What happens to stars in front of a falling observer entering a black hole?

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SUMMARY

When a free-falling observer approaches a black hole, the redshift of stars in front of them can be expressed with the formula λ_{shift} = λ_{0} √(1 - R_{s}/R_{hover}). This formula indicates how the light from stars ahead is affected by the gravitational field of the black hole. The event horizon of a large black hole presents minimal tidal acceleration, making the crossing a non-event. Light from behind the observer is redshifted, while the black hole itself obscures most light from the opposite side, creating a dark region where background images cannot be seen.

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  • Understanding of general relativity and gravitational effects on light.
  • Familiarity with redshift and blueshift concepts in astrophysics.
  • Knowledge of Schwarzschild radius and its implications for black holes.
  • Basic grasp of gravitational lensing and its effects on light paths.
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  • Research the implications of the Schwarzschild radius on light behavior near black holes.
  • Study gravitational lensing effects and how they relate to black hole observations.
  • Explore the concept of redshift in detail, particularly in extreme gravitational fields.
  • Investigate Andrew Hamilton's work on black hole lensing and its visual representations.
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Astronomers, astrophysicists, and students studying black hole physics and gravitational effects on light. This discussion is particularly beneficial for those interested in the observational consequences of falling into a black hole.

Passionflower
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It is often said that passing the event horizon for a large black hole is basically a non event as the size of the tidal acceleration at the event horizon depends on the mass of the black hole.

But let's consider something else; what happens to the stars in front of a free falling observer falling radially at escape velocity into a black hole. Can we devise a formula that expresses the red or blue shift as seen by the observer?

We have the redshift formula for stars behind us, which is:
[tex]\sqrt { \left| \left( 1-\sqrt {{\frac {r_{{s}}}{r}}} \right) \left( <br /> 1+\sqrt {{\frac {r_{{s}}}{r}}} \right) ^{-1} \right| }{\frac {1}{<br /> \sqrt { \left| 1-{\frac {r_{{s}}}{r}} \right| }}}[/tex]
Which graphically looks like:
http://img442.imageshack.us/img442/4100/redshift.png
But what do we measure about the stars ahead of us?
 
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Yes, the result is:

[itex]\lambda_{shift}[/itex] = [itex]\lambda_{0}[/itex] [itex]\sqrt{1 - R_{s}/R_{hover}{}}[/itex]

Reference: "Black Holes A Traveler's Guide", P.37, Pickover.
 
I don't have "Traveller's guide", but the quoted expression looks like it's for a hovering observer (because of the R_hover).

The black hole itself blocks most of the light from the "other side".

For the falling case, see for instance Andrew Hamilton's webpage, http://casa.colorado.edu/~ajsh/approach.html#lensing.

Picking out the most relevant part of the webpage:

n the illustrated case, the lensing mass is a black hole. Any light rays which come within 1.5 Schwarzschild radii of the black hole fall into the black hole. Here there is a dark region, bounded by the red lines, within which images of background objects cannot appear.

For what you see after you pass through, look a bit later on the webpage, http://casa.colorado.edu/~ajsh/singularity.html, "The Schwarzschild bubble".

I've ommited some things that appear not to be directly relevant to the origianl question that are still interesting, including some interesting discussion about how and when one sees people who have previously fallen through the horizon.
 

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