref{['heq1']}-\ref{['heq2']}) if $\widetilde{n_0}(z)\!=\!\bar{n}^j\!\equiv\! n_{cr}/268.8$ ($n_{cr}\!=\! \pi mc^2/e^2\lambda^2$ is the critical density); as a result, $E/mc^2\equiv h\!=\!1.28$. Adopting $\bar{n}=\bar{n}^j$ as the density plateau maximizes the LWFA of test electrons, see section \ref{['WFA']}.B. A wavelength $\lambda=0.8\mu$m leads to a peak intensity $I\!=\!1.7\!\times\!10^{19}$W/cm$^2$ and $\bar{n}^j\!=\!6.5\times\! 10^{18}$cm$^{-3}$. (c) Corresponding phase portrait (at $\xi>l$). (d) Corresponding electron density at $t=100\lambda/c$.
  • Figure 5: Assuming the same input data as in fig. \ref{['graphsb']}, we plot: in the first row, $\check{\bm U}^{ \perp}(\xi,\xi_{{ +}})\equiv e\check {\bm A}\!^{ \perp}(\xi,\xi_{{ +}})/mc^2$ and $\hat{\bf u}^{ \perp}(\xi)\equiv e{\bm \alpha}^{ \perp}(\xi)/mc^2$ vs. $\xi$ resp. for $\xi_{{ +}}/\lambda=200,400,800$; in the second row, $V\equiv \check{\bm U}^{ \perp}{}^2(\xi,\xi_{{ +}})$ and $v\equiv \hat{\bf u}^{ \perp}{}^2(\xi)$ vs. $\xi$ resp. for $\xi_{{ +}}/\lambda=200,400,800$; in in the third row, the averages $V_a(\xi,\xi_{{ +}}),v_a(\xi)$ vs. $\xi$ resp. for $\xi_{{ +}}/\lambda=200,400,800$.
  • ...and 10 more figures

Theorems & Definitions (2)

  • Proposition 1
  • Proposition 2