190 OPTICS LETTERS / Vol. 40, No. 2 / January 15, 2015 Multi-megagauss magnetic field generation by amplitude modulated surface plasma wave over a rippled metal surface Pawan Kumar Department of Physics, Raj Kumar Goel Institute of Technology, Ghaziabad, UP-201003, India ([email protected]) Received October 7, 2014; revised November 28, 2014; accepted November 30, 2014; posted December 1, 2014 (Doc. ID 224482); published January 9, 2015 The mechanism of a self-generated megagauss magnetic field by an amplitude modulated surface plasma wave (SPW) over a rippled metallic surface is proposed. The amplitude modulated SPW exerts a ponderomotive force on free electrons in the metallic ripple, giving them an oscillatory velocity at the modulation frequency. The osNL cillatory velocity couples with the electron density in metallic ripple and drives a nonlinear current J⃗ with NL ∇ × J⃗ ≠ 0. This irrotational nonlinear current generates the megagauss magnetic field. © 2015 Optical Society of America OCIS codes: (190.4410) Nonlinear optics, parametric processes; (240.4350) Nonlinear optics at surfaces; (240.6680) Surface plasmons; (240.6690) Surface waves. http://dx.doi.org/10.1364/OL.40.000190 The surface plasma wave (SPW) plays an important role in laser coupling to metals [1–5] and overdense plasmas [6–8]. When the high intensity femtosecond laser gets mode converted into an SPW, the electric field is greatly enhanced, leading to a variety of nonlinear effects, e.g., multiphoton emission of electrons, ablation of materials, and harmonic generation [9–14]. A noteworthy feature of high power laser–matter interaction has been the generation of a multigauss magnetic field because of a variety of mechanisms, e.g., crossed density and temperature gradients, and a ponderomotive force across density gradient Weibel instability [15–18]. A large amplitude SPW is also shown to generate quasistatic current in the skin layer of the plasma that produces a magnetic field. As the electron density of the plasma is increased, the skin depth of the SPW decreases and so does the generated magnetic field. At a laser intensity of <1016 W∕cm2 , investigated magnetic fields of the order of 1 MG have been predicted [19]. Two dimensional particle-in-cell simulations for laser–overdense plasma coupling via resonant excitation of SPW and quasi-steady state magnetic field generation reveal enhanced laser absorption up to 75%, and the peak value of the steady magnetic field is 580 MG at an intensity of ∼1019 W cm−2 [8]. An SPW over a rippled metallic surface is shown to produce in the ripple region a nonlinear current that has nonzero curl and gives rise to magnetic field generation [20]. However, in these studies do not allow temporal variation of laser intensity or consider a nonperiodic variation. In this Letter, I develop a mechanism of multi megagauss magnetic field generation by an amplitude modulated SPW over a rippled metallic surface. The physics of the process is as follows: the amplitude modulated SPW imparts the oscillatory velocity to electrons to exert a ponderomotive force on them at modulation frequency. The ponderomotive force to imparts oscillatory velocity to electrons which couples with the electron density rippled and to create a nonlinear current which generates the magnetic field. This magnetic field is a function of 0146-9592/15/020190-03$15.00/0 laser intensity: as intensity increases the laser intensity magnetic field increases but our approach is none-relativistic. In other studies, the magnetic field is generated via resonantly excited nonamplitude modulated SPWs. Consider a rippled metallic-free space interface (Fig. 1), x Δ cos qz (where Δ is the height of the ripple) with x < Δ cos qz, representing the metal characterized by relative lattice permittivity εL and free electron density n0 . As one moves along ẑ in the ripple region, the electron density shows a periodic variation with z, hence, following Liu and Tripathi [4], we model the surface ripple as a density ripple with free electron density: n n0 nq ; nq n0 iqz e : 2 (1) We allow a large amplitude SPW to propagate along ẑ (cf. Fig. 1). For small Δ, as correspond to the SPW wavelength, the field of the amplitude modulated SPW can be written as [21] ⃗E 1 A ẑ kz x̂ exp−iωt − kz z expαI x; for x < 0 iαI kz x̂ exp−iωt − kz z exp−αII x; for x < 0; A ẑ − iαII (2) where A A0 1 μ cos Ωt − z∕vg α2I k2z − ω2 ∕c2 εL − ω2p ∕ω2 , α2II k2z − ω2 ∕c2 , k2z ω2 ∕c2 εm ∕1 εm , εm εL − ω2p ∕ω2 , ωp n0 e2 ∕mε0 1∕2 is the plasma Fig. 1. Surface plasma wave on metallic rippled surface. © 2015 Optical Society of America January 15, 2015 / Vol. 40, No. 2 / OPTICS LETTERS frequency, e and m are electron charge and mass, εL is lattice dielectric constant of the metal, and ε0 is the free space permittivity. We allow A to have slow t, z dependence, A A0 1 μ cos Ωt − z∕vg , where vg is the group velocity of the SPW, μ is the index of modulation, and Ω is the modulation frequency. The SPW imparts fast oscillatory velocity to electrons inside the metal: ⃗vω eE⃗ : miω (3) It also exerts a ponderomotive force on them at the modulation frequency Ω: 2 k2z ⃗F p − m ∇ ⃗vω · ⃗vω − e 1 2 2αI e2αI x 2A0 1 μ 2 4mω2 αI × cos Ωt − z∕vg ; (4) where we have assumed μ ≪ 1. The ponderomotive force imparts an oscillatory velocity to electrons: v⃗ Ω − F⃗ p e2 A20 μ1 k2z ∕α2I x̂ αI e2αI x e−iΩt−z∕vg : (5) miΩ m2 iΩω2 Had we chosen A A0 cos Ωt − z∕vg , the ponderomotive force would have a 2Ω component and the oscillatory velocity would be ⃗v2Ω − F⃗ p e2 A20 1 k2z ∕α2I 2αI x −2iΩt−z∕vg x̂ αI e e : (6) 2miΩ 4m2 iΩω2 The electron drift beats with the density ripple to produce nonlinear current: 1 NL J⃗ Ω − nq e ⃗vΩ 2 or BΩy where εeff εL − ω2p ∕Ω2 , taking ∇× of Eq. (8) and using Eq. (9), one gets ε ∂2 B⃗ ⃗ μ0 ∇ × J; ∇ × ∇ × B⃗ −∇2 B⃗ − eff c2 ∂t2 ε NL ∇2 B⃗ Ω eff Ω2 B⃗ Ω μ0 ∇ × J⃗ Ω ; x < 0 c2 ω2 ∇2 B⃗ Ω 2 B⃗ Ω 0: x > 0. c (7) The current density produces a magnetic field in compliance with Maxwell’s equations: ∇ × E⃗ − ∂B⃗ ; ∂t 1 ∂E⃗ NL ; εeff 2 ∇× B⃗ μ0 J⃗ c ∂t (8) (9) (10) We consider the following two cases: Case I: Unrippled surface Using ∂∕∂z Ω∕vg , εeff εL − ω2p ∕Ω2 , Eq. (10) may be written as 2 ∂2 B⃗ Ω Ω Ω2 ⃗ NL 2 εeff − 2 BΩ μ0 ∇ × J⃗ Ω ∂x2 c vg 2 ∂2 B⃗ Ω Ω Ω2 ⃗ x<0 2 − 2 BΩ 0: x > 0. ∂x2 c vg (11) NL NL ∂ NL ⃗ Since J⃗ Ω ‖x̂, ∇ × J⃗ Ω ŷ ∂z J Ωx i vΩg J NL Ωx , BΩ has a ycomponent. Further, the above term varies as e2αI x in medium I, ∂∕∂x 2αI μ0 iΩ∕vg J NL μ0 iΩ∕vg J NL Ωx Ωx BΩy Ω2 ≈ : 2 2 Ω 2 4α ε − 4α 2 2 I eff I c v (12) g In a vacuum, the magnetic field falls off as e−βx , where β Ω∕vg 1 − v2g ∕c2 1∕2 . Case II: Rippled surface NL J⃗ Ω has z-dependence and varies as of e−iΩt−qΩ∕vg z , one may write the magnetic field as μ0 iΩ∕vg qJ NL μ iΩ∕vg qenq e2 A20 μ1 k2z ∕α2I αI exp2αI x exp−iΩt − Ω∕vg qz Ωx 2 0 2 i h : 2 2 4α2I Ωc2 εeff − vΩg q 4α2I Ωc2 εeff − vΩg q 2m2 iΩω2 1 NL J⃗ 2Ω − nq e ⃗v2Ω : 2 191 (13) The magnetic field has been calculated for moderate intensity (I L 1016 W∕cm2 ) and the following parameters: jvω j∕c 0.1, nq ∕n0 1∕2, Ω 6 × 1012 rad∕s, e∕m 1.6 × 1011 , qc∕ωp 1∕20, and εL 9 (gold). The magnetic field jBΩy j is a function of ω∕ωp and plotted in Fig. 2. The maximum magnetic field at this intensity is 3 MG. The figure shows that the magnetic field increases with plasma frequency, but at a higher frequency it decreases. This is because, as the electron density increases, the skin depth of the SPW decreases and the generated magnetic field also decreases at a higher 192 OPTICS LETTERS / Vol. 40, No. 2 / January 15, 2015 associated with the generation of the magnetic field and relevant for many applications of interests. Fig. 2. Magnetic field if function of frequency. frequency the coupling of the SPW because of the decreasing of the skin. The rippled surface enhanced magnetic field generation via excitation of the amplitude modulated SPW. In conclusion, an amplitude modulated laser excites an amplitude modulated SPW over a rippled gold surface, leading to the generation of a magnetic field at the modulated frequency because of the quasi-static nonlinear surface current associated with it. A metallic rippled surface of suitable wave number gives rise to significant enhancement in the magnetic field. The magnetic field increases with frequency and decreases at higher frequency. When the magnetic field acquires large value, the electron cyclotron frequency becomes significant and affects the propagation of the SPW and nonlinear phenomena associated with it. A Gaussian laser pulse of half-period τL could also produce a pulsed magnetic field. When increasing the intensity of the laser, the magnetic field increased and becomes relevant in many situations of interests. The SPW can also appear on flat overdense plasmas by the decay process and is References 1. H. Raether, Springer Tracts in Modern Physics (SpringerVerlag, 1988), Vol. 111. 2. D. Sarid, Phys. Rev. Lett. 47, 1927 (1981). 3. V. M. Agranovich, Sov. Phys. Uspekhi 18, 99 (1975). 4. C. S. Liu and V. K. Tripathi, IEEE Trans. Plasma Sci. 28, 353 (2000). 5. P. K. Kaw and J. B. McBride, Phys. Fluids 13, 1784 (1970). 6. S. R. J. Brueck and D. J. Ehrlich, Phys. Rev. Lett. 48, 1678 (1982). 7. J. Kupersztych and M. Raynauda, Phys. Rev. E 59, 4559 (1999). 8. A. Bigongiari, M. Raynaud, C. Riconda, A. Heron, and A. Macchi, Phys. Plasmas 18, 102701 (2011). 9. T. Tsang, T. Srinivasan-Rao, and J. Fischer, Phys. Rev. B 43, 8870 (1991). 10. B. N. Chichkov, C. Momma, S. Nolte, F. von Alvensleben, and A. Tünnermann, Appl. Phys. A 63, 109 (1996). 11. I. Ursu, I. N. Mihăilescu, A. M. Prokhorov, V. I. Konov, and V. N. Tokarev, Physica 132C, 395 (1985). 12. N. Kroo, G. Farkas, P. Dombi, and S. Varró, Opt. Express 16, 21656 (2008). 13. T. Y. F. Tsang, Opt. Lett. 21, 245 (1996). 14. Y. Guo and M. Deutsch, Opt. Lett. 39, 3860 (2014). 15. R. J. Mason and M. Tabak, Phys. Rev. Lett. 80, 524 (1998). 16. P. Mora and R. Pellat, Phys. Fluids 22, 2408 (1979). 17. J. A. Stamper, K. Papadopoulos, R. N. Sudan, S. O. Dean, E. A. McLean, and J. M. Dawson, Phys. Rev. Lett. 26, 1012 (1971). 18. G. Chatterjee, P. K. Singh, S. Ahmed, A. P. L. Robinson, A. D. Lad, S. Mondal, V. Narayanan, I. Srivastava, N. Koratkar, J. Pasley, A. K. Sood, and G. R. Kumar, Phys. Rev. Lett. 108, 235005 (2012). 19. A. Bigongiari, M. Raynaud, and C. Riconda, Phys. Rev. E 84, 015402(R) (2011). 20. J. Parashar, Phys. Plasmas 20, 044503 (2013). 21. C. S. Liu and V. K. Tripathi, Electromagnetic Theory for Telecommunications (Cambridge University Press India, 2007).
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