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DIFFERENTIATION AND INTEGRATION

BY USING MATRIX INVERSION

Dagmara Matlak, Jarosław Matlak, Damian Słota, Roman Wituła

Institute of Mathematics, Silesian University of Technology, Gliwice, Poland [email protected]

Abstract. In the paper certain examples of applications of the matrix inverses for

generat-ing and calculatgenerat-ing the integrals are presented.

Keywords: matrix inverse, integrals, generalized McLaurin’s formula

Introduction

The first part of our discussion concerns the linear mappings defined on the

finite-dimensional space of solutions of the following system of differential

equa-tions

=

,

+ ⋯ +

,

=

,

+ ⋯ +

,

=

,

+ ⋯ +

,

.

(1)

Suppose that functions

,

, … ,

form the solution of the above system of

equations and matrix

=

,

×

of system (1) is nonsingular. Let us consider

the linear mapping

of the linear space of solutions

,

, … ,

of system (1)

onto itself defined in the following way:

=

=

,

+ ⋯ +

,

,

+ ⋯ +

,

=

,

,

,

,

=

. (2)

Matrix

is nonsingular, so there exists its inverse

. In particular, the

follow-ing equality occurs:

=

.

(3)

(2)

Therefore, if

=

, then functions

are the primitive functions

of

(

= 1,2, … ,

)

.

The current article is inspired by Swartz’s paper [1] where the author gives

some simple examples of using this procedure, among others, for generating the

integrals of functions

= e

sin

,

=

cos

, for which he obtained the

formula (the integration constants are omitted and this rule will oblige

hencefor-ward):

=

!

=

ೌೣ మ

" #

$%#

#

+

$%# &

.

(4)

1. Generalization of Swartz’s example

Let us start from the generalization of the example mentioned above. Let us take

the functions

= cosh

sin

,

= cosh

cos

,

= sinh

cos

,

= sinh

sin

.

(5)

Note that the differentiation operator for these functions is of the form

'

(

=

)

*

+

,

=

-0

0

0

0

0

0

0

0

. '

(

.

(6)

If

≠ 0

, then the inverse of matrix of operator

has the form

=

-0

0

0

0

0

0

0

0

.

.

(7)

Now we can easily integrate functions

, e.g.

/

=

+

(3)

2. Integrals of

ܛܑܖ

for odd

Consider the second derivatives of functions

= sin

,

≥ 2

. We have

sin

=

sin

cos

=

− 1

sin

sin

.

(8)

Of course for

= 1

there is

sin

=

sin

. Thus we can write the second

derivative operator for the odd powers of function

sin

, from 1 to odd

0

, in the

following matrix form:

'

sin

sin

sin

(

=

)

*

sin

sin

1

sin

2

+

,

=

'

− sin

6 sin

− 9 sin

00

− 1

sin

0

sin

(

=

=

-−1

0

0

0

3 ∙ 2

−3

0

0

0

0

00

− 1

0

. '

sin

sin

sin

(

.

(9)

The determinant of the obtained matrix is equal to:

det

= (−1)

ೖశభ

(

0

‼)

≠ 0,

0

3

. The inverse matrix is of the form

=

, ೖశభ మ × ೖశభ మ

,

(10)

where

,

=

0,

<

4

,

,

=

4

,

‼ ‼ ‼ ‼

,

>

4

.

(11)

We can deduce that for odd

there occurs (with respect to the linear element):

sin

= −

‼ ‼

()‼ ()‼

sin

,

(12)

where

: =

. For example, we get

sin

= −

sin

sin

sin

.

(13)

We note that from (12) by differentiating we obtain (see [2, 3]):

sin

= −

‼ ‼

cos

()‼ ()‼

sin

.

(14)

(4)

For example, we have

sin

= −

cos

(1 +

sin

+

sin

)

.

3. The case of the even powers of

ܛܑܖ ࢞

Consider functions of the form

= sin

೙షభ೙

sin

,

(15)

for

= 2,4,6, …

. Acting on the vector

'

(

, where

0

is even, with the second

derivative operator, like it was done in equation (9), we get the following

transfor-mation matrix:

6

'

(

=

'

(

=

=

-−2

0

0

0

2

∙ 3 4

−4

0

0

0

0

0

− 2

0

− 1

0

0

.'

(

.

(16)

The above matrix is invertible and its inversion is of the form

6

=

, ೖ మ× ೖ మ

,

(17)

where

,

=

0,

<

4

,

,

=

4

,

మ ‼ ‼ ‼ ‼

,

>

4

.

(18)

Therefore for even

n

we get the formula (exact to the linear element):

=

‼ ‼మ

‼ ‼

"

sin

sin

&

=

‼ ‼మ

"

‼ ‼

sin

− 1 +

+

sin

‼ ‼

‼ ‼

&

=

‼ ‼మ

sin

= −

sin

,

(19)

(5)

which implies the following integral identity

sin

=

‼ ‼

"

+

‼ ()‼ ⁄

&

=

‼ ‼

"

‼ ()‼()మ ⁄

sin

&

.

(20)

Hence, by differentiating we get (see [2, 3]):

sin

=

‼ ‼

"

cos

‼ ()‼ ⁄

sin

&

.

(21)

For example, we obtain

sin

=

cos

"

sin

+

sin

+

sin

&!

.

(22)

4. Integral of

ܜ܉ܖ

Let

8

be the linear space of sequences

9

:

of differentiable functions

: (

,

) →

;

. Let

<

:

8

8

be a linear operator satisfying equation

'

tan

tan

tan

(

=

< '

1

tan

tan

(

.

(23)

If

<

is represented by infinite matrix

, then from (23) matrix

has the form

=

-1

0

1

0

0

0

2

0

2

0

0

0

3

0

3

.

.

(24)

It is easy to show that

=

=

>

>

>

?

1

0

0

0

0

0

0

0

0

0

⋯@

A

A

A

B

.

(25)

However, matrix

does not represent the inverse operator

<

, since the

fol-lowing relations hold

(6)

'

tan

tan

tan

(

=

-1

0

0

0

−1

0

0

0

0

1

0

0

0

−1

0

0

0

0

1

0

0

0

−1

0

. '

1

tan

tan

(

, (26)

resulting from the formula

"

tan

tan

&

= tan

− tan

.

(27)

Moreover, we get from this, after summing over powers in the interval

,

and

by uniform convergence (see [4]), that

tan

=

"

tan

tan

&

,

(28)

or equivalently

tan

CC

=

"

tan

tan

&

=

tan

,

(29)

for every

,

and

= 0,1,2, …

.

From formula (28) we also get the matrix form

D<

of operator

<

, i.e. the

inverse operator of operator

<

(under assumption of its existence):

D<

=

=

>

>

>

>

>

>

?

1

0

0

0

0

0

0

0

0

0

0

0

0

0

0

0

0

@

A

A

A

A

A

A

B

.

(30)

Formula (29) is our main analytic result in this section. Why do we think so?

Because, as we show now, this formula is a generalization of the classical

MacLaurin’s formulae for

ln(

+ 1)

, i.e.

ln

+ 1

=

+

+ ⋯

,

(31)

for

−1 <

≤ 1

, found independently by Nicolaus Mercator and Saint-Vincent

(see sections 10-9 and 10-10 in [5] and page 387 in [6]), and for

arctan

, i.e.

arctan

=

+

− ⋯

,

(32)

(7)

This connection should not be surprising because of the known complex

rela-tion (see [7]):

arctan

E

=

ln

"

&

,

(33)

where

E

(−∞, −1] ∪ [1, ∞)

and where the principal branch of the

loga-rithm is under consideration. On the cuts we have

arctan(

C

) = ±

+

ln

"

&

,

(34)

for

C

∈ (−∞, −1) ∪ (1, ∞)

and where the upper/lower sign corresponds to the

right/left side of the set determining

C

. More precisely, the connection between the

arctan function and log function is obvious and the section concerns the real and

imaginary parts of

arctan

E

, since we have

arctan

E

=

arctan

"

&

+

ln

"

మ మ

&

,

(35)

where

E

=

+

C

,

|E|

< 1

. First, from equation (29) for

= 1

we get

− ln cos

=

tan

()

(36)

or

ln cos

1

arctan

√2

=

,

(37)

which by (31) implies the well known identity (since

cos

H

=

√ !"మ#

for

H

"

,

&

):

ln cos

1

arctan

√2

= −

ln

+ 1

,

(38)

i.e.

+ 1 cos

arctan

≡ 1

,

(39)

for every

I

0,1

J

.

But this formula holds for every

≥ 0

since

cos

H

=

√ !"మ#

for every

H

"

,

&

. In other words, formula (37) is equivalent to (31). For

= 0

from

(29) we get

!$% !"

=

&మ 'ೖ

,

(40)

(8)

which implies (32). Hence, for

= 1

we obtain

= 1 −

+

(

+ ⋯

(41)

That is the classical Gregory-Leibniz-Nilakantha’s formula (see [8]).

Generaliza-tions of the Gregory power series (32) are discussed in papers [9] and [10].

As seen from equation (29), the values of integrals

tan

ഏ ర

for

≥ 2

are

the translations of numbers

tan

or

ഏ ర

, depending on parity of

. For

even

we have

tan

=

ഏ ర

()ೖ ()⁄ ഏ ర

=

()ೖ ()⁄

,

(42)

whereas for odd

we get

tan

=

tan

ഏ ర

()ೖ ()⁄ ഏ ర

=

"

ln 2 −

()ೖ ()⁄

&

.(43)

5. Final remark

Some other applications of the matrix obtained by n-times differentiation of

product functions and composition functions are discussed in paper [11]. In turn, in

paper [12] the technique of the inverse matrix was used for calculating the integral

sec

, similarly as in the present study. The obtained formulae were used

there for generating the trigonometric identities.

References

[1] Swartz W., Integration by matrix inversion, Amer. Math. Monthly 1958, 65, 282-283.

[2] Prudnikov A.P., Bryczkov J.A., Mariczev O.J., Integrals and Series, Elementary Functions, Vol. 1, Nauka Press, Moscov 1986 (in Russian).

[3] Prudnikov A.P., Bryczkov J.A., Mariczev O.J., Integrals and Series, Complements Sections, Vol. 2, Nauka Press, Moscow 1986 (in Russian).

[4] Kołodziej W., Mathematical Analysis, PWN, Warsaw 1979 (in Polish).

[5] Eves H., An Introduction to the History of Mathematics, Holt, Rinehart and Winston, New York 1969.

[6] Boyer C. (revised by Merzbach U.), A History of Mathematics, Wiley, New York 1991. [7] Olver F.W.J., Lozier D.W., Boisvert R.F., Clark C.W., NIST Handbook of Mathematical

Func-tions, Cambridge Univ. Press, Cambridge 2010.

[8] Wituła R., Number π, its History and Influence on Mathematical Creativeness, Wyd. Pracowni

(9)

[9] Gawrońska N., Słota D., Wituła R., Zielonka A., Some generalizations of Gregory’s power series and their applications, J. Appl. Math. Comput. Mech. 2013, 12(3), 79-91.

[10] Wituła R., Hetmaniok E., Pleszczyński M., Słota D., Generalized Gregory’s series (in review). [11] Redheffer R., Induced transformations of the derivative - vector, Amer. Math. Monthly 1976,

83, 255-259.

[12] Wituła R., Matlak D., Matlak J., Słota D., Use of matrices in evaluation of ׬secଶ௡ାଵݔ ݀ݔ in review.

References

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