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Observable QG effects in Chern-Simons gravity--Stephon Alexander
Important talk,
http://pirsa.org/09110132/
Important talk,
http://pirsa.org/09110132/
atyy said:Cool. Danke!
marcus said:Anybody who wonders about this would do well, I think, to watch the 1hour video:
http://pirsa.org/09110138/
Stephon explains the whole idea. Michael Peskin is there grilling him with questions, and also Neil Hurok the director of PI, a cosmologist. It is a risky idea. But it gets good people's attention and intrigues them.
It assumes that there are a lot of neutrinos in the early universe, produced somehow by some reactions. Neutrinos naturally form a condensate, just like the electrons in a superconductor pair up. With electrons in superconductor, two fermions combine to make a boson. In Stephon's model four neutrinos get together. It is only a rough analogy.
You are asking "what if there wasn't this condensate?" In that case the cosmo const would I believe be ZERO, in this model universe. In this model there is no other source of the dark energy.
Lots of things could go wrong. There might not have been enough neutrinos in the universe to make this happen. And maybe neutrinos do not actually condense into foursomes the way he thinks they might.
Chern-Simons gravity is a modified theory of gravity that incorporates the concept of torsion, which is the twisting or bending of space-time. Unlike other theories of gravity, which focus on curvature of space-time, Chern-Simons gravity takes into account both curvature and torsion.
Observable QG (quantum gravity) effects in Chern-Simons gravity refer to the predicted deviations from general relativity that can be observed in certain physical phenomena, such as the bending of light around massive objects or the behavior of gravitational waves. These effects are a result of the incorporation of torsion in the theory.
Chern-Simons gravity is a classical theory of gravity, but it incorporates aspects of quantum theory. It is often used as a starting point for developing a theory of quantum gravity, as it provides a framework for studying the effects of torsion on space-time and its interactions with matter.
Stephon Alexander's work has helped to expand our understanding of Chern-Simons gravity and its potential implications for quantum gravity. His research has shed light on the observable effects of torsion in gravitational interactions and has opened up new avenues for studying the interplay between gravity and quantum mechanics.
While there is not yet any direct experimental evidence for observable QG effects in Chern-Simons gravity, there are some ongoing experiments and observations that could potentially provide support for the theory. For example, the Laser Interferometer Gravitational-Wave Observatory (LIGO) is currently searching for gravitational waves that could exhibit signatures of torsion, and future space missions such as the Laser Interferometer Space Antenna (LISA) may also provide valuable data for testing predictions of Chern-Simons gravity.