Hossless Anti-Gravity: Bojowald's Landmark Paper & Beyond

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SUMMARY

Bojowald's landmark paper on Loop Quantum Cosmology (LQC) establishes that gravity repels at extremely high densities, a finding supported by 109 subsequent articles. The original analysis focused on isotropic cases, but later research has generalized these results under less restrictive assumptions. Notably, Singh has proposed that this reversed gravitational effect could have observable signatures in Gamma-Ray Bursts (GRBs). The implications of reversed gravity are significant in addressing cosmological puzzles, particularly concerning dark energy and dark matter.

PREREQUISITES
  • Understanding of Loop Quantum Cosmology (LQC)
  • Familiarity with Gamma-Ray Bursts (GRBs)
  • Knowledge of gravitational theories and their implications
  • Basic comprehension of cosmological concepts such as dark energy and dark matter
NEXT STEPS
  • Research the implications of Bojowald's paper on Loop Quantum Gravity
  • Explore Parampreet Singh's contributions to stellar collapse models in LQC
  • Investigate observational tests for reversed gravity effects in astrophysics
  • Study the relationship between dark energy, dark matter, and gravity in cosmological contexts
USEFUL FOR

Astronomers, physicists, and researchers interested in cosmology, particularly those focused on the implications of Loop Quantum Gravity and its potential observational signatures.

marcus
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Here are 109 articles (or books)
http://arxiv.org/cits/gr-qc/0102069?skip=75&db=spires
which all cite Bojowald's landmark paper where he determined that in Loop cosmology gravity REPELS at very high density. Here is the orig:
http://arxiv.org/gr-qc/0102069

the original paper dealt with an isotropic case (the analysis was simplified by making things uniform or symmetric) but since then people have extended the result, assuming less and less, to make it more general.

AFAICS this has no direct connection with the "anti-gravitation" that Sabine H is discussing in her thread of that name. But maybe it is an amusing coincidence.

In any case there is a considerable literature now which takes seriously the possibility that the effect of gravity reverses at very high density, and becomes repellent.
Bojowald, Singh, and others have modeled stellar-size collapse in some detail and Singh has proposed that the model may have an observable signature which can be sought in GRBs.

In any case reversed gravity is a feature of the LQC model, which has the correct classical limit and is currently being studied for observational testing.
 
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Hi marcus,

that is indeed interesting! I guess the interest in such behaviour is strongly supported by the cosmological puzzles, in the first line the dark energy/dark matter problems, which indicate that we are really missing something important. That - among other things - is a reason why I think experimental focus will probably shift away from colliders and towards astro/cosmology.

B.
 
hossi said:
Hi marcus,

that is indeed interesting!

I am delighted by your interest. If you ever want to pursue the phenomenology of (loop) quantum gravity stellar collapse, let me know and I will dig up a paper or two by Parampreet Singh or an online seminar talk----something that you might find usable.
 

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