Big Bang Cosmology
The Big Bang Model is a broadly accepted theory for the origin and evolution of
our universe. It postulates that 12 to 14 billion years ago, the portion of the
universe we can see today was only a few millimeters across. It has since
expanded from this hot dense state into the vast and much cooler cosmos we
currently inhabit. We can see remnants of this hot dense matter as the now very
cold cosmic microwave background radiation which still pervades the universe and
is visible to microwave detectors as a uniform glow across the entire sky.
Foundations of the Big Bang Model
The Big Bang Model rests on two theoretical pillars:
General Relativity
Albert Einstein at the Chalkboard- source unknown
The first key idea dates to 1916 when Einstein developed his General Theory of Relativity which he
proposed as a new theory of gravity. His theory generalizes Isaac Newton's
original theory of gravity, c. 1680, in that it is supposed to be valid for
bodies in motion as well as bodies at rest. Newton's gravity is only valid for
bodies at rest or moving very slowly compared to the speed of light (usually not
too restrictive an assumption!). A key concept of General Relativity is that
gravity is no longer described by a gravitational "field" but rather
it is supposed to be a distortion of space and time itself. Physicist John
Wheeler put it well when he said "Matter tells space how to curve, and
space tells matter how to move." Originally, the theory was able to account
for peculiarities in the orbit of Mercury and the bending of light by the Sun,
both unexplained in Isaac Newton's theory of gravity. In recent years, the
theory has passed a series of rigorous tests.
The Cosmological Principle
After the introduction of General Relativity a number of
scientists, including Einstein, tried to apply the new gravitational dynamics to
the universe as a whole. At the time this required an assumption about how the
matter in the universe was distributed. The simplest assumption to make is that
if you viewed the contents of the universe with sufficiently poor vision, it
would appear roughly the same everywhere and in every direction. That is, the
matter in the universe is homogeneous and isotropic when averaged over very
large scales. This is called the Cosmological Principle. This assumption is
being tested continuously as we actually observe the distribution of galaxies on
ever larger scales. The accompanying picture shows how uniform the distribution
of measured galaxies is over a 70° swath of the sky. In addition the
cosmic microwave background radiation, the
remnant heat from the Big Bang, has a temperature which is highly uniform over
the entire sky. This fact strongly supports the notion that the gas which
emitted this radiation long ago was very uniformly distributed.
These two ideas form the entire theoretical basis for Big Bang cosmology and
lead to very specific predictions for observable properties of the universe. An
overview of the Big Bang Model is presented in a set of companion pages.
Further Reading
- Peebles, P.J.E., Schramm, D.N., Turner, E.L. & R.G. Kron 1991, "The Case for the Relativistic Hot Big Bang Cosmology", Nature, 352, 769 - 776.
- Peebles, P.J.E., Schramm, D.N., Turner, E.L. & R.G. Kron 1994, "The Evolution of the Universe'', Scientific American, 271, 29 - 33.
- Will, Clifford, "Was Einstein Right?"
Wilkinson Microwave Anisotropy Probe
