I ntrnat. J. Math. Math. Si. Vol. 2 No. 2 (1979) 325-336 325 NONLINEAR INTERACTION OF WAVES IN A HOT INHOMO.GENEOUS MAGNETIZED PLASMA TARA PRASAD KHAN Physics Department Dinabandhu Andrews College Dist- 24 Parganas, West Bengal, India MAHADEB DAS Physics Department Serampore College, Serampore Dist Hooghly, West Bengal, India LOKENATH DEBNATH Departments of Mathematics and Physics East Carolina University Greenville, N.C. 27834, U.S.A. (Received August 7, 1978 and ABSTRACT. in revised form May i, 1979) This study is concerned with the theory of parametric coupling of waves in a hot inhomogeneous magnetized plasma in which the temperature gradient has been taken into account. The general dispersion relation and the polarization of the ordinary and the extra-ordinary wave modes are discussed. The eigen-mode solutions of the coupled differential equations for the wave amplitudes are obtained in the terms of the so called three wave interaction matrix elements. The theory of nonlinear wave-wave interactions, which has been extended to the case of an inhomogeneous magnetized plasma, is used to determine the threshold value of the electric field and the frequency shift. The results of this paper are also compared NONLINEAR INTERACTION OF WAVES 326 with the other known results. It is shown that the findings of this study are in excellent agreement with the results of earlier investigators. KEY WORDS AND PHRASES. Parametric instaby, Waves in inhomogeneo plasma, wave-wave interactions, Threshold electric field and frequency shift. 1980 MATHEMATICS SUBJECT CLASSIFICATION CODES. i. 76X05, 76E30. INTRODUCTION. In recent years there has been considerable interest in the theory of parametric instability in an inhomogeneous plasma [1-8] because of its fundamental role in the study of weak plasma turbulence, and of many important physical applications. henomena In their recent research-expository and survey article on parametric in a plasma, Galeev and Sagdeev [9] reviewed the theory of parametric instabilities in an inhomogeneous plasma using the generalized Mathleu equation as a model equation. They have also presented the latest advances of the nonlinear theories of parametric instabilities based on the ideas of weakly turbulent plasma. Perkins and Flick [I0] have made an interesting study of parametric instabilities in an inhomogeneous plasmas, and then calculated the threshold electric field. It is shown that the value of the threshold electric field increases in an inhomogeneous plasma because energy propagates away from the unstable region by electron plasma waves. Thus an additional energy loss occurs and is solely responsible for the increase of the threshold electric field not observed in a homogeneous plasma. Eubank [ii] experimentally confirmed the theoretical prediction of Perkins and Flick. In a recent paper, Kroll, Ron and Rostoker [12] have suggested that the nonlinear resonance of two transverse lectromagnetic waves whose frequencies differ slightly by the electron plasma frequency can be applied to excite longitudinal electron plasma oscillations. Montgomery [13] observed certain mathematical inaccuracy and physical limitations of the work of Kroll, Ron and Rostoker, and then analyzed the problem of nonlinear wave interactions in plasma with laser beams. 327 T.P. KHAN, M. DAS AND L. DEBNATH Using the perturbation method of Krylov-Bogliubov-Mitropolskii, Montgomery obtained the amplitude-dependent frequency shift and wave number shift with physical significance. It was shown that the resonant excitation of longitudinal plasma oscillations is possible by the transverse electromagnetic waves. Etievant, Ossakow, Ozizmir and Su [14] have investigated the nonlinear wave-wave interactions of electromagnetic waves in an infinite homogeneous plasma. It is interesting and important to take into account the effects of density and temperature gradients on the above problem. The present study deals with the theory of parametric coupling of waves in a hot inhomogeneous magnetized plasma in which the temperature gradient has been The general dispersion relation and the polarization of taken into consideration. The eigen-mode solutions of the coupled two different wave modes are investigated. equations for the wave amplitudes are obtained in terms of the three wave interaction matrix elements. The theory of nonlinear wave-wave interactions is used to determine the threshold electric field and the frequency shift. The results of this analysis are found to be in excellent agreement with those of earlier workers. 2. BASIC EQUATIONS FOR TWO PLASMA MODEL. In two plasma model, the equations of motion and the continuity equation for each kind of component are in the usual notations given by Dv_n Ze Dt m V E (-Tap ) m O DO Dt + 0 V Z --v- -v v -n (2.1) (2.2) 0 eB where cm is the cyclotron frequency, v a is the collision frequency of each 328 NONLINEAR INTERACTION OF WAVES component and B B O z is the external magnetic field The subscript u stands for e or i corresponding to electrons and ions respectively, Z e electron or ion and is the charge of an is the Boltzmann Constant. The Maxwell equations are curl _E E c t 1 curl B (2.3ab) 4e(n-no) dlv_E c t 4r nev dlv B c (2.4ab) 0 We consider a plasma model whose density dlstrlbution varies as 0 a i with the density gradient (d__) and neglect the time dependence of UO due to any external electric field. < Vo x (t)e Voy t)e T The e e KT fl e Ze m e2_e 2 (2.6) (2.7) 0 3. (2 5) =x= with 0 THE FIRST ORDER EQUATIONS. _ In the first order approximation, equations (2.1) dropping the subscript - where + v --o .VTg) i (’---- Vv + I --Vl Vv o Z__e E m--o Pao zeroeth order solution of (2.1) gives me e2-)e 2) ___e pao(1-x) Zfi x -o v--i represents the first order terms in (2.2) can be written as, V’(Tp) m .VTg) (-- _Zl x v --o V_l (3.1) 329 T.P. KHAN, M. DAS AND L. DEBNATH Assuming the density gradient is small, we take the space and time dependent _ exp[i(k of the first order quantities as r- tot). The equation (3.1) can then readily be solved to obtain where vii =_ _E1 (3.2) Is the mobility tensor given by Ze [( -Pc _k when I is the unit dyadic and ( c V_o) I +-- 1 _c _k -oV 1(+ G KT m(’- k A (to- k (3.3/ to is yy) Gyy .+(_ v’+ iZao k o with -(k v v --K )2 #, + 2i(l-()k (to- k 2 v (3.6) 0 --0 is the ratio of the two specific heats. and Using equations (3.2) and taking the Maxwell equations (2.3ab) (2.4ab), it turns out that with D -- =(k to2) 2 i I c c where to 2 o (3,7) toct2 v (+ k 0- to c 4epa (3.9) m In the case of wave propagation along with x-direction (k k), we obtain 330 NONLINEAR INTERACTION OF WAVES the dispersion relation D(k, m) Det (3.10) o, There are two independent solutions of equation (3.10) in the form D (3.11) 0 ZZ which corresponds to the ordinary wave, and D xx D yy -D xy D yx (3.12) =0 which corresponds to the extra-ordinary wave, where Dxx, Dyy, D. are the elements of the matrix The first order fields for the different modes (ordinary and extra-ordinary) are obtained as g --O E with a a a A 0 0 r- t)] (3.13) exp[i(k r- m t)] (3.14) 0 Ae e e.xp[i(k --e 0 e I a o e (i b x + E __x__ and b=-ig y i D )/(1 + b2) 2 yy_ (3.15ab) (3.16) D yx where 2 YY Dyx 4. c 7 iz kv o oy (3.17) c o z (3.8) THE SECOND ORDER EQUATIONS. In the second order approximation, we obtain from equations (2.1) (2.2) T.P. KHAN, M. DAS AND L. DEBNATH 8v 2 ---+--oV Vv 2 + vI Vv I + v2 Ze VVo --E--2m -v Z v v2- 2 -o Z --o x ZR v2 x 1 Vl (4.1) + vp) m 0/ 2 with (4.2) 2 o V_l + (k- (k PO ) i _v2 (to- k / (4.3) v --0 Using the space and time dependence of all second order quantities in the form exp[i(_k Z_e v2 with Q mt)] r c m H =-v I KTm I pl(-k we find (i k Vv I I v -o o V_ l)((m-k’--i y_kpo (Y_oV)- ) I+-k v -o E_2 m + c H (4.4) i Q Vl (4.5) 2 2)i + {yk- i(y- 2) i} Po +iyp I 2 ] (4.6) Using the Maxwell equations and eliminating the second order magnetic field follows that v x (v xE) whence J2 =- @ Po + I c --v2 2E2 4 3t c 2 P2 B2, it (4.) @t o + Pl --Vl (4.8) Substituting the values of v in equation (4.4), we obtain 2 V x (V x 4im 2 c E2) + 1 c o 32E2 + @t I + 2 "’----.L -/ c m p Po + c H + - v k so--ok e o J 1 Pal o 3E 2 (4.9) 332 NONLINEAR INTERACTION OF WAVES EQUATION FOR THE INTERACTING MODES. 5. We assume a plane wave solution with an amplitude varying in the direction of propagation and write _E2 where A A (x,t) a exp[i(k (5.1) mt)] r is a slowly varying function of x and t because the nonlinearity is assumed to be weak. k2A and m2A, We next drop the second derivatives of A in comparison to + (Ul x (u2 (u 3 - )AI A3 A2 V123 (mllm21m3) + )A 3 where Ak A I A V321 (-m31m21-ml) 2 (k_2 + kl) k 3 We write the matrix elements for a and a VI2 3 e 2Ti t A exp{i(-x A k + (5.2) m)} m)}, t A (5.3) exp{i(-x A k + t A m)} (5.4) m3- (ml + m2) Am and 0 to obtain the final result exp{i(x A k AI A3 V213 (-m21-mllm3) x +)A2 E 2 D then use the linear dispersion relation I a and a a 3 (5.5ab) ae 2 where are defined in (3.15ab). (" PO {-i(al * 3 c 2 a3)(3 ( Ze a2) m( 0 3 2 * 3 (a I 12 I and Ze m ms(m 2 3a (k 2 a3)(k3 c i6) Vox)(m 2 k3 + Z o + k2. Vox)A2 (m 2 2 2) .+ (al "(’a3) (k--2-i) "c (2 k2 o 11I k2Vx)m (2 -k2 V_ox) m2 a + k2Vox) 2 k 2 V or) 1 a2 b2 (5.6) T.P. KHAN, M. DAS AND L. DEBNATH V321 is obtained by interchanging m V231 2i [ PZe (a2 , + a 2 m 2 =__.i We consider , V -o m and I k 2 A2 mZe i+b22 , k, Ak real and A 3 V123 and c 2{k3( 33 e 2 (--2_k2V_ox) b2+Z flo) -( in m3 333 k3 3(i --klVox) "al) + + kl kl (5.4). (5.7) )l(3-k3Vox is the pump of fixed amplitude. amplitudes are described by equations (5.2) 3 l(al’e "a3)}] We take A’s The small to be space independent so that t A A dt}] [ep{i 1 (5.8) o and then we find [22 + t where - 9 2 I[AI I exp{i (V123 e Neglecting i A m t assumes the form t + (A4m)2] i A m V 2 13 A e 2@ 2 (5.10) 3 it follows that the solution of g(t)dt} + B exp{-i 2 o (5.9) (59) by W.K B method g(t)dt}] (5.11) o with i g IV123 V213 A32 (A 24i (5.12) When the wave packet drifts along x the time-increment dt can be written as dt (dx) ) to obtain AI xt g(x) dx] [exp ) (5.13) o where the integration is limited to the instability zone. It is interesting to note that the threshold value of the wave can be calculated when g < 0 334 NONLINEAR INTERACTION OF WAVES Am A3= (5.14) 2/V123V213 Thus the value of the frequency shift can be obtained from (5.14) as i Am 2A 3 IV123V213 -{(m 2- mA2 k2Vox)b2- + m2 (m2-k2Vox) b 2-o 2 k3 (m3-k3Vox) (m2-k2Vox) m 2 where the assumption o} 3 (ml-klVox) >> m m / e kl + 2 m I (m3-k3Vox) I] (5.15) is invoked. j / /m With the following numerical values m k w 2 k 3 of Montgomery Am 1015 sec =5 6x i011 sec k 2 a3- al it turns out that e 2.7 x 108 -i -i -i 19 cm I 106 3 sec e.s. -i U/cm which is in good agreement with that 13] Similarly, considering the space dependence only, one can calculate the wave number shift from equations (5.2) 6 (5.4). DISCUSSION. The general features of density gradient and magnetic field in the nonlinear interactions of plasma oscillations have been investigated. This is important in connection with its use as an optical density probe suggested by Kroll, Ron and 335 T.P. KHAN, M. DAS AND L. DEBNATH Rostoker [13] or as a controlled source of plasma oscillations conceived by Montgomery [13] the frequency shift will deviate with the increased value of the density gradient. However, strong magnetic field will have only influence on the frequency shift. ACKNOWLEDGMENT. This work was partially supported by a summer grant from the East Carolina University Research Committee. Authors express their sincere thanks to Mrs. Lela Skinner for typing the final manuscript. REFERENCES i. Liu, C. S. and Rosenbluth, M. N. Parametric decay of electromagnetic Waves into two plasmons and its consequences, Phys. Fluids. 19 (1976) 967-971. 2. Liu, C. S., Rosenbluth, M. N., and White, R. B. Raman and Brillouin scattering of electromagnetic waves in inhomogeneous plasmas, Phys. Fluids. 17 (1974) 1211-1219. 3. Nicholson, D. R. 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