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Matrix Representation of a Star
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Journal of Applied & Computational Mathematics

ISSN: 2168-9679

Open Access

Research - (2020) Volume 9, Issue 4

Matrix Representation of a Star

Mohamed Moktar Chaffar*
*Correspondence: Mohamed Moktar Chaffar, Lycee Georges Brassens Villeneuve-le-Roi France and Temporary Professor at the University of Paris-Est Cr eteil (Paris 12) and at the Galilee Villetaneuse Institute (Paris 13), Paris, France, Tel: 0642448449, Email:
Lycee Georges Brassens Villeneuve-le-Roi France and Temporary Professor at the University of Paris-Est Cr eteil (Paris 12) and at the Galilee Villetaneuse Institute (Paris 13), Paris, France

Received: 23-May-2020 Published: 02-Jun-2020 , DOI: 10.37421/2168-9679.2020.9.448
Copyright: © 2020 Mohamed Moktar Chaffar. This is an open-access article distributed under the terms of the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited.

Abstract

In the present paper we define an oriented Star with imageα coefficient α 1 and we further develop the procedure for finding eigenvalues and eigenvectors for an (5 × 5) Starmatrix directly or (5 × 5) Star-matrix indirectly. we give an overview of the methods to compute matrix-multiplication of a Star image α (generally square 5 × 5) with particular emphasis on the oriented matrix.

Keywords

Matrix orientation • Coefficient star-matrix

Introduction

In this article, we propose a matrix representation of an oriented star with α coefficient imageα [1] and define two directions of orientation. It is therefore possible to orient a star with imageα coefficient α in two different ways, directly and indirectly (Figure 1).

applied-computational-mathematics

Figure 1.

A star with α coefficient is composed of five numbers outside a, b, c, d, e and five numbers inside T1, T2, T3, T4, T5, These last five numbers are written in the form of 5-tuple (T1, T2, T3, T4, T5) (Figure 2).

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Figure 2a.

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Figure 2b.

The scalars α are called the star coefficient if α is a solution of equation α = T1 (α) + T2(α) + T3(α) + T4(α) + T5(α) (Noted by αimage), a vector (T1, T2, T3, T4, T5) is called a solution vector of this Star-System with coefficient α in five unknowns.

The present paper is organized as follows: In Section 2, we present some preliminary results and notations that will be useful in the sequel. In Section 3, we will use the convention here that the star imageα has a positive or a negative (picture 1) orientation besides orientation of a star imageα. Another way to think of a positive orientation is that as we traverse the path following the positive orientation the star imageα must always be on the left (that is, one may also speak of orientation of a (5 × 5) matrix, polynomial of degree 5, etc.). We present some examples of Star-matrix directly or indirectly.

Some Basic Definitions and Notations

In this section, we introduce some notations and star-system with coefficient α defined.

A star-system with coefficient α

Definition 1: Let a, b, c, d, and e and α be real numbers, and let T1, T2, T3, T4, T5 be unknowns (also called variables or indeterminates). Then a system of the form

image

is called a star-system with coefficient α in five unknowns. We have also noted image [a, b, c, d, e; α] = α. The scalars a, b, c, d, e is called the coefficients of the unknowns, and α is called the constant “Chaff” of the star-system in five unknowns.

A vector (T1, T2, T3, T4, T5) in R5 is called a star-solution vector of this star-system

If and only if image[a, b, c, d, e; α] = α.

The solution of a Star-system is the set of values for T1, T2, T3, T4 and T5 that satisfies five equations simultaneously.

A star-element

A star-element is a term of the five-tuple (T1, T2, T3, T4, T5) solution of a star-system image[a, b, c, d, e; α] = α, where (T1, T2, T3, T4, T5) ∈ R5.

Star-Coefficient or Constant “Chaff”

The star-Coefficient or Constant”Chaff” is also noted by α? and is a solution of equation α= T1(α )+T2 (α )+T3 (α )+T4 (α )+T5 (α ), where (T1, T2, T3, T4, T5) is solution of a star-system image [a, b, c, d, e; α] = α.

Star-matrix

The star-system with coefficient α can be written in matrix form

image

Mimage or MStaris called the star-Matrix of the star-system with coefficient α (image[a, b, c, d, e; α] = α).

Mimage a matrix is said to be of dimension 5 × 5. A value called the determinant of Mimage that we denote by |MStaris| or |Mimage|, corresponds to square matrix Mimage. Consequently, the determinant of Mimage is |Mimage| = 2.

Set-star

The set-star is constructed from the solution set of linear star-system with coefficient α ([a, b, c, d, e; α] = α). The Set-star will be noted by Simage

Star-System equivalent

Equivalent Star-Systems are those systems having exactly same solution, i.e. two star-systems are equivalent if solution of on star system is the solution of other, and vice-versa.

Parameterized curves

A parameterized differentiable curve is simply a specific subset of R5 with which certain aspects of differential calculus can be applied.

Definition 2: A parameterized differentiable curve is a differentiable map α: I → R5 of an open interval I = (a, b) of the real line R in to R5

Regular curves

A parameterized differentiable curve α: I → R5, We call any point that satisfies α 0 (t) = 0 a singular point and we will restrict our study to curves without singular points.

Definition 3: A parametrized differentiable curve is a differentiable α: I → R5 is said to be regular if α'(t)≠0 for all t ∈ I

Parametric arclength

Generalized, a parametric arclength starts with a parametric curve in R5. This is given by some parametric equations T1(t), T2(t), T3(t), T4(t), T5(t), where the parameter t ranges over some given interval. The following formula computes the length of the arc between two points a, b.

Lemma 1: Consider a parametric curve T1(t),T2(t),T3(t),T4(t),T5(t), where t ∈ (a, b). The length of the arc traced by the curve as t ranges overt (a, b) is

image

Thereafter I start with several examples with detailed solutions are presented.

Orientation of a Star with Coefficient A and Matrix Multiplication

Orientation of a Star

In this section, We choose two directions of travel on this Star with coefficient α can be classified as negatively oriented (clockwise), positively oriented ( counterclockwise).

Where image+ is a star oriented contraclockwise (positively oriented) (Figure 3):

applied-computational-mathematics

Figure 3a.

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Figure 3b.

In the first case, one obtains a new matrix noted image called the star matrix directly

image

We note image- is a star oriented clockwise (negatively oriented) (Figure 4):

applied-computational-mathematics

Figure 4.

In the second case, one obtains a new matrix noted image - called the star matrix indirectly

image

Image of a five prime numbers.

Example 1: We consider the Star-System with coefficient image [3,7,11,13,17; α] = α of Linear Equations, we can easily solve this using Star- Matrix image (Figure 5).

applied-computational-mathematics

Figure 5.

image

The solution of the Star-system image is therefore image

So the overall solution is the star-set: imageimage

in a particular case if image Then

• The Star-coefficient:image

• The star-element is (2,18,−4,10,8) (Figure 6)

applied-computational-mathematics

Figure 6.

image

and the star matrix indirectly

image

The determinant of a matrix image is denoted detimage, after numerous calculations det image 1181 is a prime number because it has only two distinct divisors: 1 and itself (1181).

The characteristic polynomial of a matrix image

image

The characteristic polynomial of a matrix image noted image

image

image

image

Where

image

called the matrix multiplication or chaffar-matrix. These results verified:

image

image

A Surprise Result image where one of the eigenvalues is repeated noted

image

Now we look at matrix image where one of the eigenvalues is repeated noted image We shall see that this.

Eigenvalues: imageimage

image

image

Investigate carefully the eigenvectors associated with the repeated eigenvalue

image

The eigenvectors associated with the eigenvalue image =41.2085820470714

image

The eigenvectors associated with the eigenvalue image8.91508947299477

image

The eigenvectors associated with the eigenvalue image 8.91508947299477

image

The eigenvectors associated with the eigenvalue image 11.2856288661062

image

The Eigenvalues of matrix image α2- =0.12957478575019, α3-=41.8947762503062, α4=−14.0769629109033,

image

The eigenvectors associated with the repeated eigenvalue image=0.12957478575019

image

The eigenvectors associated with the eigenvalue image =41.8947762503062

image

The eigenvectors associated with the eigenvalue image−14.0769629109033

image

The conclusion is that since image is 5×5 and we can obtain five linearly

Independent eigenvectors then image be diagonalized.

On the other hand

image

image

Matrix multiplication and Star-function

As we will see in the next subsection, matrix multiplication exactly corresponds to the composition of the corresponding linear transformations.

Example 2. Let α ∈R , for all t ∈R the star-system image[t,2t,3t,4t,5t;α]= α has a unique solution

image

So the overall solution is the Star-set:

image

If image Then

• The Star-coefficient: α* =10t

• The star-function: (t,5t,−t,3t,2t) (Picture 7)

In the special case t=3

• The Constant”Chaff”: α = 30

• The Star-set: image

The star matrix directly

image

The star matrix indirectly

image

After numerous calculations det image ×243, 243 is a prime number.

The characteristic polynomial of a matrix image

image

The characteristic polynomial of a matrix image

image

The following product was obtained from the two matices imageimage

we get the following matrix:Called Chaffar-matrix

image

It should be hard to believe that our complicated formula for matrix multiplication actually means something intuitive such as chaining two transformations together.

Let image and image be linear transformations, and let image andimage be their standard matrices, respectively, soimage is is an 5×5 matrix and image is an 5×5 matrix.

Then image is a linear transformation, and its standard matrix is the product image that is to sayimage

we have

image

So

image

A Surprise Result

image

Eigenvalues of matrix image = 35.5216112793007,

image

The eigenvectors associated with the repeated eigenvalue image=-8.63341670127017

image

The eigenvectors associated with the eigenvalue image35.5216112793007

image

The eigenvectors associated with the eigenvalue image−14.0769629109033

image

The eigenvectors associated with the eigenvalue image−14.0769629109033

image

image is 5×5 and we can obtain five linearly independent eigenvectors then image be diagonal-Eigenvalues of matrix image = 34.7324078557174,

image

The eigenvectors associated with the repeated eigenvalue image= −6.82337727172845

image

The eigenvectors associated with the eigenvalue image34.7324078557174

image

The eigenvectors associated with the eigenvalue image16.2578297114104

image

The eigenvectors associated with the eigenvalue image7.65651697632905

image

Similarly is that since image is 5×5 and we can obtain five linearly independent eigenvectors then image be diagonalized.

More generally,

For all t ∈ R − {0} the star-system image[t,2t,3t,4t,5t;10t] = 10t has a unique solution (t,5t,−t,3t,2t), the Star-coefficient αimage = 10t and the star-function: t 7→ (t,5t,−t,3t,2t) (Figure 7)

applied-computational-mathematics

Figure 7.

The star matrix directly

image

image

The characteristic polynomial of a matrix image

image

image

image

We get the star matrix indirectly

image

image

The characteristic polynomial of a matrix image

For all (t,λ) ∈R−{0}×R,

image

image

The following product was obtained from the two matices image andimage

image

Chaffar-Matrix image is a matrix independent of t

image

it should be hard to believe that our complicated formula for matrix multiplication actually means something intuitive such as chaining two transformations together.

The following results are obtained:

image

The relationship between two matrices image and image is a convenient method of visualizing relationships quickly and definitively. One way of looking at it is that the result of matrix multiplication is important in research afterwards.

References

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Citations: 1282

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