Bojowald 3 week gig at KITP quantum NONsingularities

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SUMMARY

The forum discussion centers on the upcoming mini-program titled "The Quantum Nature of Spacetime Singularities," organized by Martin Bojowald and Gary T. Horowitz at the KITP in Santa Barbara from January 8 to January 26, 2007. This event aims to address fundamental issues in quantum gravity, particularly regarding singularities in black holes and the early universe. Key topics include string gas cosmology, tachyon condensation, and loop quantum gravity, which posits a discrete nature of space. The discussion highlights Bojowald's contributions to the field, including his Living Reviews article and his role in establishing a singularity-free framework in quantum cosmology.

PREREQUISITES
  • Understanding of quantum gravity concepts
  • Familiarity with string theory and its implications
  • Knowledge of loop quantum gravity principles
  • Awareness of cosmological models and singularity theories
NEXT STEPS
  • Research "string gas cosmology" and its relevance to quantum gravity
  • Study "loop quantum cosmology" and its implications for singularities
  • Examine the AdS/CFT correspondence in the context of black hole physics
  • Explore the concept of naked singularities and their physical interpretations
USEFUL FOR

Researchers, physicists, and students interested in quantum gravity, cosmology, and the theoretical frameworks addressing spacetime singularities will benefit from this discussion.

marcus
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Francesca flagged this January 2007 event

francesca said:
I look forward for next January! Bojowald and Horowitz are organizing in Santa Barbara a mini-program lasting 3 weeks in http://www.kitp.ucsb.edu/activities/auto2/?id=332" :-p
We will see...
 
Last edited by a moderator:
Physics news on Phys.org
http://www.kitp.ucsb.edu/activities/auto2/?id=332

------quote-----
The Quantum Nature of Spacetime Singularities

(Martin Bojowald, Robert H. Brandenberger, Gary T. Horowitz, Hong Liu)

Jan 8, 2007 - Jan 26, 2007



One of the main goals of quantum gravity is to provide a better understanding of physics near the big bang and inside black holes where general relativity breaks down. Recently, there has been considerable progress toward this goal in both of the main approaches to quantum gravity. In string theory, this includes string gas cosmology, tachyon condensation, and holographic descriptions using the AdS/CFT correspondence. In loop quantum gravity, space is fundamentally discrete, and evolution in symmetric cosmological models is nonsingular. This three week miniprogram will combine experts in both areas and on the classical approach to singularities to make further progress on this fundamental problem.

------endquote-------

Francesca's post
https://www.physicsforums.com/showthread.php?p=976175#post976175
was #17 in this thread
https://www.physicsforums.com/showthread.php?t=119156
 
Bojowald has also been invited to give a week of lectures in September at the Brazil School of Cosmology and Gravitation
http://www.cbpf.br/~cosmogra/bscgxxii.htm

His singularity-free version of quantum cosmology is getting to look
kind of standard. Thanks to Christine for this news!

Probably his authorship of the Living Reviews article helped solidify that
and then his writing the Elsevier Encyclopedia of Mathematical Physics
article on Quantum Cosmology
http://arxiv.org/abs/gr-qc/0603110

When you write the encyclopedia article on Quantum Cosmology that sort of makes it official that your version is the standard benchmark.

Living Reviews has a similar feel
http://arxiv.org/abs/gr-qc/0601085
That one was specifically on LOOP quantum cosmology.
 
Last edited:
I wonder how they are triying to interpret two oof the most relvants, IMHO consecuences of the yet made analisys.

Concretely the change of orientation of the 3 space when the singularity is crossed. In fact all the physics interpretation of evolution through the singularity is a chalenge.

For example it seemengly opens the issue of aparence of naked singularitys. If so, where do they appear?
 

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