The evolution of scientific thought from Newton to EinsteinD'Abro, A. (Aram)
Science
The evolution of scientific thought from Newton to Einstein
D'Abro, A. (Aram)
Relativity (Physics); Science -- Methodology
Suppose, then, we wish to express the distance between two points
and , defined by the intersections of a certain line
with two successive lines (Fig. II). The co-ordinates of the two
points are () and (), respectively, where
represents the increase in the value of as we pass
from to on the line.
On no account may we say that the distance (which we shall call
) is given by the value , for is
nothing but a difference between numbers serving to localise points;
it has nothing in common with a distance. In order to dispel any
doubts on this score, we may notice that if we compare the lines
to parallels and the lines to meridians, the points and
will be given by the intersections of two consecutive meridians
[Pg 86]
with the same parallel. In this case would correspond
to the difference in longitude between the two points; and obviously
a difference in longitude is no criterion of a distance, since for
the same difference in longitude the distance decreases from equator
to pole. In short, the distance between and
cannot be fully determined by .
Yet, on the other hand, just as the distance between two points lying
on the same parallel is affected by their difference in longitude,
so now the distance between and must be a
function of the co-ordinate difference . A sufficiently
general expression of a quantity when defined in terms of
another quantity on which it depends is given by
where , , are appropriate magnitudes. If, however,
we consider points exceedingly close together, becomes
exceedingly small in value, and as a result and
, etc., are many times smaller still. At the limit,
therefore, when the two points are at an infinitesimal distance apart,
the higher powers of become so insignificant that
they can be neglected in comparison with . We thus obtain
, and in order to specify that we are considering
infinitesimal distances we replace the symbol by and
obtain
It is customary to designate by so that, using
squares, our formula becomes
[Pg 87]
And now we have to consider an important question. What is ?
What does it represent? We do not propose to enter into its full
mathematical significance, but we may mention certain of its important
characteristics. In our illustration of meridians and parallels,
let us consider the various points of intersection defined by the
intersections of the successive parallels with two fixed meridians.
The difference in longitude between these various point pairs
will, of course, be constant and will be given by the same
invariable quantity . Inasmuch as the distance
between these point pairs varies from pole to equator, we see from
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