Predictability in Spatially Extended Systems with Model Uncertainty. II

Macroscopic models for spatially extended systems under random influences are often described by stochastic partial differential equations. Some techniques for understanding solutions of such equations, such as estimating correlations, Liapunov exponents and impact of noises, are discussed. They are...

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Опубліковано в: :Электронное моделирование
Дата:2009
Автор: Duan, J.
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Мова:Англійська
Опубліковано: Інститут проблем моделювання в енергетиці ім. Г.Є. Пухова НАН України 2009
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Цитувати:Predictability in Spatially Extended Systems with Model Uncertainty. II / J. Duan // Электронное моделирование. — 2009. — Т. 31, № 3. — С. 21-35. — Бібліогр.: 7 назв. — рос.

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author Duan, J.
author_facet Duan, J.
citation_txt Predictability in Spatially Extended Systems with Model Uncertainty. II / J. Duan // Электронное моделирование. — 2009. — Т. 31, № 3. — С. 21-35. — Бібліогр.: 7 назв. — рос.
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container_title Электронное моделирование
description Macroscopic models for spatially extended systems under random influences are often described by stochastic partial differential equations. Some techniques for understanding solutions of such equations, such as estimating correlations, Liapunov exponents and impact of noises, are discussed. They are relevant for understanding predictability in spatially extended systems with model uncertainty, for example, in physics, geophysics and biological sciences. The presentation is for a wide audience. Рассмотрены некоторые методы представления решений стохастических дифференциальных уравнений в частных производных, в частности в задачах корреляции оценки, экспоненты Ляпунова и воздействие шумов. Методы пригодны для понимания предсказуемости в пространственно распределенных системах с неопределенностью модели, например, в физике, геофизике и биологических науках. Розглянуто деякі методи представлення розв'язків стохастичних диференціальних рівнянь у частинних похідних, зокрема у задачах кореляції оцінки, експоненти Ляпунова та впливу шумів. Методи придатні для розуміння передбачуваності у просторово розподілених системах з невизначеністю моделі, наприклад, у фізиці, геофізиці та біологічних науках.
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fulltext J. Duan Department of Applied Mathematics Illinois Institute of Technology (Chicago, IL 60616, USA, E-mail: duan@iit.edu) Predictability in Spatially Extended Systems with Model Uncertainty *. II Macroscopic models for spatially extended systems under random influences are often described by stochastic partial differential equations. Some techniques for understanding solutions of such equations, such as estimating correlations, Liapunov exponents and impact of noises, are dis- cussed. They are relevant for understanding predictability in spatially extended systems with model uncertainty, for example, in physics, geophysics and biological sciences. The presentation is for a wide audience. Ðàññìîòðåíû íåêîòîðûå ìåòîäû ïðåäñòàâëåíèÿ ðåøåíèé ñòîõàñòè÷åñêèõ äèôôåðåíöèàëüíûõ óðàâíåíèé â ÷àñòíûõ ïðîèçâîäíûõ, â ÷àñòíîñòè â çàäà÷àõ êîððåëÿöèè îöåíêè, ýêñïîíåíòû Ëÿïóíîâà è âîçäåéñòâèå øóìîâ. Ìåòîäû ïðèãîäíû äëÿ ïîíèìàíèÿ ïðåäñêàçóåìîñòè â ïðîñò- ðàíñòâåííî ðàñïðåäåëåííûõ ñèñòåìàõ ñ íåîïðåäåëåííîñòüþ ìîäåëè, íàïðèìåð, â ôèçèêå, ãåîôèçèêå è áèîëîãè÷åñêèõ íàóêàõ. K e y w o r d s: Stochastic partial differential equations, correlation, Liapunov exponents, pre- dictability, uncertainty, invariant manifolds, impact of noise 4. Correlation. In this section, we discuss correlation of solutions, at different time instants, of some linear SPDEs. We first recall some information about Fourier series in Hilbert space. Hilbert-Schmidt theory and Fourier series in Hilbert space. A separable Hilbert space H has a countable orthonormal basis{ }en n� � 1. Namely, e em n mn, �� , where �mn is the Kronecker delta function. Moreover, for any h �H, we have Fourier series expansion h h e en n n � � � � , 1 . ISSN 0204–3572. Ýëåêòðîí. ìîäåëèðîâàíèå. 2009. Ò. 31. ¹ 3 21 * J. Duan. Predictability in Spatially Extended Systems with Model Uncertainty. I. — Ýëåêòðîí- íîå ìîäåëèðîâàíèå, ¹ 2, 2009. This work was partly supported by the NSF Grants 0542450 and 0620539. In the context of solving stochastic PDEs, we may choose to work on a Hilbert space with an appropriate orthonormal basis. This is naturally possible with the help of the Hilbert-Schmidt theory [1, p. 232]. The Hilbert-Schmidt theorem [1, p. 232] says that a linear compact symmet- ric operator A on a separable Hilbert space H has a set of eigenvectors that form a complete orthonormal basis for H. Moreover, all the eigenvalues of A are real, each non-zero eigenvalue has finite multiplicity, and two eigenvectors that cor- respond to different eigenvalues are orthogonal. This theorem applies to a strong (self-adjoined) elliptic differential operator B Bu D a x D u m � � � � � ( ) ( ( ) ) , 1 0 � � � � , x D n � � , where the domain of definition of B is an appropriate dense subspace of H L D� 2( ), depending on the boundary condition specified for u (x). In this case, A := B–1 is a linear symmetric compact operator in a Hilbert space, e. g., H L D� 2( ). We may consider A := (B + aI)–1 for some real number a. This may be necessary in order for the operator to be invertible, i.e., no zero eigenvalue, such as in the case of Laplace operator with zero Neumann boundary condition. By the Hilbert-Schmidt theorem, eigenvectors (also called eigenfunctions in this context) of A = B–1 form an orthonormal basis for H L D� 2( ). Note that A and B share the same set of eigenfunctions. So we can claim that the strong ellip- tic operator B’s eigenfunctions form an orthonormal basis for H L D� 2( ). In the case of one spatial variable, the elliptic differential operator is the so called Sturm-Liouville operator [1, p. 245]. For example Bu pu qu� � � � ( ) , x l ( , )0 where p x( ), �p x( )and q x( )are continuous on (0, l). This operator arises in the method of separating variables for solving linear (deterministic) partial differential equations in the next section. By the Hilbert-Schmidt theorem, eigenfunctions of the Sturm-Liouville operator form an orthonormal basis for H L l� 2 0( , ). The wave equation with additive noise. Consider the stochastic wave equa- tion with additive noise u c u Wtt xx t� 2 º , 0 0� � �x l t, , u t u l t( , ) ( , )0 0� � , u x f x( , ) ( )0 � , u x g xt ( , ) ( )0 � , where º is a real parameter modeling the noise intensity, c > 0 is a constant (wave speed), and Wt is a Brownian motion taking values in Hilbert space H L l� 2 0( , ). J. Duan 22 ISSN 0204–3572. Electronic Modeling. 2009. V. 31. ¹ 3 Method of eigenfunction expansion: u u t e xn n n� � � � 1 ( ) ( ), W q W t e xt n n n n � � � � ( ) ( ) 1 , where e x l n x l n ( ) sin� 2 � , � �n n� ( )2, n �1 2, , ... . The final solution u x t A l cn q cn l sdW sn n t n( , ) sin ( ) cos� � � � � � � � � � � � � �� �º � � 0 cn l t n � � � � 1 � � � � � � � � � � � �� �B l cn q cn l sdW s cn l t en n t nº � � � 0 cos ( ) sin n x( ) , where A f en n� , , B l cn g en n� � , . When the noise is at one mode, say at the first mode e x1( ) (i.e., q1 > 0 but qn = = 0, n = 2, 3, ...), we see that the solution contains randomness only at that mode. So for the linear stochastic diffusion system, there is no interactions between modes. In other words, if we randomly force a few fast modes, then there is no impact on slow modes. Mean value for the solution: �u x t A cn t l B cn t l n n n ( , ) cos sin� ! " # $ % ! " # $ % � �� � � � � � � 1 � � e xn ( ). Covariance for the solution: now we calculate the covariance of solution u at different time instants t and s, i. e. � � �� � � �u x t u x t u x s u x s( , ) ( , ), ( , ) ( , ) . Us- ing the Ito’s isometry, we get � � �� � � � �u x t u x t u x s u x s( , ) ( , ), ( , ) ( , ) � � � � � & � º 2 2 2 2 2 0 2l q c n cn r l dr cn t l cn s l n t s � � � � sin cos cos n� � � 1 � & � 0 2 t s cn r l dr cn t l cn s l cos sin sin � � � Predictability in Spatially Extended Systems with Model Uncertainty. II ISSN 0204–3572. Ýëåêòðîí. ìîäåëèðîâàíèå. 2009. Ò. 31. ¹ 3 23 � & � 0 t s cn r l cn r l dr cn t l cn s l cn s l sin cos cos sin cos s � � � � � in cn t l � ! " # $ % � � � � . After integrations, we get the covariance as Cov u x t u x s u x t u x t u x s u x s( ( , ), ( , )) ( , ) ( , ), ( , ) ( , )� � � �� � � � � � & �� �� � � � � º 2 2 2 2 2 1 2 2 2l q c n t s cn t s l l cn cn n � � � ( ) cos ( ) sin n t s l cn t s l � �( ) cos ( )& & � �l cn cn t s l cn t s l l cn cn t s l2 2 2� � � � � cos ( ) sin ( ) sin ( ) �� � � & �� �� � � � º 2 2 2 2 2 1 2 2 l q c n t s cn t s l l cn cnn n � � � ( ) cos ( ) sin �( ( ))t s t s l � & � 2 � � �� l cn cn t s l2 � � sin ( ) . In particular, for t = s we get the variance. Variance for the solution: Var u x t l c n q t l cn cn l tn( ( , )) sin� � �� � ! " # $ º 2 2 2 2 2 1 2 4 2 � � � % � ��� � � n 1 . Energy evolution for the solution: E t u c u dxt x l ( ) [ ]� � 1 2 2 2 2 0 . Taking time derivative, � ( ) [ ] ( , ) � ( )E t u u c u dx u x t W x dxt tt xx l t t l � � �� � 2 0 0 º . Or in integral form, E t E u x t dW x dx t s s l ( ) ( ) ( , ) ( )� � �0 0 0 º . J. Duan 24 ISSN 0204–3572. Electronic Modeling. 2009. V. 31. ¹ 3 It can be shown that �E t E( ) ( )� 0 , Var E t u x s dW dx l t s t ( ( )) ( , )� ! " " # $ % %� �' (2 0 0 2 � , where Wt is in the following form W W t q W t e xt n n n n � � � � �( ) ( ) ( ) 1 , and ( t u can be written in the following form : ( � � � � t n nu A cn l cn t l B cn l cn t l � ��� � ! " # $ % � sin cos � � � � �' � � q cn s l dW s cn t l n t n 0 sin ( ) sin � �� � � �� 0 t n n cn s l dW s cn t l e xcos ( ) cos ( ) � � . Set cn l n� )/ � and rewrite ( ' ) ) ) )t n n t n n n n nu F t q s t s t dW s� � �( ) (sin sin cos cos ) ( ) 0� � � � � � � � � � �� � � � �� �� e xn ( ) � � � � � �� � � � �� �� F t q t s dW s e xn n t n n n( ) cos ( ) ( ) ( )' ) 0 , where F t A s t B s tn n n n n n n( ) : sin cos� � ) ) ) ) , n = 1, 2, ... . For the simplicity of notations, set G t F t q t s dW sn n n t n n( ) : ( ) cos ( ) ( )� ��' ) 0 , n = 1, 2, ... , then we have ( t n nu G t e x�� ( ) ( ). Thus � � 0 0 2 0 l t s t l n n s nu x s dW dx q e x u dW� � � ! " " # $ % % � � � � � ( ( , ) ( ) ( )s dx t n 0 2 1 �� # $ % % � � � � ! " " � � � � � � � � � � � � ���� � � � q u e x dW s dxn s n n tl n ( ) ( ) 00 2 1 Predictability in Spatially Extended Systems with Model Uncertainty. II ISSN 0204–3572. Ýëåêòðîí. ìîäåëèðîâàíèå. 2009. Ò. 31. ¹ 3 25 �� q e x G s e x dx dWn n t n j j j l � � � � � � �� � � � ! " " # $ % % 1 0 10 ( ) ( ) ( ) n s( ) � � � � � 2 � � � � # $ % % � � � � � � � �� q G s e x e x dx dW sn n t j j n j l n 1 0 1 0 ( ) ( ) ( ) ( ) � � � � ! " " � 2 � � � � � � � � � � � � � � � � �� �q G s dW s q G s dn n t n n n n t n 1 0 2 1 0 2( ) ( ) ( ) s � � � � � � � � � � �� � � � �q F s q s r dW r dn n t n n n s n 1 0 0 2 � ( ) cos ( ) ( )' ) s �� q F s dsn n t n � � � � 1 0 2( ) � � � � � � � � � � � � � ��� ' )*q s r dr dsn n s n t 2 1 0 2 0 cos ( ) � ! " � �� � # $ % � � � q A t t B t n n n n n n n n 1 2 2 2 2 2 1 4 2 2 1 4 ) ) ) ) ) sin n n tsin2) ! " # $ %� � � � �� � � � �1 2 1 2 4 1 8 1 22 1 2 2 A B t q t n n n n n n n ) ) ' ) *( cos ) ( cos )n t) � � � � � � . Therefore, Var E t q A t t Bn n n n n n( ( )) sin� � ! " # $ % � � � � � � ' ) ) )* 1 2 2 2 1 4 2 n n n n t t2 2 2 1 4 2) ) ) ! " # $ %�sin � � � �� � � � � � � �1 2 1 2 4 1 8 12 1 2 2 A B t q t n n n n n n n ) ) ' ) +( cos ) ( cos )2)n t � � � is obtained. The diffusion equation with multiplicative noise. Consider the stochastic diffusion equations with zero Dirichlet boundary condition u u uwt xx t� º � , 0 1� �x , u x f x( , ) ( )0 � , (2) J. Duan 26 ISSN 0204–3572. Electronic Modeling. 2009. V. 31. ¹ 3 where wt is a scalar Brownian motion. We take Hilbert space H L� 2 0 1( , ) with an orthonormal basis e n xn � 2sin ( )� . We use the method of eigenfunction expansion: u x t u t e xn n( , ) ( ) ( )�� , u u t e x u t n e xxx n n n n� � �� �( ) �� ( ) ( )( ) ( )� 2 . Putting these into the above SPDE (2), with � �n n� ( )2, we get � ( ) ( ) ( )( ) ( ) ( ) � .u t e x u t e u t e x wn n n n n n n t� � �� � � º We further obtain the following system of SODEs: du t u t u t dw tn n n n( ) ( ) ( ) ( )� � � º , n = 1, 2, 3, ... . Thus u t u t w tn n n( ) ( ) exp ( )� � � ! " # $ % ! " # $ %0 1 2 2� º º , where u x f x f x e x e x u e xn n n n( , ) ( ) ( ), ( ) ( ) ( ) ( )0 0� ��� � �� . Therefore, the final solution is: u x t a e x b t wn n n t( , ) ( ) exp( ),� � º with a f x e xn n�� �( ), ( ) and bn n� � � ! " # $ %� 1 2 2 º . Note that � �exp( ) exp( ) exp( ) exp( ) expb t w b t w b t tn t n t n � � ! º º º 1 2 2 " # $ % � � �exp( )� n t . Therefore, we can find out the mean, variance, covariance and cor- relation of the solution: E u x t a e x tn n n( ( , )) ( ) exp( )� �� � , Var u x t u x t E u x t u x t E u x t( ( , )) ( , ) ( ( , )), ( , )) ( ( , ))� � � �� � � ��a t tn n 2 22 1exp( )[exp( ) ]� º . For , � t we have � �exp{ ( )} exp{ ( ) }º º ºw w w w wt t � � �, , ,2 � � �� �exp{ ( )} exp{ }º ºw w wt , ,2 � �� � � � � � � &exp ( ) exp{ } exp [( ) ( )] 1 2 2 1 2 22 2 2 º º ºt t t, , , ,� � � � � � . Predictability in Spatially Extended Systems with Model Uncertainty. II ISSN 0204–3572. Ýëåêòðîí. ìîäåëèðîâàíèå. 2009. Ò. 31. ¹ 3 27 Therefore, by direct calculation, we can get Cov u x t u x a b t tn n( ( , ), ( , )) exp( ( ) (( ), , ,� � � � � 2 21 2 2º ( )))t & , � � � ! " # $ %� �exp( ( )) exp exp� , � , � ,n n n n nt b t t t b 1 2 2 º ! " # $ % � � � � 1 2 2 º , � � & ��a t tn n 2 2 1exp{ ( )}[exp{ ( )} ]� , ,º and Corr u x t u x Cov u x t u x Var u x t V ( ( , ), ( , )) ( ( , ), ( , )) ( ( , )) , , � ar u x( ( , )), � � � & � � �a t t a t n n n n 2 2 2 1 2 exp{ ( )}[exp{ ( )} ] exp( )[ex � , , � º p{ ) ] exp( )[exp{ ) ]� �� � �º º 2 2 21 2 1t an n� , , . 5. Lyapunov Exponents. Lyapunov exponents are tools for quantifying growth or decay of linear systems (e. g., PDEs or SPDEs). The following discus- sions are from [2, 3]. A deterministic PDE system. Let us first look at the following deterministic PDE: ( ( � u t u uxx� , (3) u x f x( , ) ( )0 � , (4) u x t( , ) �0, x D ( , (5) where D x x� � �{ : }0 1 and the function f L 2 0 1( , ). An orthonormal basis for L2 0 1( , ) is { ( )}e xn , n = 0, 1, 2, ..., ( �xx j j je e� � . Note that 0� -�� j . We then can write: f f ej j j � � � � 0 , (6) where f f ej j� , . By using the method of eigenfunction expansion, it is known that the unique solution to the problem is given below: u x t t f e xj j j j ( , ) exp( ( )) ( )� � � � � � � 0 , t ./01 (7) J. Duan 28 ISSN 0204–3572. Electronic Modeling. 2009. V. 31. ¹ 3 Theorem 2. Let us fix a non-zero initial condition f. Let j0 be the smallest integer j . 0 in the expansion (6) of f such that f j0 02 . Then the Lyapunov expo- nent of the system (3)—(5) exists as a limit and is given by � � �u jf( ) � � 0 . P r o o f. For a class of initial conditions f we calculate the Lyapunov expo- nents, which are defined as �u t L f t u t( ) lim sup log� 3� 1 2( ) . By applying (7), we obtain the Lyapunov exponents regarding to PDE sys- tem (3)—(5), � � �u t j j j j f t t f e x( ) lim sup log exp( ( )) ( )� � 3� � � �1 0 . On the one hand, 1 0t t f e xj j j j log exp( ( )) ( )� � � � � � � � � ! " " # $ % % � � � � �1 1 0 0 0 2 1 2 t t f t j j j j jlog exp( ( )) / � � � � log f . On the other hand, 1 0t t f e xj j j j log exp( ( )) ( )� . � � � � � . � � � � 1 1 0 0 0 0t t f t fj j j jlog exp( ( )) log� � � � . A SPDE system. We now consider the following SPDE dv v v dt vdwxx t� ( ) 4 , (8) v x f x( , ) ( )0 � , x D , (9) v x t( , ) �0 , x D ( , (10) where wt is a scalar Brownian motion. The conditions (9) and (10) hold for a.a. 5 6. We seek the solution with expansion with respect to the basis { }e j (see the last subsection) v x t y t e xj j j ( , ) ( ) ( )� � � � 0 , (11) Predictability in Spatially Extended Systems with Model Uncertainty. II ISSN 0204–3572. Ýëåêòðîí. ìîäåëèðîâàíèå. 2009. Ò. 31. ¹ 3 29 where y tj ( ), for j = 0, 1, 2, … satisfy the following stochastic ordinary differen- tial equations: dy t y t dt y t dwj j j j t( ) ( ) ( ) ( )� � � 4 , y fj j( )0 � . So y t w t fj t j j( ) exp( ) exp� � � ! " # $ % ! " # $ %4 � 4 1 2 2 . Thus from (11), we obtain, v x t w t f et j j j j ( , ) exp( ) exp� � � ! " # $ % ! " # $ % � � � 4 � 4 1 2 2 0 . Observe that v x t w t u t xt( , ) exp( ) exp ( ( , )� ! " # $ % ! " # $ %4 ��7 4 1 2 2 , (12) where u (t, x) is the solution to the above deterministic PDE (3)—(5). By (12), we can calculate the Lyapunov exponent of the stochastic system (8)—(10) as a function of the Lyapunov exponent of the deterministic system (3)—(5) as follows: �v t f t v t( ) lim sup log� � 3� 1 ( ) � � ! " # $ % ! " # $ % 3� lim sup log exp( ) exp ( t t t w t u 1 1 2 24 ��7 4 ( )t � � �� �7 � 8 * 4*u f( ) ( , a.s. by the strong law of large number. Let us state the result in the following theorem. Theorem 3. Let f 2 0. Then the Lyapunov exponent of the SPDE (8)—(10) almost surely exists as a limit, is non-random and is given in the fol- lowing formula: � � �7 � 8 * 4*v uf f( ) ( ) (� � , a. s. Remark 7. Let us consider a special case when � � . Then by the above theorem, for a fixed initial condition f, the Lyapunov exponent of the stochastic system (8)—(10) is � � � 8 * 4*v uf f( ) ( )� , J. Duan 30 ISSN 0204–3572. Electronic Modeling. 2009. V. 31. ¹ 3 which obviously is smaller than the Lyapunov exponent of the corresponding deterministic system (3)—(5). The result implies that this stochastically per- turbed system is more stable than the original deterministic system. 6. Impact of Uncertainty. In this section, we first recall some inequalities for estimating solutions of SPDEs, and then we estimate the impact of noises on solutions of the nonlinear Burgers equation. Differential and integral inequalities. G r o n w a l l i n e q u a l i t y: D i f f e - r e n t i a l f o r m [4]. Assuming that y t( ) . 0, g (t) and h (t) are integrable, if dy dt � g t y h t( ) ( ) for t t. 0, then y t y t e h s e ds g d g d t t t t t t ( ) ( ) ( )[ ] ( ) ( ) � � � �0 0 0 0 , , , , , t t. 0. In particular, if dy dt gy h� for t t. 0 with g, h being constants and t0 = 0, we have y t y e h g egt gt( ) ( ) ( )� �0 1 , t . 0 . Note that when constant g < 0, then lim ( ) t y t h g3� � � . G r o n w a l l i n e q u a l i t y: I n t e g r a l f o r m [5, 6]. If u (t), v (t) and c (t) are all non-negative, c (t) is differentiable, and v t c t u s v s ds t ( ) ( ) ( ) ( )� � 0 for t t. 0, then v t v t e c s e ds u d u d t t t t s t ( ) ( ) ( )[ ] ( ) ( ) � � � � �0 0 0 , , , , , t t. 0. In particular, assuming that y (t) . 0 and is continuous and y t C K y s ds t ( ) ( )� � 0 , with C, K being positive constants, for t > 0. Then y t CeKt( ) � , t . 0. Sobolev inequalities. We first introduce some common Sobolev spaces. For k = 1, 2, ..., we define H l f f f f L lk k( , ) : { : , , ..., ( , )}( )0 02� � . Each of these is a Hilbert space with the scalar product u v uv u v u v dx k k k l , [ ... ]( ) ( )� � � � 0 , Predictability in Spatially Extended Systems with Model Uncertainty. II ISSN 0204–3572. Ýëåêòðîí. ìîäåëèðîâàíèå. 2009. Ò. 31. ¹ 3 31 and the norm u u u u u u dx k k k l � � � �, [ ( ) ... ( ) ]( )2 2 2 0 . For k = 1, 2, ... and p . 1, we further define another class of Sobolev spaces W D u u Du D u L D kk p p, ( ) { : , , ..., ( ), }� �� � with norm u u k p L p p, � ! " � # $ %u u L p k L p p p p ... ( ) 1 . Moreover, H lk 0 0( , )denotes the closure ofC lc � ( , )0 in H lk ( , )0 (i.e., under the norm 9 k ). It is a sub-Hilbert space in H lk ( , )0 . Similarly,W lk p 0 0, ( , ) denotes the closure of C lc � ( , )0 in W lk p, ( , )0 (i.e., under the norm 9 k p, ). It is a sub-Hilbert space inW lk p, ( , )0 . Standard abbreviations L L D2 2� ( ), H H Dk k 0 0� ( ), k = 1, 2, ..., are used for the common Sobolev spaces in fluid mechanics, with < 9 , 9 > and 9 denoting the usual (spatial) scalar product and norm, respectively, in L D2( ): � � � �f g fgdxdy D , : , f f f f x y dxdy D : , ( , )� � � � � . C a u c h y - S c h w a r z i n e q u a l i t y. In the space L D2( ) of square-integrable functions defined on a domain D n� � : f x g x dx f x dx g x dx D D D ( ) ( ) ( ) ( )� � �� 2 2 . H ��o l d e r i n e q u a l i t y. In the space L Dr ( ) of functions defined on a do- main D n� � : f x g x dx f x dx g x dx D p D p q D ( ) ( ) ( ) ( )� � �� ! " " # $ % % ! " " # $ % % 1 1 q . M i n k o w s k i i n e q u a l i t y. In the space L Dp ( )of functions defined on a domain D n� � : f x g x dx f x dx g x p D p p D p p ( ) ( ) ( ) ( ): ! " " # $ % % � ! " " # $ % % � � 1 1 dx D p � ! " " # $ % % 1 . J. Duan 32 ISSN 0204–3572. Electronic Modeling. 2009. V. 31. ¹ 3 P o i n c a r e i n e q u a l i t y [4]. For g H D 0 1( ), g g x y dxdy D g dxdy D g D D 2 2 2 2� � ; � ;� �( , ) � � , where D is the Lebesgue measure of the domain D. For u W Dp 0 1, ( ),1� � �p and D n� � a bounded domain u C u p p � ; , where C is a positive constant depending only on the domain D. Let u W Dp 1, ( ),1� � �p and D n� � a bounded convex domain. Let S � D be a measurable subset, and define the spatial average of u over S by u S udxS D � � 1 (here S is the volume or Lebesgue measure of S). Then u u C uS p p � � ; , where C is a positive constant depending only on the domain D and S. A g m o n i n e q u a l i t y [4]. Let D n� � . There exists a constant C depend- ing only on domain D such that u C u u L D H D H D n n� � � ( ) ( ) ( ) 1 2 1 2 1 2 1 2 , for n odd, u u u L D H D H D n n� � � ( ) ( ) ( ) 2 2 2 2 1 2 1 2 , for n even. In particular, for n = 1 and u H l 1 0( , ), u C u u L l L l H l � � ( , ) ( , ) ( , )0 0 1 2 0 1 2 2 1 . Moreover, for n = 1 and u H l 0 1 0( , ), u C u u L l L l x L l � � ( , ) ( , ) ( , )0 0 1 2 0 1 2 2 2 . Stochastic Burgers equation.We now consider the Burgers equation with additive noise forcing as in [7]: ( ( ( <t x x tu u u v u W � 2 � , u t( , )0 0� , u l t( , ) �0, u x u x( , ) ( )0 0� , whereWt is a Brownian motion, with covariance Q, taking values in the Hilbert space L2(0, l) with the usual scalar product 9 9, . We assume that the trace Tr (Q) is finite. So �Wt is noise colored in space but white in time. Predictability in Spatially Extended Systems with Model Uncertainty. II ISSN 0204–3572. Ýëåêòðîí. ìîäåëèðîâàíèå. 2009. Ò. 31. ¹ 3 33 Taking F u u dx u u l ( ) ,� �� 1 2 1 2 2 0 and applying the Ito’s formula, we obtain 1 2 1 2 2 2d u u dW u vu uu lTr Q dtt xx x� � � �� � �� , , ( )< < . Thus d dt u u vu uu lTr Q v u lTr Qxx x x� 2 2 2 22 2� � � � , ( ) ( )< < . By the Poincare inequality u c ux 2 2� for some positive constant depending only on the interval (0, l), we have d dt u v c u lTr Q� 2 2 22 � � < ( ). Then using the Gronwall inequality, we finally get � �u u e c lTr Q e v c t v c t 2 0 2 2 2 2 1 2 1� � � � < ( )[ ] . Note that the first term in this estimate involves the initial data, and the second term involves the noise intensity < as well as the trace of the noise covariance. We finally consider the Burgers equation with multiplicative noise forcing ( ( ( <t x x tu u u v u uw � 2 � , with the same boundary condition and initial condi- tion as above, where wt is a scalar Brownian motion (e. g., with covariance Q = 1 and the trace Tr (Q) = 1). So �Wt is noise homogeneous in space but white in time. By the Ito’s formula, we obtain 1 2 1 2 2 2 2 d u u udw u vu uu u dtt xx x� � � �� � �� , ,< < . Thus d dt u u vu uu u v u u v c uxx x x� 2 2 2 2 2 2 2 2 2 2 2 � � � � � � ! " # $ %, < < < . Therefore, � �u u e v c t 2 0 2 22 � � ! " # $ %< . J. Duan 34 ISSN 0204–3572. Electronic Modeling. 2009. V. 31. ¹ 3 Note here that the multiplicative noise affects the mean energy growth or de- cay rate, while the additive noise affects the mean energy upper bound. Likelihood for staying bounded. By the Chebyshev inequality, we can esti- mate the likelihood of solution orbits staying inside or outside a bounded domain in Hilbert space H L l� 2 0( , ). Taking the bounded domain as a ball centered at the origin with radius � > 0. For example, for the above Burgers equation with multiplicative noise, we have � � � ( : )5 � � �* * < u u u e v c t . � � � ! " # $ %1 2 0 2 22 and � � � ( : ) ( : )5 � 5 � �* < u u u e v c t � � � . . � � ! " # $ % 1 1 0 2 22 . I would like to thank Hongbo Fu and Jiarui Yang for helpful comments. Ðîçãëÿíóòî äåÿê³ ìåòîäè ïðåäñòàâëåííÿ ðîçâ'ÿçê³â ñòîõàñòè÷íèõ äèôåðåíö³àëüíèõ ð³âíÿíü ó ÷àñòèííèõ ïîõ³äíèõ, çîêðåìà ó çàäà÷àõ êîðåëÿö³¿ îö³íêè, åêñïîíåíòè Ëÿïóíîâà òà âïëèâó øóì³â. Ìåòîäè ïðèäàòí³ äëÿ ðîçóì³ííÿ ïåðåäáà÷óâàíîñò³ ó ïðîñòîðîâî ðîçïîä³ëåíèõ ñèñòå- ìàõ ç íåâèçíà÷åí³ñòþ ìîäåë³, íàïðèêëàä, ó ô³çèö³, ãåîô³çèö³ òà á³îëîã³÷íèõ íàóêàõ. 1. Zeidler E. Applied Functional Analysis: Applications to Mathematical Physics. — New York: Springer, 1995. 2. Caraballo T., Langa J. A Comparison of the Longtime Behavior of Linear Ito and Stra- tonovich Partial Differential Equations // Stochastic Anal. Appl. — 2001. — 19, ¹ 2. — P. 183—195. 3. Kwiecifinska A. A. Stabilization of Evolution Equations by Noise//Proc. Amer. Math. Soc. — 2002. — 130, ¹ 10. — P. 3067—3074. 4. Temam R. Infinite-dimensional Dynamical Systems in Mechanics and Physics. — New York: Springer-Verlag, Second Edition, 1997. 5. Coddington E. A., Levinson N. Theory of Ordinary Differential Equations. — New York McGraw Hill, 1955. 6. Guckenheimer J., Holmes P. Nonlinear Oscillations, Dynamical Systems and Bifurcations of Vector Fields. — New York: Springer-Verlag, 1983. 7. Blomker D., Duan J. Predictability of the Burgers Dynamics under Model Uncertainty. In Boris Rozovsky 60th Birthday Volume Stochastic Differential Equations: Theory and Ap- plications, P. Baxendale and S. Lototsky (Eds.) — New Jersey: World Scientific, 2007. — P. 71—90 Ïîñòóïèëà 08.12.08 Predictability in Spatially Extended Systems with Model Uncertainty. II ISSN 0204–3572. Ýëåêòðîí. ìîäåëèðîâàíèå. 2009. Ò. 31. ¹ 3 35
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language English
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publishDate 2009
publisher Інститут проблем моделювання в енергетиці ім. Г.Є. Пухова НАН України
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Predictability in Spatially Extended Systems with Model Uncertainty. II / J. Duan // Электронное моделирование. — 2009. — Т. 31, № 3. — С. 21-35. — Бібліогр.: 7 назв. — рос.
0204-3572
https://nasplib.isofts.kiev.ua/handle/123456789/101491
Macroscopic models for spatially extended systems under random influences are often described by stochastic partial differential equations. Some techniques for understanding solutions of such equations, such as estimating correlations, Liapunov exponents and impact of noises, are discussed. They are relevant for understanding predictability in spatially extended systems with model uncertainty, for example, in physics, geophysics and biological sciences. The presentation is for a wide audience.
Рассмотрены некоторые методы представления решений стохастических дифференциальных уравнений в частных производных, в частности в задачах корреляции оценки, экспоненты Ляпунова и воздействие шумов. Методы пригодны для понимания предсказуемости в пространственно распределенных системах с неопределенностью модели, например, в физике, геофизике и биологических науках.
Розглянуто деякі методи представлення розв'язків стохастичних диференціальних рівнянь у частинних похідних, зокрема у задачах кореляції оцінки, експоненти Ляпунова та впливу шумів. Методи придатні для розуміння передбачуваності у просторово розподілених системах з невизначеністю моделі, наприклад, у фізиці, геофізиці та біологічних науках.
This work was partly supported by the NSF Grants 0542450 and 0620539. I would like to thank Hongbo Fu and Jiarui Yang for helpful comments.
en
Інститут проблем моделювання в енергетиці ім. Г.Є. Пухова НАН України
Электронное моделирование
Математические методы и модели
Predictability in Spatially Extended Systems with Model Uncertainty. II
Article
published earlier
spellingShingle Predictability in Spatially Extended Systems with Model Uncertainty. II
Duan, J.
Математические методы и модели
title Predictability in Spatially Extended Systems with Model Uncertainty. II
title_full Predictability in Spatially Extended Systems with Model Uncertainty. II
title_fullStr Predictability in Spatially Extended Systems with Model Uncertainty. II
title_full_unstemmed Predictability in Spatially Extended Systems with Model Uncertainty. II
title_short Predictability in Spatially Extended Systems with Model Uncertainty. II
title_sort predictability in spatially extended systems with model uncertainty. ii
topic Математические методы и модели
topic_facet Математические методы и модели
url https://nasplib.isofts.kiev.ua/handle/123456789/101491
work_keys_str_mv AT duanj predictabilityinspatiallyextendedsystemswithmodeluncertaintyii