Gravitational Waves: Definition & General Overview

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SUMMARY

Gravitational waves are disturbances in spacetime that can transmit energy, but defining them universally remains complex. The discussion highlights that in general relativity (GR), particularly in asymptotically flat spacetimes, the Bondi news function can be utilized to determine radiation presence. The Petrov classification serves as an analogy for electromagnetic (EM) waves, indicating that gravitational waves may not always conform to traditional definitions. The challenge lies in the lack of a comprehensive definition for gravitational field energy in GR.

PREREQUISITES
  • Understanding of general relativity (GR)
  • Familiarity with the Bondi news function
  • Knowledge of Petrov classification
  • Basic concepts of electromagnetic (EM) waves
NEXT STEPS
  • Research the Bondi news function in detail
  • Explore the Petrov classification and its applications in gravitational wave theory
  • Study the implications of asymptotically flat spacetimes in general relativity
  • Investigate the energy definitions of gravitational fields in various contexts
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Physicists, astrophysicists, and students of general relativity seeking to deepen their understanding of gravitational waves and their theoretical implications.

martinbn
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What are gravitational waves in general, not just in the weak field/linearized theory?
 
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Interesting question.

I'm not sure that the issue is really the weak field approximation. Isn't the real issue something that occurs in other contexts, e.g., plain old E&M on a flat background? Say I have a space that's empty except for a point charge. In the rest frame of the charge, this is a static field. In a frame where the charge is moving, an observer at a particular point will see a time variation in the field, and will probably interpret this as a wave disturbance passing by. Indeed, according to this observer, energy is being transported by the field. However, there is no energy being transported to infinity.

For gravity, in spacetimes with special symmetries, I guess one way to go is to use the Petrov classification. This is analogous to defining (pure) EM waves as null fields (although there are exceptions).

If the spacetime is asymptotically flat, I believe you can compute the Bondi news function to decide whether there is radiation.

I doubt that there is a definition that works in general. To call something a gravitational wave, you want it to be something that's transmitting energy. But in GR we don't have a definition of the energy of the gravitational field, except in special cases such as asymptotically flat spacetimes.
 
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