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skydivephil
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Will the results from the PLanck satellite shed any light on Loop Quantum Cosmology or any other form of matter bounce?
skydivephil said:Wow that's a lot to be getting on with, thanks.
The short answer is: probably not much. It will add further constraints to the available parameter space, but it isn't likely to be enough to really constrain inflation (which is where LQC comes into play).skydivephil said:Will the results from the PLanck satellite shed any light on Loop Quantum Cosmology or any other form of matter bounce?
marcus said:But Phil! You don't have to even glance at any of it!
My feeling about this is that you have asked an extremely interesting question, that we should be following over the next 12 months. And that right now IMHO we don't know the answer. Even experts don't yet know what bearing Planck will have on LQG/LQC.
The only thing I know to do is to read (or skim) the brief summaries, and the conclusion sections, of the papers by phenomenologists like Barrau. (and Grain, Mielczarek etc.) And get a sense of it, how definite are they being, how reserved, what do they think?
I don't think there is a sure conclusive answer to the question yet. But it is something to watch.
I do know that two major leaders in LQG are Rovelli and Ashtekar---and before 2006 Ashtekar was doing comparatively little in cosmology, now it is his main focus. And before 2009 Rovelli was not doing LQC at all---now LQG application to cosmology is a major interest of his (several papers per year). People get to be leaders by knowing what to work on---it is a sign that Loop cosmo is ripe when it has drawn their attention away from the main
theory. From the general to the critical application.
Loop Quantum Cosmology (LQC) is a theoretical framework that combines principles of quantum mechanics and general relativity to study the evolution of the universe on a small scale. It proposes a discrete structure of space-time, where space is made up of tiny loops and time is quantized into discrete units.
The Planck Satellite is a space observatory launched by the European Space Agency in 2009 with the primary goal of studying the Cosmic Microwave Background (CMB). The CMB is the oldest light in the universe and contains valuable information about the early universe. The Planck Satellite has provided precise measurements of the CMB, which can be used to test and refine theories such as LQC.
LQC proposes that the Big Bang was not a singularity, as predicted by general relativity, but rather a "bounce" from a previous contracting phase. This bounce occurs when the universe reaches a minimum size, and the repulsive forces of quantum gravity cause it to expand again. This avoids the singularity and provides a more complete understanding of the early universe.
One of the main differences between LQC and other theories, such as String Theory, is that LQC is based on a discrete structure of space and time, while other theories assume a continuous space-time. LQC also provides a more complete and self-consistent framework for studying the universe on a quantum level, while other theories may have limitations or require additional assumptions.
One of the main challenges is that the Planck Satellite was not specifically designed to test LQC, so the data must be carefully analyzed and interpreted in the context of the theory. Additionally, LQC is still a developing and evolving theory, so there may be discrepancies or uncertainties in predicting certain phenomena. Further research and collaboration between cosmologists and quantum physicists is needed to fully explore the potential of LQC with the data from the Planck Satellite.