A Level Physics Notes: Cosmology – The Future of the Universe
The Universe is expanding, but that might be a temporary thing.
Some observers say that the rate of expansion is increasing. Some say
that the mutual gravitational attraction of all the matter and
energy in the universe is slowing the expansion of the Universe down,
At some point in the future the Universe may or may not stop
expanding and start contracting, ending in a Big Crunch – the
Universe would in this case be closed. This is illustrated on the
diagram below by the curve
![]()
The parameter
is
the ratio
where
is
the critical density, the density the universe would have to keep
expanding, but constantly decelerating, with the expansion coming to
a stop at infinite time, and
is
the present density of the universe. The density of the universe, all
things considered, seems to be suspiciously close to the critical
density, which is about
Kg
per cubic m but recent evidence suggests the rate of expansion may be
increasing, so the Universe is open. Open Universes are illustrated
by the three top curves on the diagram above.
To complicate things the Universe is pervaded by a mysterious substance called Dark Matter, about which we know very little, but which may contribute greatly to the mass of the Universe.