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Handbook of mathematics for engineers and scienteists part 205 ppt

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To solve this integral equation, direct and inverse Laplace transforms are used.. The right-hand side f x of the integral equation must satisfy certain relations... The integral equation

Trang 1

1 To solve this integral equation, direct and inverse Laplace transforms are used The

solution can be represented in the form

y (x) = f (x) –

 x

Here the resolvent R(x) is expressed via the kernel K(x) of the original equation as follows:

R (x) = 1

2πi

 c+i∞

c–i∞

2

R (p)e px dp, R2(p) = K2(p)

1+ 2K (p),

2

K (p) =



0 K (x)e

px dx.

2◦ Let w = w(x) be the solution of the simpler auxiliary equation with a =0and f ≡ 1:

w (x) +

 x

Then the solution of the original integral equation with arbitrary f = f (x) is expressed via

the solution of the auxiliary equation (2) as

y (x) = d

dx

 x

a w (x – t)f (t) dt = f (a)w(x – a) +

 x

a w (x – t)f



t (t) dt.

T11.3 Linear Equations of the First Kind

with Constant Limits of Integration

1.

 b

a |x– t| y(t) dt = f (x), 0a < b < ∞.

Solution:

y (x) = 12f 

xx (x).

The right-hand side f (x) of the integral equation must satisfy certain relations The general form of f (x) is as follows:

f (x) = F (x) + Ax + B,

A= –12

F 

x (a) + F x  (b)

, B = 12

aF 

x (a) + bF x  (b) – F (a) – F (b)

,

where F (x) is an arbitrary bounded twice differentiable function (with bounded first

deriva-tive)

2.

 a

0

y(t)

|x– t| dt = f (x), 0 < a∞.

Solution:

y (x) = – A

x1 4

d dx

 a

x

dt

(t – x)1 4

 t

0

f (s) ds

s1 4(t – s)1 4



8πΓ2(3/4).

Trang 2

 b

a

y(t)

|x– t| k dt = f (x), 0 < k < 1.

It is assumed that|a|+|b|<∞ Solution:

y (x) = 1

2π cot(12πk) d

dx

 x

a

f (t) dt (x – t)1–k

1

π2 cos2(12πk)

 x

a

Z (t)F (t) (x – t)1–k dt,

where

Z (t) = (t – a)1+k2 (b – t)1–k2 , F (t) = d

dt

 t

a

(t – τ ) k

 b

τ

f (s) ds

Z (s)(s – τ )1–k



4.

 b

0

y(t)

|xλ – t λ|k dt = f (x), 0 < k < 1, λ> 0.

Solution:

y (x) = –Ax λ(k–21) d

dx

" b

x

t λ(3 – 2k)–2

(t λ – x λ)1–2k

 t

0

s λ(k+1 )– 2

2 f (s) ds (t λ – s λ)1–2k

# ,

A= λ

2

2π cos



πk

2



Γ(k)

 Γ

1

+ k

2

–2 , whereΓ(k) is the gamma function.

5.



–∞

y(t)

|x– t|1–λ dt = f (x), 0 < λ < 1.

Solution:

y (x) = λ

2π tan

πλ 2

 

–∞

f (x) – f (t)

|x – t|1 +λ dt.

It assumed that the condition ∞

|f (x)| p dx<∞ is satisfied for some p,1< p <1

6.



sign(x – t)

|x– t|1–λ y(t) dt = f (x), 0 < λ < 1.

Solution:

y (x) = λ

2π cotπλ

2

 

f (x) – f (t)

|x – t|1 +λ sign(x – t) dt.

7.



–∞

a + b sign(x – t)

|x– t|1–λ y(t) dt = f (x), 0 < λ < 1.

Solution:

4π

a2cos2 1

2πλ

+ b2sin2 12πλ 

 –∞

a + b sign(x – t)

|x – t|1 +λ



f (x) – f (t)

dt

Trang 3



0

y(x + t) – y(x – t)

Solution: y(x) = – 1

π2



0

f (x + t) – f (x – t)

 In equations T11.3.9 and T11.3.10 and their solutions, all singular integrals are

under-stood in the sense of the Cauchy principal value.

9.



y(t) dt

t – x = f (x).

Solution: y(x) = – 1

π2



f (t) dt

t – x .

The integral equation and its solution form a Hilbert transform pair (in the asymmetric form)

10.

 b

a

y(t) dt

t – x = f (x).

This equation is encountered in hydrodynamics in solving the problem on the flow of an

ideal inviscid fluid around a thin profile (axb) It is assumed that|a|+|b|<∞.

1 The solution bounded at the endpoints is

y (x) = – 1

π2

(x – a)(b – x)

 b

a

f (t)

(t – a)(b – t)

dt

t – x,

a

f (t) dt

(t – a)(b – t) =0

2◦ The solution bounded at the endpoint x = a and unbounded at the endpoint x = b is

y (x) = – 1

π2

x – a

b – x

 b

a

b – t

t – a

f (t)

t – x dt.

3 The solution unbounded at the endpoints is

π2

(x – a)(b – x)

 b

a

(t – a)(b – t)

t – x f (t) dt + C

 ,

where C is an arbitrary constant The formula  b

a y (t) dt =

C

π holds

11.

 b

a e

λ|x–t|y(t) dt = f (x), ∞ < a < b < ∞.

Solution:

y (x) = 1

2λ



f 

xx (x) – λ2f (x)

The right-hand side f (x) of the integral equation must satisfy certain relations The

general form of the right-hand side is given by

f (x) = F (x) + Ax + B,

bλ – aλ –2



F 

x (a) + F x  (b) + λF (a) – λF (b)

, B = –1

λ



F 

x (a) + λF (a) + Aaλ + A

,

where F (x) is an arbitrary bounded, twice differentiable function.

Trang 4

 b

a ln|x– t| y(t) dt = f (x).

Carleman’s equation.

1◦ Solution for b – a≠ 4:

π2

(x – a)(b – x)

 b

a

(t – a)(b – t) f t  (t) dt

1

ln1

4(b – a)



 b

a

f (t) dt

(t – a)(b – t)



2◦ If b – a =4, then for the equation to be solvable, the condition

 b

a f (t)(t – a)

– 1 2(b – t)– 1 2dt=0

must be satisfied In this case, the solution has the form

π2

(x – a)(b – x)

 b

a

(t – a)(b – t) f t  (t) dt

 ,

where C is an arbitrary constant.

13.

 b

a ln|x– t| + β

y(t) dt = f (x).

By setting

x = eβ z, t = eβ τ, y (t) = Y (τ ), f (x) = eβ g (z),

we arrive at an equation of the form T11.3.12:

 B

A ln|z – τ|Y (τ ) dτ = g(z), A = ae β , B = be β

14.

 a

a



ln A

|x– t|



y(t) dt = f (x), –axa.

Solution for 0< a <2A:

y (x) = 1

2M  (a)



d da

 aa w (t, a)f (t) dt



w (x, a)

– 1 2

 a

|x| w (x, ξ)

d dξ

 1

M  (ξ)

d dξ

 ξ –ξw (t, ξ)f (t) dt



– 1 2

d dx

 a

|x|

w (x, ξ)

M  (ξ)

 ξ –ξw (t, ξ) df (t)



, where the prime stands for the derivative and

M (ξ) =



ln2A ξ

–1 , w (x, ξ) = M (ξ)

π

ξ2– x2.

Trang 5

 a

0

ln

x x + t – ty(t) dt = f(x).

Solution:

y (x) = – 2

π2

d dx

 a

x

F (t) dt

t2– x2, F (t) =

d dt

 t

0

sf (s) ds

t2– s2.

16.



0

cos(xt)y(t) dt = f(x).

Solution: y(x) = 2

π



0 cos(xt)f (t) dt.

Up to constant factors, the function f (x) and the solution y(t) are the Fourier cosine

transform pair

17.



0

sin(xt)y(t) dt = f(x).

Solution: y(x) = 2

π



0 sin(xt)f (t) dt.

Up to constant factors, the function f (x) and the solution y(t) are the Fourier sine

transform pair

18.

 π/2

0

y(ξ) dt = f (x), ξ = x sin t.

Schl¨omilch equation.

Solution:

y (x) = 2

π



f(0) + x π/2



ξ (ξ) dt

 , ξ = x sin t.

19.

 2π

0

cot t – x

2



y(t) dt = f (x), 0x2π.

Here the integral is understood in the sense of the Cauchy principal value and the right-hand side is assumed to satisfy the condition 2π

0 f (t) dt =0

Solution:

y (x) = – 1

4π2

 2π

0 cot

t – x 2



f (t) dt + C, where C is an arbitrary constant.

It follows from the solution that

 2π

0 y (t) dt =2πC The equation and its solution form a Hilbert transform pair (in the asymmetric form)

20.



0

tJ ν (xt)y(t) dt = f(x), ν > – 1 2

Here, J ν (z) is the Bessel function of the first kind.

Solution:

y (x) =



0 tJ ν (xt)f (t) dt.

The function f (x) and the solution y(t) are the Hankel transform pair.

Trang 6



∞ K0 |x– t| y(t) dt = f (x).

Here, K0(z) is the modified Bessel function of the second kind.

Solution:

y (x) = – 1

π2



d2

dx2 –1 

∞ K0 |x – t| f (t) dt.

22.



∞ K(x – t)y(t) dt = f (x).

The Fourier transform is used to solve this equation

1 Solution:

y (x) = 1

2π



2f(u)

2

K (u) e iux du, 2f(u) = √1

2π

 ∞ f (x)e

iux dx, K2(u) = √1

2π

 ∞ K (x)e

iux dx.

The following statement is valid Let f (x)  L2(–∞, ∞) and K(x)  L1(–∞, ∞).

Then for a solution y(x)L2(–∞, ∞) of the integral equation to exist, it is necessary and

sufficient that 2f (u)/ 2 K (u)L2(–∞, ∞).

2◦ Let the function P (s) defined by the formula

1

P (s) =

 ∞ e

–stK (t) dt

be a polynomial of degree n with real roots of the form

P (s) =

1– s

a1



1– s

a2



.



1– s

a n

 Then the solution of the integral equation is given by

y (x) = P (D)f (x), D= d

dx

23.



0

K(x – t)y(t) dt = f (x).

Wiener–Hopf equation of the first kind This equation is discussed in the books by Gakhov

and Cherskii (1978), Mikhlin and Pr¨ossdorf (1986), Muskhelishvili (1992), and Polyanin and Manzhirov (1998) in detail

T11.4 Linear Equations of the Second Kind

with Constant Limits of Integration

1. y(x) – λ

 b

a (x – t)y(t) dt = f(x).

Solution:

y (x) = f (x) + λ(A1x + A2),

Trang 7

A1= 12f1+6λ (f1Δ2–2f2Δ1)

λ2Δ4

–12f2+2λ(3f2Δ2–2f1Δ3)

λ2Δ4

f1=

 b

a f (x) dx, f2=

 b

a xf (x) dx, Δn= b n – a n

2. y(x) + A

 b

a |x– t| y(t) dt = f (x).

1◦ For A <0, the solution is given by

y (x) = C1cosh(kx) + C2sinh(kx) + f (x) + k

 x

a sinh[k(x – t)]f (t) dt, k=

–2A, (1)

where the constants C1and C2are determined by the conditions

y 

x (a) + y  x (b) = f x  (a) + f x  (b),

y (a) + y(b) + (b – a)y x  (a) = f (a) + f (b) + (b – a)f x  (a). (2)

2◦ For A >0, the solution is given by

y (x) = C1cos(kx) + C2sin(kx) + f (x) – k

 x

a sin[k(x – t)]f (t) dt, k=

2A, (3)

where the constants C1and C2are determined by conditions (2)

3◦ In the special case a = 0and A > 0, the solution of the integral equation is given by formula (3) with

C1= k Is(1+ cos λ) – Ic(λ + sin λ)

2+2cos λ + λ sin λ , C2= k

Issin λ + Ic(1+ cos λ)

2+2cos λ + λ sin λ ,

k=

2A , λ = bk, Is=

 b

0 sin[k(b – t)]f (t) dt, Ic =

 b

0 cos[k(b – t)]f (t) dt.

 In equations T11.4.3 and T11.4.4 and their solutions, all singular integrals are

under-stood in the sense of the Cauchy principal value.

3. Ay(x)+ B

π

 1

–1

y(t) dt

t – x = f (x), –1 < x < 1.

Without loss of generality we may assume that A2+ B2=1

1 The solution bounded at the endpoints:

y (x) = Af (x) – B

π

 1 – 1

g (x)

g (t)

f (t) dt

t – x , g (x) = (1 + x) α(1– x)1–α, (1)

where α is the solution of the trigonometric equation

on the interval0< α <1 This solution y(x) exists if and only if 1

– 1

f (t)

g (t) dt=0

... (x)

The right-hand side f (x) of the integral equation must satisfy certain relations The

general form of the right-hand side is given by

f (x) =...

Wiener–Hopf equation of the first kind This equation is discussed in the books by Gakhov

and Cherskii (1978), Mikhlin and Prăossdorf (1986), Muskhelishvili (1992), and Polyanin and Manzhirov... y (t) dt =2πC The equation and its solution form a Hilbert transform pair (in the asymmetric form)

20.



0

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