The nature of the physical worldEddington, Arthur Stanley, Sir
Philosophy
The nature of the physical world
Eddington, Arthur Stanley, Sir
Physics -- Philosophy; Science -- Philosophy
Two “particles” in the four-dimensional world are shown in Fig.
5, namely yourself and myself. We are not empty
space so there is no limit to the kind of curvature entering into
our composition; in fact our unusual sort of curvature is what
distinguishes us from empty space. We are, so to speak, ridges in
the four-dimensional world where it is gathered into a pucker. The
pure mathematician in his unflattering language would describe us as
“singularities”. These two non-empty ridges are joined by empty space,
which must be free from those kinds of curvature described by the
ten principal coefficients. Now it is common experience that if we
introduce local puckers into the material of a garment, the remainder
has a certain obstinacy and will not lie as smoothly as we might wish.
[Pg 128]
You will realise the possibility that, given two ridges as in Fig. 5,
it may be impossible to join them by an intervening valley without the
illegal kind of curvature. That turns out to be the case. Two perfectly
straight ridges alone in the world cannot be properly joined by empty
space and therefore they cannot occur alone. But if they bend a little
towards one another the connecting region can lie smoothly and satisfy
the law of curvature. If they bend too much the illegal puckering
reappears. The law of gravitation is a fastidious tailor who will not
tolerate wrinkles (except of a limited approved type) in the main area
of the garment; so that the seams are required to take courses which
will not cause wrinkles. You and I have to submit to this and so our
tracks curve towards each other. An onlooker will make the comment that
here is an illustration of the law that two massive bodies attract each
other.
We thus arrive at another but equivalent conception of how the earth’s
spiral track through the four-dimensional world is arrived at. It is
due to the necessity of arranging two ridges (the solar track and
the earth’s track) so as not to involve a wrong kind of curvature in
the empty part of the world. The sun as the more pronounced ridge
takes a nearly straight track; but the earth as a minor ridge on the
declivities of the solar ridge has to twist about considerably.
Public-domain text, read in full here on John Shaqi.
Reviews
Reviews
No reviews yet
Be the first to share your thoughts on this work.
Elsewhere in the archive
Join the Discussion
Join the discussion
Sign in to leave a comment or review.
Sign InorCreate an account