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 introduces the concept of time into intimate relationship with
the spatial coordinate system. And at once we feel the lack of a
concrete, visualized fourth dimension.]* [If we want to fix objects
in the floor alone, the edge of the room running toward the ceiling
would become unnecessary and could be dropped from our coordinate
system. That is, we need only two coordinates to fix the position of a
point in a plane. Suppose instead of discarding the third coordinate,
we use it to represent units of time. It then enables us to record
the time it took a moving point in the floor to pass from position
to position. Certain points in the room would be vertically above
the corresponding points occupied by the moving point in its path
across the floor; and the vertical height above the floor of such
points corresponds to a value of the time-coordinate which indicates
the time it took the point to move from position to position.]152
[Just as the path of the point across the floor is a continuous curve
(for the mathematician, it should be understood, this term "curve"
includes the straight line, as a special case in which the curvature
happens to be zero); so the series of points above these in the room
forms a continuous curve which records for us, not merely the path of
the point across the floor, but in addition the time of its arrival
at each of its successive positions. In the algebraic work connected
with such a problem, the third coordinate behaves exactly the same,
regardless of whether we consider it to represent time or a third
spatial dimension; we cannot even tell from the algebra what it
does represent.
When we come to the more general case of a point moving freely through
space, we have but three coordinates at our disposal; there is not
a fourth one by aid of which we can actually diagram its time-space
record. Nevertheless, we can write down the numerical and algebraic
relations between its three space-coordinates and the time which it
takes to pass from one position to another; and by this means we can
make all necessary calculations. Its motion is completely defined
with regard both to space and to time. We are very apt to call
attention to the fact that if we did have at our disposal a fourth,
space-coordinate, we could use it to represent the time graphically,
as before, and actually construct a geometric picture of the path of
our moving point with regard to space and time. And on this account
we are very apt to speak as though the time measurements constituted
a fourth coordinate, regardless of any question of our ability to
construct a picture of this coordinate. The arrival of a point in
a given position constitutes an event; and this event is completely
defined by means of four coordinates--three in space, which we can
picture on our coordinate axes, and one in time which we cannot.
Public-domain text, read in full here on John Shaqi.
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