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Einstein summation notation (Topic)

In much of the material of related to physics, one finds it expedient to adapt the summation convention first introduced by Einstein. Let us consider first the set of linear equations

a1x + b1y + c1z  =   d1

a2x + b2y + c2z  =   d2
a3x + b3y + c3z  =   d3
(1)

We shall find it to our advantage to set x = x1, y = x2, z = x3. The superscripts do not denote powers but are simply a means for distinguishing between the three quantities x, y, and z. One immediate advantage is obvious. If we were dealing with 29 variables, it would be foolish to use 29 different letters, one letter for each variable. The single letter x with a set of superscripts ranging from 1 to 29 would suffice to yield the 29 variables, written x1, x2, x3, , x29. Our reason for using superscripts rather than subscripts will soon become evident. Equations (1) can now be written

a1x1 + b1x2 + c1x3  =  d1
a2x1 + b2x2 + c2x3  =  d2
a3x1 + b3x2 + c3x3  =  d3
(2)

Equations (2) still leave something to be desired, for if there were 29 such equations, our patience would be exhausted in trying to deal with the coefficients of x1, x2, x3, , x29. Let us note that in (2) the coefficients of x1, x2, x3 may be expressed by the matrix

(            )
   a1  b1  c1
(  a2  b2  c2)
   a   b   c
    3   3   3
(3)

By defining a1 = a11, b1 = a12, c1 = a13, a2 = a21, b2 = a22, c2 = a23, a3 = a31, b3 = a32, c3 = a33, the matrix (3) becomes

(  a11  a12  a13 )
(                )
   a21  a22  a23
   a31  a32  a33
(4)

One advantage is immediately evident. The single element aij lies in the ith row and jth column of the matrix (4). Equations (1) can now be written

a11x1 + a12x2 + a13x3  =   d1
a21x1 + a22x2 + a33x3  =   d2
a  x1 + a  x2 + a  x3  =   d
  31      32      33         3
(5)

Using the familiar summation notation of mathematics, we rewrite (5) as

∑3                 ∑3                ∑ 3
    a1rxr = d1        a2rxr = d2         a3rxr = d3
r=1                r=1                r=1
(6)

or in even shorter form

∑3
    airxr =  di    i = 1,2,3
r=1
(7)

The system of equations

∑3      r
    airx  = di     i = 1,2,3,...,n
r=1
(8)

represents n linear equations.

Einstein noticed that it was excessive to carry along the sign in (8). we may rewrite (8) as

a xr =  d     i = 1,2,3,...,n
 ir      i
(9)

provided it is understood that whenever an index occurs exactly once both as a subscript and superscript a summation is indicated for this index over its full range of definition. In (9) the index r occurs both as a subscript (in air) and as a superscript (in xr), so that we sum on r from r = 1 to r = n. In a four-dimensional spacetime (x1 = x,x2 = y,x3 = z,x4 = ct) summation indices range from 1 to 4. The index of summation is a dummy index since the final result is independent of the letter used. We can write

    r       j       α
airx  ≡ aijx ≡  aiαx
(10)

We may also write (9) as

 i r    i
arx  = d      i = 1, 2,3,...,n
(11)

where the element ari belongs to the ith row and jth column of the matrix

(                    )
   a11  a12   ...  a1n
||  a21  a22   ...  a2n ||
(  ...  ...  ...  ...)
    n    n         n
   a1   a2   ...  an
(12)

0.1 References

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

This entry is a derivative of the Public domain work [1].


"Einstein summation notation" is owned by bloftin.
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Other names:  Einstein summation convention, summation notation, summation convention

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Cross-references: work, domain, spacetime, system, matrix, powers, Einstein
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This is version 1 of Einstein summation notation, born on 2010-02-15.
Object id is 842, canonical name is EinsteinSummationNotation.
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Physics Classification02. (Mathematical methods in physics)
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