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Precession can be demonstrated effectively through a spinning top. If a spinning top is placed on a flat surface near the surface of the Earth at a vertical angle and is not spinning, it will fall over due to the force of gravity producing a torque acting on its center of mass. However, if the top is spinning on its axis, it precesses about the vertical direction, rather than topple over due to this torque. Precessional motion is a combination of a steady circular motion of the axis and the...
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Precession Caused by Gravitational Waves.

Ali Seraj1, Blagoje Oblak2

  • 1Centre for Gravitational Waves, Université Libre de Bruxelles and International Solvay Institutes, CP 231, B-1050 Brussels, Belgium.

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|August 26, 2022
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Summary
This summary is machine-generated.

Gravitational waves cause gyroscopes to precess, extending the Lense-Thirring effect. This "gyroscopic memory" effect, measurable by observatories like LIGO, offers new insights into gravitational waves and black hole mergers.

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Area of Science:

  • * Astrophysics
  • * General Relativity
  • * Gravitational Wave Astronomy

Background:

  • * The Lense-Thirring effect describes how massive rotating objects warp spacetime, causing nearby objects to precess.
  • * Gravitational waves are ripples in spacetime caused by accelerating masses, detected by observatories like LIGO.
  • * Understanding the interaction between gravitational waves and matter is crucial for testing general relativity.

Purpose of the Study:

  • * To demonstrate that gravitational waves induce gyroscope precession.
  • * To extend the stationary Lense-Thirring effect to dynamic gravitational wave sources.
  • * To identify and analyze the
  • Main_Methods
  • Main_Results
  • Conclusions

Main Methods:

  • * Theoretical analysis of gyroscope motion in the spacetime of gravitational waves.
  • * Calculation of precession rates and their dependence on source distance and Noether currents.
  • * Estimation of the gyroscopic memory effect's magnitude for observed gravitational wave signals.

Main Results:

  • * Gravitational waves cause freely falling gyroscopes to precess relative to distant stars.
  • * The precession rate is inversely proportional to the square of the distance to the gravitational wave source.
  • * A novel
  • gyroscopic memory
  • effect is identified, including a contribution from gravitational electric-magnetic duality.

Conclusions:

  • * Gravitational waves possess a previously unrecognized effect on gyroscope orientation.
  • * The gyroscopic memory effect offers a new observable for gravitational wave astronomy.
  • * This phenomenon may be more pronounced for supermassive black hole mergers, providing a target for future observations.