by Markus Schwarz » Fri Sep 09, 2011 1:45 pm
Dear babaonet,
Friedmann and others were searching for solutions to Einstein's new theory of gravitation (general relativity).
Since the equations are quite complicated, Friedmann made the simplifying assumption that the universe is homogenous and isotropic.
These are technical terms, which translate into plain English as the words you highlighted above. So, under this assumption he was able to
find a solution to Einstein's theory.
The question remained whether this solution is actually a good description of the universe we live in. The answer hinges on if we can find evidence or proof of this. In the 40ies, based on Friedmann's solution, Gamow predicted that there would be a "cosmic background radiation" with certain specific properties. It took another 20 years until Penzias and Wilson discovered this radiation. It was the missing proof to show that the universe is homogenous and isotropic. They were awarded the Nobel prize for it.
Hope that helps.
Dear babaonet,
Friedmann and others were searching for solutions to Einstein's new theory of gravitation (general relativity).
Since the equations are quite complicated, Friedmann made the simplifying assumption that the universe is homogenous and isotropic.
These are technical terms, which translate into plain English as the words you highlighted above. So, under this assumption he was able to
find a solution to Einstein's theory.
The question remained whether this solution is actually a good description of the universe we live in. The answer hinges on if we can find evidence or proof of this. In the 40ies, based on Friedmann's solution, Gamow predicted that there would be a "cosmic background radiation" with certain specific properties. It took another 20 years until Penzias and Wilson discovered this radiation. It was the missing proof to show that the universe is homogenous and isotropic. They were awarded the Nobel prize for it.
Hope that helps.