Its sunny and breezy out here in San Fran. Although I'm tempted to go out for a run, I've been here for last couple hours thinking about cutoffs in field theory and its effect on cosmology. Marvin Weinstein (see my previous post on him) and I got in a fight the other day (typical Bronx versus Brooklyn brawl).
Marvin: So whaddya want to do, what are your trying to get at and don't gimme no bullshit
Stephon: I've been telling you that non-perturbative effects like gravitational instantons can be induced during inflation to kill the cosmological constant!
Marvin: You didnt solve a damn thing.
Stephon: Where you going with that Marv, my starting point is no different than Woodards. I say lets start with a huge cosmological constant, space-time will naturally be in a de Sitter phase. Now we have to
ask, by what dynamics is it killed. . .
Marvin: Yeah, except that its infinite. Not even Woodard solves that! Look, I'm a simple man-if you put in cutoffs then you have a very non trivial problem, nobody talks about it but its there o.k?
Stephon: So why don't you write it up! Didn't you and Ratin in your recent paper on Quantum de Sitter cover that ? see: http://arXiv.org/abs/hep-th/0312249
Marvin: Its there but not explicit-Look, I only write things up when I have something to say, I don't waste paper.
Stephon: So whaddya you want me to do? No one knows what to do with cutoffs in a dynamical space-time -especially non compact ones, I mean Jacobson and his students are currently studying this. I tried ok? See you next week ol man
-So the battle continues, Me, Marvin and the rest of the species trying to understand why Lambda_cc is small and positive today!