chavvdarrr said:
And according to few of my old classmates who work in places like CERN and the Chicago accelarator (its name went out my mind), many experiments always give same results : "we have nice fit with the thoery and we need more $$$ in order to go ahead" . Like the experiment for calculating gravity speed 1-2 years ago using gravity field of Jupiter... a friend of mine told me what the results will be BEFORE the experiment was made ! No, he wasn't working on that project
Well, we've expected for a very long time what the speed of gravity must be. Gravity waves propagating at the speed of light has been in Einstein's theory since the inception of GR. So of course your friend expected that result.
But there are some (including the resident GR expert here at Davis) who believe that the experiment you mention doesn't actually measure the speed of gravity, but rather just the speed of light.
Anyway, the really exciting thing about physics today is that we don't know what to expect. In both the fields of high energy physics and cosmology, we expect to be able to gain exciting new information out of upcoming experiments, but we really haven't nailed down much at all as to what that information should be. Different theories predict radically different behavior in upcoming experiments.
One really interesting and brand-new result came out of the 3rd-year WMAP data, which was just released a couple of weeks ago. The really exciting measurement is that they find, with the simplest models, a deviation of the scale factor from one by about 4 sigma (i.e. ruled out at the 99.9968% level).
The idea is that there were some primordial quantum mechanical perturbations in the very early universe that gave rise to all structure we see today. Different scales of perturbations would have been generated at different times: perterbations earlier-on would have expanded more, and would be responsible for the largest-scale structure. Our current universe, then, is highly dependent upon the amplitude of each of these perturbations. Since the universe had expanded many fold between the generation of the largest scale structure and the smallest, we don't expect the amplitudes of these perturbations to be completely independent of scale. The scale factor parameterizes this expectation, and if it differs from one, then we detect that different perturbation scales actually had different amplitudes.
So, the existence of this measured variation in amplitude based upon scale could give us a window into the possible models for inflation.