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Analytical properties of Graetz modes in parallel and concentric configurations

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(1)Open Archive Toulouse Archive Ouverte OATAO is an open access repository that collects the work of Toulouse researchers and makes it freely available over the web where possible. This is an author’s version published in: https://oatao.univ-toulouse.fr/26478. Official URL : https://doi.org/10.1007/s11012-020-01192-4. To cite this version: Pierre, Charles and Plouraboué, Franck Analytical properties of Graetz modes in parallel and concentric configurations. (2020) Meccanica, 55. 1545-1559. ISSN 0025-6455. Any correspondence concerning this service should be sent to the repository administrator: tech-oatao@listes-diff.inp-toulouse.fr.

(2) Analytical properties of Graetz modes in parallel and concentric configurations Charles Pierre . Franck Plouraboue´. Abstract The generalized Graetz problem refers to stationary convection–diffusion in uni-directional flows. In this contribution we demonstrate the analyticity of generalized Graetz solutions associated with layered domains: either cylindrical (possibly concentric) or parallel. Such configurations are considered as prototypes for heat exchangers devices and appear in numerous applications involving heat or mass transfer. The established framework of Graetz modes allows to recast the 3D resolution of the heat transfer into a 2D or even 1D spectral problem. The associated eigenfunctions (called Graetz modes) are obtained with the help of a sequence of closure functions that are recursively computed. The spectrum is given by the zeros of an explicit analytical series, the truncation of which allows to approximate the eigenvalues by solving a polynomial equation. Graetz mode computation is henceforth made explicit and can be performed using standard software of formal calculus. It permits a direct and mesh-less computation of the. C. Pierre Laboratoire de Mathe´matiques et de leurs Applications, UMR CNRS 5142, Universite´ de Pau et des Pays de l’Adour, Pau, France e-mail: charles.pierre@univ-pau.fr F. Plouraboue´ (&) Institut de Me´canique des Fluides de Toulouse (IMFT), CNRS, INPT, UPS, Universite´ de Toulouse, Alle´e du Professeur Camille Soula, 31400 Toulouse, France e-mail: fplourab@imft.fr. resulting solutions for a broad range of configurations. Some solutions are illustrated to showcase the interest of mesh-less analytical derivation of the Graetz solutions, useful to validate other numerical approaches. Keywords Heat and mass transfer  Convection– diffusion  Reduced problem  Separation of variables  Analytical solutions. 1 Introduction Parallel convective heat exchangers are relevant in many application contexts such as heating/cooling systems [23], dialysis’s [9], as well as convective heat exchangers [14]. A number of works devoted to parallel convective heat exchangers in simple two dimensional configurations [11, 12, 15, 16, 24, 25, 27, 28] can be found to cite only a few, whilst many others can be found in a recent review [6]. As quoted in [6] conjugate heat transfer are mixed parabolic/hyperbolic problems which makes them numerically challenging. In many applications the ratio between the solid and fluid thermal conductance is high (larger than one thousand in many cases). The convection is dominating, so that the ratio of convection to diffusion effects provided by the so-called Pe´clet number is very high (e.g. larger than 105 in.

(3) [20, 21]). When dealing with such highly hyperbolic situations, numerical convergence might be an issue. The increase in computer power has permitted and popularized the use of direct numerical simulations to predict heat exchangers performances [7, 13, 20, 21, 26]. The derivation of analytic mesh-less reference solutions allows to evaluate the accuracy and the quality of the discrete solutions, as done in [2, 5, 8, 17, 18] in a finite-element framework. In most cases, it is interesting to validate the numerical solution in simple configurations as well as being able to test the solution quality for extreme values of the parameters, when rapid variations of the temperature might occur in localized regions. However, few analytic solutions are known, apart from very simplified cases. Namely, such analytic solutions can be obtained for axi-symmetric configurations, when the longitudinal diffusion has been neglected whilst assuming a parabolic velocity profile, as originally studied by Graetz [10]. In this very special case, the Graetz problem maps to a Sturm–Liouville ODE class, and the resulting analytic solutions can be formulated from hyper-geometric functions, see [4] or for example [25]. In this contribution we introduce analytic generalized Graetz modes: including longitudinal diffusion, for any regular velocity profile, and for general boundary conditions. The derivation of the generalized Graetz modes follows an iterative process that can be performed using a standard formal calculus software. Then, Sect. 2.1 sets notations (mainly for the cylindrical case) and provides the physical context as well as the constitutive equations under study. Section 2.2 gives the necessary mathematical background for the subject, with an emphasis on most recent results useful for the presented analysis. Section 3.1 shows that discrete mode decomposition also holds for non-axi-symmetric configuration. Section 3.3 gives the central result of this contribution regarding the analyticity of the generalized Graetz modes. Finally Sect. 4 illustrate specific applications obtained with the method with explicit analytic computations.. 2 Setting the problem 2.1 Physical problem We study stationary convection–diffusion in a circular duct made of several concentric layers (fluid or solid). The domain is set to X  ða; bÞ with ða; bÞ  R an interval and X the disk with center the origin and radius R. The longitudinal coordinate is denoted by z and cylindrical coordinates ðr; uÞ are used in the transverse plane. Then X is split into m different compartments Xj , j ¼ 1. . .m, either fluid or solid and centered on the origin: X1 is the disk of radius r1 whereas Xj , j  2, is the annular with inner and outer radius rj1 and rj for a given sequence 0\r1 \    \rm ¼ R. Two such configurations are depicted on Fig. 1. The physical framework is set as follows: 1. Velocity: vðr; u; zÞ ¼ vðrÞ ez with ez the unit vector along the z direction. We denote vj ¼ vjXj ¼ vj ðrÞ ez the restriction of the velocity to compartment Xj . In case this compartment is solid we have vj ðrÞ ¼ 0. We make the mathematical assumption that each vj ðrÞ is analytic, though v(r) is allowed to be discontinuous at each interface. 2. Conductivity: kðr; u; zÞ ¼ kðrÞ and moreover kjXj ¼ kj [ 0 is a constant. The general equation for stationary heat convection–diffusion reads. Fig. 1 Two possible configurations. Above: fluid flowing inside a circular tube with a solid wall. Below: fluid flowing inside an annular between a solid core and a solid external wall.

(4)   divðr;u;zÞ vT  krðr;u;zÞ T ¼ 0: With the assumptions we have made, it simplifies to divðkrTÞ þ ko2z T ¼ voz T. in X  ða; bÞ;. ð1Þ. where we denoted by div ¼ divðr;uÞ and r ¼ rðr;uÞ the gradient and divergence operators restricted to the transverse plane. The following boundary conditions, either of Dirichlet or Neumann type, are considered T ¼ gðzÞ. or krT ¼ gðzÞ. on oX  ða; bÞ: ð2Þ. 2.2 Mathematical background Problem reformulation Adding a supplementary vector unknown p: X ! R2 , problem (1)–(2) has been reformulated in [2, 8, 17, 18] into a system of two coupled PDEs of first order: oz W ¼ AW with W ¼ ðT; pÞ;  1   k1 divðÞ vk ; A¼ kr 0 on the space H ¼ L2 ðXÞ  ½L2 ðXÞ2 and involving the differential operator A: DðAÞ  H ! H. The definition of the domain D(A) of the operator A depends on the chosen Dirichlet or Neumann boundary condition. For simplicity we briefly recall the properties of operator A in the Dirichlet case, as presented in [8, 18]. These properties have been extended to the Neumann case in [17] and to the Robin case in [3]. For a Dirichlet boundary condition, we set DðAÞ ¼ H10 ðXÞ H div ðXÞ. Then A is self-adjoin with compact resolvent. Apart from the kernel space K :¼ kerA ¼ fð0; pÞ; p 2 H div ðXÞ; div p ¼ 0g the spectrum of A is composed of a set K of eigenvalues of finite multiplicity. It has been shown in [18] that K decomposes into a double sequence of eigenvalues ki , 1.  ki      k1 \0\k1 .     ki ! þ1:. ð3Þ. We call upstream eigenvalues the positive eigenvalues fki ; i\0g and downstream eigenvalues the negative ones fki ; i [ 0g. The associated eigenfunctions ðWi Þi2ZH form an orthogonal (Hilbert) basis of K ? . Eigenmodes Let us write Wi ¼ ðHi ; pi Þ the eigenfunctions. Their vector component satisfies. pi ¼ krHi =ki . It is important to understand that Hi : X7!R only is the scalar component of the associated eigenfunction Wi . As a result the ðHi Þi2ZH are not eigenfunctions themselves, they are neither orthogonal nor form a basis of L2 ðXÞ. To clarify this distinction we refer to Hi as an eigenmode associated with ki . Eigenmodes can be directly defined through a generalized eigenvalue problem. A function H: X ! R is an eigenmode if H 2 H1 ðXÞ, krH 2 H div ðXÞ and their exists a scalar k so that div ðkðrÞrHÞ þ k2 kðrÞH ¼ kvðrÞH on X;. ð4Þ. with H ¼ 0 or rH  n ¼ 0 on oX depending on the considered Dirichlet or Neumann boundary condition. In that situation, k is an eigenvalue of A associated with the eigenfunction Wi ¼ ðH; krH=kÞ. As a consequence, the eigenmodes always are real functions since the operator A is symmetric. The upstream and downstream eigenmodes have the following important property (proved in [8]): • The upstream eigenmodes fHi ; i\0g form a (Hilbert) basis of L2 ðXÞ. • The downstream eigenmodes fHi ; i [ 0g also form a basis of L2 ðXÞ. Problem resolution The problem (1)–(2) can be solved by separation of variables. General solutions for non-homogeneous boundary conditions of Dirichlet, Neumann or Robin type have been derived in [2, 3, 8, 17, 18]. Such solutions are detailed in Sect. 4. We simply recall their formulation for a homogeneous Dirichlet boundary condition: X ci ðzÞHi ðr; uÞ eki z : Tðr; u; zÞ ¼ i2ZH. The functions ci ðzÞ are determined with the help of the eigenmodes, of the boundary condition g(z) and of the inlet/outlet conditions. As an illustration, we precise that derivation in two cases. In the case of a homogeneous boundary condition gðzÞ ¼ 0 in (2), then ci ðzÞ ¼ ci 2 R are constant scalars. On a semiinfinite domain X  ð0; þ 1Þ, the upstream coefficients are zero, ci ¼ 0 for i\0, and.

(5) Tðr; u; zÞ ¼. X i2Z. ci Hi ðr; uÞ eki z :. þ. The coefficients ci for i [ 0 are given by the inlet condition T i ¼ Tjz¼0 X Ti ¼ ci Hi : i2Z. þ. If the domain is finite, equal to X  ð0; LÞ, then the upstream coefficients are no longer equal to zero, the upstream and downstream coefficients ci satisfy X X Ti ¼ ci Hi þ ci Hi eki L ; i2Z. i2Zþ. To ¼. X. ci Hi eki L þ. X. Tn;k ðrÞ r n. as. r ! 0þ :. where T o ¼ Tjz¼L is the outlet condition.. ð7Þ. An eigenmode H associated with the eigenvalue k decomposes as a finite sum of terms of the form Tn;k ðrÞ cosðnuÞ or Tn;k ðrÞ sinðnuÞ. The eigenvalue set K decomposes in the Dirichlet case as [   Kn ; Kn ¼ k 2 C; Tn;k ðRÞ ¼ 0 ; K¼ ð8Þ n2N. and in the Neumann case as  [ K¼ Kn ; Kn ¼ k 2 C;. ci Hi ;. i2Z. i2Zþ. Lemma 1 For all k 2 C and all n 2 N there exists a unique function Tn;k ðrÞ: ð0; RÞ ! R that satisfies (5)– (6) together with the normalization condition. n2N. d Tn;k ðRÞ ¼ 0 dr. ð9Þ. Finally, if k 2 Kn , then the associated eigenmodes are Tn;k ðrÞ cosðnuÞ and Tn;k ðrÞ sinðnuÞ.. 3 Analyticity of the generalized Graetz modes 3.1 Series decomposition To take advantage of the azimuthal symmetry of the physical problem we perform the Fourier decomposition of the eigenmodes. Their Fourier series expansion is composed by terms of the form TðrÞ cosðnuÞ or TðrÞ sinðnuÞ. We prove here that we have a finite number of such terms and characterize T(r). Let us introduce the operator Dn   1d d n2 r f  2 f: Dn f ¼ r dr dr r Consider H an eigenmode associated with k 2 K and assume that Hðr; uÞ ¼ TðrÞ cosðnuÞ or Hðr; uÞ ¼ TðrÞ sinðnuÞ. Then T is a solution of the following ODEs k2 kj T þ kj Dn T ¼ kvj T;. on. ðrj1 ; rj Þ;. that are coupled with the transmission conditions kj. d d Tðrj Þ ¼ kjþ1 Tðrjþ Þ; dr dr. • for n [ 0, one solution is Oðr n Þ at the origin and the second is Oðrn Þ, • for n ¼ 0, one solution is O(1) at the origin and the second is OðlogðrÞÞ,. j ¼ 1. . .m; ð5Þ. Tðrj Þ ¼ Tðrjþ Þ;. Proof of Lemma 1 The well posedness of the function Tn;k definition is obtained by induction on the intervals ½rj1 ; rj . Assume that Tn;k is given on ½rj1 ; rj  for some j  1. On ½rj ; rjþ1  the ODE (5) is regular and has a space of solution of dimension two, therefore Tn;k is uniquely determined by the two initial conditions (6). Now on ½0; r1 : the ODE (5) is singular at r ¼ 0. The Frobenius method (see e.g. [22]), with the assumption that v(r) is analytic on ½0; r1 , states that the space of solutions is generated by two functions whose behavior near r ¼ 0 can be characterized:. Therefore condition (7) ensures existence and uniqueness for Tn;k . Let H be an eigenmode for k 2 K. On each subdomain Xj , Eq. (4) can be rewritten as. j ¼ 1. . .m  1:. ð6Þ. DH ¼.  1 kvj ðrÞH  k2 H : kj. Using the assumption that vj ðrÞ is analytic on ½rj1 ; rj , elliptic regularity properties imply that H 2 C1 ðXj Þ..

(6) Moreover, since H 2 H1 ðXÞ and krH 2 H div ðXÞ, it follows that H and krH  n are continuous on each interface between Xj and Xjþ1 . We consider the Fourier series expansion for H X hn ðrÞeinu : H¼ n2Z. Sect. 3.2.1 and their construction with the help of closure problems is given in Sect. 3.2.2. A consequence is that the spectrum in (8) and (9) are given by the zeros of the following analytical series ( ) [ X p K¼ Kn ; Kn ¼ k 2 C; cn;p k ¼ 0 ; n2N. p2N. 1. Since H 2 C ðXj Þ we can differentiate under the sum to obtain X Dn ðhn ðrÞÞeinu : DH ¼ n2Z. and so Eq. (4) ensures that each Fourier mode hn ðrÞ satisfies the ODEs (5). It also satisfies the transmission conditions (6) because of the continuity of H and of krH  n at each interface. We already studied the behavior of the solution of (4) at the origin. Among the two possible behaviors characterized by the Frobenius method, H 2 H1 ðXÞ and rH 2 L2 ðXÞ ensure that hn ðrÞ ¼ Oðr jnj Þ. As a result we have hn ðrÞ ¼ ajnj Tjnj;k ðrÞ. Finally, H being a real function, we can recombine the Fourier modes to get, X X bjnj Tn;k ðrÞ cosðnuÞ þ cjnj Tn;k ðrÞ sinðnuÞ: H¼ n0. n[0. We also proved that each term Tn;k ðrÞ cosðnuÞ or Tn;k ðrÞ sinðnuÞ itself is an eigenmode for k which obviously are linearly independent. But each eigenvalue k 2 K being of finite multiplicity, the sums above are finite. h. ð11Þ where the coefficients cn;p are given by cn;p ¼ tn;p ðRÞ in the Dirichlet case or by cn;p ¼ drd tn;p ðRÞ in the Neumann case. In practice: 1. By truncating the series in Eq. (11) at order M, we can compute approximate eigenvalues by searching the zeros of the polynomial in k PM p p¼0 cn;p k ¼ 0. 2. If k is an approximate eigenvalue, the correspondP ing approximate eigenmode is M tn;p ðrÞkp . p¼0. For more simplicity we fix in the sequel the value of n 2 N and denote tn;p ¼ tp and Tn;k ¼ Tk . 3.2.1 Definition We consider the ODEs, for j ¼ 1. . .m, kj Dn tp þ kj tp2 ¼ vðrÞtp1. on ðrj1 ; rj Þ;. ð12Þ. together with the transmission conditions for j ¼ 1. . .m  1, tp ðrjþ Þ ¼ tp ðrj Þ;. kj. d d tp ðrjþ Þ ¼ kjþ1 tp ðrj Þ; dr dr ð13Þ. 3.2 Closure functions and the normalization condition at the origin, Assuming the following decomposition: X Tn;k ðrÞ ¼ tn;p ðrÞkp ; p2N. lim ð10Þ. and formally injecting this expansion into problem (5) provides recursive relations on tn;p ðrÞ, kj Dn tn;p þ kj tn;p2 ¼ vðrÞtn;p1 : which allows an explicit analytic computation of the functions tn;p ðrÞ. We prove in Sect. 3.3 that such a decomposition exists. The functions tn;p are called the closure functions. They are precisely defined in. r!0. tp ðrÞ ¼ 0: rn. ð14Þ. Lemma 2 Setting t1 ¼ 0 and t0 ¼ r n , then the closure functions ðtp ðrÞÞp  1 satisfying (12)–(14) for p  1 are uniquely defined. The proof is set-up by construction in Sect. 3.2.2..

(7) X. 3.2.2 Construction. Tn;k ðrÞ ¼. We assume that for some p  1, tp2 ðrÞ and tp1 ðrÞ are known. We hereby derive tp ðrÞ. Let us first introduce the operators Fj for j ¼ 1; . . .m, defined for a function f Z r Z x 1 n ynþ1 f ðyÞ dydx; Fj ½f ðrÞ :¼ r ð15Þ 2nþ1 rj1 x rj1. Xd d Tn;k ðrÞ ¼ tn;p ðrÞkp ; on ½rj1 ; rj ; j ¼ 1. . .m; dr dr p2N. tn;p ðrÞkp ; on ½0; R. p2N. which is the inverse of operator Dn . We denote w1 ðrÞ ¼ r n and w2 ðrÞ ¼ r n if n [ 0 or w2 ðrÞ ¼ lnðrÞ if n ¼ 0, that are the basis solution of Dn f ¼ 0. We consider the right hand side fp1 v fp1 :¼ tp1  tp2 : k. ð16Þ. Then on each compartment ðrj1 ; rj Þ, tp ðrÞ is solution of (12) and therefore reads, tp ðrÞ ¼ aj w1 ðrÞ þ bj w2 ðrÞ þ Fj ½fp1 ðrÞ: We finally show how to compute the constants aj and bj . First compartment ½0; r1  Assume that tp1 ¼ Oðr n Þ and fp1 ¼ Oðr n Þ at r = 0, which is true for p ¼ 1. We get that F1 ½fp1  ¼ Oðr nþ2 Þ and the normalization condition (13) sets a1 ¼ b1 ¼ 0. We then have, tp ðrÞ ¼ F1 ½fp1 ðrÞ. on ½0; r1 :. ð17Þ. It follows that tp ¼ Oðr nþ2 Þ ¼ Oðr n Þ and fp ¼ Oðr n Þ. Further compartments ½rj ; rjþ1 , j  1 We assume that tp ðrÞ has been computed on the compartment ½rj1 ; rj  and determine tp ðrÞ on ½rj ; rjþ1 , j  1. We clearly have Fjþ1 ½f ðrj Þ ¼ 0 and drd Fj ½f ðrj Þ ¼ 0. Then Eq. (13) at rj reformulates as aj w1 ðrj Þ þ bj w2 ðrj Þ ¼ tp ðrj Þ d d kj d tp ðrj Þ; aj w1 ðrj Þ þ bj w2 ðrj Þ ¼ kjþ1 dr dr dr. which equation has a unique solution since w1 and w2 form a basis for the solutions of the homogeneous equation Dn f ¼ 0. 3.3 Series expansion of the eigenmodes Our main result is the following.. where the ðtn;p ðrÞÞp2N are the closure functions introduced in the previous section. 3.3.1 Proof of Theorem 1 We fix the value of n 2 N and simply denote tn;p ¼ tp and Tn;k ¼ Tk . Assume that the three functions Tk ðrÞ, drd Tk ðrÞ and Dn Tk ðrÞ are analytic for r 2 ½rj1 ; rj  and k 2 C. We P can write Tk ðrÞ ¼ p  0 sp ðrÞkp . The derivation theP orem imply that drd Tk ðrÞ ¼ p  0 drd sp ðrÞkp and that P Dn Tk ðrÞ ¼ p  0 Dn sp ðrÞkp . Injecting this in (5) shows the sp ðrÞ satisfy (5). Similarly the transmission and normalization conditions (6)–(7) imply that the sp ðrÞ satisfy (13)–(14). Uniqueness in Lemma 2 then imply that sp ðrÞ ¼ tp ðrÞ. Let us then prove that Tk ðrÞ, drd Tk ðrÞ and Dn Tk ðrÞ are analytic for r 2 ½rj1 ; rj  and k 2 C for all j ¼ 1. . .m. We proceed by induction. Assume that this is true on ½rj1 ; rj . Then the initial data k ! Tk ðrj Þ and k ! or Tk ðrj Þ are analytic. On ½rj ; rjþ1 , Tk is the solution of the regular ODE (5) that analytically depends on k, r and whose initial conditions (6) at rj also analytically depend on k. Classical results on ODEs (see e.g. [1, section 32.5]) state that Tk ðrÞ analytically depends on k and r on ½rj ; rjþ1 . This is also true for Dn Tk since Dn Tk ¼ k2 Tk þ kv=kTk . Finally this is also true for drd Tk by integration. It remains to prove the result for r 2 ½0; r1 . This is harder because of the singularity at r ¼ 0. The problem being local at r ¼ 0, we can assume r1  1: We formally introduce the series, X tp ðrÞkp ; Ak ðrÞ ¼ p0. Xd tp ðrÞkp ; dr p0 X Dn tp ðrÞkp : Ck ðrÞ ¼ Bk ðrÞ ¼. p0. Theorem 1. The functions Tn;k satisfy,. Let us denote F½f  ¼ F1 ½f  for F1 ½f  defined in (15). We introduce F ðiÞ ¼ F . . . F the ith iterate of.

(8) F. Let us define si ¼ F ðiÞ ½t0  for t0 ðrÞ ¼ r n the 0th closure function. It is easy to compute si , si ðrÞ ¼ Ki r nþ2i ;. Ki1 ¼ 22i i!ði þ 1Þ. . .ði þ nÞ: ð18Þ. We consider the constant M ¼ maxðkv=kk1 ; 1Þ  1. If r1  1, then on ½0; r1  we have,. d. jtp ðrÞj  ap ; tp ðrÞ.  ap ; jDn tp ðrÞj  ap : dr. Lemma 3. with ap ¼ ð2MÞp Ki1 for p ¼ 2i or p ¼ 2i þ 1. With definition (18) of the coefficients Ki , it is clear P that the series p  0 ap kp converges over C. The three series Ak ðrÞ, Bk ðrÞ and Ck ðrÞ therefore are normally converging for r 2 ½0; r1  and for k in any compact in C. As a result the integration theorem implies that Bk ¼ or Ak and Ck ¼ Dn Ak . Relation (12) ensures that Ak satisfies (5) whereas relation (14) together with t0 ¼ r n ensures that Ak satisfies (7). Uniqueness in Lemma 1 then implies that Ak ¼ Tk . This proves Theorem 1 on [0, R] and ends this proof. Proof of Lemma 3 We will systematically use that r  1, that Ki and si ðrÞ in (18) are decreasing and that the operator F satisfies, h1  h2 ) F½h1   F½h2 ;. jF½hj  F½jhj:. From that last inequality it is easy to check that jtp j þ jtp1 j  2ð2MÞp Ki r nþ2i if p ¼ 2i or p ¼ 2i þ 1. For p ¼ 2i or p ¼ 2i þ 1 it follows that   fp ¼ jDn tpþ1 j  M jtp j þ jtp1 j  ð2MÞpþ1 Ki r nþ2i : This gives the third inequality in Lemma 3. By differentiating (17) we get, Z r Z x d 1 n1 tpþ1 ðrÞ ¼nr ynþ1 fp ðyÞ dydx 2nþ1 dr 0 x 0 Z 1 r nþ1 þ n y fp ðyÞ dy r 0 It follows that. d. tpþ1 ðrÞ  ð2MÞpþ1 Ki C;. dr. with, C ¼ nr. n1. 1 þ n r  nr n1 þ. 1 rn. Z. r. 0 r. Z. 0. dy. Z. 0. 1 x2nþ1. 0. y2nþ2iþ1 dydx. 2nþ2iþ1. y r. x. x2nþ1. 0. Z. Z. 1. Z. x. y2n dydx. 0. r. y2n dy ¼. nr n þ r nþ1  1; 2n þ 1. implying the second inequality in Lemma 3. h. With definitions (16)–(17) we have the upper bound, jtp j  F½jfp1 j  MðF½jtp1 j þ F½jtp2 jÞ: By recursion, we obtain an upper bound involving the si ¼ F ðiÞ ðt0 Þ of the form X M nk smk : jtp j  k. The number of terms in the sum is less than 2p . Index nk is smaller than p and M nk  M p . The minimal value for mk is i if p ¼ 2i or i þ 1 if p ¼ 2i þ 1, so that smk  si or smk  siþ1 respectively. Therefore,  if p ¼ 2i ð2MÞp Ki r nþ2i jtp j  p nþ2ðiþ1Þ ð2MÞ Kiþ1 r if p ¼ 2i þ 1;. 3.4 Extension to planar configurations We consider layered planar configurations as depicted on Fig. 2. The transverse coordinate perpendicular to the layers is denoted by x. The coordinate x is homologous to the radial coordinate r in the cylindrical case. The origin is set at the center so that R  x  R with 2R the total thickness of the geometry. Actually, the results that we obtained for concentric cylindrical configurations are easier to establish in the. which upper bound ensures the first inequality in Lemma 3.. Fig. 2 Example of a planar configurations.

(9) case of layered planar configurations. This is because  d2  2 the operator Dn :¼ dx associated with the y2 þ n periodic decomposition Hðx; yÞ ¼. X. Tn;k ðxÞ cosðn2pyÞ þ. n0. X. k i and T i depend on the nature of the boundary condition (Dirichlet or Neumann). 4.1.1 Dirichlet boundary condition. Tn;k ðxÞ sinðn2pyÞ;. n[0. is no more singular in Cartesian coordinates. Hence, the technical issues associated with the proof of analyticity in the variable k for the functions Tk , dTk = dr and Dn Tk are no longer present in this case. Furthermore, each step of the proofs provided in Sects. 3.1 and 3.2 directly apply to the planar case, so that Theorem 1 also holds.. For the lateral Dirichlet boundary condition in Eq. (2), the temperature solution are given in [2] for the cylindrical case X ai ci ðzÞTi ðrÞ eki z ; Tðr; zÞ ¼ gðzÞ þ i2ZH. with, denoting k the conductivity in the boundary annular: ai ¼. 4 Examples of applications In this section we develop various examples of solutions so as to illustrate the versatility and usefulness of the previously presented theoretical results. In Sect. 4.1 we first give explicit general solutions adapted for two families of geometries, i.e planar or cylindrical, for general boundary conditions. We pursue towards illustrating interesting and relevant solutions considering two idealized but non trivial configurations in the subsequent sections. In Sect. 4.2 we showcase how a localized heat source can lead to a ‘hot spot’ of temperature in its neighborhood, and illustrate how our mesh-less analytic method can effectively capture the temperature peak. A second example is provided in Sect. 4.3 where we examine a double-pass configuration in the planar framework for which, again, a localized heat source is imposed nearby the origin. 4.1 Explicit families of solutions As in Eq. (2), we will consider symmetric boundary conditions (only depending on z). Thus we will consider the spectrum K0 in definitions (8)–(9) for   n=0. In the Dirichlet case K0 ¼ k 2 C;  T0;k ðRÞ ¼ 0 and in the Neumann case K0 ¼ k 2 C; dT0;k = drðRÞ ¼ 0g. The spectrum is computed with the closure functions as in Eq. (11). It decomposes as in Eq. (3): K0 ¼ fkþi ; ki ; i 2 NH g with kþi \0 the upstream modes and ki [ 0 the downstream modes. We will simply denote T i ¼ Tk i;0. Remember that. 2pR dTi ðRÞ: k dr k2i. This adapts to the parallel planar configuration with

(10) k dTi dTi ðRÞ þ ðRÞ ai ¼ 2 dr ki dr In both cylindrical and planar cases, the functions ci ðzÞeki z are given by the convolution between dg= dz and the exponentially decaying modes Z þ1 ci ðzÞ ¼ g0 ðnÞeki n dn z ð19Þ Z z cþi ðzÞ ¼  g0 ðnÞekþi n dn; 1. for the upstream modes and downstream modes respectively. 4.1.2 Neumann boundary condition and nonbalanced case Consider now a Neumann boundary conditions (2) in R the case where Q :¼ X vdx 6¼ 0, i.e. the total convective flux is not zero. Then from [2] the solution reads X P Tðr; zÞ ¼ GðzÞ þ ai ci ðzÞTi ðrÞ eki z ; ð20Þ Q i2ZH. Rz. with GðzÞ ¼ 1 gðnÞdn the primitive of the heat source g(z) and P the perimeter of the external cylinder. Note that the temperature indeed is defined up to an additive constant that has been fixed by setting T1 ¼ 0 here. For the cylindrical configuration, we choose a Poiseuille velocity profile vðrÞ ¼ Peð1  ðr=r0 Þ2 Þ,.

(11) where Pe is the Pe´clet number that quantifies the ratio between convection and diffusion (here based on the maximal velocity in the tube). We have P=Q ¼ 4R=ðPer02 Þ and 2pR ai ¼ Ti ðRÞ: ki. ð21Þ.  1 Ti ðRÞ þ Ti ðRÞ : ki. ð22Þ. In both cases, the functions ci ðzÞeki z are given by the convolution between the imposed flux at the boundary and the exponentially decaying modes ci ðzÞ ¼. Z. þ1. gðnÞeki n ;. cþi ðzÞ ¼ . Z. ðvT0  kÞr dr. z. gðnÞekþi n dn;. ; b¼. a2 R. Z. R. ð2k  vT0 ÞT0 r dr þ a T0 ðRÞ. 0. ð26Þ whereas for parallel planar configuration the parameters a and b read 2. ; ðvT0  kÞ dr Z R a ð2k  vT0 ÞT0 dr þ aðT0 ðRÞ þ T0 ðRÞÞ=2: b¼ 2 R ð27Þ 0 2. 4.2 Locally heated pipe and non-balanced case Q 6¼ 0. 1. z. ð23Þ for the upstream modes and downstream modes respectively. 4.1.3 Neumann boundary condition and balanced case Consider now a Neumann boundary conditions (2) in the case where the total convective flux cancels out: R Q :¼ X vdx ¼ 0. This is the case of a balanced exchanger. In this case, the solution displays a distinct form (see [2]) involving the (adiabatic) kernel T0 solution of div ðkrT0 Þ ¼ v ;. 0. R. a ¼RR. Whereas, for parallel planar configurations: ai ¼. a ¼ RR. rT0  njR ¼ 0:. ð24Þ. In the Sect. 4.3 we will consider an example of such a configuration for which we will give an explicit solution of the kernel T0 . In general form, the complete solution associated with balanced case Q ¼ 0, reads Tðr; zÞ ¼ aGðzÞ þ GðzÞðaT0 þ bÞ þ. X i2Z. ai ci ðzÞTi ðrÞ eki z ;. We illustrate the use of explicit computation of the eigenmode decomposition, through the recursive relations (12) and (13), in a simple and classical configuration: sometimes referred to as ‘generalized Graetz’ configuration. Two concentric cylinders are thus considered. A central one, for which r 2 ½0; r0  and whereby the fluid convects the temperature, and an external one, r 2 ½r0 ; R where temperature conduction occurs. The dimensionless axi-symmetric longitudinal velocity v(r) inside the inner cylinder is chosen such as vðrÞ ¼ Peð1  ðr=r0 Þ2 Þ, where Pe is the Pe´clet number which quantifies the ratio between convection and diffusion. The domain dimensions are r0 ¼ 1 and R ¼ 2. The conductivity is set to k ¼ 1. The solution is defined up to an additive constant that is fixed by setting T1 ¼ 0. A Neumann boundary condition krT ¼ gðzÞ is set. The applied boundary condition is chosen so as to present a localized (and regular) heat flux nearby the origin, with z0 ¼ 1=2 here: gðzÞ ¼ 1  cosð2pðz  z0 ÞÞÞ. H. ð25Þ Rz with GðzÞ ¼ 1 GðnÞdn, the second primitive of the heat source g(z), ai and ci ðzÞ again given by (20) and (23) and where a and b are two constants characterizing the heat exchange with values detailed below. Note that for this configuration the temperature field is defined up to C1 ðz þ T0 Þ þ C2 , see details in [2]. In cylindrical configuration the parameters a and b are given by. for. z 2 ½z0  1=2; z0 þ 1=2;. ð28Þ. and gðzÞ ¼ 0 otherwise. With these conditions, a simple balance on the domain allows to compute Tþ1 : R þ1 Z 1 2pR 1 gðzÞ dz 4R Rr Tþ1 ¼ ¼ gðzÞ dz; Pe r0 0 2p 0 0 vðrÞr dr so that Tþ1 ¼ 8=Pe here. Using Neumann boundary condition (28) and Eq. (20) one is able to provide a mesh-less explicit analytic solution for the.

(12) temperature, illustrated in Fig. 3 for various values of Pe varying between 100 to 0.1 so as to show-case the drastic effect of convection on the temperature profiles. Figure 3a exemplifies that, when convection dominates in the center line r ¼ 0, the effect of the heat source nearby the origin is weak. The local temperature is almost zero at r ¼ 0 for z 2 ½1; 0, since the prescribed temperature at z ! 1 is zero. Nevertheless, a slight tilt of the center line temperature profile is noticeable as z [ 0 so that it barely reaches the non-zero asymptotic downstream constant temperature Tþ1 at z ¼ 10. On the contrary to the center line profile, the wall profile at r ¼ R displays a strong deflection with a maximum located at the heat source maximum z ¼ 1=2, and both upstream and. (a). Pe=100. Temperature profiles inside a cylinder. 1.2. r=R r = (R + r0 )/2 r = r0 r = r0 /2 r=0. 1 0.8. T. 0.6 0.4 0.2. T+∞ = 0.08. 0. (b). −4 Pe=10. −2. 0. 2. 4. 1.5 1. T+∞ = 0.8. 0.5 0. (c). −4. −2. 0. 2. 4. 2. 4. z. Pe=1. 10 8. T+∞ = 8. T 6 4. (d) 80. T. −4. −2. 0. z. Pe=0.1 T+∞ = 80. 77.5 75 −4. 4.3 Parallel configuration and balanced case Q¼0. z. 2. T. downstream decay from this maximum. The typical downstream decay length is related to the convection ability to transport the heat flux downstream. Hence the larger the Pe´clet, the longer the downstream decay length. The upstream decay length, on the contrary both depends on the solid conduction and the wall radius. In the case of small solid walls thickness, some asymptotic behavior have been documented [19]. The other radially intermediate temperature profiles shown in Fig. 3a display a medium behavior between the center line and the wall profile. The closer to the outer cylinder wall, the closer the temperature peak to the wall profile. Figure 3b–d display the effect of decreasing the convection on the temperature profile. From one hand, these profiles display smoother and smaller peaks at the heat source as convective effects are weakened. On the other hand, the profiles are increasingly non-symmetric at smaller Pe´clet numbers, with an increasing downstream temperature Tþ1 ¼ 8=Pe.. −2. 0. 2. 4. z. Fig. 3 Temperature profiles at various radial distances from center r ¼ 0 to solid edge r ¼ R and for various Pe´clet numbers. An identical scaling in z has been set to focus on the heated region (dashed vertical lines). Away from the heated region, the temperature exponentially goes to T1 ¼ 0 when z ! 1 and to Tþ1 as z ! þ1. Here we consider a parallel planar geometry in a double-pass configuration for which the upper fluid is re-injected into the lower one at one end as in [12]. An exchanger with total thickness 2R is considered. A fluid is flowing for jxj  x0 surrounded by solid walls for x0  jxj  R. We consider the zero total flux for which the upper fluid is convected along þ z direction for x 2 ½0; x0 , and on the opposite one for x 2 ½ x0 ; 0. Within ½ x0 ; x0 , the velocity profile reads   jxj jxj ; ð29Þ 1 vðxÞ ¼ 6 rðxÞ Pe x0 x0 rðxÞ being the sign of x, with Pe´clet number Pe ¼ Rx vx0 =D (built from the average velocity v ¼ 0 0 v dx=x0 , x0 the fluid channel half-gap and the diffusivity D). At x ¼ R, adiabatic conditions are prescribed, (i.e rT  njR ¼ 0) for jzj [ 1=2 whereas the flux (28) (with zo ¼ 0 here) is imposed for z 2 ½1=2; 1=2. In this case the adiabatic kernel T0 solution of (24) is given by: for jxj  x0.

(13) T0 ðxÞ ¼ rðxÞPe.  x  3 x2 x  2x2 x0 þ 2x30  rðxÞPe 0 ; 2 2 2x0. ð30Þ whereas for jxj  x0 T0 ðxÞ ¼ rðxÞPex20 =2:. ð31Þ. The two constants a and b defined in (27) read a¼. 35 ; b ¼ 0: þ 35R. 13Pe2 x30. at the surface x ¼ R, is weakly affected by the increase of the Pe´clet number except for small Pe´clet (where one has to translate back the reference temperature chosen at 1, so as to obtain true physical ‘‘hot-spot’’ temperature). Nevertheless, further-down inside the solid the temperature rise is weakened by increasing fluid convection, as expected. Also, convection drops down the outlet temperature, as expected from heatflux balance argument.. ð32Þ. Figure 4 illustrates the temperature profiles along the longitudinal direction z at various transverse heights x, either in the center of the channel (x ¼ 0), at the interface between the liquid and the solid (x ¼ x0 ) or at the solid exterior edge (x ¼ R). One can observe that the ‘‘hot-spot’’ temperature located very close at z ¼ 0 (a). (b). 5 Conclusion This contribution has provided the mathematical proof, as well as the effective algorithmic framework for the computation of generalized Graetz mode decomposition in cylindrical or parallel configurations. We have shown that, in these special configurations, the Graetz functions analyticity enables meshless explicit computation of the steady-state temperature even when boundary condition with source terms are considered. The method has been illustrated in two complementary cases (cylindrical/non balanced and parallel/balanced) in order to showcase its various aspects. Most of the presented computations have required few minutes or less in a 8  3:2 GHz Intel processor running on a Linux station, with less than 5Go RAM. Compliance with ethical standards. (c). Conflict of interest The authors declare that they have no conflict of interest. Appendix Cylindrical heated pipe case Q 6¼ 0 (d). The solution provided by (20) is X 8 Tðr; zÞ ¼ GðzÞ þ ai ci ðzÞTi ðrÞ eki z ; Pe H. ð33Þ. i2Z. Rewritting (28) as     1 gðzÞ ¼ HðzÞHð1  zÞ 1  cos 2p z þ 2 Fig. 4 Temperature profile inside a parallel channel with counter-current flow (29) along z. A heat source term (28) is located within z 2 ½1=2; 1=2 (dotted lines). with H(z) the Heaviside function, and using.

(14) integration by parts leads to the primitive GðzÞ ¼ Rz 0 0 1 gðz Þdz equals to    1 1 : GðzÞ ¼ HðzÞHð1  zÞ z  sinð2p z þ 2p 2 The function ci ðzÞ in (33) are given by (23), the integration by part of which gives cþi ðzÞ ¼ gðzÞ.   eki z Hð1  zÞ k þ 2 sinð2pzÞ þ cosð2pzÞ : ki ki þ 4p2 2p. The eigenfunctions Ti are provided by the k-analytical decomposition (10) upon functions tp ðrÞ such that Ti ðrÞ ¼. Np X. tp ðrÞkpi ;. ð34Þ. where each eigenvalue ki of the discrete spectrum sets its eigenfunctions Ti from (34). Here, Neumann adiabatic boundary condition at R ¼ 2, combined with—truncated—decomposition (34) provide a— hence finite—polynomial condition for ki whose zeros are the approximated discrete spectrum. We hereby provide the first three elements of both downstream and upstream spectrum computed with finite truncation Np ¼ 20 in (34) and parameter Pe ¼ 1, with a formal calculus Maple software: k1 ¼ 0:674240, k2 ¼ 3:306258, k3 ¼ 4:936416, k1 ¼ 0, k2 ¼ 1:027741, k3 ¼ 2:35726. Function tp ðrÞ, p 2 f0; 5g are also hereby given by the following piece-wise continuous analytic functions of r along the fluid-solid domains r 2 ½0; 1 [ ½1; 2. p¼0. . r 2 ½0; 1. t0 ¼ 1. r 2 ½1; 2 8 > < r 2 ½0; 1. t0 ¼ 1. > : r 2 ½1; 2 8 > > < r 2 ½0; 1 > > : r 2 ½1; 2 8 > > < r 2 ½0; 1 > > : r 2 ½1; 2 8 > > < r 2 ½0; 1 > > : r 2 ½1; 2 8 > > < r 2 ½0; 1 > > : r 2 ½1; 2. 5 4 r þ 5=2 r 2 8 15 5 þ lnðr Þ t1 ¼ 8 2 1 25 r 4 125 r 6 25 r8 t2 ¼  r 2 þ  þ 16 144 256 4 2 1825 r 175 lnðr Þ  þ t2 ¼ 2304 4 96 5 r 4 25 r6 875 r 8 445 r 10 125 r 12 t3 ¼  þ  þ  16 48 2304 4608 18432 2 4385 5 r 155 lnðr Þ 5 2 þ þ  r lnðr Þ t3 ¼  18432 32 4608 8 r 4 25 r6 1325 r 8 839 r 10 10975 r 12 3175 r 14 625 r 16 t4 ¼  þ  þ  þ 64 192 9216 9216 331776 602112 2359296 2 319528919 2375 r 847715 lnðr Þ r 4 175 r 2 lnðr Þ  þ þ  t4 ¼  9216 64 1040449536 3096576 384 5 r 6 95 r 8 575 r 10 3755 r 12 51755 r 14 779375 r 16 3201125 r 18 125 r 20 t5 ¼  þ  þ  þ  384 3072 18432 221184 8128512 520224768 18728091648 18874368 2 2789680345 5005 r 9747175 lnðr Þ 15 r 4 155 r 2 lnðr Þ 5 r 4 lnðr Þ   þ  þ t5 ¼  512 74912366592 73728 231211008 18432 128 ð35Þ t1 ¼ .

(15) Finally, each parameter ai of (33) is given by (22) using the closure function Ti ðR ¼ 2Þ and its corresponding eigenvalue ki . Parallel configuration and balanced case Q ¼ 0 The theoretical solution detailed in Sect. 4.1.3 is hereby detailed. From (25) we recall the temperature solution X ai ci ðzÞTi ðrÞ eki z ; Tðr; zÞ ¼ aGðzÞ þ gðzÞaT0 þ i2ZH. ð36Þ involving the constant a given in (32) and the function g(z) given in (28). Rewritting (28) as     1 ; gðzÞ ¼ HðzÞHð1  zÞ 1  cos 2p z þ 2 with H(z) the Heaviside function, and using integraRz tion by parts leads to a primitive GðzÞ ¼ 1 gðz0 Þdz0 equals to     1 1 : GðzÞ ¼ HðzÞHð1  zÞ z  sin 2p z þ 2p 2 Again, the functions ci ðzÞ are given by (23), the integration by part of which gives cþi ðzÞ ¼ gðzÞ.   eki z Hð1  zÞ k þ 2 sinð2pzÞ þ cosð2pzÞ ki ki þ 4p2 2p. The eigenfunctions Ti are provided by the k-analytical decomposition (10) upon functions tp ðrÞ such that. 8 > r 2 ½2; 1 > > > > > > > > > < r 2 ½1; 0 > > > r 2 ½0; 1 > > > > > > > : r 2 ½1; 2. Ti ðrÞ ¼. Np X. tp ðrÞkpi ;. ð37Þ. p¼0. where each eigenvalue ki of the discrete spectrum sets its eigenfunctions Ti from (37). Here again, Neumann boundary condition at R ¼ 2, combined with— truncated—decomposition (37) provide a polynomial condition for ki the zeros of which are the approximated discrete spectrum. We hereby provide the five first elements of this spectrum computed with finite truncation Np ¼ 20 in (37) and parameter Pe ¼ 50, computed with a formal calculus Maple software. k1 ¼ 1:738793, k2 ¼ 1:738793, k3 ¼ 1:585275, k4 ¼ 1:3093020, k5 ¼ 1:011529. Function tp ðrÞ, p 2 f0; 5g are also hereby given by the following piece-wise continuous polynomial functions of r along the various solid-fluid domains ½2; 1 [ ½1; 0 [½0; 1 [ ½1; 2. Starting with t0 ¼ 1 identically equal to 1, we recursively compute the following (polynomial) functions tp ðrÞ 8 r 2 ½2; 1 t1 ¼ 0 > > > < r 2 ½1; 0 t1 ¼ 25 ðr  1Þð1 þ r Þ3 > r 2 ½0; 1 t1 ¼ 25 r 4 þ 50 r3  50 r  25 > > : r 2 ½1; 2 t1 ¼ 50 ð38Þ. Parameter ai of (36) is given by (22) using closure function Ti ðR ¼ 2Þ and its corresponding eigenvalue ki .. 1 ð r þ 2Þ 2 2 1347 2236 r r 2 3750 r 7 1875 r 8 þ þ   1250 r 3  1875 r 4  750 r 5 þ 500 r 6 þ t2 ¼ 2 7 14 14 7 7 1347 2236 r r 2 3750 r 1875 r8 þ t2 ¼ þ   1250 r 3  625 r 4 þ 750 r 5 þ 500 r 6  2 7 14 14 7 13014 r r 2 t2 ¼ 1248   2 7 t2 ¼ . ð39Þ.

(16) 8 r 2 ½2; 1 > > > > > > > r 2 ½1; 0 > > > > > > < r 2 ½0; 1 > > > > > > > > > > > > > : r 2 ½1; 2. t3 ¼ 0.   5ð1 þ rÞ3 11661  20261 r þ 96921 r 2 þ 226961 r 3 þ 8750 r4  362250 r5  322000 r 6  18500 r 7 þ 84375 r8 þ 28125 r 9 462 19435 19730 r 25r2 101200r3 78125r 4 33610r5 74965r6 31250r7 103125r8 3125r9 72500r10 t3 ¼ þ þ   þ þ    þ 2 21 14 7 6 7 14 3 21 154 33 11 12 140625r 46875r  þ 77 154 14580 t3 ¼  100 r þ 25 r2 11 t3 ¼. ð40Þ 8 > > r 2 ½2; 1 > > > > > > > > > r 2 ½1; 0 > > > > > > > > > < > > > r 2 ½0; 1 > > > > > > > > > > > > > > > > > : r 2 ½1; 2. 1 ðr þ 2Þ4 24 21071161 3288262 r 1347 r2 209989 r3 33452423 r4 95900 r5 2031875 r6 15973250 r 7 2275625 r8 2028125 r9    þ þ þ  t4 ¼ þ  28 33 1848 11 42 147 28 63 504504 9009 10 11 12 13 14 15 16 4179325 r 7640625 r 2265625 r 421875 r 60968750 r 234375 r 234375 r   þ þ þ þ  36 77 66 91 7007 77 616 21071161 3288262 r 1347 r2 209989 r 3 21791423 r 4 101400 r 5 2019625 r6 796750 r7 10902625 r 8 2018875 r 9   þ þ þ   t4 ¼þ þ  28 33 1848 11 42 147 196 63 504504 9009 10 11 12 13 14 15 16 14244725 r 609375 r 8828125 r 421875 r 60968750 r 234375 r 234375 r þ   þ  þ þ 252 77 462 91 7007 77 616 22888172 1164110834 r 2169 r3 2 þ  624 r þ t4 ¼ 7 1617 63063. t4 ¼. ð41Þ 8 r 2 ½2; 1 > > > > > > > r 2 ½1; 0 > > > > > > > > > > > > > > > > < r 2 ½0; 1 > > > > > > > > > > > > > > > > > > > > > > > : r 2 ½1; 2. t5 ¼ 0 5 ð1 þ r Þ3  1594383325  582590385 r  978868182 r 2 þ 74397416190 r3 þ 111713337741 r 4 þ 410289881841 r 5  1279496305500 r 6 162954792  741396373500 r 7 þ 1797598889250 r 8 þ 3506620554250 r 9 þ 1894060853250 r10  1117168905750 r11  2202785812500 r 12  1228317562500 r 13  156926250000 r 14 þ 140323125000 r15 þ 68527265625 r 16 þ 9789609375 r 17. t5 ¼. 7971916625 3500466325 r 19435 r 2 50174095 r 3 2038131125 r 4 25775835 r5 19508095 r 6 250061555 r 7 þ þ þ þ    162954792 27159132 308 22932 252252 4004 308 6468 132625865 r 8 37396250 r 9 251021875 r 10 269196250 r11 1040385625 r 12 170490000 r 13 74039375 r14 þ þ   þ þ  1176 231 1764 1617 19404 1001 924 62421875 r 15 434609375 r 16 7008984375 r17 4114843750 r 18 17578125 r 19 3515625 r 20  þ þ  þ  1617 24024 476476 357357 5852 11704 96144058760 83080 r 7290 r 2 50 r 3 25 r4 t5 ¼  þ  þ  20369349 33 11 3 12 t5 ¼. ð42Þ. References 1. Arnold V (1973) Ordinary differential equations, 10th edn. MIT Press, Cambridge 2. Bouyssier J, Pierre C, Plouraboue´ F (2014) Mathematical analysis of parallel convective exchangers with general lateral boundary conditions using generalized Graetz modes. Math Models Methods Appl Sci 24(04):627–665 3. Debarnot V, Fehrenbach J, de Gournay F, Martire L (2018) The case of Neumann, robin and periodic lateral condition for the semi infinite generalized Graetz problem and applications. arXiv preprint arXiv:1803.00834 4. Deen WM. Analysis of transport phenomena. Oxford University Press, New York 5. Dichamp J, Gournay FD, Plouraboue´ F (2017) Theoretical and numerical analysis of counter-flow parallel convective. 6. 7.. 8.. 9. 10. 11.. exchangers considering axial diffusion. Int J Heat Mass Transf 107:154–167 Dorfman A, Renner Z (2009) Conjugate problems in convective heat transfer. Math Probl Eng 2009:927350 Fedorov AG, Viskanta R (2000) Three-dimensional conjugate heat transfer in the microchannel heat sink for electronic packaging. Int J Heat Mass Transf 43(3):399–415 Fehrenbach J, De Gournay F, Pierre C, Plouraboue´ F (2012) The generalized Graetz problem in finite domains. SIAM J Appl Math 72:99–123 Gostoli C, Gatta A (1980) Mass transfer in a hollow fiber dialyzer. J Membr Sci 6:133–148 Graetz L (1885) Uber die Wa¨rmeleitungsfa¨higkeit von Flu¨ssigkeiten. Ann Phys 261(7):337–357 Ho C-D, Yeh H-M, Yang W-Y (2002) Improvement in performance on laminar counterflow concentric circular.

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