crazco said:
there was a singularity, what made it expand
i so confused
A singularity is a breakdown in a theory. A place where some model blows up and stops being applicable. Typically singularities get fixed by modifying the model---this has happened with other theories in other branches of physics. At present there is no reason to believe that a singularity occurred. As Einstein-Online says, most cosmologists would be quite surprised if there turned out to have been one.
However "what made it expand?" is a very good question. Whatever was there at the start of expansion, why did it begin expanding?
nicksauce said:
No one knows the answer to this question. It is an open area of research. The relatively new field of Quantum Cosmology tries to answer such questions.
Nick is right! No one knows. There are theories (in the new field of Quantum Cosmology) which give answers. But they have not yet been tested.
Here are the papers in QC written since 2005.
http://www.slac.stanford.edu/spires/find/hep/www?rawcmd=dk+quantum+cosmology+and+date%3E2005&FORMAT=WWW&SEQUENCE=citecount%28d%29
There are 362 papers that appeared in the four years 2006-2009 alone. That is about 90 papers per year.
If you look at the first 50 papers listed, that is, at the most often cited ones, they are almost all using bounce models where there is no singularity but rather there is a prior contraction, and quantum effects kick in at very high density making gravity repel strongly instead of attract. So the whole things begins expanding.
Quantum gravity as these researchers have formulated it, has a natural brief inflation episode.
For a further discussion of how Quantum Cosmology (with the bounce feature) relates to inflation you could look at Ashtekar's recent paper:
http://arXiv.org/abs/0912.4093
So the answer to your question is that nobody knows but they have several interesting ideas, and the field is called QC, and they are working on it pretty hard.
And currently one of the areas of QC getting a lot of attention is
how to test the models.
There is an international workshop on that coming up this year in Stockholm.
Here is a sample paper addressing the QC testing problem, if you are curious. It talks about "footprints" of QC to look for in the temperature map of the cosmic microwave background. Observable features of the CMB.
http://arXiv.org/abs/0902.0145