Loop Quantum Cosmology dual to Randall-Sundrum Model

In summary, Parampreet Singh's recent paper reports a connection between loop quantum gravity and string theory, where loop cosmological dynamics and dualities are studied in relation to Randall-Sundrum braneworld scenarios. The paper discusses the role of discrete quantum geometric effects in dynamical evolution, leading to quadratic energy density modifications to the Friedmann equation. The presence of an extra (large) time-like dimension is of particular interest, as it is usually considered unphysical in string theory. The paper also explores the relationship between the expanding phase, contracting phase, and phantom phase in loop quantum cosmology, and shows dual relationships with Randall-Sundrum cosmology. Further analysis and discussion on this connection between loop quantum gravity and string theory is warranted.
  • #1
yanniru
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Specifically LGC is dual to RS theory with an extra (large) time-like dimension, as reported by Parampreet Singh today in:
http://arxiv.org/PS_cache/gr-qc/pdf/0603/0603043.pdf

This is the first connection between loop quantum gravity and string theory that I am aware of. The need for an extra time-like dimension is of particular interest as multiple timelike dimensions appear in string theory only under specific instances such as N=2 supersymmetry and 26 dim string theory and both are considered unphysical. Comments on what this means are appropriate. Here is the abstract and a couple quotes from the summary of the paper.
Richard


Loop cosmological dynamics and dualities with Randall-Sundrum braneworlds
Authors: Parampreet Singh
The discrete quantum geometric effects play an important role in dynamical evolution in the loop quantum cosmology. These effects which are significant at the high energies lead to the quadratic energy density modifications to the Friedmann equation, as in the Randall-Sundrum braneworld scenarios but with a negative sign. We investigate the scalar field dynamics in this scenario and show the existence of a phase of super-inflation independent of the inverse scale factor modifications as found earlier. In this regime the scalar field mimics the dynamics of a phantom field and vice versa. We also find various symmetries between the expanding phase, the contracting phase and the phantom phase in the loop quantum cosmology. We then construct the scaling solutions in the loop quantum cosmology and show their dual relationship with those of the Randall-Sundrum cosmology.

We have shown that in this case the Friedmann equations gets a rho squared modification similar to the Randall-Sundrum scenario but with a negative sign(which also arises in a modified Randall-Sundrum model with a time-like extra dimension).

We find that the scaling solutions in the effective theory are dual to those of the Randall-Sundrum scenario if the critical density arising in LGC is identified with the brane tension.
 
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  • #2
Oh my. I saw Singh's paper when I was surfing the arxiv yesterday, and wondered "Can this be for real?" Since you bring it up here I'm going to have to dig into it and see what I think. I especially want to see what he means by "loop quantum gravity" because sometimes string physicists have definitions of that that would seem strange to the LQG community.
 

FAQ: Loop Quantum Cosmology dual to Randall-Sundrum Model

What is Loop Quantum Cosmology dual to Randall-Sundrum Model?

Loop Quantum Cosmology dual to Randall-Sundrum Model is a theoretical framework that combines concepts from Loop Quantum Gravity and the Randall-Sundrum Model in order to address the problems of quantum gravity and the cosmological constant in cosmology. It proposes a way to reconcile the differences between these two theories and provide a more complete understanding of the universe.

How does Loop Quantum Cosmology dual to Randall-Sundrum Model explain the cosmological constant problem?

The cosmological constant problem is the discrepancy between the observed value of the cosmological constant and the predicted value from quantum field theory. Loop Quantum Cosmology dual to Randall-Sundrum Model offers a solution by introducing a new mechanism for generating the cosmological constant that is based on the principles of Loop Quantum Gravity. This mechanism predicts a value that is consistent with observations and helps to resolve the problem.

What is the role of extra dimensions in Loop Quantum Cosmology dual to Randall-Sundrum Model?

In the Randall-Sundrum Model, the presence of extra dimensions is used to explain the hierarchy problem in particle physics. In Loop Quantum Cosmology dual to Randall-Sundrum Model, these extra dimensions are also present but they play a different role. They are used to provide a new perspective on the origin of the universe and to address the problems of quantum gravity and the cosmological constant.

What are the key differences between Loop Quantum Cosmology and Randall-Sundrum Model?

The main difference between Loop Quantum Cosmology and Randall-Sundrum Model is that the former is a quantum theory of gravity while the latter is a classical theory with extra dimensions. Loop Quantum Cosmology also takes into account the effects of quantum gravity on the early universe, while the Randall-Sundrum Model is primarily concerned with the hierarchy problem in particle physics.

Is there any observational evidence for Loop Quantum Cosmology dual to Randall-Sundrum Model?

Currently, there is no direct observational evidence for Loop Quantum Cosmology dual to Randall-Sundrum Model. However, the predictions of this theory are still being studied and tested through various experiments and observations. Some potential evidence may come from observations of the cosmic microwave background, gravitational waves, and the large-scale structure of the universe. Further research and observations are needed to confirm the validity of this theory.

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