You are right about interpreting what they say in that paper---a submission to the FQXi essay contest. I was wrong in my interpretation of what they seem to be saying.
Now I am puzzled. Maybe they mean something new by "singularity", maybe what they are talking about is what arises in nature
instead of the infinite density, infinite curvature glitch.
It could be that my concepts are obsolete in this case. Could singularity mean something new, that we don't yet know what it is?
I should apologize for an apoplectic moment of strident overstatement. Your reading sounds modest and levelheaded, Sbrothy.
But "infinite density/curvature" doesn't mean anything to me. At the relevant scale geometry would be quantum and we don't know what spacetime is in quantum regime, or so I imagine. The question is still, for me, what in reality replaces the classical singularity?
And if they want to call it a singularity----a new kind of singularity, say a "quasi-singularity" or a "quantum spacetime singularity"---I can't object. I have great respect for Jacobson.
I wish they'd use a different word because traditionally it means a breakdown of some manmade theory, or the place where the breakdown occurs---not something in nature.
What he actually said at the KITP workshop, with Steven Shenker pushing him to hazard a hunch, is that he thinks "time evolution continues."
At the pit of a black hole, where classically the time-evolution stops, where timelike geodesics terminate, there (said TJ) in a quantum treatment they wouldn't end. Time-evolution would continue on thru somehow. If pushed to say, that was his hunch.
Maybe we are coming to where we will apply the term "quantum spacetime singularity" to that situation----where the classical singularity has been avoided or resolved---where in a conventional mathematicians sense there is a
non-singularity
I should get the link to that KITP discussion session that TJ co-led, in case anyone is interested.
http://online.itp.ucsb.edu/online/singular_m07/
The discussion started out being led by Gary Horowitz and then TJ took over halfway through, around minute 30:
http://online.itp.ucsb.edu/online/singular_m07/babybh/
The critical segment was minute 42-45. Steve Shenker pressed TJ to say what his hunch was. The discussion got lively. His hunch was time evolution continued thru the pit of a black hole---into something. The word "quasi-singularity" was used, I think by Shenker or maybe Horowitz.
If you download the quicktime movie you can then drag the pointer to minute 42 and start there. You don't have to watch the first 42 minutes unless you want to.