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
We shall find it to our advantage to set , , . The superscripts do not denote powers but are simply a means for distinguishing between the three quantities , , and . 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 with a set of superscripts ranging from 1 to 29 would suffice to yield the 29 variables, written , , , , . Our reason for using superscripts rather than subscripts will soon become evident. Equations (1) can now be written
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 , , , , . Let us note that in (2) the coefficients of , , may be expressed by the matrix
By defining , , , , , , , , , the matrix (3) becomes
One advantage is immediately evident. The single element lies in the i th row and j th column of the matrix (4). Equations (1) can now be written
Using the familiar summation notation of mathematics, we rewrite (5) as
or in even shorter form
The system of equations
represents linear equations.
Einstein noticed that it was excessive to carry along the sign in (8). we may rewrite (8) as
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 occurs both as a subscript (in ) and as a superscript (in ), so that we sum on from to . In a four-dimensional spacetime () 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
We may also write (9) as
where the element belongs to the i th row and j th column of the matrix