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Multi-dimensional Vlasov simulations on trapping-induced sidebands of Langmuir waves

Y. Chen Key Laboratory for Micro-/Nano-Optoelectronic Devices of Ministry of Education, School of Physics and Electronics, Hunan University, Changsha, 410082, China Institute of Applied Physics and Computational Mathematics, Beijing, 100094, China    C. Y. Zheng Institute of Applied Physics and Computational Mathematics, Beijing, 100094, China HEDPS, Center for Applied Physics and Technology, Peking University, Beijing 100871, China Collaborative Innovation Center of IFSA (CICIFSA), Shanghai Jiao Tong University, Shanghai 200240, China    Z. J. Liu Institute of Applied Physics and Computational Mathematics, Beijing, 100094, China HEDPS, Center for Applied Physics and Technology, Peking University, Beijing 100871, China    L. H. Cao Institute of Applied Physics and Computational Mathematics, Beijing, 100094, China HEDPS, Center for Applied Physics and Technology, Peking University, Beijing 100871, China Collaborative Innovation Center of IFSA (CICIFSA), Shanghai Jiao Tong University, Shanghai 200240, China    C. Z. Xiao [email protected] Key Laboratory for Micro-/Nano-Optoelectronic Devices of Ministry of Education, School of Physics and Electronics, Hunan University, Changsha, 410082, China Collaborative Innovation Center of IFSA (CICIFSA), Shanghai Jiao Tong University, Shanghai 200240, China
Abstract

Temporal evolution of Langmuir waves is presented with two-dimensional electrostatic Vlasov simulations. In a muti-wavelength system, trapped electrons can generate sidebands including longitudinal, transverse and oblique sidebands. We demonstrated that oblique sidebands are important decay channels of Langmuir waves, and the growth rate of oblique sideband is smaller than the longitudinal sideband but higher than the transverse sideband. When the amplitudes of sidebands are comparable with that of Langmuir wave, vortex merging occurs following the broadening of longitudinal and transverse wavenumbers, and finally the system is developed into a turbulent state. In addition, the growth of sidebands can be depicted by the nonlinear Schrödinger model (Dewar-Rose-Yin (DRY) model) with non-Maxwellian Landau dampings. It shows the significance of particle-trapping induced nonlinear frequency shift in the evolution and qualitative agreement with Vlasov simulations.

I Introduction

In common electron-ion plasmas, some collective modes of interaction or eigenmodes can be found. And these waves are related to the charge density fluctuations. A low frequency one called ion acoustic wave corresponds to the characteristic frequency determined by ions and a high frequency one called Langmuir wavekruer ; Nicholson corresponds to the characteristic frequency determined by electrons. In inertial confinement fusion (ICF),ICF1 ; I_D ; Tik an incident pump laser can easily decay to a reflected electromagnetic wave and a Langmuir wave, which is the so-called stimulated Raman scattering (SRS).chen ; chen1 ; Brunner1 ; xiao1 ; xiao2 ; xiao3 ; xiao4 ; xiao5 Because this instability consumes pump energy and produces hot electrons, which are detrimental to fusion, it is crucial to find the saturation mechanism of SRS.Estabrook ; Vu ; yin ; Lin

At 1960s1960s, Kruer etet al.al. revealed a trapped-particle instability that Langmuir wave can decay to sidebands,KDS and it can serve as a saturation mechanism of SRS.Brunner1 The so-called Kruer, Dawson, and Sudan (KDS) model achieves great success in explaining the longitudinal sidebands in one dimension.Brunner2 ; Krasovsky Recently, Friou et al. studied sidebands of Langmuir waves as a saturation of SRS by using Vlasov and particle in cell (PIC) code in one dimensional geometry,Friou the results from different codes agree with each other and they found that the amplitude of growth rates of longitudinal sidebands have scaling law γg1ϕg2\gamma\sim g_{1}\phi^{g_{2}}, where g20.60.9g_{2}\sim 0.6-0.9 for different wavenumber of Langmuir waves. Also, another theoretical model given by Dewar, Kruer and Manheimer is used to study the sideband instability.Dewar This model is based on the nonlinear Schrödinger equation and shows that the sidebands are originated from the nonlinear frequency shift by trapped electrons.Berger1 Dewar’s model was also be extended to two dimensions (so called Dewar-Rose-Yin model, i.e.i.e. DRY model) to analyze the filamentation of Langmuir wave.rose1 ; rose2 ; winjum

Recently, the transverse decay channels of plasma waves get many attentions.Berger2 ; Denis1 ; Denis2 ; Chapman Berger etet al.al. used both generalization of KDS model (GKDS) and DRY model to study the transverse sidebands of Langmuir wave.Berger2 The growth rates of transverse sidebands of Langmuir wave are obtained from these two models and reasonably agreed with their single-wavelength Vlasov simulations. They found that transverse sidebands can lead to the filamentation of Langmuir wave. Also, D. A. Silantyev etet al.al. studied the transverse sideband of Langmuir waves.Denis1 ; Denis2 They found the scaling of the maximum growth rate is γmaxϕ\gamma_{max}\propto\sqrt{\phi} by using Vlasov-Possion simulations, where ϕ\phi is the electrostatic potential of Langmuir waves. Similarly, Chapman etet al.al. observed that the ion acoustic waves (IAW) have the longitudinal decay channel, two-ion decay (TID), and the transverse decay channel, off-axis instability (OAI). Although they failed to explain OAI by existing theories, they conjectured the OAI is an ion-driven trapped particle instability.Chapman We should note that the nature of TID instability is different from sideband instability. These works indicate that trapped particles can generate both longitudinal and transverse instabilities. Inspired by the transverse modulation of plasma waves, we believe that sidebands of Langmuir wave is a muti-dimensional instability, and the oblique sidebands whose wavevector has an oblique angle to the wavevector of Langmuir wave should be considered. In Berger’s Vlasov simulations, they only considered one longitudinal wavelength of Langmuir wave, thus they cannot observe the longitudinal and oblique sidebands.Berger2 Now, we fill this gap by using multi-wavelength Vlasov simulations and DRY model to study the sidebands of Langmuir waves in multi-dimensions .

In this paper, first, we use two-dimensional Vlasov-Poisson simulations to observe the nonlinear evolution of sidebands of Langmuir waves, including longitudinal sidebands, oblique sidebands and transverse bands. We should note that the oblique sidebands are just the trapped particle instability in a new direction. We find that oblique sidebands are important decay modes of Langmuir waves, which is similar to longitudinal sidebands and transverse sidebands. When the amplitudes of sidebands are comparable with that of Langmuir wave, sidebands saturate through a violent process featured as vortex merging in the phase space. This phenomenon is firstly discovered by Brunner etet atat.Brunner2 Recently, Yang etet al.al. also studied vortex merging by Vlasov simulations.yang The kxk_{x}, kyk_{y} component of modes then broaden rapidly. Finally, the system is developed into a turbulent state lasting from tωpe=880t\omega_{pe}=880 to the end of simulations. Second, we extent the DRY model to two dimension and obtain the growth rates of sidebands. The Landau damping of Langmuir waves in a non-Maxwellian distribution is considered. In simulations, we obtain the scaling law for longitudinal sidebands is γϕ0.75\gamma\sim\phi^{0.75}, and that for oblique sideband with ky=0.03125k_{y}=0.03125 is γϕ0.85\gamma\sim\phi^{0.85}. The g2g_{2} for longitudinal sidebands in our paper agree with the results in Friou’s work,Friou g20.60.9g_{2}\sim 0.6-0.9. In our theoretical results, the scaling law for longitudinal sidebands is γϕ0.5\gamma\sim\phi^{0.5}, and that for oblique sideband with ky=0.03k_{y}=0.03 is γϕ0.66\gamma\sim\phi^{0.66}. Our theoretical model can describe the longitudinal sidebands, oblique sidebands, and transverse sidebands. The growth rates of sidebands qualitatively agree with our Vlasov simulation results.

This paper is structured in the following ways. Firstly, in Sec. II, we use Vlasov simulations to study the nonlinear evolution of the sidebands of Langmuir waves in two dimensions. Secondly, DRY model are performed to study the growth rate of sidebands in Sec. III. At last, the conclusion and discussion are shown in Sec. IV.

II Two dimensional Vlasov simulations

II.1 Excitation of Langmuir waves

The evolution of Langmuir waves is governed by Vlasov-Poisson equations. In two-dimensional (2D) and multi-wavelength system, the Vlasov-Poisson equations are given by

fet+vxfex+vyfeyeExmefevxeEymefevy=0,2ϕx2+2ϕy2=ρEx=ϕx+Eext,Ey=ϕy,\begin{split}&\frac{\partial f_{e}}{\partial t}+v_{x}\frac{\partial f_{e}}{\partial x}+v_{y}\frac{\partial f_{e}}{\partial y}-\frac{eE_{x}}{m_{e}}\frac{\partial f_{e}}{\partial v_{x}}-\frac{eE_{y}}{m_{e}}\frac{\partial f_{e}}{\partial v_{y}}=0,\\ &\frac{\partial^{2}\phi}{\partial x^{2}}+\frac{\partial^{2}\phi}{\partial y^{2}}=\rho\\ &E_{x}=-\frac{\partial\phi}{\partial x}+E_{ext},E_{y}=-\frac{\partial\phi}{\partial y},\end{split} (1)

where fef_{e} is the distribution function, ExE_{x} and EyE_{y} are the electrostatic field at longitudinal and transverse direction, respectively, ϕ\phi is electrostatic potential, and ρ\rho is the charge density. EextE_{ext} is an external electric field, longitudinally driving the Langmuir wave. Ion motion is not considered in our paper since we mainly focus on the Langmuir wave.

Refer to caption
Figure 1: kLλDe=1/3k_{L}\lambda_{De}=1/3, the spatial space is Lx=20λLL_{x}=20\lambda_{L}, Ly=32λLL_{y}=32\lambda_{L}. (a) The temporal evolution of field energy EfieldE_{field} (blue line), electron kinetic energy EkineticE_{kinetic} (red line) and the total energy Etotal=Efield+EkineticE_{total}=E_{field}+E_{kinetic} (black dashed line). The field energy times 22 for better view. (b) is the temporal evolution of envelope of ExE_{x} and EyE_{y} at the center of the simulation box. (c) and (d) are the ExE_{x} and EyE_{y} at t=200ωpe1t=200\omega_{pe}^{-1}. (e) and (f) are the corresponding spectrum at kxk_{x}-kyk_{y} space.

We have developed a 2D version of Vlasov-Poisson code, PLAW2d (2D Plasma Wave simulation), which uses Van Leer scheme (VL3)VL ; VL2 to solve the Vlasov equation and fast Fourier transform (FFT) to solve the Poisson equation yang ; yangs ; feng . The spatial domain occupies X[0,Lx]X\in[0,L_{x}] and Y[0,Ly]Y\in[0,L_{y}], and the boundary conditions are periodic at each side. The lengths of simulation box are Lx=20λLL_{x}=20\lambda_{L} and Ly=32λLL_{y}=32\lambda_{L}, where λL=2π/kL\lambda_{L}=2\pi/k_{L} is the wavelength of Langmuir wave and kL=1/3λDe1k_{L}=1/3\lambda_{De}^{-1} is the corresponding wavenumber. We choose kL=1/3λDe1k_{L}=1/3\lambda_{De}^{-1} as the wavenumber in simulation because it corresponds to the kinetic regime of SRS in ICF. Some nonlinear effects by particle trapping will occur in kinetic regime, such as trapped particle instability (TPI), inflation of SRS because of the decreasing of Landau damping of Langmuir wave, and spatially auto-resonant Stimulated Raman Scattering due to the nonlinear frequency shift in inhomogeneous plasma. The physical spaces are discretized by Δx=1.0471λDe\Delta x=1.0471\lambda_{De} and Δy=6.032λDe\Delta y=6.032\lambda_{De}, where λDe\lambda_{De} is the electron Debye length. The velocity domain is vx,y[12vte,12vte]v_{x,y}\in[-12v_{te},12v_{te}] and they are discretized by Δvx=Δvy=0.1vte\Delta v_{x}=\Delta v_{y}=0.1v_{te}, where vte=Te/mev_{te}=\sqrt{T_{e}/m_{e}} is the thermal velocity of electrons, TeT_{e} and mem_{e} are the temperature and mass of electrons, respectively. Therefore, the four dimensional meshgrids are 360×100×241×241360\times 100\times 241\times 241. Electrons in plasma are initialized by 2D Maxwellian distribution function, fe0(vx,vy)=12πvteexp(vx2+vy22vte2)f_{e0}(v_{x},v_{y})=\frac{1}{2\pi v_{te}}exp(-\frac{v_{x}^{2}+v_{y}^{2}}{2v_{te}^{2}}). The total simulation time is ttotal=2500ωpe1t_{total}=2500\omega_{pe}^{-1}, and the time step is dt=0.1ωpe1dt=0.1\omega_{pe}^{-1}, where ωpe=4πnee2/me\omega_{pe}=\sqrt{4\pi n_{e}e^{2}/m_{e}} is the plasma frequency and nen_{e} is the electron density of plasma. We should notice that in the remaining paper the units are normalized to electron unit, such as, vte=1v_{te}=1, ωpe=1\omega_{pe}=1 and λDe=1\lambda_{De}=1, etc.

At the drive phase shown in Fig. 1(a) , t=0200ωpe1t=0\sim 200\omega_{pe}^{-1}, an external electrostatic field

Eext=Eextmax[1+(tττ)n]1sin(kLxωLt),E_{ext}=E_{ext}^{max}\left[1+(\frac{t-\tau}{\triangle\tau})^{n}\right]^{-1}sin(k_{L}x-\omega_{L}t), (2)

is used to induce the Langmuir waves, where Eextmax=0.01meωpevte/eE_{ext}^{max}=0.01m_{e}\omega_{pe}v_{te}/e is the amplitude of pump drive, τ=100ωpe1\tau=100\omega_{pe}^{-1}, τ=50ωpe1\triangle\tau=50\omega_{pe}^{-1}, n=10n=10 and ωL=ωpe2+3kL2vte2\omega_{L}=\sqrt{\omega_{pe}^{2}+3k_{L}^{2}v_{te}^{2}} is the Bohm-Gross dispersion relation of Langmuir wave and the phase velocity is vϕ=ωL/kLv_{\phi}=\omega_{L}/k_{L}. In stage I shown in Fig. 1(a), the field energy and electron kinetic energy increase exponentially because the Langmuir waves are resonant excited. Fig. 1(b) is the time history of ExE_{x} and EyE_{y} envelopes at the center of the simulation box, and it shows the amplitude of ExE_{x} increases to 0.20.2 at t=200ωpe1t=200\omega_{pe}^{-1}. Fig. 1(c) to (f) are ExE_{x} and EyE_{y} in physical space and the their spectra in kxkyk_{x}-k_{y} space at t=200ωpe1t=200\omega_{pe}^{-1}, respectively. In Fig. 1(c), there occupies the longitudinal Langmuir wave with 2020 wavelengths, but no fields are observed in the transverse direction as shown in Fig. 1(d). Correspondingly, the Langmuir wave (LW) mode are clearly excited at kx=1/3,ky=0k_{x}=1/3,k_{y}=0 in Fig. 1(e), and no mode are shown in the transverse directions in Fig. 1(f).

II.2 Growth of sidebands

Refer to caption
Figure 2: (a) and (b) are the ExE_{x} and EyE_{y} at t=560ωpe1t=560\omega_{pe}^{-1}. (c) and (d) are the corresponding spectrum at kxk_{x}-kyk_{y} space. In (c), the red diamonds stand for the selected sidebands of Langmuir waves. (e) The evolution of Langmuir wave (black line), the growth of longitudinal sideband(blue line), oblique sidebands (red and orange lines) and transverse sidebands(violet, green and manganese purple lines).

At t=200ωpe1t=200\omega_{pe}^{-1}, the external field is turned off, leaving the Langmuir waves propagating freely. The excited wave is, however, unstable to many instabilities, such as sideband instability, modulational instability, and filamentation instability etc. The trapped-particle-induced sidebands of Langmuir wave are the earliest-developing ones. In Fig. 1(a), the stage II (t=200880ωpe1t=200\sim 880\omega_{pe}^{-1}) is defined as the growth of sidebands where three kinds of sidebands are observed. The first one is the longitudinal sideband, i.e.i.e. kxkL,ky=0k_{x}\neq k_{L},k_{y}=0. This kind of sideband is well-studied in one-dimensional systems.Brunner1 ; KDS ; Brunner2 ; Dewar ; yang The second one is the transverse sideband defined by kx=kL,ky0k_{x}=k_{L},k_{y}\neq 0 and discussed by Berger et al. Berger2 The last kind is called the oblique sideband, i.e.i.e. kxkLk_{x}\neq k_{L} and ky0k_{y}\neq 0, which exists in multi-wavelength and multi-dimensional systems and has never been discovered before.

Refer to caption
Refer to caption
Figure 3: (a) Distribution function of electrons in vxv_{x}-vyv_{y} space at tωpe=200t\omega_{pe}=200. (b) Distribution function of electrons in vxv_{x}-vyv_{y} space at tωpe=600t\omega_{pe}=600.

Fig. 2(a) and (b) are ExE_{x} and EyE_{y} in the physical space at t=560ωpe1t=560\omega_{pe}^{-1}. In addition to the nearly unchanged longitudinal fields, modes with small amplitudes are observed in Fig. 2(b), which imply sidebands with ky0k_{y}\neq 0 are excited. Fig. 2(c) and (d) are the corresponding spectra of sidebands in kxk_{x}-kyk_{y} space where longitudinal sidebands, transverse sidebands and oblique sidebands emerge clearly. In Fig. 2 (c), we pick some modes for further analyses: LW represents the Langmuir wave at kx=1/3,ky=0k_{x}=1/3,k_{y}=0; LS stands for the longitudinal sidebands with the maximum growth rate at kx=0.25,ky=0k_{x}=0.25,k_{y}=0; OS1 and OS2 are two chosen oblique sidebands for kx=0.2667,ky=0.03125k_{x}=0.2667,k_{y}=0.03125 and kx=0.2833,ky=0.0625k_{x}=0.2833,k_{y}=0.0625; TS1, TS2 and TS3 are three transverse sidebands at kx=kLk_{x}=k_{L} and ky=0.03,0.04167k_{y}=0.03,0.04167 and 0.10.1, respectively.

Refer to caption
Figure 4: (a) and (b) are the electron trapped structures at t=500ωpe1t=500\omega_{pe}^{-1} and t=1500ωpe1t=1500\omega_{pe}^{-1}. (c) and (d) are the temporal evolution of kxk_{x} and kyk_{y} spectrum. toff=200ωpe1t_{off}=200\omega_{pe}^{-1} is the time when the external driver is turned off, tmerge=880ωpe1t_{merge}=880\omega_{pe}^{-1} is when the vortex merging happens. (e) and (f) are the ExE_{x} and EyE_{y} at t=1500ωpe1t=1500\omega_{pe}^{-1}. (g) and (h) are the corresponding spectrum at kxk_{x}-kyk_{y} space.

The growth of these sidebands are shown in Fig. 2(e). When resonant excited, the Langmuir wave (black line) gives its energy to other modes and particles. The fastest growing mode is the longitudinal sideband denoted by the blue line, and then it comes the oblique sidebands (the red line and the orange line), slowing down with the increase of kyk_{y}. The transverse sidebands are the slowest ones as indicated by the purple, green, and pink lines. As kyk_{y} increases the growth rate of transverse sideband increases first and then decreases, showing the same features revealed by Berger et al. Berger2 The maximum growth rate of the transverse sideband is located at ky=0.04167k_{y}=0.04167. However, this is valid only when t=200600ωpe1t=200\sim 600\omega_{pe}^{-1}, since a two-stage growth of transverse sidebands is observed. When 600ωpe1<t<1000ωpe1600\omega_{pe}^{-1}<t<1000\omega_{pe}^{-1}, a rapid growth of the transverse sideband emerges, violating the linear growth pattern of sideband instabilities. Two-stage growth of sidebands can also be seen in earlier works.Brunner2 ; Berger2 ; Denis1 However, no excellent explanation of this phenomenon was provided by early works. Fig. 3 shows the phase space structures in vxv_{x} and vyv_{y} at two typical times t=200ωpe1t=200\omega_{pe}^{-1} and t=600ωpe1t=600\omega_{pe}^{-1}. Based on the discovery of a recent work,yanxia when the beam-like distribution function of electron was formed, there will be a beam plasma instability induced by the beam of electrons. The average beam velocity is equal to the phase velocity of Langmuir wave. This instability may lead to the two-stage growth of initially slower growing modes. Accordingly, the beam-like of distribution function of electron is also formed in Fig. 3(b). So,we guess the two-stage growth of initially slower growing modes may be related to the beam-plasma instability.

We summarize the results above that sidebands of the Langmuir wave can be excited by trapped electrons. In a two-dimensional and multi-wavelength system, there are sidebands in three kinds of directions, i.e. longitudinal sidebands, transverse sidebands and oblique sidebands. The maximum growth occurs with the longitudinal sideband, and the second maximum growth belongs to the oblique sideband, which is the trapping-induced sideband in a new direction. The slowest is transverse sideband.

II.3 Vortex merging and wave-particle-interaction-induced turbulence

At t900ωpe1t\approx 900\omega_{pe}^{-1} in Fig. 1(a), there exists a violent energy exchange between kinetic and field energy, which implies strong wave-particle interactions. Also, in Fig. 1(b), ExE_{x} and EyE_{y} become unprecedentedly oscillative, revealing a whole new stage. This specific stage III is termed as the turbulent state. The term, turbulent state, means an utter destruction of the coherent phase-space structures into chaos, which is described in a recent one-dimensional study.Brunner2 ; yang

When different modes have similar amplitudes comparable to the fundamental Langmuir wave, they will interact with the BGK structure of Langmuir waves.Shoucr1 ; Shoucr2 ; Shoucr3 At t880ωpe1t\approx 880\omega_{pe}^{-1}, it hits the critical point and then vortex merging happens. In Fig. 4(a), there are 2020 vortices in the phase space before vortex merging, but after that only 1515 vortices are left with irregular trajectories shown in Fig. 4(b). The transition is demonstrated clearly in Fig. 4(c) and (d), which plot the temporal evolutions of ExE_{x} in kxk_{x} and kyk_{y} space, respectively. The black dashed lines, kx=1/3k_{x}=1/3 in 4(c) and ky=0k_{y}=0 in 4(d) represent the Langmuir wave. After turning off the driver, the longitudinal sidebands with the maximum growth rates occur along the black dashed lines (kLxδkk_{Lx}-\delta_{k} and kLx+δkk_{Lx}+\delta_{k}) in Fig. 4(c). Oblique and transverse sidebands are subsidiary signals apart from the main Langmuir wave and longitudinal sidebands signals. An abrupt transition occurs at tmerge=880ωpe1t_{merge}=880\omega_{pe}^{-1}, and within less than 50ωpe150\omega_{pe}^{-1} the spectrum explodes. After that transition, the broadening spectrum seems to be a long-term and stable structure, so we suppose the final state of the Langmuir wave is reached. Since the spectrum is much like the turbulence structure, we term the final state as the wave-particle-interaction-induced turbulent state.

The turbulent states in physical space and spectral space are shown in Figs. 4(e) to (h) at t=1500ωpe1t=1500\omega_{pe}^{-1}. Filaments-like structures are easily observed in Fig. 4(e) and (f). These structures are characterized by the stripes in the kxk_{x}-kyk_{y} space resulting from nonlinear expansions of the sidebands along kyk_{y}.

II.4 Amplitude dependence of sidebands

Refer to caption
Figure 5: Vlasov simulation results. (a) The positions of oblique sidebands for different amplitude of field at kxk_{x}-kyk_{y} space. (b) The scaling law of growth rates of sidebands are obtained by using power law fitting γ=g1ϕg2\gamma=g_{1}\phi^{g_{2}}. We find that g2=0.75g_{2}=0.75 for longitudinal sideband and g2=0.85g_{2}=0.85 for oblique sideband with ky=0.03125k_{y}=0.03125.

By changing the starting amplitude of Langmuir wave potential, we find the nonlinear evolution experiencing such processes is rather robust. Here, only the amplitude of Langmuir wave potential is changed and other parameters keep the same as discussed above.

When the amplitude is getting larger, the number of trapped electrons also increases, leading to an increase of the frequency shift.Berger2 The amplitude dependence of positions of the brightest sideband signals in kxk_{x}-kyk_{y} space are shown in Fig 5 (a). The |kxkL||k_{x}-k_{L}| for oblique sidebands increases with the electrostatic fields, which is similar to the longitudinal sidebands. And the maximum value of kyk_{y} for oblique sidebands also increases with the electrostatic fields, which is similar to the transverse sidebands.

In Fig. 5 (b), we extract the maximum growth rates of longitudinal sidebands (red circles) and the growth rate of the oblique sideband with ky=0.03125k_{y}=0.03125 (blue squares). Especially, the dependence on the amplitude for longitudinal sideband is obtained by power law fitting γ=g1ϕg2\gamma=g_{1}\phi^{g_{2}} with g2=0.75g_{2}=0.75, and that for oblique sideband is g2=0.85g_{2}=0.85. Our scaling law for longitudinal sideband agree with early work g20.60.9g_{2}\sim 0.6-0.9.Friou g2g_{2} for sidebands are close to 0.50.5, which reminds us the sideband instability has a strong relationship with the trapped-particle induced nonlinear frequency shift, which is also the starting point of our theoretical model of multidimensional sideband instability.

III Theoretical Model: sidebands of Langmuir waves

The Dewar-Rose-Yin (DRY) model was first used to study the 1D modulation instability of Langmuir wave and then extended to study 2D modulation and filamentation instabilities.Dewar ; rose1 ; rose2 ; Berger2 Here we reuse this model to predict the sidebands of Langmuir wave. In 2D situation, the modulation instability can be described by nonlinear Schrödinger equation,

i(t+ωkkxx+υ)ϕk+(122ωkky22y2+122ωkkx22x2+Δω)ϕk=0,\begin{split}i&\left(\frac{\partial}{\partial t}+\frac{\partial\omega_{k}}{\partial k_{x}}\frac{\partial}{\partial x}+\upsilon\right)\phi_{k}\\ &+\left(\frac{1}{2}\frac{\partial^{2}\omega_{k}}{\partial k_{y}^{2}}\frac{\partial^{2}}{\partial y^{2}}+\frac{1}{2}\frac{\partial^{2}\omega_{k}}{\partial k_{x}^{2}}\frac{\partial^{2}}{\partial x^{2}}+\Delta\omega\right)\phi_{k}=0,\end{split} (3)

where ϕk(x,y,t)\phi_{k}(x,y,t) is the envelope of potential, ν\nu is the Landau damping, and ωk\omega_{k} is the root of the dispersion relation ϵ(k,ω)=0\epsilon(\vec{k},\omega)=0. The fluid type of dispersion relation is used,

ϵ(k,ω)=ϵ(k,ω)=1ωpe2ω23k2vte2,\epsilon(\vec{k},\omega)=\epsilon(k,\omega)=1-\frac{\omega_{pe}^{2}}{\omega^{2}-3k^{2}v_{te}^{2}}, (4)

where k=|k|=kx2+ky2k=|\vec{k}|=\sqrt{k_{x}^{2}+k_{y}^{2}} is the wavenumber of sidebands. The nonlinear term causing instability is the trapped-particle induced nonlinear frequency shift, Δω\Delta\omega. To express it analytically, we use the adiabatic driven formula, Berger1

Δωωpe=α2π(kLλDe)2eEmaxTekL(v21)exp(v22)|v=vϕ/vte.\frac{\Delta\omega}{\omega_{pe}}=-\frac{\alpha}{\sqrt{2\pi}(k_{L}\lambda_{De})^{2}}\sqrt{\frac{eE_{max}}{T_{e}k_{L}}}(v^{2}-1)exp(-\frac{v^{2}}{2})|_{v=v_{\phi}/v_{te}}. (5)

where α=0.544\alpha=0.544, vϕv_{\phi} is the phase velocity of Langmuir wave and Emax=0.2meωpevte/eE_{max}=0.2m_{e}\omega_{pe}v_{te}/e is the electron field amplitude of the Langmuir wave, which corresponds to a potential of |eϕ/Te|=0.6|e\phi/T_{e}|=0.6.

In order to find instability growth rate of Eq. 3, we assume two small sidebands ωk=ωL±Ω\omega_{k}=\omega_{L}\pm\Omega, kx=kL±Δkxk_{x}=k_{L}\pm\Delta k_{x} and ky=kLy±Δkyk_{y}=k_{Ly}\pm\Delta k_{y} where ωL\omega_{L}, kLk_{L} are linear frequency and wavenumber of Langmuir wave, and in our consideration, kLy=0k_{Ly}=0. Let the Landau damping ν\nu be absorbed by Ω\Omega. Assuming a trial solution ϕ(x,y,t)=1/2(ϕk(x,y,t)exp(ikxiωkt)+c.c.)\phi(x,y,t)=1/2(\phi_{k}(x,y,t)exp(i\vec{k}\cdot\vec{x}-i\omega_{k}t)+c.c.) for Eq. 3, we can obtain the dispersion relation,

(ΩΔkxωkkx)2=(Δkx222ωkkx2+Δky222ωkky2)(Δkx222ωkkx2+Δky222ωkky2+Δω2),\begin{split}&\left(\Omega-\Delta k_{x}\frac{\partial\omega_{k}}{\partial k_{x}}\right)^{2}=\left(\frac{\Delta k_{x}^{2}}{2}\frac{\partial^{2}\omega_{k}}{\partial k_{x}^{2}}+\frac{\Delta k_{y}^{2}}{2}\frac{\partial^{2}\omega_{k}}{\partial k_{y}^{2}}\right)\\ &\left(\frac{\Delta k_{x}^{2}}{2}\frac{\partial^{2}\omega_{k}}{\partial k_{x}^{2}}+\frac{\Delta k_{y}^{2}}{2}\frac{\partial^{2}\omega_{k}}{\partial k_{y}^{2}}+\frac{\Delta\omega}{2}\right),\end{split} (6)

where Δkx=kxkL\Delta k_{x}=k_{x}-k_{L}, Δky=ky\Delta k_{y}=k_{y}. The growth rate of sideband is

γ(kx,ky)=Im(Ω)+υ.\gamma(k_{x},k_{y})=Im(\Omega)+\upsilon. (7)
Refer to caption
Figure 6: (a) Contours of solutions to the Langmuir wave when |eϕ/Te|=0|e\phi/T_{e}|=0 and ky=0k_{y}=0, blue line stands for the real part of dielectric function, red line is the imaginary part of dielectric function. (b) Contours of solutions to the Langmuir wave when |eϕ/Te|=0.6|e\phi/T_{e}|=0.6 and ky=0k_{y}=0. (c) Contours of solutions to the Langmuir wave when |eϕ/Te|=0.6|e\phi/T_{e}|=0.6 and ky=0.12k_{y}=0.12. (d) The Landau damping as a function of kyk_{y} with different amplitudes.

The imaginary part of Ω\Omega exists only when (Δkx22ωkkx2+Δky22ωkky2)Δω<0(\Delta k_{x}^{2}\frac{\partial^{2}\omega_{k}}{\partial k_{x}^{2}}+\Delta k_{y}^{2}\frac{\partial^{2}\omega_{k}}{\partial k_{y}^{2}})\Delta\omega<0. Since 2ωkkx2=2ωkky23vte2/ωL\frac{\partial^{2}\omega_{k}}{\partial k_{x}^{2}}=\frac{\partial^{2}\omega_{k}}{\partial k_{y}^{2}}\approx 3v_{te}^{2}/\omega_{L}, thus modulation instability exists only when Δω<0\Delta\omega<0. The maximum value of Im(Ω)Im(\Omega) and its location are easily solved from Eq. (6),

(Im(Ω))m=Δω4,\displaystyle(Im(\Omega))_{m}=\frac{\Delta\omega}{4}, (8)
(kxkL)2+ky2=ΔωωL6vte2.\displaystyle(k_{x}-k_{L})^{2}+k_{y}^{2}=\frac{\Delta\omega\omega_{L}}{6v_{te}^{2}}. (9)

Since Δω\Delta\omega is independent of kk, if no damping is considered ν=0\nu=0, a constant maximum growth rate is located along a circle of the initial Langmuir wavenumber, (kL,0)(k_{L},0). This is, of course, not consistent with our simulation results, so we must consider the distribution of Landau damping, υ=υ(kx,ky)\upsilon=\upsilon(k_{x},k_{y}).

Refer to caption
Figure 7: (a) The growth rates of sidebands obtained by DRY model, |eϕ/Te|=0.6|e\phi/T_{e}|=0.6. (b) The growth rates of longitudinal sidebands. (c) The growth rates of transverse sidebands. (d) The growth rates of oblique sidebands with ky=0.03k_{y}=0.03.

To do so, we must calculate the Landau damping in a trapping distribution function, such as the one presented at t=200ωpe1t=200\omega_{pe}^{-1} in our simulation. Following the treatment of early works,Berger2 ; Divol a two-dimensional trapping distribution function is artificially constructed,

f0(vx,vy)=Nef0,x(vx)f0,y(vy),f0,y(vy)=fM(vy),f0,x(vx)=fM(vx)+δfxflat(u),δfxflat(u)=P(u)12vteexp(u2/2),P(u)=βu+γ(u21),u=(vxvϕ)/δv,\begin{split}&f_{0}(v_{x},v_{y})=N_{e}f_{0,x}(v_{x})f_{0,y}(v_{y}),\\ &f_{0,y}(v_{y})=f_{M}(v_{y}),\\ &f_{0,x}(v_{x})=f_{M}(v_{x})+\delta f_{x}^{flat}(u),\\ &\delta f_{x}^{flat}(u)=P(u)\frac{1}{\sqrt{2}v_{te}}exp(-u^{2}/2),\\ &P(u)=\beta u+\gamma(u^{2}-1),\\ &u=(v_{x}-v_{\phi})/\delta v,\end{split} (10)

where fM(vx)f_{M}(v_{x}) and fM(vy)f_{M}(v_{y}) are one-dimensional Maxwellian distributions. δv=2eϕ/Te\delta v=2\sqrt{e\phi/T_{e}} is the width of the plateau around the phase velocity. β\beta and γ\gamma are the first and second derivatives of f0,x(vx)f_{0,x}(v_{x}) at phase velocity,

β=(δv~)v~exp(v~2/2)|v~=vϕ/vte,γ=δv~3(1v~2)exp(v~2/2)|v~=vϕ/vte,\begin{split}&\beta=(\delta\tilde{v})\tilde{v}exp(-\tilde{v}^{2}/2)|_{\tilde{v}=v_{\phi}/v_{te}},\\ &\gamma=\frac{\delta\tilde{v}}{3}(1-\tilde{v}^{2})exp(-\tilde{v}^{2}/2)|_{\tilde{v}=v_{\phi}/v_{te}},\\ \end{split} (11)

where δv~=δv/vte\delta\tilde{v}=\delta v/v_{te}. The constructed distribution function resembles Fig. 3(a), which enables the zero Landau damping near the phase velocity vϕ=ωL/kLv_{\phi}=\omega_{L}/k_{L}. The kinetic dispersion function under the non-Maxwellian distribution function is

ϵ(ω,k)=1ωpe2k2Pvf0dvvω/kiπωpe2k2|vf0|v=ωk,\epsilon(\omega,k)=1-\frac{\omega_{pe}^{2}}{k^{2}}P\int^{\infty}_{-\infty}\frac{\nabla_{v}f_{0}\cdot d\textbf{v}}{v-\omega/k}-i\pi\frac{\omega_{pe}^{2}}{k^{2}}|\nabla_{v}f_{0}|_{v=\frac{\omega}{k}}, (12)

where PP means the Cauchy principal value, v=(vx,vy)\textbf{v}=(v_{x},v_{y}), and k=kx2+ky2k=\sqrt{k_{x}^{2}+k_{y}^{2}}.

Refer to caption
Figure 8: Theoretical results obtained by DRY model. (a) and (b) use α=0.544\alpha=0.544, which corresponds to adiabatic approximation.Berger1 (a) The positions of oblique sidebands for different amplitude of field at kxk_{x}-kyk_{y} space. (b) The amplitude of field dependence of growth rate of longitudinal sideband with maximum growth rate(blue squares) and the growth rates of oblique sideband with ky=0.03k_{y}=0.03. (c) and (d) are the same results by using α=0.823\alpha=0.823, which corresponds to sudden approximation.Berger1

Since the distribution function is almost flattened near the Langmuir wave phase velocity but decreases dramatically when kyk_{y} increases, we assume the Landau damping varies with kyk_{y} but is constant along Δkx\Delta k_{x}. Then we can numerically solve the dispersion function Eq. (12) along kx=kLk_{x}=k_{L} and obtain the Landau damping as a function of kyk_{y} in Fig. 6. When |eϕ/Te|=0|e\phi/T_{e}|=0, it backs to the Maxwellian distribution function, so the Landau damping is 0.026ωpe-0.026\omega_{pe} as shown in Fig. 6(a). Fig. 6(b) shows the Landau damping at ky=0k_{y}=0 when eϕ/Te=0.6e\phi/T_{e}=0.6, and the evaluated Landau damping being 0 satisfies our designed distribution function. As kyk_{y} increases to 0.120.12 in Fig. 6(c), the phase velocity of sidebands becomes away from the trapped plateau, so the Landau damping increases to 0.0296ωpe-0.0296\omega_{pe}. Fig. 6(d) shows the overall Landau damping increases with kyk_{y}. And the Landau damping will decrease with the potential, because when |eϕ/Te||e\phi/T_{e}| increases from 0.60.6 to 1.21.2, the width of trapped region becomes larger in accordance with our expectation. We should note that the distribution in Eqs. 10 is artifical, thus, vϕv_{\phi} in Eqs. 10 and Eqs. 11 is adjustable to make sure the Landau damping equals to 0, when|eϕ/Te|0|e\phi/T_{e}|\neq 0 and ky=0k_{y}=0.

Refer to caption
Figure 9: Theoretical results by DRY model for kλDe=1/3k\lambda_{De}=1/3 with sudden approximation. The scaling law of growth rates of sidebands are obtained by using power law fitting γ=g1ϕg2\gamma=g_{1}\phi^{g_{2}}. We find that g2=0.5g_{2}=0.5 for longitudinal sideband and g2=0.66g_{2}=0.66 for oblique sideband with ky=0.03k_{y}=0.03.

Fig. 7 shows the final theoretical growth rates of sidebands obtained when |eϕ/Te|=0.6|e\phi/T_{e}|=0.6. The shape of sidebands in Fig. 7(a) resembles the spectrum in Fig. 2(c). We pick out three kinds of sidebands in Fig. 7(b), (c) and (d). Fig. 7(b) represents the longitudinal sidebands, where its maximum growth rate locates at kx=0.2733,ky=0k_{x}=0.2733,k_{y}=0 and the maximum growth rate is γLS=0.0103ωpe\gamma_{LS}=0.0103\omega_{pe}. In our simulations, the corresponding quantities are kx=0.25,ky=0k_{x}=0.25,k_{y}=0, and γLS=0.02199ωpe\gamma_{LS}=0.02199\omega_{pe}. The DRY model underestimates δk\delta_{k} and the growth rate of sideband perhaps due to the underestimation of the nonlinear frequency shift Δω\Delta\omega in Eq. 5. Fig. 7(c) is the transverse sidebands with kx=kLk_{x}=k_{L}. The position of transverse sideband with the maximum growth rate locates at kx=kL,ky=0.04k_{x}=k_{L},k_{y}=0.04, and the maximum growth rate of transverse sideband is γTS=0.0052ωpe\gamma_{TS}=0.0052\omega_{pe}. While in simulations they are kx=kL,ky=0.04167k_{x}=k_{L},k_{y}=0.04167 and γTS=0.00588ωpe\gamma_{TS}=0.00588\omega_{pe}, respectively, which show good consistencies for transverse sidebands. This is because the transverse sidebands are mostly affected by Landau damping of sidebands,Berger2 showing the Landau damping in our calculation is accurate. Fig. 7(d) stands for the growth rates of oblique sidebands with ky=0.03k_{y}=0.03, which is between the longitudinal and transverse sidebands as indicated by our Vlasov simulations.

Refer to caption
Refer to caption
Figure 10: Vlasov simulation results with |eϕ/Te|=0.6|e\phi/T_{e}|=0.6. (a) The spectrum of ExE_{x} in kxk_{x}-ω\omega space with a time window tωpe=01000t\omega_{pe}=0\sim 1000. The green line represents the dispersion relation of Langmuir wave. (b) The spectrum of ExE_{x} in kyk_{y}-ω\omega space with a time window tωpe=01000t\omega_{pe}=0\sim 1000.

The theoretical shapes of sidebands with the maximum growth rates and the corresponding growth rates as a function of potential amplitude are shown in Fig. 8. To compare with the Vlasov results, a sudden driven model of nonlinear frequency shift is plotted in Fig. 8(c) and (d), in addition to the adiabatic model shown in Fig. 8(a) and (b). The difference is that in a sudden driven model, α=0.823\alpha=0.823 in Eq. 5,Berger1 which permits a higher Langmuir wave frequency shift. Fig. 8(a) shows the amplitude dependence of the positions of sidebands. As compared with Fig. 5(a), the shape and dependence on amplitude are similar, but it shrinks inward. When turning to the sudden driven model with Δωsudden1.5Δωadiabatic\Delta\omega_{sudden}\approx 1.5\Delta\omega_{adiabatic}, the shapes get large. In Fig. 8(b) and (d), the growth rates of longitudinal sidebands scale linearly with |eϕ/Te|1/2|e\phi/T_{e}|^{1/2}, which agrees with early theoretical results.Dewar ; Berger2 As the nonlinear frequency shift gets larger, Fig. 8(d) shows a better agreement with the simulation results in Fig. 5(b). In Fig. 9, we obtain the scaling law for sidebands by power law fitting under sudden approximation. g2=0.5g_{2}=0.5 for longitudinal sideband and g2=0.66g_{2}=0.66 for oblique sideband with ky=0.03k_{y}=0.03. Both in simulation and theoretical results, g2g_{2} for oblique sideband is a little larger than that of longitudinal sidebands. This may be because the influence of Landau damping on oblique sidebands.

However, there still exist discrepancies between Vlasov simulations and DRY model, especially when |eϕ/Te||e\phi/T_{e}| is large. We suspect that it is due to the underestimation of Δω\Delta\omega in DRY model. Therefore, in Fig 10(a) and (b), we plot the spectra of ExE_{x} in the kxk_{x}-ω\omega space and the kyk_{y}-ω\omega from Vlasov simulations with |eϕ/Te|=0.6|e\phi/T_{e}|=0.6, respectively. The observed nonlinear frequency shifts of Langmuir wave and sidebands is on the order of Δω0.1ωpe\Delta\omega\approx 0.1\omega_{pe}, however, theory predicts that Δωadiabatic=0.0413ωpe\Delta\omega_{adiabatic}=0.0413\omega_{pe} for adiabatic approximation and Δωsudden=0.0624ωpe\Delta\omega_{sudden}=0.0624\omega_{pe} for sudden approximation. Though with some flaws, the DRY model is good enough to capture the main physics of sidebands of Langmuir waves, and the growth rates of sidebands are qualitatively agreed with our 2D electrostatic Vlasov simulations.

IV Conclusion and discussion

In this paper, first, we study the evolution of Langmuir waves in a muti-wavelength system through 2D Vlasov simulations. There are three stages in our simulations. In the drive phase, an external driver is used to excited a monochromatic Langmuir waves. In the phase of sideband growth, the sidebands of Langmuir waves are excited because of the trapped electrons. Three kinds of sidebands are observed, which are the longitudinal sidebands, oblique sidebands and transverse sidebands. The oblique sidebands are arc-shaped in the k-space. The growth rates of oblique sidebands are smaller than that of the longitudinal sideband with the maximum growth rate but higher than the transverse sideband. In the turbulent state, the vortex merging happens when the amplitudes of sidebands are comparable with that of Langmuir waves. After vortex-merging, 2020 vortices merges to 1515 vortices. And The spectra of kxk_{x} and kyk_{y} become broader, inducing the filamentation of Langmuir waves. The amplitude dependence of sidebands are also studied by Vlasov simulations. We find that Δkx\Delta k_{x} of longitudinal sidebands and Δkx\Delta k_{x} and Δky\Delta k_{y} of oblique sidebands increase with the amplitude. Next, we reuse the DRY model to study the sidebands of Langmuir waves. Based on the early work,Berger2 the Landau damping with kyk_{y} should be considered. The growth rates of three kinds of sidebands are finally obtained by DRY model, and they are qualitatively agreed with our Vlasov simulations.

The sideband instability is a saturation mechanism of SRS in ICF, and in earlier works, researchers mostly focused on the Longitudinal sidebands of Langmuir wave.Brunner1 ; Friou The Vlasov simulations and theoretical results show clearly that sideband of Langmuir wave is a multidimensional instability. So, the sidebands of Langmuir wave in oblique and tranverse direction should also be considered. In this paper, we only consider the situation in two dimensions. The sideband with kzk_{z} component might also exist. Besides, in early works, some kinetic effects by particle trapping have been studied by using particle in cell (PIC) simulations, such as Langmuir wave bowingyin ; Lin the trapped particle side loss hxvu3 in multidimensions. These works indicate that Multidimensional effects are important for instabilities in ICF. In the future works, PIC simulations will be used to study the sidebands of Langmuir wave in multidimensions.

Acknowledgements

We are pleased to acknowledge useful discussions with T. Yang, Y. Z. Zhou and S. X. Xie. This work was supported by the Strategic Priority Research Program of Chinese Academy of Sciences (Grant No. XDA25050700), National Natural Science Foundation of China (Grant Nos. 11805062, 11875091 and 11975059), Science Challenge Project, No. TZ2016005 and Natural Science Foundation of Hunan Province, China (Grant No. 2020JJ5029).

DATA AVAILABILITY

The data that support the findings of this study are available from the corresponding author upon reasonable request.

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