J. Korean Math. Soc. 48 (2011), No. 2, pp. 311–327 DOI 10.4134/JKMS.2011.48.2.311
SIMPLIFIED TIKHONOV REGULARIZATION FOR TWO KINDS OF PARABOLIC EQUATIONS
Li Jing and Wang Fang
Abstract. This paper is devoted to simplified Tikhonov regularization for two kinds of parabolic equations, i.e., a sideways parabolic equation, and a two-dimensional inverse heat conduction problem. The measured data are assumed to be known approximately. We concentrate on the convergence rates of the simplified Tikhonov approximation of u(x, t) and its derivative u
x(x, t) of sideways parabolic equations at 0 ≤ x < 1, and that of two-dimensional inverse heat conduction problem at 0 < x ≤ 1, respectively.
1. Introduction
In several engineering contexts, there is sometimes a need to determine the temperature on both sides of a thick wall, but one side is inaccessible to measure (see e.g. [7]). In one-dimensional setting, this problem occasionally leads to the following parabolic equation in the quarter plane:
u t = a(x)u xx + b(x)u x + c(x)u, x > 0, t > 0, (1)
u(1, t) = g(t), t > 0, (2)
u(x, 0) = 0, x > 0, (3)
where a, b and c are given functions such that there exist λ, Λ > 0, λ ≤ a(x) ≤ Λ, c(x) ≤ 0, x ∈ R + .
For simplicity, we suppose that
a(x) ∈ C 2 ( R + ), b(x) ∈ C 1 ( R + ), c(x) ∈ C(R + ).
We want to know u(x, t) for 0 ≤ x < 1. This is a severely ill-posed problem (cf. [2, 4]), i.e., if small changes of g(t) with
(4) ∥g − g δ ∥ ≤ δ,
Received October 4, 2009; Revised December 21, 2009.
2010 Mathematics Subject Classification. 35K05, 47A52, 65J10, 65N21.
Key words and phrases. Fourier transformation, simplified Tikhonov regularization, con- vergence rate, sideways parabolic equations, inverse heat conduction problems.
This work was partially supported by NNSF of China Grant No.10671211 and Hunan Provincial Natural Science Foundation of China Grant No. 07JJ3005.
⃝2011 The Korean Mathematical Societyc
311
there may be dramatically large errors in the solution u(x, t).
To solve this difficulty, the most popular method is regularization [3, 9, 10, 17], i.e., using the solutions of well-posed problems to approximate the solutions of the original problems. A lot of authors deal with the above ill- posed problems by different methods. Roughly speaking, the methods involved are simplified Tikhonov regularization [4], Fourier method [2, 4], Wavelet Mayer method [2, 15], numerical method [1, 5, 13, 16, 8].
In [4], using simplified Tikhonov regularization, Fu discussed the convergence rate of the approximate solution to u(x, t) at 0 < x < 1 with g(t) replaced by g δ (t). Under the condition that ∥f∥ = ∥u(0, t)∥ ≤ E, the convergence rate of the approximate solution of the sideways parabolic equation may attain O(δ x ), 0 < x < 1. However, he did not use this method to investigate the convergence rate at the boundary x = 0. The present work is aimed to study the convergence rate of the approximation of u(x, t) and u x (x, t) for all 0 ≤ x < 1. In addition, for two-dimensional inverse heat conduction problems (IHCP), suppose the data at x = 0 are observed, we also need to get the information for 0 < x ≤ 1. Up to now, many authors put forward methods on this topic, we can refer to [11, 14, 18]. However, few authors have investigated the convergence rate. Here, by simplified Tikhonov regularization, we can obtain the convergence rate of the approximate solution exactly.
The structure of this paper is as follows. In Section 2, we present some definitions and theorems that we need for our results and give the convergence rates of approximation of u(x, t) and u x (x, t) for a sideways parabolic equation at 0 ≤ x < 1. The convergence rate of approximate solution of the two- dimensional inverse heat conduction problem for 0 < x ≤ 1 is outlined in Section 3 when the available data are inaccurate. Our results improve and generalize many known results in this field [4].
2. Convergence rate for sideways parabolic equations For brevity, the notation ∥ · ∥ denotes L 2 -norm, and
ˆ h(ξ) = 1
√ 2π
∫ + ∞
−∞
e −iξt h(t)dt is the Fourier transform of function h(t), then
h(t) = 1
√ 2π
∫ + ∞
−∞
e iξt ˆ h(ξ)dξ.
As we consider the problem in L 2 ( R) with respect to variable t, we extend u(x, ·), g(·) = u(1, ·), f(·) = u(0, ·) and other functions appearing in the section to be zero for t < 0. To obtain our convergence rate, we need the following assumptions and lemmas first. We assume that there exists a priori bound for the function f (t) = u(0, t):
(5) ∥f∥ ≤ E
or
(6) ∥f∥ p ≤ E, p ≥ 0,
where ∥f∥ p is defined by
∥f∥ p ≜
(∫ + ∞
−∞
(1 + ξ 2 ) p | ˆ f (ξ) | 2 dξ )
12.
Lemma 1 ([7]). Let v(x, ξ) be the solution of the following boundary value problem for ordinary differential equation
iξv(x, ξ) = a(x)v xx + b(x)v x + c(x)v, x > 0, ξ ∈ R, v(0, ξ) = 1,
x lim →∞ v(x, ξ) = 0, ξ ̸= 0
for ξ = 0 we require v(x, 0) be bounded as x tends to ∞. Suppose that the direct
problem
u t = a(x)u xx + b(x)u x + c(x)u, u(x, 0) = 0,
u(0, t) = f (t) has a solution u(x, t). Then
(7) u(x, t) = 1
√ 2π
∫ + ∞
−∞
e iξt v(x, ξ) ˆ f (ξ)dξ, x > 0 and
ˆ
u(x, ξ) = v(x, ξ) ˆ f (ξ).
Remark 1. From Lemma 1, it is obvious that if u is the solution of the above direct problem, then ˆ u(1, ξ) = v(1, ξ) ˆ f (ξ) = ˆ g(ξ) and ˆ g(ξ) = v(1,ξ) v(x,ξ) u(x, ξ). So, ˆ
ˆ
u x (x, ξ) = v x (x, ξ) ˆ f (ξ) = v x (x, ξ) v(1, ξ) ˆ g(ξ).
Lemma 2 ([7]). There exist constants c k , k = 1, 2, 3, 4, such that for x ∈ [0, 1]
and |ξ| large enough, say |ξ| ≥ ¯ξ, c 1 e −A(x)
√ |ξ|/2 ≤ |v(x, ξ)| ≤ c 2 e −A(x)
√ |ξ|/2 ; (8)
c 3
√ |ξ|e −A(x) √
|ξ|/2 ≤ |v x (x, ξ) | ≤ c 4
√ |ξ|e −A(x) √
|ξ|/2 , (9)
where A(x) = ∫ x 0
√ 1
a(s) ds. Especially, the right-hand side inequalities in (8) and (9) are valid for all ξ ∈ R with other constants c ′ 2 and c ′ 4 .
Lemma 3 ([7]). If the boundary value problem
a(x)v xx (x) + b(x)v x (x) + c(x)v(x) = 0, 0 < x < ∞;
v(0) = 1, v(x) is bounded as x → ∞
has a unique solution, then there exist constants c ′ 1 and c ′ 2 such that c ′ 1 e −A(1)
√ |ξ|/2 ≤ |v(1, ξ)| ≤ c ′ 2 e −A(1)
√ |ξ|/2 , ∀ξ ∈ R.
Refer to [4], for all 0 ≤ x < 1, we can define an operator K(x) : L 2 ( R) → L 2 ( R) by
K(x)h(x, ξ) = \ v(1, ξ) v(x, ξ)
ˆ h(x, ξ).
Let u(x, t) be the solution of (1)-(3). Then (1)-(3) can be rewritten as (10) K(x)u(x, t) = g(t), 0 ≤ x < 1.
Since (1)-(3) is ill-posed, as we all know, to solve this difficulty, we often use the solution of Tikhonov function
(11) min {∥K(x)h − g δ ∥ 2 + α ∥h∥ 2 }
over all h(x, ·) in L 2 ( R) to approximate to u(x, t) for 0 ≤ x < 1, where α > 0 is the regular parameter.
By mathematical analysis, we can easily get the following results.
Lemma 4. For 0 ≤ x ≤ 1, α > 0, there hold the inequalities:
(1) sup s ≥0 1+αe e(1−x)s2s ≤ α (x −1)/2 , sup s ≥0 1+αe exs2s ≤ α −x/2 ; (2) sup s ≥0 1+αe e(2−x)s2s ≤ α (x −2)/2 , sup s ≥0 e 1+αe(1+x)s2s ≤ α −(1+x)/2 . Definition 1 (cf. [4]). Let
≤ α −x/2 ; (2) sup s ≥0 1+αe e(2−x)s2s ≤ α (x −2)/2 , sup s ≥0 e 1+αe(1+x)s2s ≤ α −(1+x)/2 . Definition 1 (cf. [4]). Let
≤ α −(1+x)/2 . Definition 1 (cf. [4]). Let
(12) u δ (x, t) ≜ 1
√ 2π
∫ + ∞
−∞
e iξt (v(x, ξ)/v(1, ξ))ˆ g δ (ξ) 1 + α |1/v(1, ξ)| 2 dξ
and it is called a simplified Tikhonov approximate solution of u(x, t) of problem (1)-(3). Then ˆ u δx = (vx(x,ξ)/v(1,ξ))ˆ g
δ(ξ)
1+α |1/v(1,ξ)|
2.
In [4], for 0 < x < 1, Fu investigated the convergence rate of the above simplified Tikhonov approximate solution with α = ( E δ ) 2 under the condition that (5) holds,
(13) ∥u δ (x, ·) − u(x, ·)∥ ≤ Cδ
A(x)A(1)E 1 −A(x)A(1).
We are now in the position to formulate the convergence rate for all 0 ≤ x <
1.
Theorem 1. Suppose problem (1)-(3) has a unique solution, let u(x, t) given by (7) be the exact data at 0 ≤ x < 1, and u δ (x, t) be the simplified Tikhonov regularized approximation to u(x, t). In addition, assume that the measured history (noisy data) g δ (t) satisfy (4) and priori condition (6) be valid, then if α = ( E δ ) γ , 1 ≤ γ ≤ 2, there holds
∥u δ (x, ·)−u(x, ·)∥= O(δ 1 −γ/2 · δ
γA(x)2A(1))+O(δ γ −1 · δ
2A(1)A(x)(ln E δ ) −p+
A(x)p 2A(1)
)
(14)
+ O(δ
γA(x) 2A(1)
(ln E
δ ) −2p ), p ≥ 0, 0 ≤ x < 1.
Proof. The same argument as Theorem 2.4 in [4], we can obtain
∥ˆu(x, ·) − ˆu δ (x, ·)∥ 2 ≤ 2
∫ + ∞
−∞ |ˆg(ξ) − ˆg δ (ξ) | 2 I 1 dξ + 2α 2
∫ + ∞
−∞ | ˆ f (ξ) | 2 I 2 dξ
≜ J 1 + J 2 , where with 2s = √
2 |ξ|, C 1 , C 2 > 0, (15) I 1 = |v(x, ξ)/v(1, ξ)| 2
(1 + α |1/v(1, ξ)| 2 ) 2 ≤ C 1
( e (A(1) −A(x))s 1 + αe 2A(1)s
) 2
≤ C 1 α (A(x) −A(1))/A(1) ; and
(16) I 2 = |1/v(1, ξ)| 2 · |v(x, ξ)/v(1, ξ)| 2 (1 + α |1/v(1, ξ)| 2 ) 2 ≤ C 2
( e (2A(1) −A(x))s 1 + αe 2A(1)s
) 2
.
Thus, J 1 ≤ 2δ 2 sup ξ ∈R I 1 ≤ 2C 1 δ 2 α (A(x) −A(1))/A(1) = 2C 1 δ α2 · α
A(x)A(1). Next, it remains to give the estimation of J 2 .
Setting ξ 0 = 2[ 2A(1) 1 ln( E δ (ln E δ ) −p )] 2 , by Lemma 4, we come to the relation
J 2 ≤ 2C 2 α 2
∫ + ∞
−∞ | ˆ f (ξ) | 2
( e (2A(1) −A(x))s 1 + αe 2A(1)s
) 2
dξ
= 2C 2 α 2
∫
|ξ|≤ξ
0| ˆ f (ξ) | 2 (1 + ξ 2 ) p
[ e (2A(1) −A(x))s (1 + αe 2A(1)s )(1 + ξ 2 )
p2] 2 dξ
+ 2C 2 α 2
∫
|ξ|≥ξ
0| ˆ f (ξ) | 2 (1 + ξ 2 ) p
[ e (2A(1) −A(x))s (1 + αe 2A(1)s )(1 + ξ 2 )
p2] 2
dξ
≤ 2C 2 α 2 E 2 (e (2A(1) −A(x))s0| s0= √
= √
ξ
0/2 ) 2 + 2C 2 α 2 E 2 α A(x)/A(1) −2 ξ 0 −2p
= 2C 2 E 2 α 2 ( E
δ ) 2 −A(x)A(1)(ln E
δ ) −2p+A(x)pA(1) + 2C 2 E 2 ξ 0 −2p α A(x)/A(1)
= 2C 2 E 4 −
A(x) A(1)
( α
δ ) 2 δ
A(x) A(1)
(ln E
δ ) −2p+
A(x)p
A(1)
+ 2C 2 E 2 ξ −2p 0 α A(x)/A(1) . Consequently, with the help of Parseval equality,
∥u(x, ·) − u δ (x, ·)∥ 2
= ∥ˆu(x, ·) − ˆu δ (x, ·)∥ 2
≤ 2C 1
δ 2
α · α
A(x)A(1)+ 2C 2 E 4 −A(x)A(1)( α
δ ) 2 δ
A(x)A(1)(ln E
δ ) −2p+A(x)pA(1)
+ 2C 2 E 2 ξ 0 −2p α A(x)/A(1)
= O(δ 2 −γ · δ γA(x)/A(1) ) + O(δ 2(γ −1) δ A(x)/A(1) (ln E δ ) −2p+
A(x)p A(1)
)
+ O(δ γA(x)/A(1) (ln E δ ) −4p ).
Hence the assertion follows. □
Remark 2. From the discussion above, it follows that if γ = 2, p ≥ 0,
∥u(x, ·) − u δ (x, ·)∥ ≤ Cδ
A(x)A(1), 0 < x < 1, which is the optimal order (see [4]).
Remark 3. Especially, to get the convergence rate of the approximate solutions at x = 0, we only need to fix p > 0, 1 ≤ γ < 2.
In heat conduction applications, u(x, t) in (1)-(3) denotes the temperature, and u x (x, t) denotes its flux, thus it is also valuable to estimate the approxi- mation of u x (x, t).
Theorem 2. Suppose problem (1)-(3) has a unique solution, let u(x, t) given by (7) be the exact data at 0 ≤ x < 1, and u δ (x, t) be the simplified Tikhonov regularized approximation to u(x, t). In addition, assume that the measured history (noisy data) g δ (t) satisfy (4) and priori condition (6) with p ≥ 1/2 be valid, then if α = E δ , there holds
(17) ∥u δx (x, ·) − u x (x, ·)∥ = O(δ
14) + O(δ
2A(1)A(x)[(ln E
δ ) −p+A(x)p2A(1) + (ln E
δ ) 1 −2p ]).
Proof. Along the line of the proof of Theorem 2.4 in [4], we can obtain
|ˆu x (x, ·) − ˆu δx (x, ·)| 2 ≤ 2 | v v(1,ξ)x(x,ξ) | 2 · | ˆ g δ − ˆg| 2
[1 + α | v(1,ξ) 1 | 2 ] 2 + 2α 2 | v(1,ξ) 1 | 2 · | v v(1,ξ)x(x,ξ) | 2 · | ˆ f | 2 [1 + α | v(1,ξ) 1 | 2 ] 2
= 2 | ˆ g δ − ˆg| 2 I 1 + 2α 2 | ˆ f | 2 I 2 . By Lemma 2 and Lemma 3, with 2s = √
2 |ξ|, one has
I 1 = | v v(1,ξ)x(x,ξ) | 2
[1 + α | v(1,ξ) 1 | 2 ] 2 ≤ 2 ( c c4′
1
) 2 |ξ|e (A(1) −A(x)) √
2 |ξ|
[1 + ( c 1′
2
) 2 αe A(1)
√ 2 |ξ| ] 2
≤ 2 ( c c4′
1
) 2 |ξ|e (A(1) −A(x)) √
2 |ξ|
min {1, ( c 1′ 2
) 2 }[1 + αe A(1) √
2 |ξ| ] 2
≤ C 1
[ se (A(1) −A(x))s 1 + αe 2A(1)s
] 2
. Similarly,
I 2 = | v(1,ξ) 1 | 2 · | v v(1,ξ)x(x,ξ) | 2 [1 + α | v(1,ξ) 1 | 2 ] 2 ≤ C 2
[ se (2A(1) −A(x))s 1 + αe 2A(1)s
] 2
.
m M 0
1
Figure 1
Define p(s) ≜ e
A(1)2s −s. Then p min = p(s 0 ) | s
0=
A(1)2ln
A(1)2= A(1) 2 (1 −ln A(1) 2 ).
Thereby, if A(1) 2 ≤ e, then p min ≥ 0 and s ≤ e
A(1)2s , ∀s ∈ R + ; Else if A(1) 2 > e, from Figure 1, we know that there exist m = m(A(1)), M = M (A(1)) such that if s ≤ m or s ≥ M, s ≤ eA(1)2 s , and if m < s < M, s ≥ eA(1)2 s . Therefore, according to Lemma 4,
s . Therefore, according to Lemma 4,
I 1 ≤ C 1
[ se (A(1) −A(x))s 1 + αe 2A(1)s
] 2
≤ C 1 max
{[ M e (A(1) −A(x))s 1 + αe 2A(1)s
] 2
,
[ e 3A(1)s/2 1 + αe 2A(1)s
] 2 } (18)
≤ C 1 max {M 2 α
A(x)−A(1)A(1), 3
32α −3/2 }.
Remember that
∥ˆu x (x, ·) − ˆu δx (x, ·)∥ 2 ≤ 2
∫
R | ˆ g δ − ˆg| 2 I 1 dξ + 2α 2
∫
R | ˆ f | 2 I 2 dξ ≜ J 1 + J 2 . Here,
J 1 = 2
∫
R | ˆ g δ − ˆg| 2 I 1 dξ ≤ 2C 1 max {M 2 αA(x)−A(1)A(1) , 3
32α −3/2 }δ 2 = O(δ 1/2 );
(19)
J 2 = 2α 2
∫
R | ˆ f | 2 I 2 dξ (20)
≤ 2C 2 α 2
∫
R | ˆ f | 2 (1 + ξ 2 ) p
[ se (2A(1) −A(x))s (1 + αe 2A(1)s )(1 + 4s 4 ) p/2
] 2
.
Note that if 0 ≤ s ≤ 1, then s ≤ (1 + 4s 4 ) p/2 , i.e., (1+4s s4)
p/2 ≤ 1. And if s ≥ 1, we also have (1+4s s4)
p/2 ≤ (4s4s )
p/2 = 2 −p s 1 −2p ≤ 1.
)
p/2≤ (4s4s )
p/2 = 2 −p s 1 −2p ≤ 1.
Consequently, setting ξ 0 = 2[ 2A(1) 1 ln( E δ (ln E δ ) −p )] 2 , we get
J 2 ≤ 2C 2 α 2
∫
|ξ|≤ξ
0| ˆ f | 2 (1 + ξ 2 ) p
[ se (2A(1) −A(x))s (1 + αe 2A(1)s )(1 + 4s 4 ) p/2
] 2 (21)
+ 2C 2 α 2
∫
|ξ|≥ξ
0| ˆ f | 2 (1 + ξ 2 ) p
[ se (2A(1) −A(x))s (1 + αe 2A(1)s )(1 + 4s 4 ) p/2
] 2
≤ 2C 2 E 2 α 2 sup
|ξ|≤ξ
0[ e (2A(1) −A(x))s 1 + αe 2A(1)s
] 2
+ 2C 2 E 2 α 2 sup
|ξ|≥ξ
0[ se (2A(1) −A(x))s (1 + αe 2A(1)s )(1 + 4s 4 ) p/2
] 2
≤ 2C 2 E 2 α 2 (e (2A(1) −A(x))s0| s0= √
= √
ξ
0/2 ) 2 + 2C 2 E 2 α 2 αA(x)A(1)−2 s 2 0 −4p
= 2C 2 E 4 −A(x)A(1)( α
δ ) 2 δ
A(x)A(1)(ln E
δ ) −2p+A(x)pA(1) + 2C 2 E 2 s 2 0 −4p α
A(x)A(1)
= O(δ
A(x) A(1)
[(ln E
δ ) −2p+
A(x)p
A(1)
+ (ln E
δ ) 2 −4p ]).
Combing (18)-(20) with (21), we can get the assertion immediately. □
3. Convergence rate for two-dimensional inverse heat conduction problems
In this section, we study a two-dimensional inverse heat conduction problem in a semi-infinite slab [11, 14], i.e.,
u t (x, y, t) = u xx (x, y, t) + u yy (x, y, t), 0 < x < 1, y > 0, t > 0, (22)
u(0, y, t) = φ(y, t), y > 0, t > 0, (23)
with corresponding measured data function φ δ (y, t), u x (0, y, t) = 0, y ≥ 0, t ≥ 0, (24)
u(x, y, 0) = 0, 0 < x < 1, y > 0, (25)
u(x, 0, t) = 0, 0 < x < 1, t ≥ 0.
(26)
Now, we wish to determine the temperature u(x, y, t) for 0 < x ≤ 1 from temperature φ δ (y, t). In order to use some results from Fourier analysis, we extend the function u(x, ·, ·), φ(·, ·), φ δ ( ·, ·) and ψ(·, ·) = u(1, ·, ·) to whole real (y, t) plane by defining them to be zero everywhere in {(y, t), y < 0, t < 0}.
We also assume that these functions are in L 2 ( R 2 ) and use the corresponding
L 2 norm, as defined below
(27) ∥φ∥ =
(∫
R
2|φ(y, t)| 2 dydt )
12.
We now could assume that the measured data function φ δ (y, t) satisfies
(28) ∥φ − φ δ ∥ ≤ δ,
where δ > 0 represents a bound on the measurement error.
Let
(29) φ(ξ, τ ) = ˆ 1
2π
∫
R
2φ(y, t)e −i(ξy+τt) dydt be the Fourier transform of a function φ(y, t). Then
φ(y, t) = 1 2π
∫
R
2ˆ
φ(ξ, τ )e i(ξy+τ t) dξdτ.
Taking Fourier transformation to (22), then
bu xx (x, ξ, τ ) = (iτ + ξ 2 )ˆ u(x, ξ, τ ).
Suppose u is the solution of (22)-(26), we can easily get the solution by condi- tions (23) and (24) (one can refer to [5, 6, 12]), i.e.,
ˆ
u(x, ξ, τ ) = ˆ φ(ξ, τ ) cosh(xθ), 0 ≤ x ≤ 1, ξ, τ ∈ R, (30)
u(x, y, t) = 1 2π
∫
R
2ˆ
φ(ξ, τ ) cosh(xθ)e i(ξy+τ t) dξdτ, (31)
here θ is the principal value of √
iτ + ξ 2 :
θ = √
iτ + ξ 2 =
√√ τ 2 + ξ 4 + ξ 2
2 + isign(τ )
√√ τ 2 + ξ 4 − ξ 2
2 .
Setting a =
√√ τ2+ξ
4+ξ
2
2 , b =
√√ τ2+ξ
4−ξ
2
2 , σ = sign(τ ). Then θ = a + iσb. It is obvious that
ψ(ξ, τ ) = ˆ ˆ u(1, ξ, τ ) = ˆ φ(ξ, τ ) cosh θ.
Since | cosh(xθ)| is unbounded for 0 < x ≤ 1, from (31) we can see that small errors in the data can blow up and completely destroy the solution for 0 < x ≤ 1, thus the two-dimensional IHCP is ill-posed. Here, we use the simplified Tikhonov regularization to solve this difficulty.
Define K(x) : L 2 ( R 2 ) → L 2 ( R 2 ) by
(32) K(x)u(x, ξ, τ ) = \ u(x, ξ, τ ) ˆ cosh(xθ) . Then (22)-(26) can be rewritten as
K(x)u(x, y, t) = φ(y, t), 0 ≤ x < 1.
We use the solution of the following functional
(33) min
h(x, ·,·)∈L
2( R
2) J (x), J (x) = ∥K(x)h − φ δ ∥ 2 + α ∥h∥ 2 to approximate to u(x, y, t), where α > 0 is the regular parameter.
Lemma 5. There exists a unique solution to the above minimization problem (33). It is given by
(34) h δ (x, y, t) = 1 2π
∫
R
2e i(ξy+τ t) cosh(xθ) ˆ φ δ
1 + α | cosh(xθ)| 2 dξdτ.
Proof. Let I denote the identity operator in L 2 ( R 2 ) and K ∗ (x) be the adjoint of K(x). Then, the unique solution of the minimization problem (33) is given by
(35) h δ = [K ∗ (x)K(x) + αI] −1 K ∗ (x)φ δ . By Parseval formula, one has
(36) ⟨ \ K(x)u, ˆ v ⟩ = ⟨K(x)u, v⟩ = ⟨u, K ∗ (x)v ⟩ = ⟨ˆu, \ K(x) ∗ v ⟩.
According to (32),
⟨ \ K(x)u, ˆ v ⟩ = ⟨ 1
cosh(xθ) u, ˆ ˆ v ⟩ = ⟨ˆu, 1 cosh(xθ) v ˆ ⟩.
This immediately leads to,
K \ ∗ (x)v = 1 cosh(xθ) ˆ v.
Consequently,
K ∗ (x)K(x)v = \ 1
| cosh(xθ)| 2 v. ˆ In view of
K ∗ (x)K(x)h \ δ + αc h δ = K \ ∗ (x)φ δ ,
we obtain (
1
| cosh(xθ)| 2 + α )
ˆ h δ = 1 cosh(xθ) φ ˆ δ . It turns out that
ˆ h δ =
1 cosh(xθ) φ ˆ δ α + | cosh(xθ)| 1
2= cosh(xθ) ˆ φ δ 1 + α | cosh(xθ)| 2 .
Using the inverse Fourier transformation, we can get the assertion. □
Definition 2. Let
u δ (x, y, t) = 1 2π
∫
R
2e i(ξy+τ t) cosh(xθ) ˆ φ δ
1 + α | cosh θ| 2 dξdτ
and it is called a simplified Tikhonov approximate solution of u(x, y, t) of prob- lem (22)-(26).
Lemma 6 ([14]). If a ≥ b ≥ 0, x ≥ 0, τ ∈ R, then (1) | cosh(a + iσb)| ≥ ce a , 0 < c =
√ 1 −2e−π/2
2 < 1;
(2) | cosh(x(a + iσb))| ≤ e xa .
Theorem 3. Suppose problem (22)-(26) has a unique solution, let u(x, y, t) given by (31) be the exact data at 0 < x ≤ 1, and u δ (x, y, t) be the simplified Tikhonov regularized approximation to u(x, y, t). Besides, assume φ δ satisfy (28) and
(37) ∥ψ∥ p ≤ E, p ≥ 0,
where ∥ · ∥ p denotes the norm in Sobolev space H p ( R 2 ) defined by
∥ψ∥ p ≜ (∫
R
2(1 + ξ 2 + τ 2 ) p | ˆ ψ(ξ, τ ) | 2 dξdτ )
12. If α = ( E δ ) γ , 1 ≤ γ ≤ 2, then for ∀0 < x ≤ 1,
∥u δ (x, ·, ·) − u(x, ·, ·)∥
≤ O(δ (1 −γ/2)x + δ γ −(1+x)/2 · (ln E
δ ) −(x+1)p/2 + (ln E
δ ) −p δ γ(1 −x)/2 ).
Proof. Since
|ˆu δ − ˆu| 2 =
ˆφcosh(xθ) − ˆφ δ · cosh(xθ) 1 + α | cosh θ| 2
2
=
( ˆ φ − ˆ φ δ ) cosh(xθ) + α ˆ φ cosh(xθ) · | cosh θ| 2 1 + α | cosh θ| 2
2
≤ 2 | ˆ φ − ˆ φ δ | 2 · | cosh(xθ)| 2
[1 + α | cosh θ| 2 ] 2 + 2α 2 | ˆ φ cosh θ | 2 · | cosh θ| 2 · | cosh(xθ)| 2 [1 + α | cosh θ| 2 ] 2
= 2 | ˆ φ − ˆ φ δ | 2 · | cosh(xθ)| 2
[1 + α | cosh θ| 2 ] 2 + 2α 2 | ˆ ψ | 2 · | cosh θ| 2 · | cosh(xθ)| 2 [1 + α | cosh θ| 2 ] 2
≤ 2| ˆ φ − ˆ φ δ | 2 · I 1 + 2α 2 | ˆ ψ | 2 · I 2 , where
I 1 = | cosh(xθ)| 2
[1 + α | cosh θ| 2 ] 2 , I 2 = | cosh θ| 2 · | cosh(xθ)| 2 [1 + α | cosh θ| 2 ] 2 . By Lemma 4 and Lemma 6, we know that
I 1 ≤ |e xa |
(1 + αc 2 e 2a ) 2 ≤ c −2 |e xa | 2
(1 + αe 2a ) 2 ≤ c −2 α −x ;
I 2 ≤ |e a | 2 · |e xa | 2
(1 + αc 2 e 2a ) 2 ≤ c −2 |e (1+x)a | 2
(1 + αe 2a ) 2 ≤ c −2 α −(1+x) . Therefore,
∥ˆu δ (x, ξ, τ ) − ˆu(x, ξ, τ)∥ 2 ≤ 2
∫
R
2| ˆ φ − ˆ φ δ | 2 I 1 dξ + 2α 2
∫
R
2| ˆ ψ | 2 I 2 dξ (38)
≤ 2c −2 δ 2 α −x + 2α 2
∫
R
2| ˆ ψ | 2 I 2 dξ.
Setting m = 1 2 ln( E δ (ln E δ ) −p ), define Ω m = {(ξ, τ) ∈ R 2 | m ξ22 + 4m τ24 ≤ 1}.
≤ 1}.
It is easy to show that
(ξ, τ ) ∈ Ω m ⇔ a ≤ m and
(ξ, τ ) ∈ R 2 \ Ω m ⇒ (1 + ξ 2 + τ 2 ) −p2 ≤ m −p . 2α 2
∫
R
2| ˆ ψ | 2 I 2 dξ (39)
≤ 2c −2 α 2
∫
Ω
m| ˆ ψ | 2 (1 + ξ 2 + τ 2 ) p
{ e (1+x)a
(1 + αe 2a )(1 + ξ 2 + τ 2 )
p2} 2
+ 2c −2 α 2
∫
R
2\Ω
m| ˆ ψ | 2 (1 + ξ 2 + τ 2 ) p
{ e (1+x)a
(1 + αe 2a )(1 + ξ 2 + τ 2 )
p2} 2
≜ J 1 + J 2 .
Since 1 + ξ 2 + τ 2 ≥ 1, a ≤ m as (ξ, τ) ∈ Ω m and the function f (s) = 1+α s2s is increasing for s ≥ 0, then
J 1 ≤ 2c −2 α 2 E 2 sup
0 ≤a≤m
( e (1+x)a 1 + αe 2a
) 2 (40)
≤ 2α 2 E 2 c −2
( e (1+x)m 1 + αe 2m
) 2
≤ 2E 2 c −2 α 2 e 2(1+x)m
= 2E 2 c −2 α 2 ( E δ (ln E
δ ) −p ) 1+x
= C 1 α 2 δ −(1+x) · (ln E
δ ) −(1+x)p . And
J 2 ≤ 2c −2 α 2 E 2 sup
R
2\Ω
m{ e (1+x)a
(1 + αe 2a )(1 + ξ 2 + τ 2 )
p2} 2
(41)
≤ 2c −2 E 2 m −2p α 1 −x = 2 2p+1 c −2 E 2 [ln( E δ (ln E
δ ) −p )] −2p α 1 −x
= 2 2p+1 c −2 E 2 (ln E
δ − p ln(ln E
δ )) −2p α 1 −x ≤ C 2 (ln E
δ ) −2p α 1 −x .
Inserting (39)-(41) into (38), we get
∥ˆu δ (x, ξ, τ ) − ˆu(x, ξ, τ)∥ 2
≤ O(δ 2 α −x + (α 2 δ −(1+x) · (ln E
δ ) −(1+x)p + (ln E
δ ) −2p α 1 −x ). □
0 0.5 1 1.5 2 2.5 3 3.5 4
0 0.5 1 1.5 2 2.5 3 3.5
Exact solution Approximate solution
Figure 2. x = 0, p =
1
3 , E = ∥f∥13 ≤ 3, δ = 0.001.
0 0.5 1 1.5 2 2.5 3 3.5 4
0 0.2 0.4 0.6 0.8 1 1.2 1.4 1.6 1.8 2
Exact solution Approximate solution
Figure 3. x = 0.3, p = 1 3 , E = ∥f∥
13
≤ 3, δ = 0.001.
0 0.5 1 1.5 2 2.5 3 3.5 4
0 0.5 1 1.5
Exact solution Approximate solution
Figure 4. x = 0.5, p = 1 3 , E = ∥f∥
13≤ 3, δ = 0.001.
0 0.5 1 1.5 2 2.5 3 3.5 4
0 0.2 0.4 0.6 0.8 1 1.2 1.4
Exact solution Approximate solution
Figure 5. x = 0.7,
p = 1 3 , E = ∥f∥
13≤ 3,
δ = 0.001.
0 0.5
1
0 1 2 3 4 0 0.5 1 1.5 2 2.5 3 3.5
t x
Exact solution
0 0.5
1
0 2 4 0 0.5 1 1.5 2 2.5 3 3.5
t x
Tikhonve Regularization
Figure 6. x = 0, p = 1 3 , E = ∥f∥
13≤ 3, δ = 0.001.
0 0.5 1 1.5 2
0 1 2 3 4 5 6
Exact solution Tikhonov regularization
Figure 7. x = 0, p =
1
3 , E = ∥f∥13 ≤ 3, δ = 0.001.
0 0.5 1 1.5 2
0 0.5 1 1.5 2 2.5 3
Exact solution Tikhonov regularization
Figure 8. x = 0.5, p = 1 3 , E = ∥f∥
13≤ 3, δ = 0.001.
4. Numerical experiments Example 1. It is easy to verify that
u(x, t) = {
x+1
t
3/2e −(x+1)24t , t > 0, 0 ≤ x ≤ 1,
0, t ≤ 0,
0 0.5 1 1.5 2 0
0.5 1 1.5 2 2.5 3 3.5
Exact solution Tikhonov regularization
Figure 9. x = 0.3, p = 1 3 , E = ∥f∥
13≤ 3, δ = 0.001.
0 0.5 1 1.5 2
0 0.5 1 1.5 2 2.5
Exact solution Tikhonov regularization
Figure 10. x = 0.7, p = 1 3 , E = ∥f∥
13≤ 3, δ = 0.001.
0 0.5
1
0 1 2 3 4
−4
−2 0 2 4
t x
Exact solution
0 0.5
1
0 1 2 3 4
−4
−2 0 2 4
t x
Tikhonve Regularization
Figure 11. x = 0, p = 1 3 , E = ∥f∥
13