Spaces of \(N\) Dimensions
A point in three-dimensional space is a set of three numbers, its coordinates, in a chosen
frame of reference: for example \((x,y,z)\), \((\rho,\phi,z)\) and \((r,\theta,\phi)\) in rectangular,
cylindrical and spherical coordinates. By analogy, a point in \(N\)-dimensional space is a set of \(N\)
numbers \((x^1,x^2,\dots,x^N)\); here \(1,2,\dots,N\) are superscripts, not exponents.
That we cannot visualize spaces of more than three dimensions has no bearing on their existence.
Coordinate transformations Let \((x^1,x^2,\dots,x^N)\) and \((\bar x^1,\bar x^2,\dots,\bar x^N)\)
be the coordinates of a point in two frames of reference, related by \(N\) independent relations
\[
\begin{aligned}
\bar x^1&=\bar x^1(x^1,x^2,\dots,x^N),\\
\bar x^2&=\bar x^2(x^1,x^2,\dots,x^N),\\
&\ \,\vdots\\
\bar x^N&=\bar x^N(x^1,x^2,\dots,x^N),
\end{aligned}
\]
or briefly
\begin{equation*}\tag{15.1}
\bar x^k=\bar x^k(x^1,x^2,\dots,x^N),\qquad k=1,2,\dots,N,
\end{equation*}
where the functions are single-valued and continuously differentiable. Conversely, to each
\((\bar x^1,\dots,\bar x^N)\) there corresponds a unique \((x^1,\dots,x^N)\) given by
\begin{equation*}\tag{15.2}
x^k=x^k(\bar x^1,\bar x^2,\dots,\bar x^N),\qquad k=1,2,\dots,N.
\end{equation*}
Relations (15.1) and (15.2) define a transformation of
coordinates.
Summation convention The sum \(a_1x^1+a_2x^2+\cdots+a_Nx^N=\sum_{j=1}^Na_jx^j\) is written
simply \(a_jx^j\): an index (subscript or superscript) repeated in a term is summed from \(1\) to \(N\)
unless otherwise specified. This is the summation convention. The letter is immaterial
(\(a_jx^j=a_px^p\)); a repeated index is called a dummy or umbral index.
An index occurring only once in a term is a free index and stands for any of \(1,2,\dots,N\),
like \(k\) in (15.1) or (15.2), each of which represents \(N\) equations.