Table of Contents
Despite its successes, the standard big bang cosmology has some problems
that are difficult to resolve. Among these are:
The inflationary model addresses all these issues by presuming that what we call the observable universe is actually a very small portion of the initial universe that underwent a de Sitter phase of exponential expansion around the time of the GUT epoch. This model posits that what became our observable universe was small enough to be in causal contact at the big bang; it then grew at an exponential rate during the inflationary epoch. The exponential growth had the effect of flattening out any curvature, stretching the geometry of the universe so much that it became flat. Any massive GUT particles were diluted, spread out over this now fantastically huge domain to an extremely tiny density, so that they no longer are observable. Quantum fluctuations in the vacuum are preserved and "blown up" to large scales by the expansion, providing the seeds for structure formation.
The source of this exponential growth was a negative pressure produced by a nonzero vacuum energy. A nonzero vacuum energy could result from quantum processes in the early universe. In quantum field theory, a field is associated with each particle, and the field in turn is related to a potential, the latter being a function which describes the energy density of the field. The right potential would result in a false vacuum, a situation in which the field was zero but the corresponding potential was not zero. The false vacuum state could have provided a vacuum energy that would behave exactly like a positive (repulsive) cosmological constant, resulting in a temporary de Sitter phase during which the patch of universe grew by a factor of perhaps 10100 or more. Eventually, however, this vacuum energy was converted into real particles and the field found its way to the true vacuum, bringing the inflation to a halt. The universe then continued to evolve from this point as in our standard model.
The inflationary model is an area of active research. It makes some predictions about the structures in the universe which are consistent with the COBE data, although not yet proven, and it predicts that the present universe should be flat. This may present a problem for the model since most measurements of Omega give < 1. Furthermore, Omega=1 models are too young for the larger Hubble values that tend to be measured by recent techniques. Moreover, the particle that might have provided the vacuum energy density is still unidentified, even theoretically; it is sometimes called the inflaton because its sole purpose seems to be to have produced inflation. Despite these outstanding questions, it seems difficult to understand how the horizon problem could be explained unless something like inflation occurred. Research continues along all these lines of investigation.
|Points to Ponder|
|Questions & Answers||
Questions and Answers related to Chapter 15.
|Web World||The topics touched on in this chapter are at the frontiers of modern cosmological research. For additional descriptions of this type of work, see the Research on Cosmology at the University of Illinois web pages.|