basic tensor (original) (raw)

The present entry employs the terminology and notation defined and described in the entry on tensor arrays. To keep things reasonably self-contained we mention that the symbol Tp,q refers to thevector spaceMathworldPlanetmath of type (p,q) tensor arrays, i.e. maps

where I is some finite list of index labels, and where 𝕂 is a field.

We say that a tensor array is a characteristic array, a.k.a. abasic tensor, if all but one of its values are 0, and the remaining non-zero value is equal to 1. For tuples A∈Ip andB∈Iq, we let

denote the characteristic array defined by

(εAB)j1⁢…⁢jqi1⁢…⁢ip={1 if (i1,…,ip)=A and (j1,…,jp)=B,0 otherwise.

The type (p,q) characteristic arrays form a natural basis forTp,q.

Furthermore the outer multiplication of two characteristic arrays gives a characteristic array of larger valence. In other words, for

A1∈Ip1,B1∈Iq1,A2∈Ip2,B2∈Iq2,

we have that

where the productPlanetmathPlanetmath on the left-hand side is performed by outer multiplication, and where A1⁢A2 on the right-hand side refers to the element of Ip1+p2 obtained by concatenating the tuplesA1 and A2, and similarly for B1⁢B2.

In this way we see that the type (1,0) characteristic arraysε(i),i∈I (the natural basis of 𝕂I), and the type(0,1) characteristic arrays ε(i),i∈I (the natural basis of(𝕂I)*) generate the tensor array algebra relative to the outer multiplication operationMathworldPlanetmath.

The just-mentioned fact gives us an alternate way of writing and thinking about tensor arrays. We introduce the basic symbols

subject to the commutation relationsMathworldPlanetmath

ε(i)⁢ε(i′)=ε(i′)⁢ε(i),i,i′∈I,

add and multiply these symbols using coefficients in𝕂, and use

ε(j1⁢…⁢jp)(i1⁢…⁢iq),i1,…,iq,j1,…,jp∈I

as a handy abbreviation for

ε(i1)⁢…⁢ε(iq)⁢ε(j1)⁢…⁢ε(jp).

We then interpret the resulting expressions as tensor arrays in theobvious fashion: the values of the tensor array are just the coefficients of the ε symbol matching the given index. However, note that in the ε symbols, the covariant data is written as asuperscript, and the contravariant data as a subscript. This is done to facilitate the Einstein summation convention.

By way of illustration, suppose that I=(1,2). We can now write down a type (1,0) tensor, i.e. a column vectorMathworldPlanetmath

as

Similarly, a row-vector

can be written down as

In the case of a matrix

we would write

M=M11⁢ε(1)(1)+M21⁢ε(1)(2)+M12⁢ε(2)(1)+M22⁢ε(2)(2).