Red shift frequency from a black hole

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SUMMARY

The discussion centers on the redshift frequency of electromagnetic (EM) radiation near a black hole, specifically addressing the relationship between photon frequency and gravitational potential energy as one approaches the event horizon. The equation presented, (f1 - f2)/(f1 + f2) = GM(1/r1 - 1/r2), is used to analyze frequency changes at varying distances from the black hole. It is concluded that the event horizon is a fixed boundary, independent of the light's frequency, contradicting the notion that different frequencies would have varying event horizons. The conversation emphasizes the necessity of understanding general relativity (GR) to accurately interpret these phenomena.

PREREQUISITES
  • Understanding of general relativity (GR) principles
  • Familiarity with electromagnetic (EM) radiation and photon behavior
  • Knowledge of gravitational potential energy and its mathematical representation
  • Basic grasp of black hole physics and event horizon characteristics
NEXT STEPS
  • Study the implications of general relativity on black hole physics
  • Explore the concept of gravitational redshift in detail
  • Investigate the mathematical derivation of the Schwarzschild radius
  • Learn about the curvature of spacetime and its effects on light propagation
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Astronomers, physicists, and students of theoretical physics who are interested in black hole dynamics, gravitational effects on light, and the principles of general relativity.

Tyro
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Can someone tell me if these statements are right/wrong, and if wrong, why they are wrong?

Lets say you have a light (or more generally, EM) source a distance r from a black hole's core, with r > event horizon radius.

As you move closer towards the black hole, since the energy of a photon = hf, with h = constant, and the gravitational PE varies as 1/r...therefore the frequency fall due to red shifting falls as 1/r as well.

I get this equation relating the frequencies at 2 points and the radius from the black hole: (f1 - f2)/(f1 + f2) = GM(1/r1 - 1/r2)

If the above are true, then the event horizon for different frequencies of light varies. High frequency EM radiation will have a larger event horizon than low frequency EM radiation.

AFAIK, the event horizon is a fixed distance for light...

Am I looking at the problem too "classically"?
 
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Another way of looking at the event horizon is looking at how spacetime curves once you go past it. An escape velocity of c, according to GR, denotes such an extreme curvature of spacetime that it literally doubles back on itself. So, it doesn't matter what the light's frequency is, beyond the event horizon nothing can escape the curvature of spacetime.
 

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