PlanetPhysics/Examples of Einstein Summation Notation

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Some examples of applying the [[../EinsteinSummationNotation/|Einstein summation notation]].

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Example 1 . Let us consider the quantity

S=aαβxαxβ

for a three dimensional space. Since the index α occurs as both a subscript and a superscript, we sum on α from 1 to 3. This yields

S=a1βx1xβ+a2βx2xβ+a3βx3xβ

Now each term of S is such that β is both a subscript and superscript. Summing on β from 1 to 3 as prescribed by our summation convention yields the quadratic form

S=a11x1x1+a12x1x2+a13x1x3+a21x2x1+a22x2x2+a23x2x3+a31x3x1+a32x3x2+a33x3x3

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Example 2 . If x1,x2,x3,,xn is a set of independent variables, then

x1x1=x2x2=x3x3==xnxn=1

and if ij

x1x2=0,xixj=0

We may write

xixjδji{=1=if=i=j=0=if=ij

The symbol δji is called the Kronecker delta. We have

δαα=δ11+δ22++δnn=n

Let us now assume that the quadratic form at the end of example 1 vanishes identically for all values of the independent variables x1,x2, x3, and aij to be constant. Differentiating S=aαβxαxβ=0 with respect to a given variable, say xi, yields

Sxi=aαβxαxβxi+aαβxβxαxi=0Sxi=aαβxαδiβ+aαβxβδiα=0Sxi=aαixα+aiβxβ=0

Now differentiating with respect to xi yields

2Sxjxi=aαiδjα+aiβδiβ=0

so that aji+aij=0 or aij=aji for i,j=1,2,3.

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Example 3 . We define ϵij,i,j=1,2, to have the following numerical values: Let ϵ11=ϵ22=0,ϵ12=1,ϵ21=1. We now consider the expression

D=ϵijai1aj2

Expanding (2) by use of our summation convention yields

D=ϵ11a11a12+ϵ12a11a22+ϵ21a21a12+ϵ22a21a22=a11a22a21a12

The reader who is familiar with second-order [[../Determinant/|determinants]] quickly recognizes that

ϵijai1aj2=|a11a21a12a22|

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Example 4 . The [[../SimilarityAndAnalogousSystemsDynamicAdjointnessAndTopologicalEquivalence/|system]] of equations

(y1=y1(x1,x2,,xn)y2=y2(x1,x2,,xn)yn=yn(x1,x2,,xn))

represents a coordinate transformation from an (x1,x2,,xn) coordinate system to a (y1,y2,,yn) coordinate system. From the calculus we have

dyi=yix1dx1+yix2dx2++yixndxni=1,2,,n

dyi=yiyαdxα

The α in the term yixα is to be considered as a subscript. If, furthermore, the xi, i=1,2,,n, can be solved for the y1,y2,,yn, and assuming differentiability of the xi with respect to each yi, one obtains

yiyjδji=yixαxαyj

Differentiating this expression with respect to yk yields

0=yixα2xαykyi+2yixβxαxβykxαyj

Multiplying both sides of this equation by xσyi amd summing on the inex i yields

0=xσyiyixα2xαykyj+2yixβxαxβykxαyjxσyi

or

0=δασ2xαykyj+2yixβxαxβykxαyjxσyi

which yields

2xσykyj=2yixβxαxβykxαyjxσyi

In particular, if y=f(x), then

d2xdy2=d2ydx2(dxdy)3

References

[1] Lass, Harry. "Elements of pure and applied mathematics" New York: McGraw-Hill Companies, 1957.

This entry is a derivative of the Public [[../Bijective/|domain]] [[../Work/|work]] [1].

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