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The Universe consists mostly of hydrogen, which makes up almost three-quarters of all conventional (baryonic)
mass. It also contains
about 24% by weight of Helium-4 (helium atoms with nuclei that
consist of two protons and two neutrons), and smaller amounts of
Deuterium (Hydrogen-2), Helium-3 and
Lithium-6. These are thought to have been manufactured early in
the Big Bang, when the
Universe was between about one second and 100 seconds old. At that time, the temperature of the Universe would have approached
a thousand million degrees, and the Universe would have been so dense
that nuclear reactions would have been common. These would have
fused almost all the neutrons available in the early Universe with
protons to make nuclei of Helium-4, with just a few neutrons left
over to make Deuterium and Helium-3. Some of the these lighter elements would have been combined to
make most of the Lithium-7 seen in the Universe today. However, this
mechanism would not have been able to make heavier elements,
most of which are known to have been made in the stars that formed
later. Calculations of light-element production agree very well with the
astrophysical observations, as shown in the picture on the right. It can be seen
that the observations agree with the calculations, if the total amount
of conventional matter in the Universe is a few per cent of the critical
density required to reverse the expansion of the Universe, as
shown by the vertical pink stripe.
This estimate agrees, to within a factor of about two, with an
entirely independent estimate based on observations of the cosmic background radiation. The
agreement between the two estimates is a powerful confirmation of
the Big Bang model. In order to calculate accurately the amounts of the different light
elements, it is necessary to know how quickly the Universe was
expanding when it was very young, which depends on the number of
different types of particles present at the time. In particular, the
light-element calculations are sensitive to the total number of
different types of light neutrinos. Experiments at the LEP particle accelerator showed
that there are just three different types of neutrino, in which
case the light-element calculations work particularly well. This
success provides further confirmation of the Big Bang model. |
Other Big Bang subsections Last updated July 2, 2001![]()
Cosmological Inflation
Cosmic Background (CMB) Radiation
Antimatter
Dark Matter
Particles and Accelerators
Telescopes
Missing Laws?![]()