International Review of Chemical Engineering (I.RE.CH.E.), Vol. 4, N. 5 ISSN 2035-1755 September 2012 Special Section on Open Door Initiative (ODI) – 3rd edition An Exercise with the He’s Variation Iteration Method to a Fractional Bernoulli Equation Arising in Transient Conduction with Non-Linear Heat Flux at the Boundary
Jordan Hristov
Abstract – Surface temperature evolution of a body subjected to a nonlinear heat flux involving counteracting convection heating and radiation cooling has been solved by the variations iteration method (VIM) of He. The surface temperature equations comes as a combination of the time-fractional (half-time) subdiffusion model of the heat conduction and the boundary condition relating the temperature field gradient at the surface through the Riemann-Liouville fractional integral. The result of this equation is a Bernoulli-type ordinary fractional equation with a non- linear term of 4th order. Two approaches in the identification of the general Lagrange multiplier and a consequent application of VIM have been applied. The common method replaces the fractional integral (in the Riemann-Liouville sense) by an integer order integral. The more exact method of Wu uses an initial Laplace transform of the fractional integral in the iteration formula to find correctly the Lagrange multiplier. Both approaches yield different Lagrange multipliers which results in different numerical results.The article discusses the origin of these differences in the light of correct application of VIM. The developed approximate solutions have been used in numerical simulation showing the effect of Biot number and the radiation-conduction number on the surface temperature evolution. Copyright © 2012 Praise Worthy Prize S.r.l. - All rights reserved.
Keywords: Variational Iteration Method, Bernoulli-Like Fractional Equation, Lagrange Multiplier, Surface Temperature Evolution
Nomenclature Greek Letters α Fractional order, dimensionless a Thermal diffusivity, ms2 ε Emissivity of cooled surface, b Sample (slab) thickness, m dimensionless General Lagrange multiplier h Heat transfer coefficient, WmK2 λ (τ ) k Thermal conductivity, WmK λH Lagrange multiplier defined by the method of He (see also the articles 2 qts′′ () Surface flux density, Wm of S. Momani et al.) t Time, s λW Lagrange multiplier defined by the tba* = 2 Time scale (heat diffusion), s method of G. C. Wu [24], [25] (see Eq.(13c)) Ambient temperature, K Ta σ Stefan Boltzmann constant Reference temperature, K Tref Γ(•) Gamma function T Surface temperature, K s θ = TTs a Dimensionless temperature Initial temperature of the body, K T∞ θ (s) Laplace transform of the x Space co- ordinate, m dimensionless temperature θ y ()t Casual function ξ = x b Dimensionless space co-ordinate τ Dummy variable in the fractional Dimensionless Numbers integrals and derivatives Bi= bh k Biot number Subscripts *2Fourier number Fotttab== n Number of iteration 3 Radiation conduction number NbTk= σε a
Manuscript received and revised August 2012, accepted September 2012 Copyright © 2012 Praise Worthy Prize S.r.l. - All rights reserved
489
Jordan Hristov
Superscripts equation with zero initial condition. Now, we stress the C Cooling attention on a fractional-time equation arising in transient H Heating heating of bodies where (1a) is related to the time- R Radiative evolution of surface temperature and the solution is developed without the temperature field in the depth of the body. I. Introduction The heat transfer problems are among those with II. Problem Formulation and Model intensive applications of new analytical and numerical methods for solving new emerging practical situations. The flash heating of powder for example is a The present article addresses two principle issues. technique widely applied for de-hydroxylation of First of all, a problem of surface heating of body kaolinite. This mineral ( Al23 Oii 2SiO 2 2H 2 O ) undergoes subjected to a non-linear heat flux compromising a an endothermic reduction (loss) of the amount of the convective heating and a counteracting radiation cooling hydroxyl water at about 600°C resulting in meta-kaolin. is formulated. The problem formulation uses half-time This final form is strongly dependent on the rate of fractional model (in the Riemann-Liouville sense) to heating during the flash process. The kaolinite particles create an ordinary fractional differential equation are in the micro-size range but form aggregates that get (OFDE). forms of flakes which to some extent can be accepted as This allows elimination of cumbersome solutions of plates when the thermal treatment process has to be the temperature file in the depth of the thermally treated modelled. In accordance with the model of Davies [11] body. Second, the fractional model of surface the kaolinite aggregates are assumed as plates of temperature evolution is of Bernoulli type OFDE which thickness b heated by convection passing rapidly is solved by the variational iteration method (VIM) of through a furnace and cooled be thermal radiation. It is He. The main problem is the correct identification of the well-known that such models have no analytical general Lagrange multiplier. All these problems are solutions due to the non-linearity of the boundary consequently developed in the article. conditions at the interface. The process of flash heating of plate relevant to I.1. Non-Linear Boundary Condition due to thermal treatment of kaolinite has been modelled by Convection and Thermal Radiation Davies [11] and solved approximately by the heat- balance integral method of Goodman [12]. The transient heating of flat surfaces is a common The same method has been applied to radiation thermal problem solved by many methods and under cooling of finite solids [13] and plates by convention- various boundary conditions. radiation [14]. The heat balance integral solution allows It is impossible to encompass all of them, relevant the surface temperature to be estimated by developing an especially to the flash heating of bodies used in the approximated temperature profile in the depth of body, chemical, metallurgical and mineral industries. We stress then defining the temperature gradient required to solve the attention to 1-D transient heat conduction with a (1a) with respect to T . The main drawback of this nonlinear boundary condition in the form: s solution is that the temperature gradient at the interface depends on the choice of the approximate profile [12] ∂T −=−±−khTTTTs CRσε 4 (1a) and its calibration [15],[16]. ()()ssref ref ∂x x=0 The present work considers the transient heat conduction in a plate of thickness b which is heated by In (1a) the reference temperature is [1],[2] is defined convection and cooled by thermal radiation. This is, in in accordance with the direction of heat fluxes fact, the problem considered by Davies [11], namely towards/from the interface, namely: for cooling: ∂∂TT2 k C R = a,a,xb=≤≤0 (2a) TT= a and TT= a (1b) 2 ref ref ∂tC∂x ρ p for heating: with: H R TT= a and TT= R (1c) ∂T ref ref = 0atx = b (2b) ∂x In the light of application of the He’s VIM (see refs [3]-[8]) to solve nonlinear conduction equations this and: boundary condition has been recently used for solving convective–radiative cooling of lumped system (fin ∂Ts 44 conduction problem) [9],[10]; as an independent −khTTTTx=−−()saσε () s − aat = 0 (2c) ∂x x=0
Copyright © 2012 Praise Worthy Prize S.r.l. - All rights reserved International Review of Chemical Engineering, Vol. 4, N. 5 Special Section on Open Door Initiative (ODI) – 3rd edition
490
Jordan Hristov
The problem of interest is the time evolution of the problem at issue. surface temperature Ts which to some extent could be ¾ Note: In order to be correct, a variable uT= ∞ − T transforms the initial condition of Eq. (2a) to zero accepted with an initial condition Tts ()==00 for one, which simplifies the problem with application simplicity of the solution. It can be solved by either of the RL derivative. Similar problem, with only approximate analytical methods as those mentioned radiative cooling, i.e., qTxT4 above or numerically. However, with all these methods s =−∂∂()∂=x 0 =µ s the main errors come from the approximate and the variable uT= ∞ − T through the relationship determination of the space derivative Tx [12], ()∂∂x=0 ∗ −∗12 4 ∗ (4b) yields TTDTss(τµ) =−∞ ()τ , where τ [15],[16]. In order to find an effective solution of the is dimensionless time. The variable uT= − T problem where only the surface temperature Ts is of ∞ interest (it is the upper limit to which the body should be means only a shift of the origin of the co-ordinate heated; determined by technological conditions, for systems, that is equivalent to the assumption that example) we refer to the possibility to split (2a) into a T∞ = 0 at t = 0 : fractional (half-time) heat conduction equation, namely: k ∂12T 1 −=−−−s hT Tσε T44 T (5b) 12 ()s asa() ∂∂2Tx,t() Tx,t() α ∂t =− a (3a) 1 ∂x ∂t 2 Equation (5a) is expressed in a dimensional form but after non-dimensialization of the basic model (2a,b,c) with a fractional half-time derivative in the Riemann- * * 2 with θ = TTs a , ξ = x b and Fott= ( tba= ), we Liouville sense: get:
12 t RL 12 ∂ Tx,t() 1 d Tx,u() ∂∂θθ2 0 Ddut == (3b) = , 01≤≤ξ (6a) 12 Γ 12 dt ∫ 2 ∂−+ttu()0 ∂Fo ∂ξ
The surface flux and the temperature at the interface with: are interrelated by (3a) setting x = 0 : ∂θ = 0atξ ==xb 1 (6b) ∂ξ k ⎡⎤∂12T,t()0 T q,t′′ 0 =−∞ (4a) s () ⎢⎥12 α ⎣⎦⎢⎥∂ttπ and: ∂θ − s =−−−Bi()θθ11at0 N4 x = (6c) ∂ξ ss() with TT()x=0 = s x=0
−12 bh α ∂ ⎣⎦⎡⎤q,ts′′ ()0 Bi =−Biot Number (7a) T,t()0 =+ T (4b) k k −12 ∞ ∂t
bTσε 3 with: N =−a Radiation-conduction number (7b) ∂T k −=kqt′′ () ∂x s x=0 Now, using the relationship (4a) in a dimensionless form we get: T∞ in (4a),(4b) is the initial temperature of the body. Therefore, expressing the surface flux by (4a) and the 1 RL DBiN2θθ= −−11 θθ4 − , = 0 (8a) boundary condition (2c) we get: 0 Fo ss()() ss()Fo=0
After rearranging the RHS of (8a) we get a fractional k ⎡⎤∂12T T −−=−−−s ∞ hT Tσε T44 T (5a) (half –time) Bernoulli equation, namely: ⎢⎥12 ()s asa() απ⎣⎦⎢⎥∂tt 1 RL DABC2θ =+θθ + 4 (8b) at x = 0 . 0 Fo s ss
In accordance with the assumption that Tt= 00= s () A = NBi,BBi−=and C =− N (8c) we may suggest T∞ = 0 in (4a),(4b) that simplifies the
Copyright © 2012 Praise Worthy Prize S.r.l. - All rights reserved International Review of Chemical Engineering, Vol. 4, N. 5 Special Section on Open Door Initiative (ODI) – 3rd edition
491
Jordan Hristov
This fractional-time Bernoulli equation was not resulting in λ = −1. The result is the same as for the encountered in the literature so far, even with arbitrary fractional Riccati equations [17],[18] because both the fractional order 01<<α similar to the fractional Riccati linear and the non-linear terms in the RHS of (11b) are equation; expressed through the Caputo derivatives [16] restricted variations. Therefore, the correctional or modified Riemann-Liouville (Jumarie’s) derivatives functional (10a) for 01< α < (omitting the subscript Fo ) [17], namely: should be:
C α 2 0111Dytt ()=+ At () Bty () + C () ty,01 <<α (9) θ =−θθθθRLIDαα⎡ RL −− ABC − 4 ⎤ (11c) nnt+100 ⎣ n nn⎦
III. Solution by VIM However, following the rules defined by (11a),(11b) we may write the correction functional also as: In accordance with the VIM methodology, we have to construct a correction functional for (8b) in the form: Fo ⎡ RL α 4 ⎤ θnn+10=−θθθθτ∫ ⎣ DABCd Fonnn −− − ⎦ (11d) ⎡⎤⎛⎞RL α 0 RL α 0 DAFoθ n −+ θθnnt+1 =+I ⎢⎥ λτ()⎜⎟ (10a) 0 ⎢⎥⎜⎟4 ⎣⎦⎝⎠−−BCθθnn i.e. the Riemann-Liouville integral is replaced by an integer-order Riemann integral where: Therefore, there are two options in the successive iterations after determination of the Lagrange multiplier, Fo RL α 1 α −1 namely: It θ ()Fo=−()() Foτθ Fo d τ (10b) 0 Γ α ∫ 1) Approach 1 - Option 1 (A1-O1), λH = −1 and ()0 Riemann integration by (11d) is a fractional integral in the Riemann-Liouville sense. 2) Approach 1 - Option 2 (A1-O2), λH = −1 and The crucial step defining the successful application of Riemann-Liouville integration by (11c) VIM is the determination of the general Langrage • The subscript "H"indicate that this multiplier is multiplier λ (τ ) . The problems existing in its identified by rules drawn by J.H-He (see III.3 for detailed comments) determination are discussed next. These two options will be commented and numerically exemplified further in this article. III.1. Lagrange Multiplier Determination Approach 2: The main problem emerging through the identification Avoiding the problem with the impossible integration of the general Lagrange multiplier in case of fractional by parts with the integral Iα in (10a), we apply the equations is the fact that with the integral Iα in the approach of Wu [24], [25] which has two principle steps: correctional functional the integration by parts cannot be a) By an initial Laplace transform to (10a) we get: applied [3],[4]. We will discuss two approaches existing in the literature and providing different Lagrange ⎡ t RL α ⎤ multipliers. ⎛⎞0 DAθn −+ θθnn+1 ()ssLt,=+()⎢ λτ ( )⎜⎟⎥ (12a) ⎢∫ ⎜⎟−−BCθθ4 ⎥ Approach 1: ⎣ 0 ⎝⎠nn⎦ Following Momani and Odibat [19]-[21] and other articles devoted to similar problems [17], [18], [22], [23] The Lagrange multiplier is assumed in the form the iteration formula (10a) is replaced by: λ (t,τλτ) = ( t − ) allowing:
Fo RL α 4 ⎡ t ⎤ θnn+10=+θλτθ()⎡⎤DABCd Fonnn −− θθτ − (11a) RL α 4 ∫ ⎣⎦ Lt,D⎢ λτ()()0 θnnn−− ABC θ − θ⎥ (12b) 0 ∫ ⎣⎢ 0 ⎦⎥
The stationary condition of the functional leads too: to be considered as convolution of λ ()t and: Fo dθn δθ=+ δθ δ λ() τd τ =0 (11b) RL α 4 nn+1 ∫ dτ DABCθ −−θθ − 0 ( 0 nnn)