Calculating Differential Precession of Gyroscopes Due to Gravitational Waves

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SUMMARY

The discussion focuses on calculating the differential precession of gyroscopes due to gravitational waves, referencing Andy Strominger's paper on the Sagnac shift of counterrotating beams. It explores the potential for computing this precession using the magnetic part of the Riemann tensor and the twist of freely falling gyroscopes. Additionally, it raises the question of whether a memory effect exists post-gravitational wave passage, potentially resulting in a permanent shift of the gyroscopes' axes. The implications of gravitational waves on galaxy formation and cosmic microwave background (CMB) imprinting are also considered.

PREREQUISITES
  • Understanding of gravitational waves and their properties
  • Familiarity with the Riemann tensor in general relativity
  • Knowledge of gyroscopic motion and precession
  • Basic concepts of cosmic microwave background (CMB) physics
NEXT STEPS
  • Research the Sagnac effect and its implications in relativistic contexts
  • Study the magnetic part of the Riemann tensor and its applications
  • Investigate the memory effect in gravitational wave physics
  • Explore the relationship between gravitational waves and cosmic structure formation
USEFUL FOR

Physicists, astrophysicists, and researchers interested in gravitational wave effects, gyroscopic dynamics, and cosmic evolution will benefit from this discussion.

WannabeNewton
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To motivate the question, Andy Strominger recently put out a paper on calculating the Sagnac shift of counterrotating beams due to the angular momentum flux of a passing gravitational wave.

See here: http://arxiv.org/abs/1502.06120.

But consider now two nearby freely falling gyroscopes initially at rest in some background inertial frame and a weak gravitational wave passing by them. Is there a way to compute the differential precession of the gyroscopes due to the angular momentum of the gravitational wave, say by looking at the magnetic part of the Riemann tensor and/or the twist of a congruence of freely falling gyroscopes? Has such a calculation been done in the literature?

To clarify, I don't mean the precession of a single gyroscope relative to the axes of the TT-gauge coordinates.

Furthermore, would there also be a memory effect after the gravitational wave has gone to future null infinity, say in terms of a permanent relative shift of the gyroscopes' axes?
 
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This topic is way beyond my technical ability but the paper you refer to has a section on the memory effect where two inertial objects can be permanently moved apart ( and together ) by a passing energy pulses. I may have misinterpreted that so please correct me if necessary.

I was struck by two possible effects

1. Galaxy formation via collapse of a gigantic hydrogen cloud is affected by sound waves with colossal wavelengths which cause compressed regions where star formation is accelerated. Could GWs do this ?

2. the matter distribution just before transparency could also be affected, imprinting on the CMB.
 

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