CEJM 3(3) 2005 508–515 Radial-type complete solutions for a class of partial differential equations Ayşegül Çetinkaya1∗, Nuri Özalp2† 1 Department of Mathematics, Faculty of Arts and Sciences, Gazi University, 40100, Kirsehir, Turkey 2 Department of Mathematics, Faculty of Sciences, Ankara University, Beşevler, 06100 Ankara, Turkey Received 17 November 2004; accepted 1 June 2005 Abstract: We give some fundamental solutions of a class of iterated elliptic equations including Laplace equation and its iterates. c Central European Science Journals. All rights reserved. Keywords: Complete solutions, iterated equations, Almansi’s expansion, Kelvin principle MSC (2000): 35A08, 35C05, 35G99 1 Introduction Much of the physical problems are solved in spherical or cylindrical domains. It means, most of the time, that the solutions are symmetric functions with respect to a point or with respect to an axis. That is why, when investigating the solutions, we see a frequent use of the type of solutions in terms of a variable r defining a distance to a point. For some of the research have been done for various type of problems, we refer to the references [1-9]. Here in this study, we apply the idea to a class of linear partial differential equations of second order and its iterates. ∗ † Let us consider the class of equations p n 2 X 1 ∂u γu 2∂ u Lu = xi 2 + αi xi + p =0 xi ∂xi ∂xi r i=1 E-mail: [email protected] E-mail: [email protected] (1) A. Çetinkaya, N. Özalp / Central European Journal of Mathematics 3(3) 2005 508–515 509 where γ, αi (i = 1, 2, ..., n) are real parameters, p (> 0) is a real constant and r is defined by r p = xp1 + xp2 + ... + xpn . (2) The domain of the operator L is the set of all real valued functions u(x) of the class C (D), where x = (x1 , x2 , ..., xn ) denotes points in Rn and D is a regularity domain of u in Rn . 2 Almansi gave an expansion formula for the solutions of Laplace equation [1]. Lyakhov and Ryzhkov, [5], obtained Almansi’s expansions for B- polyharmonic equation i.e. obtained the solutions of the equation ∆m B f = 0, where ∆B = n X J=1 Bj + N X ∂2 , 2 ∂x i i=n+1 Bj = ∂ 2 /∂x2j + γj ∂ . xj ∂x Altın generalized the idea to a class of singular partial differential equations and obtained a Lord Kelvin principle and radial type solutions for this class of equations [2,3,4,9]. In [7], Özalp and Çetinkaya gave an expansion formula and Kelvin principle for the class of equations given by (1). More precisely, they proved that if ui (x), i = 1, ..., k − 1 are any k solutions of the equation (1), then the functions w= k−1 X r jpui (x) i,j=0 and w=r −φ k−1 X i=0 r ip ui x 1 , 2 r x2 xn , ..., r2 r2 are solutions of the iterated equation Lk u = 0 . In [6], it is shown that, if u = f (r m ), f ∈ C 2 , then r p L(u) = ′′ m2 v 2 f (v) + m (m − p + n(p − 1) + Pn i=1 ′ αi ) vf (v) + γf (v) = 0 with v = r m . Since, this is an Euler equation, and the solutions of Euler equation are in the form f (r m ) = r cm ,( where c is a root of the characteristic equation), we conclude that equation (1) have solutions depending on powers of r m . We call these type of solutions as r m − type solutions. Here, in this study we first give r m − type solutions for the iterates of the equation (1) (i.e. for the equation Lk u = 0 ) and we generalize the idea to the equations of the form Lkq q ...Lk22 Lk11 u = 0 (3) 510 A. Çetinkaya, N. Özalp / Central European Journal of Mathematics 3(3) 2005 508–515 where q, k1 , ..., kq are positive integers, p n 2 X ∂ γv 1 (v) 2 ∂ Lv = xi 2 + αi xi + p. xi ∂xi ∂xi r i=1 (4) (v) Here, γv , αi (v = 1, 2, .., q; i = 1, 2, ...n) are real constants, and the operator Lkvv denotes, as usual, the successive applications of the operator Lv onto itself, that is Lkvv u = Lv (Lkvv −1 u). 2 rm type solutions for Lk u = 0 We borrow the following result from [7]. Lemma 2.1. For any real or complex parameter m, Lk (r m ) = k−1 Y [(m − pj)(m − pj + 2ψ) + γ] r m−pk (5) j=0 where the integer k is the iteration number and 2ψ = −p + n(p − 1) + n X αi i=1 Now, we are ready to generate the r m type solutions of the iterated equation Lk u = 0. Let Φ(m) = m(m + 2ψ) + γ. Then, equation (5) becomes Lk (r m ) = k−1 Y Φ(m − pj)r m−pk . j=0 On the other hand, for each j(= 0, 1, ...k − 1), the roots of the quadratic equations Φ(m − pj) = 0 are p (1) m = pj − ψ + ψ2 − γ j (6) p m(2) = pj − ψ − ψ 2 − γ. j Thus, we can rewrite (5) as k m L (r ) = k−1 Yh j=0 i (1) (2) (m − mj )(m − mj ) r m−pk . (7) A. Çetinkaya, N. Özalp / Central European Journal of Mathematics 3(3) 2005 508–515 511 From (7), we conclude that (1) u = r mj , (2) u = r mj (j = 1, 2, ..., k − 1), are solutions of Lk u = 0. Since the operator L is linear, by the superposition principle, the function k−1 X (1) (2) (1) (2) u= Aj r mj + Aj r mj j=0 (1) (2) is a complete solution of the iterated equation Lk u = 0. Here Aj and Aj are arbitrary constants. To generate the real valued solutions, we have three cases for the roots of the quadratic equations Φ(m − pj) = 0 for each fixed j. (1) ψ 2 − γ > 0, i.e. mj (i) (2) and mj (1) are two different real roots. In this case, r mj and (2) r mj are real valued linearly independent solutions of Lk u = 0. (1) (2) (ii) ψ 2 − γ = 0, i.e. mj = mj = pj − ψ is a multiple real root. In this case, from the theory of elementary differential equations we know that r pj−ψ and r pj−ψ ln r are real valued linearly independent solutions of Lk u = 0. (iii) ψ 2 − γ < 0, i.e. the roots are complex conjugates. Once p again from the pj−ψ theory of p elementary differential equations we know that r cos( γ − ψ 2 ln r) and r pj−ψ cos( γ − ψ 2 ln r) are real valued linearly independent solutions of Lk u = 0. Now let us define three auxiliary functions as 1, if ψ 2 − γ > 0 Λ1 = , 0, else 1, if ψ 2 − γ = 0 Λ2 = , 0, else 1, if ψ 2 − γ < 0 Λ3 = . 0, else Hence, we can give the following result: Theorem 2.2. Real valued r m type solutions of the iterated equation Lk u = 0 is given 512 A. Çetinkaya, N. Özalp / Central European Journal of Mathematics 3(3) 2005 508–515 by the formula u= k−1 X j=0 + (1) (2) (1) (2) Λ1 Aj r mj + Aj r mj k−1 X j=0 + k−1 X (1) (2) Λ2 r pj−ψ Bj + Bj ln r Λ3 r pj−ψ j=0 (i) (i) (i) where Aj , Bj , Cj 3 r m (8) hp i hp i (1) (2) 2 2 Cj cos γ − ψ ln r + Cj sin γ − ψ ln r (i = 1, 2) are arbitrary constants. kq k2 k1 type solutions for Lq ...L2 L1 u = 0 Now let v and q be positive integers, 1 ≤ v ≤ q, 2ψv = −p + n(p − 1) + n X (v) αi (9) Φv (m) = m(m + 2ψv ) + γv (10) i=1 and Then, for any positive integer kv , from (5) we have Lkvv (r m ) = kY v −1 Φv (m − pj)r m−pkv j=0 = kY v −1 [(m − pj)(m − pj + 2ψv ) + γv ] r m−pkv (11) j=0 Lemma 3.1. For any positive integer q, the following equality holds. " q k −1 !# v−1 v YY X Pq m k2 k1 kq Φv m − p(j + kl ) r m−p( l=1 kl ) . Lq ...L2 L1 (r ) = v=1 j=0 Here, we assume that P0 l=1 l=1 kl = 0. Proof. We use induction argument on q. For q = 1, (12) is reduced to Lk11 (r m ) = kY 1 −1 j=0 Φ1 (m − pj)r m−pk1 (12) A. Çetinkaya, N. Özalp / Central European Journal of Mathematics 3(3) 2005 508–515 513 which gives (11) for v = 1. Now assume that (12) holds for q − 1. Now, for q, we get kq−1 Lkq q ...Lk22 Lk11 (r m ) = Lkq q Lq−1 ...Lk22 Lk11 (r m ) = Lkq q "q−1 k −1 v YY Φv m − p(j + v=1 j=0 = "q−1 k −1 v YY Φv v−1 X ! kl ) r l=1 m − p(j + v=1 j=0 v−1 X kl ) l=1 !# P m−p( q−1 l=1 kl ) P q−1 Lkq q (r m−p( l=1 # kl ) ) kl ) ) On the other hand, from (11) we have kq −1 P q−1 Lkq q (r m−p( l=1 kl ) ) = Y Φq (m − p( j=0 q−1 X P q−1 kl ) − pj)r m−p( l=1 kl )−pkq l=1 . Thus, "q−1 k −1 v YY Φv Lkq q ...Lk22 Lk11 (r m ) = m − p(j + v=1 j=0 = "q−1 k −1 v YY Φv m − p(j + Φq m − p( j=0 = " q k −1 v YY v−1 X kl ) !# l=1 kq −1 × kl ) !# l=1 v=1 j=0 Y v−1 X q−1 X kl ) − pj l=1 Φv m − p(j + v=1 j=0 v−1 X l=1 ! kl ) P q−1 Lkq q (r m−p( P q−1 r m−p( !# l=1 kl )−pkq Pq r m−p( l=1 l=1 kl ) . Hence the proof is completed. Since for any fixed v, the roots of the quadratic equation ! v−1 X Φv m − p(j + kl ) = 0 l=1 are p Pv−1 (1) m = p(j + k ) − ψ + ψv 2 − γv l v j,v l=1 we can rewrite (12) as (13) p m(2) = p(j + Pv−1 kl ) − ψv − ψv 2 − γv j,v l=1 " q k −1 # v YY Pq (1) (2) Lkq q ...Lk22 Lk11 (r m ) = (m − mj,v )((m − mj,v ) r m−p( l=1 kl ) . v=1 j=0 (14) 514 A. Çetinkaya, N. Özalp / Central European Journal of Mathematics 3(3) 2005 508–515 Hence, we see that for each integer v, the functions (1) (2) u = r mj,v , u = r mj,v (j = 1, 2, ..., kv − 1), kq k2 k1 are solutions of the iterated equations Lq ...L2 L1 u = 0. Since the operator Lv is linear for each v, by the superposition principle, the function u= kX v −1 (1) (1) (2) (2) Aj,v r mj,v + Aj,v r mj,v j=0 k (1) (2) is a complete solution of the iterated equation Lq q ...Lk22 Lk11 u = 0. Here Aj,v and Aj,v are arbitrary constants. Now let us define three auxiliary functions as 1, if ψ 2 − γv > 0 v Λ1,v = , 0, else 1, if ψ 2 − γv = 0 v Λ2,v = , 0, else 1, if ψ 2 − γv < 0 v Λ3,v = . 0, else Hence, by generating the real valued solutions with similar arguments of the case Lk u = 0, we can give the following result: k Theorem 3.2. Real valued r m type solutions of the iterated equation Lq q ...Lk22 Lk11 u = 0 is given by the formula u= q k−1 X X Λ1,v v=1 j=0 + q k−1 X X (2) (1) (2) (1) Aj r mj,v + Aj r mj,v Λ2,v r p(j+ P v−1 kl )−ψv Bj + Bj ln r Λ3,v r p(j+ P v−1 kl )−ψv Cj cos v=1 j=0 + q k−1 X X v=1 j=0 (i) (i) (i) where Aj , Bj , Cj 4 l=1 l=1 (1) (1) (2) (15) hp i hp i (2) γv − ψv2 ln r + Cj sin γv − ψv2 ln r (i = 1, 2) are arbitrary constants. Conclusion Theorem 3.2 gives the complete solutions of the iterated equations (3) which includes a wide range of elliptic type equations with equidimensional equations. Thus, we can compute the analytical (symbolic) solutions of (3) by using (15) in a suitable algorithm. 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