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Time-dependent forces between a swift electron and a small nanoparticle within the dipole approximation

Castrejón-Figueroa, J.,Castellanos-Reyes, J. Á.,Maciel-Escudero, Carlos,Reyes-Coronado, Alejandro,Barrera, Rubén G.

Abstract

This work was supported by UNAM-PAPIIT project DGAPA IN114919. J.C.-F and J.Á.C.-R. are doctoral students from Programa de Doctorado en Ciencias Físicas, Universidad Nacional Autónoma de México (UNAM), and received scholarships 477516 and 481497, respectively, from Consejo Nacional de Ciencia y Tecnología (CONACyT), Mexico. C.M.-E. was a master student from Programa de Maestría en Ciencias Físicas, Universidad Nacional Autónoma de México (UNAM), and received scholarship 420478, from Consejo Nacional de Ciencia y Tecnología (CONACyT), Mexico.

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PHYSICAL REVIEW B 103, 155413 (2021) Time-dependent forces between a swift electron and a small nanoparticle within the dipole approximation J. Castrejón-Figueroa ,1,*J. Á. Castellanos-Reyes ,1C. Maciel-Escudero,1,2 A. Reyes-Coronado,1and R. G. Barrera 3 1Departamento de Física, Facultad de Ciencias, Universidad Nacional Autónoma de México, Ciudad Universitaria, Avenida Universidad 3000, Mexico City 04510, Mexico 2Materials Physics Center, CSIC-UPV/EHU, 20018 Donostia-San Sebastián, Spain 3Instituto de Física, Universidad Nacional Autónoma de México, Apartado Postal 20-364, Mexico City 01000, Mexico (Received 10 December 2020; revised 9 March 2021; accepted 19 March 2021; published 13 April 2021; corrected 10 May 2021) In this paper we calculate the time-dependent forces between a swift electron traveling at constant velocity and a metallic nanoparticle made of either aluminum or gold. We consider that the nanoparticle responds as an electric point dipole and we use classical electrodynamics to calculate the force on both the nanoparticle and the electron. The values for the velocity of the electron and the radius of the nanoparticle were chosen in accordance with electron microscopy observations, and the impact parameter was selected to fulfill the constraints imposed by the dipole approximation. We find that there are times when the force on the nanoparticle is attractive and others when it is repulsive, and show that this is due to the delayed electromagnetic response of the nanoparticle. To establish the limits of validity of our approach, we calculate the total linear momentum transfer to the nanoparticle, and compare it with results obtained, in frequency space, using the full multipole expansion of the fields induced on the nanoparticle, considering the effects of electromagnetic radiation. DOI: 10.1103/PhysRevB.103.155413 I. INTRODUCTION The ability to manipulate objects at deep subwavelength dimensions is an interesting research area that aims to control and engineer structures at the nanoand micrometer scales [1–5]. Since the last century, and due to its importance in technological applications, nanoand micromanipulation have been looking for techniques that allow moving, trapping, and assembling objects with accuracy. Optical tweezers are one example useful for the latter purpose. In this technique, the electromagnetic forces produced by tightly focused laser beams allow to move and hold micro objects [4–6] and even plasmonic nanoparticles [3,7,8]. In this electromagnetic context, electron beams produced in transmission electron microscopes (TEMs) have also shown to be potentially useful probes for guiding the motion of nanoparticles (NPs) [9–16]. In previous works it was demonstrated that electron beams are capable of inducing coalescence in separated nanoscale metal particles [9–12]. Interestingly, the recent ability to achieve subangstrom resolution in aberration-corrected scanning transmission electron microscopes (STEMs) [17–21] and parallel efforts to push the spectral resolution into the range of milli–electron volts [22–24] make STEM an attractive alternative tool for nanomanipulation with high spatial and spectral resolutions. Further developments of these techniques require a full understanding of the interaction between NPs and electron beams. *Corresponding author: [email protected] The interaction between spherical NPs and aloof STEM electron beams has been previously addressed by calculating the total linear momentum transferred by the electron beam to theNP[25–28]. These previous works were based on a classical electrodynamics approach, and the electromagnetic fields produced by the electron beam and the spherical NP were obtained by solving Maxwell’s equations in the frequency space (fully retarded wave solution approach). In addition, through a frequency-to-time Fourier transform of the electromagnetic fields, it was possible to calculate the forces upon the NP [28], showing that there are times when the force is attractive between the electron and the NP, while in others the force is repulsive. However, in addition to this approach being highly computationally demanding, the conclusions reached in Ref. [28] regarding the nature of the repulsive forces are different from those presented here. In this work we use a simple classical model to study, in the time domain, the electromagnetic-interaction forces between a small metallic NP and a swift electron. We first consider the electron as a classical point particle traveling in a straight line [29] and model the electromagnetic response of the NP as the one of an induced electric point dipole. We then calculate the forces between the two particles (swift electron and NP) using the Lorentz-force formula. This simple description of the system allows us to understand in detail some properties of the interparticle forces and reveals their attractive or repulsive behavior at different times. Most importantly, besides the simplicity of our approach, in its range of validity (large impact parameter to radius ratio), it quantitatively coincides with the results for the total linear momentum transfer, obtained with the fully retarded wave solution. 2469-9950/2021/103(15)/155413(11) 155413-1 ©2021 American Physical Society J. CASTREJÓN-FIGUEROA et al. PHYSICAL REVIEW B 103, 155413 (2021) FIG. 1. (a) Metallic NP (gray sphere) of radius awith dielectric function ε(ω), embedded in vacuum, interacting with a swift electron (red dot) traveling in the zdirection with constant velocity  vand impact parameter b. (b) Schematics of the dipole approximation model: a time-dependent electric point dipole  p(t) induced within the NP. II. THEORETICAL MODEL: THE (TIME-DEPENDENT) DIPOLE APPROXIMATION Typical modern STEMs pump highly energetic electron beams with an energy up to 400 keV (∼0.83c, with cthe speed of light). These electron beams produce low currents on the order of pA which are equivalent to a train of swift electrons traveling with constant speed, each one emitted approximately every 10−8s. By comparing this time interval with the typical lifetime of electronic excitations in metals (10−15 s) [31], we assume that the interaction between the electron beam and the NP can be modeled as if one single swift electron interacts with the NP [25–28,32,33]. We also assume that the NP is a nonmagnetic sphere embedded in vacuum, with radius aand characterized with an isotropic homogeneous electromagnetic response ε(ω). We consider the swift electron as a point particle with electric charge −e, traveling with constant velocity  valong the zdirection, and at a distance bfrom the origin (impact parameter) which is set at the center of the NP [see Fig. 1(a)]. Notice that at time t=0 the electron is at the position (b,0,0) [see Fig. 1(a)]. When the impact parameter is large enough compared to the radius of the NP, the NP can be regarded as an electric point dipole [33] (as we will discuss in Sec. IV). Within this approximation, we calculate the forces between the swift electron and the NP based on the Lorentz force. We will refer to this approach as the dipole approximation. The induced electric dipole moment  p(ω) within the NP is determined by the following expression:  p(ω)=ε0αs(ω) Eext 0(ω),(1) where ε0is the permittivity of vacuum,  Eext 0(ω) is the external electric field (in the frequency domain) produced by a swift electron [see Eq. (A5) in Appendix A] evaluated at the center of the NP, and αs(ω)=4πa3ε(ω)−ε0 ε(ω)+2ε0(2) is the quasistatic polarizability [34]. The validity of using αs(ω)inEq.(1) will be discussed in Sec. IV. Notice that in Eq. (1) the induced electric dipole moment,  p, is given as a function of frequency. Through a frequencyto-time Fourier transform one obtains  pas a function of time:  p(t)=ε0t −∞ αs(t−t) Eext 0(t)dt =ε0∞ 0 αs(τ) Eext 0(t−τ)dτ, (3) where τ=t−t. Furthermore, the force on the electric point dipole is given by [35]  F(t)=[ p(t)·∇] Eext 0(t)+˙  p(t)×μ0 Hext 0(t),(4) where ˙  pdenotes the time derivative of  p,μ0is the permeability of vacuum, and  Eext 0(t) and  Hext 0(t) are the external electric and H fields, respectively, produced by the swift electron [Eqs. (A3) and (A4) in Appendix A] evaluated at the center of the NP. In a similar manner, the force on the swift electron is  Fe( re;t)=−e[ Ep( re;t)+ v×μ0 Hp( re;t)],(5) where  Ep( re) and  Hp( re) are the electric and H fields, produced by the electric point dipole, evaluated at the position of the swift electron  re(t). We address the reader to Appendix A for the general expressions of both the external and the electric point dipole electromagnetic fields. As pointed out in the Introduction, the interaction between a swift electron and a NP has been studied in the frequency domain by obtaining the total linear momentum,  P, transferred by the swift electron to the NP (fully retarded wave solution) [25–28]. Thus, to corroborate the validity of the dipole approximation, we calculate  Pfor both approaches: the fully retarded wave solution and the dipole approximation. This comparison allows us to determine the accuracy of our approach. Within the dipole approximation, the total linear momentum transferred by the swift electron to the electric point dipole is obtained by integration of Eq. (4) in time:  P=∞ −∞  F(t)dt.(6) Furthermore, the total linear momentum lost by the electron is  Pe=∞ −∞  Fe(t)dt,(7) with  Fe(t) given by Eq. (5). Interestingly, the dipole approximation provides valuable information and reveals interesting properties in the interaction between a swift electron and a small NP, as we discuss in the next section. III. INTERACTION FORCES AND ELECTROMAGNETIC RADIATION EMITTED BY METALLIC NANOPARTICLES In this section we calculate the interparticle (swift electron and NP) forces within the dipole approximation for two different NPs: one made of aluminum and another one made of gold. Additionally, we obtain the electromagnetic radiation fields emitted by the NP due to the swift electron, and calculate the energy and linear momentum radiated by the NP. 155413-2 TIME-DEPENDENT FORCES BETWEEN A SWIFT … PHYSICAL REVIEW B 103, 155413 (2021) FIG. 2. (a) Attosecond timescale of F⊥calculated for an aluminum NP with a=1 nm. The swift electron is traveling with v=0.5cand b=3 nm. The red line represents the electric contribution to the force, the blue line represents the magnetic contribution to the force, and the black dashed line is the total force (sum of electric and magnetic contributions). Labels A, B, and C indicate the forces on the NP at times −20, 0, and 20 as. The horizontal green arrow points to the femtosecond timescale. (b) Femtosecond timescale of F⊥for the same NP as in (a). Labels D, E, and F in (b) indicate the forces at times 350, 640, and 930 as, respectively. The blue curves in (a) and (b) are multiplied by a factor of 10. A. Force on the nanoparticle First, we consider the case of an aluminum NP characterized by a dielectric function within the Drude model, with a plasma frequency ¯hωp=13.14 eV and a damping parameter ¯h=0.197 eV [36]. The NP has radius a=1 nm and the swift electron travels with constant speed v=0.5cand impact parameter b=3 nm. It is worth mentioning that for these parameters the aluminum NP is well described by the dipole approximation, as we will show in Sec. IV. The transverse or xcomponent [relative to the swift electron trajectory; see Fig. 1(a)]oftheforce  Fon the NP provides information on the attraction or repulsion of the NP relative to the electron beam. Thus, we focus our analysis and calculations on this component. We show in Fig. 2the transverse component of the force (F⊥, black dashed line) experienced by the aluminum NP. The force is separated in its electric (FE ⊥, red line) and magnetic (FH ⊥, blue line) contributions [first and second terms on the right-hand side of Eq. (4), respectively]. From Fig. 2one can notice two relevant time regimes for the force: (i) an attosecond regime and (ii) a femtosecond regime. At the attosecond timescale the forces are on the order of piconewtons [see Fig. 2(a)], while at the femtosecond timescale the forces oscillate between negative and positive values and their magnitude decreases about four orders of magnitude (to tens of attonewtons) compared to the attosecond regime [see Fig. 2(b)]. As can be seen from Figs. 2(a) and 2(b), the electric contribution to the force (red line) dominates over the magnetic one (blue line, amplified tenfold). Thus, the curve of the total force (black dashed line in Fig. 2) is superimposed on its electric contribution FE ⊥. At higher speeds of the swift electron (v> 0.5c; not shown here), the magnetic contribution to the force increases but never surpasses the electric contribution. A positive force (F⊥>0) implies that the NP is attracted toward the swift electron trajectory and, conversely, a negative force (F⊥<0) implies that the NP is repelled from it. In Fig. 2(a) we observe that t=−20 as and t=0 as (labels A and B, respectively) correspond to instants where the interaction between the swift electron and the NP is attractive. This period of time is followed by a repulsive regime (label FIG. 3. (a) Induced electric dipole moment (blue arrow) depicted in the plane y=0, for the six different times indicated in Fig. 2by labels A to F. The swift electron (red dot) is traveling with v=0.5c and b=3 nm nearby an aluminum NP with a=1 nm. The green dashed line joins the red dot and the origin. (b) Analogous to (a) but now v=0.01c. 155413-3 J. CASTREJÓN-FIGUEROA et al. PHYSICAL REVIEW B 103, 155413 (2021) FIG. 4. (a) Attosecond timescale of F⊥calculated for a gold NP with a=1 nm. The swift electron is traveling with v=0.5cand b=3 nm. The red line represents the electric contribution to the force, the blue line represents the magnetic contribution to the force, and the black dashed line is the total force (sum of electric and magnetic contributions). Labels A, B, and C indicate the forces on the NP at times −20, 0, and 20 as. The horizontal green arrow points to the femtosecond timescale. (b) Femtosecond timescale of F⊥for the same NP as in (a). The blue curves in (a) and (b) are multiplied by a factor of 10. C) that takes place up to t≈250 as. After this time, the force oscillates in the femtosecond timescale between positive and negative values, leading to attractive and repulsive interactions, as shown by labels D, E, and F in Fig. 2(b).The repulsive interaction is caused by a delay in the response of the induced electric dipole, as we discuss in the following. In Fig. 3(a) we show six different schematics of the induced electric dipole moment  p(t) within the NP (blue arrow) and the relative position of the swift electron at the six different times marked in Figs. 2(a) and 2(b). The size of the blue arrows in Fig. 3represents the magnitude of the induced dipole moment at each time (−20, 0, 20, 350, 640, and 930 as). Notice that the arrowhead represents effectively positive charge and the arrow tail represents effectively negative charge within the NP. To visualize the delay in the response of the induced electric dipole, we trace a green dashed line joining the position of the swift electron (red dot) and the center of the NP. At the times t=−20 as and t=0 as, one can see in Fig. 3(a), labels A and B, that the blue arrow points behind the green dashed line. For these cases the effective interaction between the swift electron and the induced electric dipole is attractive—the positive induced charge of the NP is closer to the swift electron. Conversely, for t=20 as [Fig. 3(a), label C], the effective interaction between the swift electron and  pis repulsive—at this time the negative charge of the NP is closer to the swift electron. For later times 350, 640, and 930 as, shown in Fig. 3(a) by labels D, E, and F, respectively, the swift electron is far away and the induced dipole moment  protates clockwise. This explains why the force experienced by the NP alternates between positive and negative in Fig. 2(b), meaning attraction and repulsion toward the swift electron. When the swift electron travels slow compared to c(nonrelativistic case), the induced dipole moment follows the position of the swift electron (red dot). That is,  ppoints toward the red dot at all times, as we show in Fig. 3(b). For this case we consider a swift electron traveling with v=0.01c and b=3 nm. We show three different times: −1, 0, and 1 fs. One can observe in Fig. 3(b) that  pand the green dashed line are superimposed. For this situation, the force between the swift electron and the NP is always attractive. From this analysis we conclude that if the swift electron travels with a speed comparable with the speed of light, a delay occurs in the response of the NP to the external electromagnetic fields, which leads to repulsive forces on the NP (see Fig. 2). Next, we consider the case of a NP made of gold with a dielectric function taken from Ref. [37]. In Fig. 4we show the transverse component of the force experienced by the gold NP as a function of time. The swift electron is traveling with v= 0.5cand b=3 nm. Some similarities between Figs. 2and 4 become apparent. For instance, we identify again two relevant time regimes for the force: attoseconds and femtoseconds. At the attosecond timescale the force changes from positive to negative between −20 to 20 as [see black dashed line in Fig. 4(a)] with a magnitude on the order of piconewtons. At the femtosecond timescale, the force decreases five orders of magnitude (attonewtons) and oscillates between positive and negative values. The amplitude of this oscillation monotonically decreases to zero. Notice that for both timescales [Fig. 4(a) and Fig. 4(b)] the electric contribution to the force (red line) dominates over the magnetic one (blue line, amplified tenfold). The repulsion (negative force) of the NP from the swift electron is caused by the delay in the response of the induced electric dipole, as we show in Fig. 5. We observe that at −20 as and 0 as the effective positive induced charge of the NP (head of the blue arrow in Fig. 5, labels A and B) is closer to the swift electron. Thus, the force is attractive. In contrast, at 20 as the effective induced charge of the NP is negative (tail of the blue arrow in Fig. 5, label C) which is closer to the swift electron, leading to a repulsive force. We learn from Figs. 2–5that the force experienced by the aluminum NP has a similar behavior, but a different magnitude, to the force experienced by the gold NP. To understand the difference in the magnitude of the forces (compare Figs. 2and 4), we analyze the quasistatic polarizability for both materials below. 155413-4 TIME-DEPENDENT FORCES BETWEEN A SWIFT … PHYSICAL REVIEW B 103, 155413 (2021) FIG. 5. Induced electric dipole moment (blue arrow) depicted in the plane y=0, for the three different times indicated in Fig. 4by labels A to C. The swift electron (red dot) is traveling with v=0.5c and b=3 nm nearby a gold NP with a=1 nm. The green dashed line joins the red dot and the origin. By substituting the Drude dielectric function into Eq. (2) and performing a frequency-to-time Fourier transform of the quasistatic polarizability αs(ω)→αs(τ), one obtains αs(τ)=4πa3(τ)ω2 s s e−(τ)/2sin(sτ),(8) for the aluminum NP [34]. The (τ)inEq.(8)istheHeaviside step function, ωs=ωp/√3, and s=ωs1−(/2ωs)2.(9) In Fig. 6we show αs(τ) calculated for the aluminum NP (blue line). The frequency of the oscillations of αs(τ) is equal to s [given by Eq. (9)]. It is worth noting that  p(t) is obtained as a convolution of αs(τ), an oscillating function in time, and the external nonoscillating electric field [given by Eq. (A3)]. Hence,  poscillates at the same frequency s. Additionally, the force on the NP [Eq. (4)] is proportional to  p(and ˙  p); hence the frequency at which the force oscillates at the femtosecond regime is s. We also obtain αs(τ) for a gold NP through a numerical frequency-to-time Fourier transform, shown by the red line in Fig. 6. One recognizes that αs(τ) also oscillates but not with a single frequency as in the aluminum case. Most importantly, the magnitude of αsat τ<70 as for gold is larger than that of the aluminum (blue line). This discrepancy in the magnitude FIG. 6. Quasistatic polarizability αs(τ) as a function of time, calculated for an aluminum NP with a=1 nm (blue line) and for a gold NP with a=1 nm (red line). The vertical black dashed line indicates τ=70 as. of αsexplains the difference in the magnitude of the forces in Figs. 2and 4. Also, for the same time interval, the initial slope of α(τ) for aluminum (blue curve) is smaller than the one for gold (red curve). Therefore, the induced electric dipole is delayed more in aluminum than in gold, yielding a larger repulsive-to-attractive force ratio, as can be seen by comparing Figs. 2(a) and 4(a). B. Force on the swift electron Now, we calculate the force on the swift electron by means of Eq. (5). As mentioned before, the transverse component of the force provides information on the attraction or repulsion of the electron beam toward the NP; hence we focus our analysis and calculations on this component. In Fig. 7we show the transverse component of the force on the swift electron (Fe⊥, black dashed line) when traveling at speed v=0.5c with b=3 nm nearby an aluminum NP with a=1nm.We show the electric (FE e⊥, red line) and magnetic (FH e⊥, blue line) contributions to the total force [first and second terms on the right-hand side of Eq. (5), respectively]. When Fe⊥<0 the swift electron is attracted toward the NP and, conversely, when Fe⊥>0 it is repelled. We observe that the force on the swift electron (Fig. 7) shows both attosecond and femtosecond timescales (with forces on the order of piconewtons and attonewtons, respectively). At the attosecond timescale, at times t=−20 as and t=0 as [labels A and B in Fig. 7(a)], the swift electron is attracted toward the NP. Conversely, at time t=20 as [label C in Fig. 7(a)]theswift electron is repelled. At the femtosecond timescale the force oscillates with frequency sbetween positive and negative [see Fig. 7(b)]. This repulsive interaction is due to the delayed electric point dipole, as we discussed before from Fig. 3. Additionally, from Figs. 2and 7we observe that the force on the swift electron presents similar behavior (but opposite direction) to the force on the NP (Fig. 2). However, one can notice that  Fe(t)+ F(t)=  0.(10) Nonetheless, the total linear momentum of the system is conserved, as we show in the following section. C. Radiation emitted by the nanoparticle and conservation of linear momentum By considering the linear momentum that the radiation carries, we calculate the recoil by the NP when it radiates. First, we obtain the rate of energy radiation by integrating the Poynting vector  Sin a closed surface containing the NP: dWrad dt = S( r;t)·d a,(11) with  S( r;t)= Erad p( r;t)× Hrad p( r;t),(12) where  Erad pand  Hrad pcorrespond to the radiation fields of the time-dependent electric point dipole  pinduced within the NP. The radiation fields can be extracted from Eqs. (A1) and (A2) in Appendix A, as the terms that decay as 1/r. Inserting  Erad p 155413-5 J. CASTREJÓN-FIGUEROA et al. PHYSICAL REVIEW B 103, 155413 (2021) FIG. 7. (a) Attosecond timescale of Fe⊥on a swift electron traveling with v=0.5cand b=3 nm nearby an aluminum NP with a=1 nm. The red line represents the electric contribution to the force, the blue line represents the magnetic contribution to the force, and the black dashed line is the total force (sum of electric and magnetic contributions). Labels A, B, and C indicate the forces on the swift electron at times −20, 0, and 20 as. The horizontal green arrow points to the femtosecond timescale. (b) Femtosecond timescale of Fe⊥for the same swift electron as in (a). and  Hrad pinto Eq. (12) yields  S( r;t)=μ0 16π2cr2[|¨  p(tr)|2−|ˆr·¨  p(tr)|2]ˆr,(13) where tr=t−r/cis the retarded time. By calculating the closed surface integral in Eq. (11), one obtains [38] dWrad dt =μ0 6πc|¨  p(tr)|2.(14) We show in Fig. 8the rate of electromagnetic energy radiated by the NP, Eq. (14), as a function of the retarded time tr= t−r/c, for an aluminum NP (amplified 20-fold and shown as a blue line) and for a gold NP (shown as a red line). It is clear that both NPs radiate energy (see blue and red colored areas in Fig. 8), and that the gold NP radiates most of the energy in FIG. 8. Rate of electromagnetic energy radiation as a function of retarded time (tr), emitted by an aluminum NP with a=1nm (amplified 20-fold in blue line) and by a gold NP with a=1nm (red line). We consider a swift electron with v=0.5cand b=3 nm. The colored area under the blue and red lines represents the energy radiated by the NP. a short period of time (tens of attoseconds) while the radiation by the aluminum NP spreads over a longer period of time. However, from Eq. (13), we realize that  Shas the following symmetry:  S( r)=− S(− r); (15) thus, the NP radiates the same amount of energy in one direction as in the opposite direction. From the relation between the Poynting vector and the density of electromagnetic linear momentum,  g= S/c2, we conclude that in the dipole approximation there is no radiation-reaction force on the NP. Additionally, we calculate the total linear momentum lost by the swift electron and transferred to the NP by integrating numerically the forces [Eqs. (6) and (7)], obtaining that  Pe+ P= 0 (16) for both aluminum and gold NPs. Thus, the total linear momentum gained by the NP is precisely the same as the linear momentum lost by the swift electron. It is well known that for small NPs it is necessary to consider the size corrections to the dielectric function [39] (due to the reduction of the mean-free path of electrons inside the NP). However, we have corroborated (not shown) that they yield negligible contribution to the linear momentum transfer. IV. COMPARISON OF THE DIPOLE APPROXIMATION WITH THE FULLY RETARDED WAVE SOLUTION In this section we obtain the total linear momentum  Pusing the fully retarded wave solution (briefly presented below). By comparing  Pobtained with both the fully retarded wave solution and the dipole approximation, we find the conditions in which the dipole approximation is valid, as we show in the following. As we mentioned in the Introduction, the fully retarded wave solution corresponds to the exact solution of Maxwell’s equations in frequency space. In this scheme, the electromag155413-6 TIME-DEPENDENT FORCES BETWEEN A SWIFT … PHYSICAL REVIEW B 103, 155413 (2021) netic fields scattered by the spherical NP are obtained as a multipolar expansion [32]:  Escat( r;ω)=∞  =1 m=  m=− Er ,mˆr+Eθ ,mˆ θ+Eφ ,mˆ φ, (17)  Hscat( r;ω)=∞  =1 m=  m=− Hr ,mˆr+Hθ ,mˆ θ+Hφ ,mˆ φ. (18) We refer the reader to Appendix A, where we show the relationship between the spherical components of Eqs. (17) and (18) with the elements of the scattering matrix tE and tM  [Eqs. (A15) and (A16)]. The total linear momentum that the swift electron transfers to the NP is given by  P=∞ 0 P(ω)dω, (19) where  P(ω)=1 πS Reε0 E( r;ω) E∗( r;ω) −ε0 2I ↔ E( r;ω)· E∗( r;ω)+μ0 H( r;ω) H∗( r;ω) −μ0 2I ↔ H( r;ω)· H∗( r;ω)·d a,(20) with Sa closed surface that contains the NP and does not intersect the swift electron path. The Re[z] denotes the real part of z,μ0is the vacuum permeability, I ↔is the identity tensor, and  E( r;ω) and  H( r;ω) are the total electromagnetic fields: the sum of those produced by the swift electron [Eqs. (A5) and (A6) in Appendix A] and those scattered by the NP [Eqs. (17) and (18)]. We refer the reader to Appendix Bfor a detailed derivation of Eqs. (19) and (20). In practice, the scattered fields are evaluated up to a fixed multipolar contribution max sufficiently large to achieve numerical convergence. Since we are interested in a solution for small particles, we consider max =1, and expanding tE and tM [Eqs. (A17) and (A18)] as a power series, we obtain [40] tE 1=2x3 3 m2−1 m2+2+2x5 5 (m2−1)(m2−2) (m2+2)2+O(x6),(21) tM 1=x5 45(m2−1) +O(x7),(22) with x=ωa/cthe size parameter and m2=ε(ω)/ε0. Keeping terms up to x3in Eqs. (21) and (22), one notices that only tE 1 contributes to the scattered fields: tE 1≈k3 6παs(ω),(23) where αs(ω) is the quasistatic polarizability given by Eq. (2). The other terms in Eqs. (21) and (22) are usually known as radiation corrections. We refer to the case in which tE =1is determined by Eq. (23) as the small-particle approximation (SPA). In the following, we compare the transverse component of total linear momentum (P⊥, transferred by the swift electron to the NP) obtained with the dipole approximation, SPA, and the fully retarded wave solution with max =1 and max =30. FIG. 9. Transverse component of the total linear momentum transferred, P⊥,byaswiftelectrontoagoldNPwitha=1 nm. The green line and the black dashed line correspond to P⊥obtained with the fully retarded wave solution with max =1andmax =30, respectively. The blue line corresponds to P⊥obtained with SPA, andthereddashedlinetoP⊥calculated with the dipole approximation. (a) Shows P⊥as a function of the ratio b/afor a swift electron traveling with v=0.5c.(b)ShowsP⊥as a function of the ratio v/c for a fixed impact parameter b=3 nm. In Fig. 9(a) we show P⊥as a function of b/a, assuming a swift electron traveling with constant speed v=0.5c, in the vicinity of a small gold NP of radius a=1nm.We compare P⊥calculated using our time-dependent approach [the dipole approximation, Eq. (6)], red dashed line, with (i) SPA [Eq. (23)], blue line; (ii) the fully retarded wave solution with max =1[Eq.(19)], green line; and (iii) the fully retarded wave solution with max =30 [Eq. (19)], black dashed line. We notice two general features shared by the four calculations: (i) P⊥is always positive and (ii) P⊥decreases for larger values of b/a[see Fig. 9(a)]. From these results, we conclude that the NP is attracted toward the electron beam and the closer the swift electron is to the NP the larger the linear momentum transferred. When the impact parameter b is comparable to the NP radius a, the higher-order multipolar modes (>1) contribute considerably to P⊥(compare black dashed line with the green one). As the impact parameter to radius ratio increases, the four P⊥calculations 155413-7 J. CASTREJÓN-FIGUEROA et al. PHYSICAL REVIEW B 103, 155413 (2021) converge asymptotically to the same value. We recognize that P⊥obtained with the dipole approximation superimposes P⊥obtained with the SPA for all b/aratios [compare red dashed line with the blue line in Fig. 9(a)]. These findings imply that the dipole approximation is the time counterpart of the small-particle approximation (SPA). The results obtained in Fig. 9(a) allow us to define a regime where high-order multipolar contributions (>1), as well as radiation corrections, are negligible. We refer to this as the dipolar regime. To corroborate that the dipolar regime remains valid for different swift electron speeds, we choose b/a=3 and calculate P⊥as a function of v/cfor the dipole approximation and the fully retarded wave solution (max =30). The results are shown in Fig. 9(b), where we notice that P⊥for the dipole approximation (red dashed line) follows closely the fully retarded wave solution (black dashed line) for a broad range of v/cvalues. V. CONCLUSIONS We studied the interaction in time between a swift electron and a small metallic nanoparticle by assuming the latter as an electric point dipole (dipole approximation). Within this approach, we calculated the forces between the swift electron and the nanoparticle as a function of time and we identified two different timescales: an attosecond timescale with forces on the order of piconewtons, and a femtosecond timescale with forces on the order of attonewtons. Our analysis shows that the delayed response of the induced electric point dipole leads to repulsive forces. When the electron travels slowly compared to the speed of light, the delay is negligible and therefore the forces are always attractive. In addition, we studied the electromagnetic radiation emitted by the nanoparticle. Our results show that, within the dipole approximation, there is no radiation-reaction force on the nanoparticle due to the symmetry of the Poynting vector carried by the scattered electromagnetic fields. We corroborated that the total linear momentum gained by the nanoparticle is precisely the one lost by the swift electron; hence the total linear momentum of the system is conserved. To establish the validity of the dipole approximation, we compared the total linear momentum obtained from (i) the dipole approximation and (ii) the fully retarded wave solution. We show that for large impact parameter to radius ratio, the dipole approximation is in good agreement with the fully retarded wave solution. Besides the simplicity of the dipole approximation, our findings show that this simple model exhibits important details of the interaction between small nanoparticles and swift electrons in the time domain, contributing to the understanding of fundamental interactions. ACKNOWLEDGMENTS This work was supported by UNAM-PAPIIT project DGAPA IN114919. J.C.-F and J.Á.C.-R. are doctoral students from Programa de Doctorado en Ciencias Físicas, Universidad Nacional Autónoma de México (UNAM), and received scholarships 477516 and 481497, respectively, from Consejo Nacional de Ciencia y Tecnología (CONACyT), Mexico. C.M.-E. was a master student from Programa de Maestría en Ciencias Físicas, Universidad Nacional Autónoma de México (UNAM), and received scholarship 420478, from Consejo Nacional de Ciencia y Tecnología (CONACyT), Mexico. APPENDIX A: ELECTROMAGNETIC FIELDS SCATTERED BY THE NANOPARTICLE AND PRODUCED BY THE SWIFT ELECTRON In this Appendix we present the electromagnetic fields scattered by the NP and produced by the swift electron. When the NP is modeled as an electric point dipole (dipole approximation), the scattered electromagnetic fields are determined by the following expressions [38]:  Ep( r;t)=1 4πε0r3{[3ˆrˆr−I ↔]·[ p(tr)+(r/c)˙  p(tr)] +(r/c)2[¨  p(tr)׈r]׈r},(A1)  Hp( r;t)=− 1 4πr2ˆr×[˙  p(tr)+(r/c)¨  p(tr)],(A2) where I ↔is the identity tensor,  pis the electric dipole moment, and ˙  p,¨  pare time derivatives of  p. Notice that in Eqs. (A1) and (A2),  p,˙  p, and ¨  pare evaluated at the retarded time tr= t−r/c. The time-dependent electromagnetic fields produced by the swift electron are [34]  Eext(x,y,z;t)=−e 4πε0 γ[(x−b)ˆx+yˆy+(z−vt)ˆz] [(x−b)2+y2+γ2(z−vt)2]3/2, (A3)  Hext(x,y,z;t)=−e 4π γv[(x−b)ˆy−yˆx] [(x−b)2+y2+γ2(z−vt)2]3/2, (A4) with γ=(1 −β2)−1/2the Lorentz factor and β=v/c.By a time-to-frequency Fourier transform of Eqs. (A3) and (A4), one finds that the electromagnetic fields produced by the swift electron (in cgs units) can be expressed as follows [41]:  Eext( r;ω)=−2eω v2γeiω(z/v)sgn(ω) RK1|ω|R vγ[(x−b)ˆx +yˆy]−i γK0|ω|R vγˆz,(A5)  Hext( r;ω)=2eβ Rv2γ|ω|eiω(z/v)K1|ω|R vγ[yˆx−(x−b)ˆy], (A6) with K1(x) and K2(x) the modified Bessel functions of the second kind of order 1 and 2, respectively, and R= (x−b)2+y2. The complete electromagnetic field scattered by the NP (beyond the dipole approximation) can be obtained by solving the fully retarded Maxwell’s equations in frequency space. The details for the derivation of the scattered electromagnetic fields are given in Ref. [32]. Here we show the spherical 155413-8 TIME-DEPENDENT FORCES BETWEEN A SWIFT … PHYSICAL REVIEW B 103, 155413 (2021) multipolar components (outside the NP) of Eqs. (17) and (18) in cgs units: Er ,m=eimφDscat ,m(+1)Pm (cos θ)h(+) (k0r) k0r,(A7) Eθ ,m=−eimφCscat ,m m sin θh(+) (k0r)Pm (cos θ) −eimφDscat ,m(+1)cos θ sin θPm (cos θ) −(−m+1) sin θPm +1(cos θ) ×(+1)h(+) (k0r) k0r−h(+) +1(k0r),(A8) Eφ ,m=ieimφCscat ,mh(+) (k0r)(+1)cos θ sin θPm (cos θ) −(−m+1) sin θPm +1(cos θ) +ieimφDscat ,m m sin θPm (cos θ) ×(+1)h(+) (k0r) k0r−h(+) +1(k0r),(A9) and the components of the H field are Hr ,m=eimφCscat ,m(+1)Pm (cos θ)h(+) (k0r) k0r,(A10) Hθ ,m=eimφDscat ,m m sin θh(+) (k0r)Pm (cos θ) −eimφCscat ,m(+1)cos θ sin θPm (cos θ) −(−m+1) sin θPm +1(cos θ) ×(+1)h(+) (k0r) k0r−h(+) +1(k0r),(A11) Hφ ,m=ieimφCscat ,m m sin θPm (cos θ)(+1)h(+) (k0r) k0r −h(+) +1(k0r) −ieimφDscat ,mh(+) (k0r)(+1)cos θ sin θPm (cos θ) −(−m+1) sin θPm +1(cos θ),(A12) where k0is the wave number in vacuum, h(+) (z)=ih(1) (z) with h(1) (z) the spherical Hankel function of the first kind, and Pm (x) are the associated Legendre functions. The spherical coordinate system (r,θ,φ) is determined by the spherical-toCartesian transformation: x=rsin θcos φ,y=rsin θsin φ, z=rcos θ, with (x,y,z) the Cartesian coordinate system shown in Fig. 1. The coefficients Cscat mand Dscat min Eqs. (A7) to (A12) are determined by Cscat ,m=(i)2+1 4π (−m)! (+m)! ψM,scat ,m,(A13) Dscat ,m=(i)2+1 4π (−m)! (+m)! ψE,scat ,m.(A14) The relationship between the coefficients of the external, ψE,M,ext ,m, and the scattered, ψE,M,scat ,m, scalar functions is given by the scattering matrix: ψE,scat ,m=tE ψE,ext ,m,(A15) ψM,scat ,m=tM ψM,ext ,m.(A16) The full expressions for ψE,M,ext ,mand ψE,M,scat ,mare given in Refs. [32,42]. The elements of the scattering matrix are independent of mdue to the spherical symmetry, and are given by tE =−j(x0)[xij(xi)]+εij(xi)[x0j(x0)] h(+) (x0)[xij(xi)]−εij(xi)[x0h(+) (x0)],(A17) tM =−xij(x0)j (xi)+x0j (x0)j(xi) xih(+) (x0)j (xi)−x0h(+) (x0)j(xi),(A18) where j(z) is the spherical Bessel function, xi=√εiωa/c, and the subscripts iand 0 indicate the dielectric function inside and outside the NP, respectively. The prime denotes differentiation with respect to x0or xi. Notice that from Eqs. (A7)to(A16) one obtains the relationship between the elements of the scattering matrix and the components of the scattered electromagnetic fields (as mentioned in Sec. IV). APPENDIX B: TOTAL LINEAR MOMENTUM TRANSFER WITHIN THE FULLY RETARDED WAVE SOLUTION APPROACH The total linear momentum  Pthat is transferred by the swift electron to the NP can be calculated from the linear momentum conservation law [34]: d dt [ Pmech(t)+ PEM(t)]=S T ↔( r;t)·d a,(B1) where  Pmech(t) is the mechanical linear momentum,  PEM(t) is the electromagnetic linear momentum, T ↔( r;t) is Maxwell’s stress tensor, and Sis a surface enclosing the NP. The electromagnetic linear momentum is  PEM(t)=ε0μ0V E( r;t)× H( r;t)d3r,(B2) where  E( r;t) is the total electric field,  H( r;t) is the total H field, andVis the volume enclosed by S. The Maxwell’s stress tensor is given by the following expression: T ↔( r;t)=ε0 E( r;t) E( r;t)−ε0 2I ↔ E( r;t)· E( r;t) +μ0 H( r;t) H( r;t)−μ0 2I ↔ H( r;t)· H( r;t).(B3) 155413-9