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)
This is our conception of a world, if such were possible, entirely free
from the influence of energy. We may conceive of it as an amorphous
immaterial something containing "point-events" (a point-event
being an instant of time at a point in space--a conception, not a
definition). These point-events have a fourfold order and definite
relation in this Frame, i.e. they can be specified by four variables
or coordinates in reference to some base called a reference system,
with respect to which they are forward or backward, right or left,
above or below, sooner or later. This shows the World-Frame to be
four-dimensional. Thus an aggregate of point-events (or an "event,"
which implies limited extension in space and limited duration
in time) [7] would have what we familiarly describe as length,
breadth, height and time. To express these metrical properties most
simply we must choose a four-dimensional reference system having
a particular form--rectilinear axes (Cartesian coordinates), and a
particular motion--uniform and rectilinear, i.e. unaccelerated, and
non-rotating with respect to the path of a light ray. We call this
an inertial system because Newton's Law of Inertia holds for such
a system alone. This system indicates how observers partition the
World-Frame into space and time. It restricts observers to uniform
rectilinear motion, and observations to bodies and light-pulses in
such motion. Thus gravitational and other forces are discounted,
and we obtain World-Frame conditions notwithstanding the fact that
observers are in the presence of energy.
Now the separation between point-events which have a definite relation
to each other must be absolute. The separation between two points in
a plane is defined by the unique distance between them (the straight
line joining them). Between point-events the analogue of this unique
distance, which we call the "separation-interval" (to indicate its
time-like and space-like nature), is also unique. Its unique and
absolute character give it great importance as thereby it is the same
for all observers regardless of their reference system.
If, in place of the rather cumbersome expression $X-x$ to indicate
the difference between the $x$-coordinates of two points, we employ
the more compact expression $dx$; if for the benefit of readers who
have a little algebra but no analysis we state explicitly that this
expression is a single symbol for a single quantity, and has nothing
to do with any product of two quantities $d$ and $x$; and if we
extend this notation to all our coordinates: then it is clear from
previous essays that the distance $S$ between two points in a plane
referred to a rectilinear system $OX$, $OY$, is given by the simple
equation $S^2 = (dx)^2 + (dy)^2$. Einstein and Minkowski show that
the value for the separation interval $\Omega$, the analogue of $S$,
referred to an inertial system is given by the equation
$$\Omega^2 = (dx)^2 + (dy)^2 + (dz)^2 - (dt)^2\,,$$
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