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Arizona Center for Mathematical Sciences, University of Arizona, Tucson, Arizona 85721
tex2html_wrap_inline288 Also with the Optical Sciences Center, University of Arizona, Tucson, AZ 85721
tex2html_wrap_inline436 Also with University of Ostrava, Ostrava, Czech Republic

Dynamic Spatial Replenishment of Femtosecond
Pulses Propagating in Air

M. Mlejnek tex2html_wrap_inline286 , E.M. Wright tex2html_wrap_inline288 , and J.V. Moloney

Abstract:

We present numerical simulations of nonlinear pulse propagation in air whereby an initial pulse is formed, absorbed by plasma generation, and subsequently replenished by power from the trailing edge of the pulse. This process can occur more than once for high power input pulses and produce the illusion of long distance propagation of one self-guided pulse.

The observation of long distance apparently self-guided pulses in air [1, 2, 3, 4, 5] has attracted much recent interest, with applications in communications and lightning channeling envisioned [3]. The basic phenomenon characterized by long filaments and propagation over tens of meters is not in dispute but the physical mechanism underlying it has still to be uncovered in detail. Early discussions centered on the idea that the nonlinear self-focusing (SF) in air would be countered by the defocusing effect of the electron plasma generated by multi-photon absorption (MPA), and result in a stable self-guided beam. Numerical simulations showing stabilization of the peak field intensity were presented in Refs. [1, 6], and Brodeur et. al. [5] have used the moving focus model to explain the features of their experiments.

In this Letter we present numerical simulations of nonlinear pulse propagation in air to elucidate the physical mechanisms involved. Our study includes the effects of SF, MPA, group velocity dispersion (GVD), and absorption and defocusing due to the generated electron density [7, 8]. Although our simulations have not been validated against current experiments, it was clear that they do not yield results resembling the self-guiding picture. Instead a dynamic picture emerges in which pulses form, are absorbed, and are subsequently replenished by new pulses, thereby creating the illusion of one pulse which is self-guided.

Our model for pulse propagation in air is a nonlinear extension of one due to Feit and Fleck [7]. Assuming propagation along the z-axis, the equation for the slowly varying electric field envelope tex2html_wrap_inline292 in a reference frame moving at the group velocity is [8]:

  eqnarray17

where the terms on the right-hand-side describe transverse diffraction, GVD, absorption and defocusing due to the electron plasma, MPA, and nonlinear SF. Here tex2html_wrap_inline294 is the optical frequency, tex2html_wrap_inline296 the intensity, tex2html_wrap_inline298 , tex2html_wrap_inline300 , tex2html_wrap_inline302 is the electron density, tex2html_wrap_inline304 the cross-section for inverse bremsstrahlung, tex2html_wrap_inline306 is the electron collision time, tex2html_wrap_inline308 is the K-photon absorption coefficient, and the nonlinear change in refractive-index for a continuous wave (cw) field is tex2html_wrap_inline312 . The critical power for self-focusing collapse for cw fields is then tex2html_wrap_inline314 . The normalized response function R(t) accounts for delayed nonlinear effects, and f is the fraction of the cw nonlinear optical response which has its origin in the delayed component. The evolution of the electron density is described by the Drude model [7, 8]

  equation54

The first term on the right-hand-side of this equation describes growth of the electron plasma by cascade (avalanche) ionization, the second term is the contribution of MPA, and the third term describes radiative electron recombination. We are interested in solutions of these equations for an input collimated Gaussian beam tex2html_wrap_inline320 where tex2html_wrap_inline322 is the peak input power, tex2html_wrap_inline324 the spot size, tex2html_wrap_inline326 characterizes the pulse length, and tex2html_wrap_inline328 is the Rayleigh range of the input beam.

For the numerical simulations presented here we chose an operating wavelength tex2html_wrap_inline330 nm, tex2html_wrap_inline332 mm, for which the Rayleigh range is tex2html_wrap_inline334 m, and tex2html_wrap_inline336 fs. The material parameters employed in our simulations for air at standard temperature and pressure are as follows: tex2html_wrap_inline338 , tex2html_wrap_inline340 m tex2html_wrap_inline342 /W [9], giving a critical power of tex2html_wrap_inline344 GW, tex2html_wrap_inline346 eV representative of the constituents of the air, which yields K=7 for the order of the MPA, and tex2html_wrap_inline350 m tex2html_wrap_inline352 W tex2html_wrap_inline354 for the MPA coefficient from the Keldysh theory of MPA [10], tex2html_wrap_inline356 s (typical value from [7]), tex2html_wrap_inline358 m tex2html_wrap_inline360 /s, tex2html_wrap_inline362 m tex2html_wrap_inline342 was calculated using tex2html_wrap_inline366 [7]. The GVD for air was taken as k''=2.0 fs tex2html_wrap_inline342 cm tex2html_wrap_inline372 and we shall comment on using other values. The numerical results were checked by doubling the space and time resolutions which led to no significant changes in the behaviour of the results presented here.

Nibbering et. al. [9] have shown that air exhibits a delayed nonlinear response due to rotational Raman scattering with f=1/2. Their work shows that the response function R(t) initially undergoes a damped harmonic motion, followed by spontaneous resurgences for times beyond 2 ps. For the sub-picosecond pulses considered here the resurgences are not relevant and we model the response function using a damped oscillator model tex2html_wrap_inline378 , where tex2html_wrap_inline380 , and we have used tex2html_wrap_inline382 THz and tex2html_wrap_inline384 THz to mimic the exact response function given in Refs. [9].

Fig. 1 shows the global maximum over time of the on-axis intensity as a function of propagation distance z for peak input powers of 5.5 tex2html_wrap_inline388 (dash-dashed curve), 6.0 tex2html_wrap_inline388 (long-dashed curve), and 6.5 tex2html_wrap_inline388 (solid curve). In each case the maximum intensity initially grows explosively due to SF, but is then limited by MPA and absorption and defocusing due to the electron density [1, 6]. After limiting, the intensity remains fairly constant up to a distance of around 2 m, or roughly a Rayleigh range, after which it decays. This observation is in agreement with the moving focus prediction by Brodeur et. al. [5] that light filaments should end at a Rayleigh range of the input beam, an exception being the case tex2html_wrap_inline394 which we will comment on later.

Fig. 1 reveals a notch in the curves where dI/dz is discontinuous. To analyze this we show the on-axis pulse profiles in Fig. 2(a) for z=0 m (dotted curve), z=0.55 m (dashed curve), and z=1.1 m (solid curve), for the case tex2html_wrap_inline394 , and we see that the temporal compression effect due to SF [11] has contracted the pulse resulting in a single peaked pulse. At this stage the peak intensity growth is limited but the temporal pulse compression still proceeds until it is stopped by the normal GVD [12, 13]. In general, if the normal GVD is too small this compression proceeds until the numerical scheme breaks down and/or the envelope approximations underlying the model break down. We plan to investigate other linear and/or nonlinear terms which may become important in this regime, e. g. shock and nonparaxial terms, in the future. For the value of GVD employed here the pulse compression is arrested before the model and numerics are violated. For a propagation distance of z=1.1 m (solid curve) we see that the pulse profile shows two peaks separated temporally by tex2html_wrap_inline408 fs. The leading peak occuring at earlier times is directly associated with the single peak at z=0.55 m, and the trailing peak developed out of the background. Upon further propagation the leading peak decays while the trailing one remains, until it too decays at around a Rayleigh range. The notch in the intensity curve is therefore explained as that propagation distance where the increasing trailing peak takes over as the global maximum from the decreasing leading peak. We also note that a similar notch was experimentally and numerically observed in the filament energy measurements of ref. [5].

The double pulse profile in Fig. 2(a) is reminiscent of the pulse-splitting phenomenon for nonlinear pulse propagation with normal GVD [12, 13]. Here normal GVD plays a role in that it arrests the temporal compression, but the leading pulse develops first followed by the trailing pulse, whereas in the pulse-splitting case the two pulses develop simultaneously. In analogy to pulse-splitting the signature of the double pulse in Fig. 2(a) will be a modulated spectrum [13], with period tex2html_wrap_inline412 , or for T=200 fs, tex2html_wrap_inline416 nm. Fig. 2(b) shows the spectrum of the double pulse in Fig. 2(a) and we see the development of a spectral modulation with 10 nm period.

To expose the physics of the development of the trailing edge pulse, we note that the leading edge pulse at z=0.55 m shown in Fig. 2(a) (dashed curve) has its maximum displaced by -50 fs from the input pulse (dotted curve). This occurs because as the input pulse focuses and the intensity increases, an electron density is generated via MPA and cascade ionization, which produces a defocusing effect which is more pronounced for the trailing portion of the pulse. This is confirmed by the fact that the trailing edge of the pulse (dashed curve) is reduced with respect to the input (dotted curve). To elucidate further Fig. 3 shows the spatial profiles for propagation distances tex2html_wrap_inline422 m and for the time slice t=70 fs, which is that at which the trailing pulse forms (see Fig. 2(a)). The input beam profile is Gaussian (dotted curve), but for z=0.55 m (dashed curve) the central intensity is suppressed with respect to the input, the beam power having been displaced into a spatial ring by the defocusing effect. However, for z=1.1 m (solid curve) the beam profile has relocalized on-axis: This spatial defocusing of the trailing portion of the pulse into a ring and subsequent relocalization into a strong peak via SF is the physical mechanism by which the trailing edge pulse forms. Refocusing of the trailing edge of the pulse was also noted by Kosareva et al. [14] (they do not include GVD) using similar model including tunneling ionization. There are also indications from experiments that the energy outside the self-guided channel is important for the prolonged propagation of pulses in air [4]. The process of pulse decay and replenishment can occur more than once: The solid curve in Fig. 1(a) for tex2html_wrap_inline394 shows the growth of a second trailing edge pulse beyond the Rayleigh range tex2html_wrap_inline334 m, and this is again due to the relocalization of power that is initially displaced into a spatial ring by the defocusing effect of the plasma. We remark that the occurence of the second trailing edge pulse in our numerical simulations was dependent upon including the delayed nonlinear response due to the rotational Raman scattering.

In summary, we have presented numerical simulations to expose the physics underlying long distance propagation in air. We have shown that although the maximum intensity stabilizes over roughly a Rayleigh range, in agreement with the moving focus model of Brodeur et. al. [5], the evolution of the pulse is very dynamic, involving the development of a leading edge pulse which subsequently decays and is replaced by a new pulse. In addition, our simulations indicate that the inclusion of rotational Raman scattering [9] permits high power pulses to continue the process of pulse decay and replenishment beyond the Rayleigh range limit. There is also a potential link between the spatial ring formation predicted in the present work and the conical emission observed in recent experiments [4].

Acknowledgement: Effort sponsored by the Air Force Office of Scientific Research, Air Force Materiel Command, USAF, under grant numbers AFOSR-97-1-0002 and AFOSR-94-1-0463. Ewan Wright was also supported by AFOSR contract F49620-94-1-0343.




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Zora Mlejnkova
Fri Apr 3 14:26:10 MST 1998
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