Einstein's Theories of Relativity and Gravitation: A selection of material from the essays submitted in the competition for the Eugene Higgins prize of $5,000Bird, J. Malcolm (James Malcolm)
Philosophy
Einstein's Theories of Relativity and Gravitation: A selection of material from the essays submitted in the competition for the Eugene Higgins prize of $5,000
Bird, J. Malcolm (James Malcolm)
Relativity (Physics)
It is familiar knowledge that the line, the surface and ordinary
Euclidean space are to be regarded as spaces of one, two and three
dimensions respectively and readers of this journal are aware
that a hypothetical space of four dimensions has been closely
investigated. The most convenient space to study is the surface or
two-space, since we can regard it as embedded in a three-space. If a
surface is curved it is generally impossible to draw a straight line
on it, for as we see clearly, the "straightest" line is changing its
direction at every point. To describe this property accurately it
is necessary to ascribe to each point a magnitude which expresses
what happens to the direction of a short line in the region when
displaced a short distance parallel to itself. This is called the
direction-defining magnitude. Different sets of values of this
magnitude relate to surfaces of different curvatures.
A second fundamental property has recently been pointed out. There
is inherent in every part of a space a measure of length peculiar
to that particular region and which in general varies from region
to region. To describe this variation accurately it is necessary to
ascribe to each point another magnitude called the length-defining
magnitude, which expresses the change from each point to the next of
the unit of length. These two magnitudes define the surface completely.
Similarly, a space of any number of dimensions is defined completely
by a similar pair of magnitudes. A space is the "field" of such
a magnitude-pair and the nature of these magnitudes defines the
dimensions of the space. The four-space usually described is the
Euclidean member of an infinity of four-spaces.
When we look into a mirror we see a space differing from ordinary
space in that right and left are interchanged and this is described
mathematically by saying that if we locate points as usual by
specifying three distances $X_1$, $X_2$, $X_3$ of the point from three
mutually perpendicular planes, then a point $X_1$, $X_2$, $X_3$, in
actual space corresponds with a point $X_1$, $X_2$, $ -X_3$ in the
mirrored space: in other words the mirrored space is derived from
the real space by multiplying the $X_3$ coordinates by $-1$. If we
were to multiply by $\sqrt{-1}$ instead of $-1$ we should derive a
different space; in this case, however, we have no mirror to show us
what it looks like. Such a space is said to have one negative dimension
and it has the peculiar property that in the figure derived from the
right triangle of ordinary space the square of the "hypotenuse" equals
the difference and not the sum of the squares of the other two sides,
so that the length of a line may sometimes have to be represented by
the square-root of a negative number, a "complex" number.
Public-domain text, read in full here on John Shaqi.
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