Skip to main content
9 events
when toggle format what by license comment
Oct 6, 2011 at 2:23 answer added Christina Sormani timeline score: 3
Aug 28, 2011 at 20:39 vote accept michael
Aug 28, 2011 at 20:39 vote accept michael
Aug 28, 2011 at 20:39
Aug 28, 2011 at 16:00 answer added Johan Noldus timeline score: 3
Aug 25, 2011 at 22:57 comment added michael yes, in some sense due to the remark you've just noted he has to work with the "natural" 4d-riemannian metric constructed from the lorentzian metric and the time-function. It's more or less always the case in articles i know around this subject, you look at globally hyperbolic spacetimes and in some sense you reduce your problem to a problem a riemannian geometry. i was wondering if since these results advance had been made by geometers .
Aug 25, 2011 at 22:22 comment added Ken Knox I know you have said that you are familiar with Anderson's work, but in section 5 of his paper "Cheeger-Gromov theory and applications to general relativity" (math.sunysb.edu/~anderson/cargese.pdf) he seems to indicate that this is basically an open problem, and describes why using a curvature bound without choosing coordinates can be unsatisfactory. Namely that he describes the non-compact class of "plane-fronted gravitational waves" that satisfy $|R|^2 = 0$. Of course it would also be nice to hear about newer, updated work if it exists.
Aug 25, 2011 at 22:02 comment added michael oh yes, i know his work on lorentzian versions of gromov-hausdorff distances. i was in fact wondering if there exists paper in which cheeger type compactness results or for instance pinching theorems were applied to get interesting results on lorentzian geometry.
Aug 25, 2011 at 21:25 comment added Rbega I'm far from an expert on this, but I believe articles by Johan Noldus are as good a place to start as any...
Aug 25, 2011 at 20:32 history asked michael CC BY-SA 3.0