At the April APS meeting: curing cosmic singularities

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SUMMARY

The April meeting of the American Physical Society (APS) will feature significant discussions on the resolution of classical General Relativity (GR) singularities through quantized theories. Abhay Ashtekar will present findings from Loop Quantum Gravity, highlighting how quantum geometry resolves classical singularities and provides insights into the quantum nature of the big bang and information loss. Gary Horowitz will offer perspectives from String Theory, while Jorge Pullin will discuss recent developments in Loop Quantum Gravity, particularly in mini and midi-superspace contexts. These sessions are scheduled for April 12 and April 13, 2008, respectively.

PREREQUISITES
  • Understanding of General Relativity (GR)
  • Familiarity with Loop Quantum Gravity concepts
  • Knowledge of String Theory fundamentals
  • Basic grasp of quantum mechanics and cosmology
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  • Research Loop Quantum Gravity and its implications for classical singularities
  • Explore the role of quantum geometry in cosmological models
  • Study recent advancements in String Theory related to black holes
  • Investigate the information loss paradox in quantum gravity contexts
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Physicists, cosmologists, and researchers interested in theoretical physics, particularly those focusing on quantum gravity, black hole physics, and the foundations of cosmology.

marcus
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One of the sessions at the April meeting of the American Physical Society (APS) will be on what replaces classic GR singularities (like bigbang or black hole) when you move to a quantized theory.

Abhay Ashtekar will discuss this from the Loop side.
Gary Horowitz will discuss the String side of it.

http://meetings.aps.org/Meeting/APR08/SessionIndex2/?SessionEventID=82743

This will be session B7 on the morning of 12 April. Will any PFer be there?

Here's Ashtekar's abstract
By now there are several examples in loop quantum gravity in which effects of quantum geometry became important, dominate the Planck regime and resolve classical singularities. The resulting quantum space-times are typically significantly larger than the original classical space-times. In simple examples, the physics of these quantum extensions has shed considerable light on issues such as the quantum nature of the big-bang and information loss puzzle. I will present a few examples to illustrate this growing area.

The next day Jorge Pullin will speak on
Recent developments in loop quantum gravity.
We review recent developments in loop quantum gravity emphasizing its applications in mini and midi-superspace situations.

That will be session M7, on Sunday afternoon
http://meetings.aps.org/Meeting/APR08/SessionIndex2/?SessionEventID=83486

Ashtekar and Pullin are invited speakers, giving relatively long presentations of 35 minutes. There will probably be a bunch of contributed talks---shorter in duration---on these and related topics, but I have only scanned the list of invited talks.
 
Last edited:
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Hi Marcus,
I am planning to attend this meeting.
I will try to report a brief summary of what Abhay and Gary say.
I will also try to ask them what’s inside of an astronomical sized black hole, if there’s no singularity.
In fact, I think I’ll make that a new thread on “Beyond the Standard Model”.
Jim Graber
 

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