Distinguishing Einstein Cartan from GR: Experiments

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SUMMARY

This discussion centers on distinguishing Einstein-Cartan gravity from General Relativity (GR) through experimental means. It is established that both theories agree in vacuum but differ in the presence of matter, particularly due to the torsion present in the Einstein-Cartan metric. The University of Washington's attempts to create a high angular momentum source to test spin-dependent gravity are noted, although their sensitivity remains insufficient to differentiate between the two theories. Additionally, neutron stars' spin alignment may provide insights into modifications in their equilibrium states, with references to significant works by Poplawski and others in the field.

PREREQUISITES
  • Understanding of Einstein-Cartan gravity and General Relativity
  • Familiarity with torsion in theoretical physics
  • Knowledge of spin and its implications in quantum mechanics
  • Basic principles of neutron star physics
NEXT STEPS
  • Research experimental setups for testing spin-dependent gravity
  • Explore Poplawski's contributions to Einstein-Cartan theory
  • Investigate the implications of torsion in neutron star equilibrium
  • Learn about the gauge approach to gravity as proposed by Kibble
USEFUL FOR

The discussion is beneficial for theoretical physicists, astrophysicists, and researchers interested in gravitational theories and their experimental validation.

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Are there any experiments either already performed or even simply proposed that could be used to distinguish Einstein Cartan gravity from GR?

My current understanding is that they are the same in vacuum, and only differ in matter. In matter the Einstein Cartan metric can have torsion, unlike the GR metric, but in vacuum they agree. Because of the way spin is related to torsion in Einstein Cartan and how important spin is in QM, it seems like that might be a viable candidate for GR violations.
 
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I'm not aware of any observation of torsion yet. It's difficult, because all our tests of GR vs. alternative theories of gravitation rely on huge (astronomical) macroscopic objects. So spin doesn't play a role but only macroscopic descriptions of matter (aka hydrodynamics) and the electromagnetic field, which in the gauge approach to gravity a la Kibble lead to standard GR.
 
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The University of Washington gravity guys tried to build a high angular momentum source/target. It was a mix of two materials magnetized in opposite directions, but one had more spin than the other. This would allow them to test spin-dependent gravity. I don't know how far they got with this.

Even so, this device was many tens of orders of magnitude less sensitive than they would need to distinguish GR from Einstein-Cartan.
 
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vanhees71 said:
I'm not aware of any observation of torsion yet. It's difficult, because all our tests of GR vs. alternative theories of gravitation rely on huge (astronomical) macroscopic objects. So spin doesn't play a role but only macroscopic descriptions of matter (aka hydrodynamics) and the electromagnetic field, which in the gauge approach to gravity a la Kibble lead to standard GR.

In neutron stars the spins align resulting in a total big spin. That should result in some modification in the state/equilibrium equation of the star, I think.
 
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Poplawski writes a lot about Einstein-Cartan theory. https://www.sciencedirect.com/science/article/pii/S0370269310011561 has a high citation count, it may or not be helpful. Unfortunately, I think Poplawski focuses on the aspect of the theory that predicts that BH collapse "bounces" in Einstein-Cartan theory, which may not be the sort of experimentally testable prediction you're looking for.
 
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