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  97. %%%TITLE, AUTHORS AND ABSTRACT%%%
  98. \twocolumn[
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  103. \includegraphics{head_foot/DOI} & \noindent\LARGE{\textbf{ Plasma-Induced Symmetry Breaking in a Spherical Silicon Nanoparticle}} \\%Article title goes here instead of the text "This is the title"
  104. \vspace{0.3cm} & \vspace{0.3cm} \\
  105. & \noindent\large{Anton Rudenko,$^{\ast}$\textit{$^{a}$} Tatiana E. Itina,\textit{$^{a\ddag}$} Konstantin Ladutenko,\textit{$^{b}$} and Sergey Makarov\textit{$^{b}$}
  106. \textit{$^{a}$~Laboratoire Hubert Curien, UMR CNRS 5516, University of Lyon/UJM, 42000, Saint-Etienne, France }
  107. \textit{$^{b}$~ITMO University, Kronverksiy pr. 49, St. Petersburg, Russia}
  108. } \\%Author names go here instead of "Full name", etc.
  109. \includegraphics{head_foot/dates} & \noindent\normalsize{The concept
  110. of nonlinear all-dielectric nanophotonics based on high refractive
  111. index (e.g., silicon) nanoparticles supporting magnetic optical
  112. response has recently emerged as a powerful tool for ultrafast
  113. all-optical modulation at nanoscale. A strong modulation can be
  114. achieved via photogeneration of dense electron-hole plasma in the
  115. regime of simultaneous excitation of electric and magnetic optical
  116. resonances, resulting in an effective transient reconfiguration of
  117. nanoparticle scattering properties. However, previous works assumed
  118. only homogenized plasma generation in the photoexcited nanoparticle,
  119. neglecting all effects related to inhomogeneous plasma
  120. distribution. Here numerical studying of the plasma photogeneration
  121. allows us to propose a novel concept of deeply subwavelength
  122. ($\approx$$\lambda$$^3$/100) plasma-induced nanopatterning of
  123. symmetrical silicon nanoparticle. More importantly, we reveal strong
  124. symmetry breaking in the initially symmetrical nanoparticle during
  125. ultrafast photoexcitation near the magnetic dipole resonance. The
  126. ultrafast manipulation by nanoparticle inherent structure and symmetry
  127. paves the way to novel principles for nonlinear optical nanodevices.}
  128. \end{tabular}
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  130. ]%%%END OF TITLE, AUTHORS AND ABSTRACT%%%
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  133. \section*{} \vspace{-1cm}
  134. %%%FOOTNOTES%%%
  135. \footnotetext{\textit{$^{a}$~Univ Lyon, UJM-St-Etienne, CNRS UMR 5516,
  136. F-42000, Saint-Etienne, France}} \footnotetext{\textit{$^{b}$~ITMO
  137. University, Kronverksiy pr. 49, St. Petersburg, Russia}}
  138. %Please use \dag to cite the ESI in the main text of the article. %If
  139. you article does not have ESI please remove the the \dag symbol from
  140. the title and the footnotetext below. \footnotetext{\dag~Electronic
  141. Supplementary Information (ESI) available: [details of any
  142. supplementary information available should be included here]. See DOI:
  143. 10.1039/b000000x/} %additional addresses can be cited as above using
  144. the lower-case letters, c, d, e... If all authors are from the same
  145. address, no letter is required
  146. \footnotetext{\ddag~Additional footnotes to the title and authors can
  147. be included \emph{e.g.}\ `Present address:' or `These authors
  148. contributed equally to this work' as above using the symbols: \ddag,
  149. \textsection, and \P. Please place the appropriate symbol next to the
  150. author's name and include a \texttt{\textbackslash footnotetext} entry
  151. in the the correct place in the list.}
  152. %%%END OF FOOTNOTES%%%
  153. %%%MAIN TEXT%%%%
  154. \section{Introduction}
  155. All-dielectric nonlinear nanophotonics based on high refractive index
  156. dielectric has become prospective paradigm in modern optics, owing to
  157. recent advances in harmonics generation~\cite{shcherbakov2014enhanced,
  158. yang2015nonlinear, makarov2016self, shorokhov2016multifold} and
  159. ultrafast all-optical modulation~\cite{iyer2015reconfigurable,
  160. makarov2015tuning, shcherbakov2015ultrafast, yang2015nonlinear,
  161. baranov2016nonlinear, baranov2016tuning}. In fact, all-dielectric
  162. nanoantennas and metasurfaces possess much smaller parasitic Joule
  163. losses at high intensities as compared with their plasmonic
  164. counterparts, whereas their nonlinear properties are comparable. More
  165. importantly, the unique properties of the nonlinear all-dielectric
  166. nanodevices are due to existing of both electric and magnetic optical
  167. resonances in visible and near IR
  168. ranges~\cite{kuznetsov2016optically}. For instance, even slight
  169. variation of dielectric permittivity around magnetic dipole resonance
  170. leads to significant changes of optical properties (transmittance or
  171. reflectance) of all-dielectric nanoantennas~\cite{makarov2015tuning,
  172. baranov2016nonlinear, baranov2016tuning} and
  173. metasurfaces~\cite{iyer2015reconfigurable, shcherbakov2015ultrafast,
  174. yang2015nonlinear}.
  175. In all this works on all-dielectric nonlinear nanostructures, the
  176. building blocks (nanoparticles) were considered as objects with
  177. dielectric permittivity homogeneously distributed over
  178. nanoparticle. Therefore, in order to manipulate by propagation angle
  179. of transmitted light it is necessary to use complicated nanostructures
  180. with reduced symmetry~\cite{albella2015switchable, baranov2016tuning,
  181. shibanuma2016unidirectional}.
  182. \begin{figure}[t] \centering
  183. \includegraphics[width=0.75\linewidth]{Concept}
  184. \caption{Schematic illustration of electron-hole plasma 2D and 1D
  185. distributions in silicon nanoparticle around a magnetic resonance.}
  186. \label{fgr:concept}
  187. \end{figure}
  188. In this Letter, we show that electron-hole plasma (EHP) generation in
  189. a spherical dielectric (e.g., silicon) nanoparticle leads to strongly
  190. nonhomogeneous EHP distribution. To reveal and study this effect, we
  191. for the first time provide full-wave numerical simulation of intensive
  192. femtosecond (fs) laser pulse interaction with a dielectric
  193. nanoparticle supporting Mie resonances and two-photon generation of
  194. EHP. In particular, we couple finite-difference time-domain (FDTD)
  195. method of the Maxwell's equations solving with equations describing
  196. nonlinear EHP generation and its variation of material dielectric
  197. permittivity. The obtained results propose a novel strategy to create
  198. complicated nonsymmetrical nanostructures by using only a photoexcited
  199. spherical silicon nanoparticle. Moreover, we show that dense EHP can
  200. be generated at deeply subwavelength scale
  201. ($\approx$$\lambda$$^3$/100) supporting formation of small metallized
  202. parts inside the nanoparticle which transforms all-dielectric
  203. nanoparticle to a hybrid one that extends functionality of ultrafast
  204. optical nanoantennas.
  205. %Plan:
  206. %\begin{itemize}
  207. %\item Fig.1: Beautiful conceptual picture
  208. %\item Fig.2: Temporal evolution of EHP in NP with different diameters
  209. at fixed intensity, in order to show that we have the highest
  210. asymmetry around magnetic dipole (MD) resonance. This would be really
  211. nice!
  212. %\item Fig.3: Temporal evolution of EHP in NP with fixed diameter (at
  213. MD) at different intensities, in order to show possible regimes of
  214. plasma-patterning of NP volume. It would be nice, if we will show
  215. power patterns decencies on intensity for side probe pulse to show
  216. beam steering due to symmetry breaking.
  217. %\item Fig.4: (a) Dependence on pulse duration is also interesting. We
  218. have to show at which duration the asymmetry factor is saturated. (b)
  219. 2D map of asymmetry factor in false colors, where x-axis and y-axis
  220. correspond to intensity and NP diameter.
  221. %\end{itemize} %Additionally, if you will manage to calculate
  222. evolution of scattering power pattern and show considerable effect of
  223. beam steering, we can try Nanoscale or LPR, because the novelty will
  224. be very high.
  225. \section{Modeling details}
  226. %TEI for Anton: please describe what you model first (what physical
  227. processes). Then, we speak about "pulse", but never "laser". Should we
  228. provide more details concerning irradiation source?
  229. We focus out attention on silicon because this material is promising
  230. for the implementation of nonlinear photonic devices thanks to a broad
  231. range of optical nonlinearities, strong two-photon absorption and EHP
  232. excitation~\cite{leuthold2010nonlinear}. Furthermore, silicon
  233. nanoantennas demonstrate a sufficiently high damage threshold due to
  234. the large melting temperature ($\approx$1690~K), whereas its nonlinear
  235. optical properties have been extensively studied during last
  236. decays~\cite{Van1987, Sokolowski2000, leuthold2010nonlinear}.
  237. Since the 3D modeling of EHP photo-generation in a resonant silicon
  238. nanoparticle has not been done before in time-domain, we develop a
  239. model considering incidence of ultrashort light pulse on a silicon
  240. sphere, where EHP is generated via one- and two-photon absorption
  241. processes, and then decayed via Auger recombination. Importantly, we
  242. also consider nonlinear feedback of the material by taking into
  243. account intraband light absorption on the generated free carriers. In
  244. order to simplify our model, we neglect diffusion of EHP, because the
  245. aim of our work is to study EHP dynamics \textit{during} laser
  246. interaction with the nanoparticle.
  247. \subsection{Light propagation} The propagation of light inside the
  248. silicon nanoparticle is modeled by solving the system of Maxwell's
  249. equations, written in the following way
  250. \begin{align} \begin{cases} \label{Maxwell}$$
  251. \displaystyle{\frac{\partial{\vec{E}}}{\partial{t}}=\frac{\nabla\times\vec{H}}{\epsilon_0\epsilon}-\frac{1}{\epsilon_0\epsilon}\vec{J}}
  252. \\
  253. \displaystyle{\frac{\partial{\vec{H}}}{\partial{t}}=-\frac{\nabla\times\vec{E}}{\mu_0}},
  254. $$ \end{cases} \end{align}
  255. where $\vec{E}$ is the electric field, $\vec{H}$ is the magnetizing
  256. field, $\epsilon_0$ is the free space permittivity, $\mu_0$ is the
  257. permeability of free space, $\epsilon = n^2 = 3.681^2$ is the
  258. permittivity of non-excited silicon at $800$ nm wavelength [green1995]
  259. \cite{Green1995}, and $\vec{J}$ is the nonlinear current, which
  260. includes the contribution due to heating of the conduction band,
  261. described by the differential equation derived from the Drude model
  262. \begin{equation} \label{Drude}
  263. \displaystyle{\frac{\partial{\vec{J}}}{\partial{t}} = - \nu_e\vec{J} +
  264. \frac{e^2n_e(t)}{m_e^*}\vec{E}}, \end{equation} where $e$ is the
  265. elementary charge, $m_e^* = 0.18m_e$ is the reduced electron-hole mass
  266. [sokolowski2000]\cite{Sokolowski2000}, $n_e(t)$ is the time-dependent
  267. free carrier density and $\nu_e = 10^{15} s^{-1}$ is the electron
  268. collision frequency [sokolowski2000]\cite{Sokolowski2000}. Silicon
  269. nanoparticle is surrounded by air, where the light propagation is
  270. calculated by Maxwell's equations with $\vec{J} = 0$ and $\epsilon =
  271. 1$. The system of Maxwell's equations coupled with electron density
  272. equations is solved by the finite-difference numerical method
  273. [rudenko2016]%\cite{Rudenko2016} , based on the finite-difference
  274. time-domain (FDTD) method [yee1966] \cite{Yee1966} and
  275. auxiliary-differential method for disperse media
  276. [taflove1995]\cite{Taflove1995}. At the edges of the grid, we apply
  277. absorbing boundary conditions related to convolutional perfect matched
  278. layers (CPML) to avoid nonphysical reflections [roden2000]%
  279. \cite{Roden2000} . Initial electric field is introduced as a Gaussian
  280. focused beam source as follows
  281. \begin{align}
  282. \begin{aligned}
  283. \label{Gaussian} {E_x}(t, r, z) =
  284. \frac{w_0}{w(z)}{exp}\left(i\omega{t} - \frac{r^2}{{w(z)}^2} - ikz -
  285. ik\frac{r^2}{2R(z)} + i\varsigma(z)\right)\\
  286. \times\;{exp}\left(-\frac{(t-t_0)^2}{\theta^2}\right),
  287. \end{aligned}
  288. \end{align} where $\theta$ is the pulse width at half maximum (FWHM),
  289. $t_0$ is a time delay, $w_0 = 3{\mu}m$ is the waist beam, $w(z) =
  290. {w_0}\sqrt{1+(\frac{z}{z_R})^2}$ is the Gaussian's beam spot size,
  291. $\omega = 2{\pi}c/{\lambda}$ is the angular frequency, $\lambda = 800
  292. nm$ is the laser wavelength in air, $c$ is the speed of light, ${z_R}
  293. = \frac{\pi{{w_0}^2}n_0}{\lambda}$ is the Rayleigh length, $r =
  294. \sqrt{x^2 + y^2}$ is the radial distance from the beam's waist, $R_z =
  295. z\left(1+(\frac{z_R}{z})^2\right)$ is the radius of curvature of the
  296. wavelength comprising the beam, and $\varsigma(z) =
  297. {\arctan}(\frac{z}{z_R}) $ is the Gouy phase shift.
  298. \subsection{Material ionization} To account for material ionization,
  299. we couple Maxwell's equations with the kinetic equation for EHP
  300. generation and relaxation inside silicon nanoparticle.
  301. \begin{figure*}[ht!] \centering
  302. \includegraphics[width=120mm]{fig2.png}
  303. \caption{\label{fig2} Free carrier density snapshots of electron
  304. plasma evolution inside Si nanoparticle taken a) $30$ fs b) $10$ fs
  305. before the pulse peak, c) at the pulse peak, d) $10$ fs e) $30$ fs
  306. after the pulse peak. Pulse duration $50$ fs (FWHM). Wavelength $800$
  307. nm in air. Radius of the nanoparticle $R \approx 105$ nm,
  308. corresponding to the resonance condition. Graph shows the dependence
  309. of the asymmetric parameter of electron plasma density on the average
  310. electron density in the front half of the nanoparticle. $n_{cr} =
  311. 5\cdot{10}^{21} cm^{-3}$ is the critical plasma resonance electron
  312. density for silicon.}
  313. \end{figure*}
  314. The time-dependent conduction-band carrier density evolution is
  315. described with a rate equation, firstly proposed by van Driel
  316. [van1987] \cite{Van1987}, taking into account photoionization,
  317. avalanche ionization and Auger recombination as
  318. \begin{equation} \label{Dens}
  319. \displaystyle{\frac{\partial{n_e}}{\partial t} =
  320. \frac{n_a-n_e}{n_a}\left(\frac{\sigma_1I}{\hbar\omega} +
  321. \frac{\sigma_2I^2}{2\hbar\omega}\right) + \alpha{I}n_e -
  322. \frac{C\cdot{n_e}^3}{C\tau_{rec}n_e^2+1},} \end{equation} where
  323. $I=\frac{n}{2}\sqrt{\frac{\epsilon_0}{\mu_0}}\left|\vec{E}\right|^2$
  324. is the intensity, $\sigma_1 = 1.021\cdot{10}^3 cm^{-1}$ and $\sigma_2
  325. = 0.1\cdot{10}^{-7} cm/W$ are the one-photon and two-photon interband
  326. cross-sections [choi2002, bristow2007, derrien2013] \cite{Choi2002,
  327. Bristow2007, Derrien2013}, $n_a = 5\cdot{10}^{22} cm^{-3}$ is the
  328. saturation particle density [derrien2013] \cite{Derrien2013}, $C =
  329. 3.8\cdot{10}^{-31} cm^6/s$ is the Auger recombination rate
  330. [van1987]\cite{Van1987}, $\tau_{rec} = 6\cdot{10}^{-12}$s is the
  331. minimum Auger recombination time [yoffa1980]\cite{Yoffa1980}, and
  332. $\alpha = 21.2 cm^2/J$ is the avalanche ionization coefficient
  333. [pronko1998] \cite{Pronko1998} at the wavelength $800$ nm in air. Free
  334. carrier diffusion can be neglected during and shortly after the
  335. excitation [van1987, sokolowski2000]\cite{Van1987, Sokolowski2000}.
  336. \begin{figure*}[ht!] \centering
  337. \includegraphics[width=0.9\textwidth]{Ne_105nm_800}
  338. \caption{\label{plasma-105nm} Split figure \ref{fig2} into two, this
  339. is first part.}
  340. \end{figure*}
  341. The changes of the real and imaginary parts of the permeability
  342. associated with the time-dependent free carrier response
  343. [sokolowski2000] \cite{Sokolowski2000} can be derived from equations
  344. (\ref{Maxwell}, \ref{Drude}) and are written as follows
  345. \begin{align} \begin{cases} \label{Index} $$
  346. \displaystyle{Re(\epsilon) = \epsilon
  347. -\frac{{e^2}n_e}{\epsilon_0m_e^*(\omega^2+{\nu_e}^2)}} \\
  348. \displaystyle{Im(\epsilon) =
  349. \frac{{e^2}n_e\nu_e}{\epsilon_0m_e^*\omega(\omega^2+{\nu_e}^2)}.}
  350. $$ \end{cases} \end{align}
  351. \section{Results and discussion}
  352. \subsection{Effect of the irradiation intensity on EHP generation}
  353. Fig. \ref{fig2} demonstrates EHP temporal evolution inside silicon
  354. nanoparticle of $R \approx 105$ nm during irradiation by
  355. high-intensity ultrashort laser Gaussian pulse. Snapshots of electron
  356. density taken at different times correspond to different total amount
  357. of deposited energy and, therefore, different intensities of
  358. irradiation. We introduce the parameter of EHP asymmetry $G$, defined
  359. as a relation between the average electron density generated in the
  360. front side of the nanoparticle and the average electron density in the
  361. back side, as shown in Fig. \ref{fig2}. During the femtosecond pulse
  362. interaction, this parameter significantly varies.
  363. Far before the pulse peak in Fig. \ref{fig2}(a), the excitation
  364. processes follow the intensity distribution, generating a low-density
  365. electron plasma of a toroidal shape at magnetic dipole resonance
  366. conditions. For higher intensities, the optical properties of silicon
  367. change significantly according to equations (\ref{Index}), and
  368. nonresonant electric dipole contributes to the forward shifting of EHP
  369. density maximum. Therefore, EHP is localized in the front part of the
  370. nanoparticle, increasing the asymmetry factor $G$ in
  371. Fig. \ref{fig2}(b). Approximately at the pulse peak, the critical
  372. electron density $n_{cr} = 5\cdot{10}^{21} cm^{-3}$ for silicon, which
  373. corresponds to the transition to quasi-metallic state $Re(\epsilon)
  374. \approx 0$ and to electron plasma resonance [sokolowksi2000]
  375. \cite{Sokolowski2000}, is overcome. At the same time, $G$ factor
  376. reaches the maximum value close to $2.5$ in
  377. Fig. \ref{fig2}(c). Further irradiation leads to a decrease of the
  378. asymmetry parameter down to $1$ for higher electron densities in
  379. Fig. \ref{fig2}(d, e).
  380. It is worth noting, that it is possible to achieve a formation of
  381. deeply subwavelength EHP regions due to high field localization. In
  382. particular, we observe very small EHP localization at magnetic dipole
  383. resonant conditions for $R \approx 105$ nm. The EHP distribution in
  384. Fig. \ref{fig2}(c) is the optimal for symmetry breaking in silicon
  385. nanoparticle, as results in the bigger asymmetry factor $G$ and higher
  386. electron densities $n_e$. We want to stress here that such regime
  387. could be still safe for nanoparticle due to small volume of such high
  388. EHP density, which should be diffused after some time.
  389. \subsection{Effects of nanoparticle size/scattering efficiency factor
  390. on scattering directions}
  391. \begin{figure}[ht] \centering
  392. \includegraphics[width=90mm]{fig3.png}
  393. \caption{\label{fig3} a) Scattering efficiency factor $Q_{sca}$
  394. dependence on the radius $R$ of non-excited silicon nanoparticle
  395. calculated by Mie theory; b) Parameter of forward/backward scattering
  396. dependence on the radius $R$ calculated by Mie theory for non-excited
  397. silicon nanoparticle c) Optimization parameter $K$ dependence on the
  398. average electron density $n_e^{front}$ in the front half of the
  399. nanoparticle for indicated radii (1-7).}
  400. \end{figure}
  401. Previously, the EHP kinetics has been demonstrated only for a silicon
  402. nanoparticle of a fixed radius $R \approx 105$ nm (TEI :REF
  403. ???). Here, we investigate the influence of the nanoparticle size on
  404. the EHP patterns and temporal evolution during ultrashort laser
  405. irradiation. A brief analysis of the initial intensity distribution
  406. inside the nanoparticle given by Mie theory for a spherical
  407. homogenneous nanoparticle [mie1908] \cite{Mie1908} can be useful in
  408. this case. Fig. \ref{fig3}(a, b) shows the scattering efficiency and
  409. the asymmetry parameter for forward/backward scattering for
  410. non-excited silicon nanoparticles of different radii calculated by Mie
  411. theory [mie1908]\cite{Mie1908}. Scattering efficiency dependence gives
  412. us the value of resonant sizes of nanoparticles, where the initial
  413. electric fields are significantly enhanced and, therefore, we can
  414. expect that the following conditions will result in a stronger
  415. electron density gradients. Additionally, in the case of maximum
  416. forward or backward scattering, the initial intensity distribution has
  417. the maximum of asymmetry. One can note, that for $R \approx 100$ nm
  418. and $R \approx 150$ nm both criteria are fulfilled: the intensity is
  419. enhanced $5-10$ times due to near-resonance conditions and its
  420. distribution has a strong asymmetry.
  421. In what follows, we present the calculation results obtained by using
  422. Maxwell's equations coupled with electron kinetics for different
  423. extremum radii for resonant and non-resonant conditions. One can note,
  424. that the maximum asymmetry factor of EHP $G$ does not guarantee the
  425. optimal asymmetry of intensity distribution, as the size of generated
  426. plasma and the value of the electron density equally contribute to the
  427. change of the modified nanoparticle optical response. For example, it
  428. is easier to localize high electron densities inside smaller
  429. nanoparticles, however, due to the negligible size of the generated
  430. EHP with respect to laser wavelength in media, the intensity
  431. distribution around the nanoparticle will not change
  432. considerably. Therefore, we propose to introduce the optimization
  433. factor $K = \frac{n_e(G-1)R^2}{n_{cr}G{R_0^2}}$, where $R_0 = 100$ nm,
  434. $n_{cr} = 5\cdot{10}^{21} cm^{-3}$, and $G$ is asymmetry of EHP,
  435. defined previously. The calculation results for different radii of
  436. silicon nanoparticles and electron densities are presented in
  437. Fig. \ref{fig3}(c). One can see, that the maximum value are achieved
  438. for the nanoparticles, that satisfy both initial maximum forward
  439. scattering and not far from the first resonant condition. For larger
  440. nanoparticles, lower values of EHP asymmetry factor are obtained, as
  441. the electron density evolves not only from the intensity patterns in
  442. the front side of the nanoparticle but also in the back side.
  443. To demonstrate the effect of symmetry breaking, we calculate the
  444. intensity distribution around the nanoparticle for double-pulse
  445. experiment. The first pulse of larger pulse energy and polarization
  446. along $Ox$ generates asymmetric EHP inside silicon nanoparticle,
  447. whereas the second pulse of lower pulse energy and polarization
  448. $Oz$interacts with EHP after the first pulse is gone. The minimum
  449. relaxation time of high electron density in silicon is $\tau_{rec} =
  450. 6\cdot{10}^{-12}$ s [yoffa1980] \cite{Yoffa1980}, therefore, the
  451. electron density will not have time to decrease significantly for
  452. subpicosecond pulse separations. In our simulations, we use $\delta{t}
  453. = 200$ fs pulse separation. The intensity distributions near the
  454. silicon nanoparticle of $R = 95$ nm, corresponding to maxima value of
  455. $K$ optimization factor, without plasma and with generated plasma are
  456. shown in Fig. \ref{fig4}. The intensity distribution is strongly
  457. asymmetric in the case of EHP presence. One can note, that the excited
  458. nanoparticle is out of quasi-resonant condition and the intensity
  459. enhancements in Fig. \ref{fig4}(c) are weaker than in
  460. Fig. \ref{fig4}(b).
  461. \begin{figure}[ht] \centering
  462. \includegraphics[width=90mm]{fig4.png}
  463. \caption{\label{fig4} a) Electron plasma distribution inside Si
  464. nanoparticle $R \approx 95$ nm $50$ fs after the pulse peak; Intensity
  465. distributions around and inside the nanoparticle b) without plasma, c)
  466. with electron plasma inside.}
  467. \end{figure}
  468. %\begin{figure} %\centering
  469. % \includegraphics[height=0.7\linewidth]{Si-flow-R140-XYZ-Eabs}
  470. % \caption{EHP distributions for nonres., MD, ED, and MQ nanoparticles
  471. at moderate photoexcitation. The aim is to show different possible EHP
  472. patterns and how strong could be symmetry breaking.
  473. % \label{fgr:example}
  474. %\end{figure}
  475. \subsection{Asymmetry analysis: effects of pulse duration, intensity
  476. and size} It is important to optimize asymmetry by varying pulse
  477. duration, intensity and size. TEI: for Konstantin L.: please change
  478. Mie figure and add a discussion and how the results agree, what is the
  479. difference TEI: for Anton R.: please add a discussion of the previous
  480. experiments and how the results agree
  481. TODO Kostya: add some discusion on rise-on time for optical switching
  482. like this: Small size will give as a magnetic dipole b1 resonance with
  483. Q-factor (ratio of wavelength to the resonance width at half-height)
  484. of about 8, a1 Q approx 4, the larger particle will have b2 Q approx
  485. 40. For large particle we will have e.g. at R=238.4 second order b4
  486. resonance with Q approx 800. As soon as the period at WL=800nm is 2.6
  487. fs, we need about 25 fs pulse to pump dipole response, about 150 fs
  488. for quadrupole, and about 2000fs for b4. If we think of optical
  489. switching applications this is a rise-on time.
  490. TODO Kostya: Add discussion about mode selection due to the formation
  491. of the plasma.
  492. \section{Conclusions} We have considered light interaction with a
  493. semiconductor nanoparticle under different irradiation conditions and
  494. for various particle sizes. As a result of the presented
  495. self-consistent calculations, we have obtained spatio-temporal EHP
  496. evolution for different light intensities and pulse temporal
  497. widths. It has been demonstrated that EHP generation strongly affects
  498. nanoparticle scattering and, in particular, changes the preferable
  499. scattering direction. In particular, the scattering efficiency factor
  500. is used to define the optimum nanoparticle size for preferential
  501. forward or backward scattering. Furthermore, a parameter has been
  502. introduced to describe the scattering asymmetry as a ratio of the EHP
  503. density in the front side to that in the back side of the
  504. nanoparticle. This parameter can be then used for two-dimensional
  505. scattering mapping, which is particularly important in numerous
  506. photonics applications. The observed plasma-induced breaking symmetry
  507. can be also useful for beam steering, or for the enhanced second
  508. harmonics generation.
  509. \section{Acknowledgments} TEI: need to add Acknowledgements The
  510. authors gratefully acknowledge financial support from The French
  511. Ministry of Science and Education and from France-Russia PHC
  512. Kolmogorov project. TEI: for Sergey M., please put Kivshar et al. and
  513. other Refs TEI: for Anton R., please put much more references that you
  514. have found describing experiments and previous calculations
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