1 |
% |
2 |
% $Id: notation.tex 1318 2007-09-26 04:39:14Z ksteube $ |
3 |
% |
4 |
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% |
5 |
% |
6 |
% Copyright 2003-2007 by ACceSS MNRF |
7 |
% Copyright 2007 by University of Queensland |
8 |
% |
9 |
% http://esscc.uq.edu.au |
10 |
% Primary Business: Queensland, Australia |
11 |
% Licensed under the Open Software License version 3.0 |
12 |
% http://www.opensource.org/licenses/osl-3.0.php |
13 |
% |
14 |
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% |
15 |
% |
16 |
|
17 |
\section{Einstein Notation} |
18 |
\label{EINSTEIN NOTATION} |
19 |
|
20 |
Compact notation is used in equations such continuum mechanics and linear algebra; it is known as Einstein notation or the Einstein summation convention. It makes the conventional notation of equations involing tensors more compact, by shortening and simplifying them. |
21 |
|
22 |
There are two rules which make up the convention: |
23 |
|
24 |
firstly, the rank of the tensor is represented by an index. For example, $a$ is a scalar; $b\hackscore{i}$ represents a vector; and $c\hackscore{ij}$ represents a matrix. |
25 |
|
26 |
Secondly, if an expression contains subscripted variables, they are assumed to be summed over all possible values, from $0$ to $n$. For example, for the following expression: |
27 |
|
28 |
|
29 |
|
30 |
\begin{equation} |
31 |
y = a\hackscore{0}b\hackscore{0} + a\hackscore{1}b\hackscore{1} + \ldots + a\hackscore{n}b\hackscore{n} |
32 |
\label{NOTATION1} |
33 |
\end{equation} |
34 |
|
35 |
can be represented as: |
36 |
|
37 |
\begin{equation} |
38 |
y = \sum\hackscore{i=0}^n a\hackscore{i}b\hackscore{i} |
39 |
\label{NOTATION2} |
40 |
\end{equation} |
41 |
|
42 |
then in Einstein notion: |
43 |
|
44 |
\begin{equation} |
45 |
y = a\hackscore{i}b\hackscore{i} |
46 |
\label{NOTATION3} |
47 |
\end{equation} |
48 |
|
49 |
Another example: |
50 |
|
51 |
\begin{equation} |
52 |
\nabla p = \frac{\partial p}{\partial x\hackscore{0}}\textbf{i} + \frac{\partial p}{\partial x\hackscore{1}}\textbf{j} + \frac{\partial p}{\partial x\hackscore{2}}\textbf{k} |
53 |
\label{NOTATION4} |
54 |
\end{equation} |
55 |
|
56 |
can be expressed in Einstein notation as: |
57 |
|
58 |
\begin{equation} |
59 |
\nabla p = p,\hackscore{i} |
60 |
\label{NOTATION5} |
61 |
\end{equation} |
62 |
|
63 |
where the comma ',' indicates the partial derivative. |
64 |
|
65 |
For a tensor: |
66 |
|
67 |
\begin{equation} |
68 |
\sigma \hackscore{ij}= |
69 |
\left[ \begin{array}{ccc} |
70 |
\sigma\hackscore{00} & \sigma\hackscore{01} & \sigma\hackscore{02} \\ |
71 |
\sigma\hackscore{10} & \sigma\hackscore{11} & \sigma\hackscore{12} \\ |
72 |
\sigma\hackscore{20} & \sigma\hackscore{21} & \sigma\hackscore{22} \\ |
73 |
\end{array} \right] |
74 |
\label{NOTATION6} |
75 |
\end{equation} |
76 |
|
77 |
|
78 |
The $\delta\hackscore{ij}$ is the Kronecker $\delta$-symbol, which is a matrix with ones for its diagonal entries ($i = j$) and zeros for the remaining entries ($i \neq j$). |
79 |
|
80 |
\begin{equation} |
81 |
\delta \hackscore{ij} = |
82 |
\left \{ \begin{array}{cc} |
83 |
1, & \mbox{if $i = j$} \\ |
84 |
0, & \mbox{if $i \neq j$} \\ |
85 |
\end{array} |
86 |
\right. |
87 |
\label{KRONECKER} |
88 |
\end{equation} |