Tez
Graduate Poster
- Joined
- Nov 29, 2001
- Messages
- 1,104
I just looked at Weinberg's paper again. Kinda interesting.
The way I've been thinking about it is this: There's no obvious connection between dark energy existing, and life existing. Never mind dark energy happening to become dynamically significant right when we happened to be around to see it. So how to make use of an anthropic principle? (Of course if this guy I just wrote about is right, then there's a correlation without any necessary connection/causation, which is nice..)
Anyway, as I understand it, when Weinberg (http://www.arxiv.org/astro-ph/0005265 ) and others use the anthropic principle they dont mean something so imprecise. What they look for are models wherein the SuperDuperVerse is much, much bigger than the universe which we see (some sort of New Inflation scenario), and certain initial fields have quantum fluctuations which range over values that yield the "desired" universes in suitable abundance - one of which is presumably our "visible" universe. In these models, they try and rig it so if you take any of the universe sized bubble regions of the SuperDuperverse, you'll find, with high likelihood, conditions much like the ones we see. Thus they say "we see the universe the way it is because no matter which universe you take you'll see something like the one we see".
The way I've been thinking about it is this: There's no obvious connection between dark energy existing, and life existing. Never mind dark energy happening to become dynamically significant right when we happened to be around to see it. So how to make use of an anthropic principle? (Of course if this guy I just wrote about is right, then there's a correlation without any necessary connection/causation, which is nice..)
Anyway, as I understand it, when Weinberg (http://www.arxiv.org/astro-ph/0005265 ) and others use the anthropic principle they dont mean something so imprecise. What they look for are models wherein the SuperDuperVerse is much, much bigger than the universe which we see (some sort of New Inflation scenario), and certain initial fields have quantum fluctuations which range over values that yield the "desired" universes in suitable abundance - one of which is presumably our "visible" universe. In these models, they try and rig it so if you take any of the universe sized bubble regions of the SuperDuperverse, you'll find, with high likelihood, conditions much like the ones we see. Thus they say "we see the universe the way it is because no matter which universe you take you'll see something like the one we see".