A possible trigger of it was symmetry breaking associated with the strong force, and the WMAP's finding of one-degree fluctuations in the background radiation is supporting evidence for this theory. One conclusion that can be derived from it is that there exist regions of the universe that we have not seen and which look different from the ones we know of because they fell out of thermal contact with the known regions. Applying it allows the development of models that both generate the intergalactic voids and allow for enough dark matter to ensure star rotation, and it addresses both the isotropy problem and the flatness problem, explaining t
A possible trigger of it was symmetry breaking associated with the strong force, and the WMAP's finding of one-degree fluctuations in the background radiation is supporting evidence for this theory. One conclusion that can be derived from it is that there exist regions of the universe that we have not seen and which look different from the ones we know of because they fell out of thermal contact with the known regions. Applying it allows the development of models that both generate the intergalactic voids and allow for enough dark matter to ensure star rotation, and it addresses both the isotropy problem and the flatness problem, explaining the uniformity of the background radiation as a consequence of rapid expansion after the Big Bang. Proposed by Alan Guth, FTP, identify this hypothesis which contends that the early universe quickly expanded by a factor of about 10 to the 20th.
A possible trigger of it was symmetry breaking associated with the strong force, and the WMAP's finding of one-degree fluctuations in the background radiation is supporting evidence for this theory.
inflation or inflationary hypothesis