Black Holes: Infalling Observers and BH Evaporation

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Discussion Overview

The discussion revolves around the nature of black holes, specifically addressing the behavior of infalling observers and the implications of black hole evaporation via Hawking Radiation. Participants explore theoretical aspects, observational paradoxes, and the effects of time dilation near the event horizon.

Discussion Character

  • Exploratory
  • Debate/contested
  • Technical explanation
  • Conceptual clarification

Main Points Raised

  • Some participants question how an infalling observer can cross the event horizon if black holes evaporate in a finite time from an outside observer's perspective.
  • It is suggested that the appearance of an object never entering a black hole is an optical illusion due to the time it takes for light to reach an outside observer.
  • One participant asserts that an infalling observer does reach the singularity in finite time, contrasting with the perception of freezing at the event horizon.
  • There is a discussion about the time it takes for an observer to cross the event horizon, with some suggesting it is simply a function of distance and speed.
  • Some participants argue that black holes are currently accreting matter rather than evaporating, with future evaporation dependent on temperature exceeding the cosmic microwave background radiation (CMBR) temperature.
  • Disagreement arises regarding the presence of Hawking radiation, with some asserting that it exists but is negligible compared to infalling matter.
  • Concerns are raised about the effects of tidal forces and spaghettification for infalling observers, particularly in relation to the size of the black hole.
  • Time dilation effects are discussed, noting that the perception of time for an infalling observer differs significantly from that of an external observer.

Areas of Agreement / Disagreement

Participants express multiple competing views regarding the nature of black hole evaporation, the experience of infalling observers, and the implications of time dilation. The discussion remains unresolved with no consensus reached on several key points.

Contextual Notes

Participants note that the understanding of black hole behavior is dependent on various assumptions, including the definitions of evaporation and the effects of external radiation. There are unresolved questions regarding the mathematical treatment of these phenomena.

  • #31
Naty1 said:
I believe Chronos explains this by noting that the horizon can be viewed as a light hypersurface...which is moving at lightspeed...I don't fully understand that perspective that but he's seem right about everything else.


One thing I do understand: Approaching a big BH from the exterior is no different than approaching a big dense planet...except, I guess, the BH is, well, black...the gravity itself [gravitational potential] is strong up close, but the gravitational potential gradient [the curvature of tidal force spaghettification] is nothing unusual. In other words, the gravitational gradient becomes extreme at the singularity not at the horizon; apparently the only 'unusual' thing at the horizon is a Schwarzschild coordinate ['fictitous'] singularity in time...so things appear to slow down from a stationary distant frame, but locally to a free falling observer things all seem 'normal' and no horizon can even be detected by such an soberver.

Well, I disputed this statement of Chronos, and stand by my disputation. From the point of view of the free faller, light from distant sources is not highly redshifted, and distant clocks do not appear to run very slow. On the other hand, the distant observer does see light from the infaller extremely redshifted and their clocks run slow then stop. I provided two different explanations of these facts.

The infaller continues to receive light from distant sources, with no difficulty, until catastrophe at the singularity.
 
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  • #32
Hey PAllen...

This is because the infaller approaches the speed of light as the event horizon is approached making it increasingly difficult for external photons to 'catch up' with the infaller.
I believe Chronos explains this by noting that the horizon can be viewed as a light hypersurface...which is moving at lightspeed...I don't fully understand that perspective that but he's seem right about everything else.

PAllen
Well, I disputed this statement of Chronos, and stand by my disputation.

Disputation! Cool [LOL]

Actually we agree. I was NOT trying to sneak in a 'last word' contrary view in the vain hope you would not catch me!

It took me a few moments to see my error: I should have quoted simply this from Chronos:

This is because the infaller approaches the speed of light as the event horizon is approached...

because I thought he might be adopting a perspective relative to the event horizon...I was only wondering about looking inward toward the black hole... I have never quite understood that perspective. I figure I am missing something if both he and pervect have adopted that 'frame' [bad word I know] for some reason I still do not get...

Anyway, your posted point that light from the distant cosmos is NOT radically redshifted I have read multiple times and even posted quotes supporting that view elsewhere from Kip Thorne and maybe Brian Greene. So you are in good company! Cheers.
 
  • #34
that's kind of scary, the plain one I mean
 
  • #35
This is a complex issue. I found 2 papers dealing with the subject
http://th-www.if.uj.edu.pl/acta/vol39/pdf/v39p1357.pdf
DECOUPLING OF KINEMATICAL TIME DILATION AND GRAVITATIONAL TIME DILATION IN PARTICULAR GEOMETRIES
" ... One can find that in the case of a radial fall in Schwarzschild geometry, light signal sent by an IO [remote observer] is received by an IFO [in-falling observer] as a red-shifted one"
http://www-e.unimagdeburg.de/mertens/teaching/seminar/themen/touching_ghosts.pdf
Touching ghosts: observing free fall from an infalling frame of reference into a Schwarzschild black hole
"... Less well known is the frequency ratio relation accompanying mutual signal exchange between Alice and her ‘mother station’, MS, located at r0. Namely, one finds that the frequency ratio is redshifted in both cases."
 
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  • #36
Chronos said:
This is a complex issue. I found 2 papers dealing with the subject
http://th-www.if.uj.edu.pl/acta/vol39/pdf/v39p1357.pdf
DECOUPLING OF KINEMATICAL TIME DILATION AND GRAVITATIONAL TIME DILATION IN PARTICULAR GEOMETRIES
" ... One can find that in the case of a radial fall in Schwarzschild geometry, light signal sent by an IO [remote observer] is received by an IFO [in-falling observer] as a red-shifted one"
http://www-e.unimagdeburg.de/mertens/teaching/seminar/themen/touching_ghosts.pdf
Touching ghosts: observing free fall from an infalling frame of reference into a Schwarzschild black hole
"... Less well known is the frequency ratio relation accompanying mutual signal exchange between Alice and her ‘mother station’, MS, located at r0. Namely, one finds that the frequency ratio is redshifted in both cases."

Looking at the first paper, I view it as agreeing with everything I said:

- in SC geometry you can factor gravitational and kinematic red shift
- for the infaller receiving signals from a distant observer, the two effects work against each other: gravitational blue shift reducing the kinematic red shift
- the balance of cancellation depends on where free fall starts from; starting free fall from closer to the horizon produces less red shift as the free faller crosses the horizon
- there is an extreme asymmetry in that the two effect add to each (rather than work against each other) other for signals from the infaller to the distant observer, leading to infinite redshift as the free faller approaches the horizon.
 
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  • #37
I agree gravitational redshift is a factor for an observer in free fall. Thanks for pointing that out. Apparently, however, it is not enough to entirely offset the kinematical component. Do you agree both papers assert signals from the 'mothership' to a radially infalling observer are redshifted by a non-trivial amount?
 
  • #38
Chronos said:
I agree gravitational redshift is a factor for an observer in free fall. Thanks for pointing that out. Apparently, however, it is not enough to entirely offset the kinematical component. Do you agree both papers assert signals from the 'mothership' to a radially infalling observer are redshifted by a non-trivial amount?

Yes, I agree. The amount of such redshift at time of horizon cross can be reduced, and I think even reversed, by starting free fall from sufficiently close to the horizon (with mothership far away and stationary - well defined in SC geometry).
 

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