Status of large higher dimensions

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SUMMARY

The discussion centers on the status of large higher dimensions, specifically addressing the second Randall-Sundrum model which proposes large dimensions instead of compactified ones. Recent findings from Spergel's group, based on neutron star collision data analyzed through electromagnetic (EM) and gravitational wave (GW) astronomy, have experimentally constrained spacetime dimensions to 3+1. This evidence effectively rules out models suggesting gravitational leakage into large extra dimensions, including 3-brane models embedded in higher-dimensional spaces.

PREREQUISITES
  • Understanding of the Randall-Sundrum model
  • Familiarity with gravitational wave astronomy
  • Knowledge of neutron star collision phenomena
  • Basic concepts of spacetime dimensions in theoretical physics
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  • Research the implications of the Randall-Sundrum model on modern physics
  • Explore gravitational wave detection techniques and their applications
  • Study the properties and significance of neutron star collisions
  • Investigate alternative theories to explain the weakness of gravity
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The discussion is beneficial for theoretical physicists, astrophysicists, and researchers interested in the implications of higher dimensions and gravitational theories.

Anne Ross
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The second Randall-Sundrum model was based on a large as opposed to compactified dimension. Has the possible existence of large higher dimensions been eliminated and what evidence rules them out?
 
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Recently, Spergel's group have written a paper based on last year's widely discussed neutron star collision which was detected using both EM as well as GW astronomy. The measurement experimentally constrains the amount of spacetime dimensions to 3+1 and it has therefore ruled out models based on the hypothesis that gravitational leakage occurs into large extra dimensions (which would explain the relative weakness of gravity), such as 3-brane models embedded in higher dimensional spaces.
 
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That is great Auto-Didact. Just what I needed.
 
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