- #36
skydivephil
- 474
- 9
bapowell said:Yes, indeed. To be clear, above James and I were discussing chaotic inflation, which is necessarily eternal (hence my phrasing "chaotic eternal inflation"). There are models of eternal inflation that are not technically chaotic (which refers to the distribution of the initial field values.)
Yes, but if B-modes are not detected that doesn't falsify inflation (nor does it necessarily confirm it, see the quick note by Brandenberger on some other B-mode sources: http://arxiv.org/abs/1104.3581)
Interesting. I was not aware that it was under dispute. For completeness, here's a reference to the original paper by Borde and Vilenkin: http://arxiv.org/abs/gr-qc/9312022. The later paper with Guth was an extension.
And James, for a good technical introduction to string theory try Zwiebach. I've not read it myself but it seems highly praised by many in the field. More advanced standards are the texts by Polchinski and Green, Schwarz, and Witten. The latter is a now out-dated by has its unique strengths.
Thats fascinating, i didnt realize that matter bounce in Horava gravity prodcued B mode polarisation. To be fair that's a pretty new paper. I do note that the author concluded we can still assess the different models via their tilt, so I think its still true that if we can produce the spectrum from the B mode it could be the decider on inflation, but I guess not in the same way that the Nature article implied.
As far as disputing the initial singualrity in eternal inflaiton, this is a an exmaple within the eternal inflation community:
http://arxiv.org/abs/0712.0571
Of course the loop guys wouold dispute from a very different angle ie a bouncing comsology