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Travaux sur les symétries de Lie des équations aux ... - DMA - Ens

Travaux sur les symétries de Lie des équations aux ... - DMA - Ens

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⎧Θ l 1y l 2 = −Ll 1l 1 ,l 1 ,y l 2 + 2 M l 1 ,l 2 ,x+53(3.102)⎪⎨⎪⎩+ ∑ kH k l 1M l2 ,k + 1 2 Ll 1l1 ,l 1L l 2l2 ,l 2− ∑ k+ 1 2 Ll 1l1 ,l 1Θ l 2+ 1 2 Ll 2l2 ,l 2Θ l 1− ∑ k+ M l1 ,l 2Θ 0 + 1 2 Θl 1Θ l 2.L k l 1 ,l 2L k k,k +L k l 1 ,l 2Θ k +We notice that the right-hand si<strong>de</strong> of (3.99) should be in<strong>de</strong>pen<strong>de</strong>nt of l 1 ;this phenomenon will be explained in a while.Proof. For Θ 0 x in (3.99), it suffices to put j := l 1 in (3.69).To obtain Θ 0 y l 1 , we put j := l 2 and l 2 := l 1 in (3.86), which yields:(3.103)Θ l 1 x − 1 2 Θ0 y l 1 = −1 2 Hl 1l 1 ,y l 1 ++ G l 1M l1 ,l 1− 1 2+ 1 2− 1 4∑k∑k∑kH k l 1L l 1l1 ,k − 1 4H l 1kL k l 1 ,l 1+∑Hl k 1L k k,k −kH k l 1Θ k + 1 4 Ll 1l1 ,l 1Θ 0 + 1 4 Θ0 Θ l 1.We may easily solve Θ 0 y l 1 and Θl 1 x thanks to this equation (3.103) and thanksto (3.91): in<strong>de</strong>ed, to obtain (3.100), it suffices to compute 4 3 · (3.91) + 2 3 ·(3.103); to obtain (3.101), it suffices to compute 2 3 · (3.91) + 4 3 · (3.103).Finally, (3.102) is a copy of (3.93). This completes the proof.3.104. Appearance of the crucial four families of first or<strong>de</strong>r partial differentialrelations (I), (II), (III) and (IV) of Theorem 1.7 (3). However,in solving Θ 0 x, Θ 0 , y l 1 Θl 1 x and Θ l 1from our six families of equations (3.69),y l 2(3.86), (3.89), (3.91), (3.93) and (3.96), only a subpart of these equations hasbeen used. We notice that the two families of equations (3.91) and (3.93)have been used completely and that the family of equations (3.96), whichdoes not involve Θ, coinci<strong>de</strong>s precisely with the system (IV) of Theorem1.7 (3). To in<strong>sur</strong>e that Θ 0 x , Θ0 , y l 1 Θl 1 x and Θ l 1as written in Proposi-y l 2tion 3.98 are true solutions, it is necessary and sufficient that they satisfythe remaining equations. Thus, we have to replace these solutions (3.99),(3.100), (3.101) and (3.102) in the three remaining families (3.69), (3.86)and (3.89).Firstly, let us insert insi<strong>de</strong> (3.69) the value of Θ 0 x given by the equation(3.99), in which the in<strong>de</strong>x l 1 is replaced in advance by an arbitrary

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