- #106
oldman
- 633
- 5
Chronos said:the LCDM model... handily describes the observational results. It is a very good model that explains many things.
I'm certainly not disputing this kind of general statement, Chronos, but the devil is always in the details! My original query was about one detail, namely:
my difficulty boils down to: why are large-scale temperature fluctuations not more prominent in the WMAP results?
and in a following post:
.I would like to know how one can "have one's cake" (solve the horizon problem) and at the same time "eat it" (accept the deficiency in low-l modes).
These quotes should also make it clear that I do agree with Hellfire
Hellfire said:... that inflation solves the homogeneity problem (or horizon problem) (and that)... the theory ... provide(s) a mechanism to account for the small inhomogeneities in the CMB that are the seeds of the matter structures...this mechanism could be quantum fluctuations during inflation.
But nether of you have yet mentioned the deficiency in low - l modes, which the WMAP results now seem to show are real. This conflict is what bothers me. Or am I tilting at windmills?
I hadn't seen the 2003 paper by Guth that Hellfire kindly referred me to. I've glanced at it now, and it seems to complement his 1997 book (which I have)excellently. Thanks for the reference, Hellfire.