Bell correlation between horizons

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    Bell Correlation
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SUMMARY

The discussion centers on whether polarization cross-sections from opposite microwave background n-poles violate the Bell inequality. Participants conclude that they do not, suggesting that the Cosmic Background Radiation (CBR) has been gravitationally 'twisted' into a preferred directional phase plane. The extent of polarization is identified as frequency dependent, with a proposed method for testing this hypothesis by examining near and distant galaxies along similar lines of sight for distance and frequency dependent polarization.

PREREQUISITES
  • Understanding of Bell inequalities in quantum mechanics
  • Familiarity with Cosmic Microwave Background Radiation (CBR)
  • Knowledge of polarization in astrophysics
  • Experience with observational techniques in astronomy
NEXT STEPS
  • Research methods for testing polarization in Cosmic Microwave Background Radiation
  • Explore the implications of gravitational effects on CBR
  • Study the relationship between frequency and polarization in astrophysical contexts
  • Investigate observational techniques for analyzing galaxies along similar lines of sight
USEFUL FOR

Astronomers, physicists, and researchers interested in quantum mechanics, cosmic background radiation, and the study of polarization in astrophysical phenomena.

Loren Booda
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Do polarization cross-sections from opposite microwave background n-poles disobey the Bell inequality?
 
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Interesting point. I would say it does not. Best guess is the CBR has been gravitationally 'twisted' into a preferred directional phase plane. I would also guess the extent of polarization is frequency dependent. This would be fairly easy to test. Take near and distant galaxies along similar lines of sight and check for both a distance and frequency dependent polarization.
 

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