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)
To exhibit this, we must recall a familiar proposition of geometry:
the square on the longest side of a right-angled triangle is equal
to the sum of the squares on the other two sides. It has long been
known that from this alone all the metrical properties of Euclidean
space--the space in which for 2,000 years we have imagined we were
living--can be deduced. Metrical properties are those depending upon
measurement. Now, in the geometry of any space, Euclidean or not,
there is a single proposition of a similar sort which tells us how
to find the most direct distance between any two points that are
very close together. This small distance is expressed in terms of
the two sets of distance measurements by which the end-points are
located, just as two neighboring positions of our ball were located
by two sets of four measurements each. We say by analogy that two
consecutive positions of the ball are separated by a small interval of
time-space. From the formula for the very small interval of time-space
we can calculate mathematically all the metrical properties of the time
and space in which measurements for the ball's motion must be made. So
in any geometry mathematical analysis predicts infallibly the truth
about all facts depending upon measurements from the simple formula
of the interval between neighboring points. Thus, on a sphere the sum
of the angles of any triangle formed by arcs of great circles exceeds
180°, and this follows from the formula for the shortest ("geodesic")
distance between neighboring points on the spherical surface.
We saw that it takes four measurements, one for time and three for
distances, to fix an elementary event, viz., the position of the
centre of our ball at any instant. A system of all possible such sets
of four measurements each, constitutes what mathematicians call a
four-dimensional space. The study of the four-dimensional time-space
geometry, once its shortest-distance proposition is known, reveals all
those relations in nature which can be ascertained by measurements,
that is, experimentally. We have then to find this indispensable
proposition.
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