Conundrum thinking about crossing an Event Horizon

In summary, the infalling observer crosses the event horizon because they reach a velocity of C. They cannot detect that they have crossed the horizon, and would only know if they lost communication with remote observers.
  • #1
Grinkle
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Folks usually point out that tidal forces make questions like the one I am asking below hypothetical at best, I understand that.

I am taking as an axiom that a free-falling observer observes nothing unusual when crossing an event horizon. More strongly, the free-falling observer cannot detect in any way that they have crossed an event horizon. If this isn't true, perhaps the reason why it isn't true answers my question.

From this lack of consequence to crossing an EH does it follow that as far as the free-falling observer is concerned, they haven't crossed any EH? How would they know that the singularity has now become an inevitable event for them? For a human observer curious to know if they crossed an EH, what consequence could they check for?
 
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  • #2
They could see if their wristwatch broke?
 
  • #3
Grinkle said:
From this lack of consequence to crossing an EH does it follow that as far as the free-falling observer is concerned, they haven't crossed any EH? How would they know that the singularity has now become an inevitable event for them? For a human observer curious to know if they crossed an EH, what consequence could they check for?
What they know depends on what sources of information are available to them. The most obvious would probably be that they lost communication with remote observers. But as far as I know, there's nothing they can do inside the spaceship that would tip them off.
 
  • #4
"I can't detect it" doesn't mean it hasn't happened. An infalling observer does cross the event horizon, and the event horizon is a well-defined surface in spacetime. There isn't any "for me" about it - you are inside or outside.

One simple way to determine whether you've crossed the horizon is to work out where it is by observing orbits before you drop through it. Then you can use timing or observation of marker buoys to determine when you've dropped through.

I suspect if you watch incoming starlight it may be enough to locate the horizon. All the stars will shift to a small patch of sky above you as you approach, and the angular range may be enough to determine when you've reached the horizon. Not sure - you may also need the hole mass in advance.

But in local terms, there's no way to detect horizon crossing, no.
 
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  • #5
If they looked behind them, the stars and everything else would be redshifted to the point of blackness.
 
  • #6
russ_watters said:
What they know depends on what sources of information are available to them. The most obvious would probably be that they lost communication with remote observers. But as far as I know, there's nothing they can do inside the spaceship that would tip them off.
Depends what you mean. Outside sources would always be able to communicate to them, and they would always be able to communicate with other infalling observers. They would not be able to answer non-infalling sources outside the hole, true.
 
  • #7
At the event horizon has the object reached a velocity of C?
 
  • #8
Exidor said:
If they looked behind them, the stars and everything else would be redshifted to the point of blackness.
Some care is needed here. The Doppler shift depends on the infaller's velocity, so there is no unique value of Doppler that identifies horizon crossing. I'm also not certain that the stars are red-shifted, but I will check.
 
  • #9
Exidor said:
At the event horizon has the object reached a velocity of C?
No. First - speed relative to what? A local description of crossing the horizon is that the horizon passes through you at c. But no local observer will see you doing c. A global description doesn't really have a well-defined notion of velocity except to refer you to particular families of local observers - who cannot see you doing c.
 
  • #10
Looking at the black hole from outside the event horizon everything at the event horizon and closer to the center of the black hole would appear black, wouldn't it? Is this the same as an infinite red shift?
 
  • #11
Ibix said:
Outside sources would always be able to communicate to them

If there were a pinging beacon outside the EH (say in some stable orbit around the black hole) that the traveler was monitoring, will the ping frequency combined with knowledge of the beacon orbit and the mass of the black hole tell the traveler when they have crossed the EH? I am thinking, perhaps incorrectly, that the traveler will observe the ping frequency increasing as they go deeper into the gravity well.
 
  • #12
Ibix said:
Some care is needed here. The Doppler shift depends on the infaller's velocity, so there is no unique value of Doppler that identifies horizon crossing. I'm also not certain that the stars are red-shifted, but I will check.
My calculations suggest stars are blueshifted for an infalling observer.

I wrote down a tangent vector to the worldline of a radially infalling massive observer and a radially infalling light pulse. The inner product should be proportional to the measured energy of the light, and hence its frequency. This appears to be an increasing quantity, at least as far as the horizon.


Edit: I may have a sign error - need to recheck.

Edit2: I did - this post is incorrect
 
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  • #13
Exidor said:
Looking at the black hole from outside

I think the traveler will always see only black in front of them, even after they cross the EH. If that is not the case, I am very confused.
 
  • #14
Exidor said:
Looking at the black hole from outside the event horizon everything at the event horizon and closer to the center of the black hole would appear black, wouldn't it? Is this the same as an infinite red shift?
Light does not come from the horizon, so defining the redshift of something that isn't there seems problematic to me.
 
  • #15
I would think it would slow down because of Doppler shift. But you also have time dilation as the observer approached C?
 
  • #16
Grinkle said:
If there were a pinging beacon outside the EH (say in some stable orbit around the black hole) that the traveler was monitoring, will the ping frequency combined with knowledge of the beacon orbit and the mass of the black hole tell the traveler when they have crossed the EH?
Probably. I'd need to switch to coordinates that don't fail at the horizon to answer this, and that's more maths than I'm going to do now - have to help with food prep...
Grinkle said:
I am thinking, perhaps incorrectly, that the traveler will observe the ping frequency increasing as they go deeper into the gravity well.
Based on #12, that would be my guess.

Edit: ...but #12 is wrong. See below.
 
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  • #17
Exidor said:
I would think it would slow down because of Doppler shift. But you also have time dilation as the observer approached C?
That's one way to look at it. Another is to note that the infalling light gains energy from the gravitational potential so is blue shifted - apparently more than the kinematic redshift from the observer's increasing infall speed.
 
  • #18
Does the edge of a black hole show blue shifting of light in astronomical observations?
 
  • #19
I was thinking inside a black hole C is exceeded but time becomes imaginary.
 
  • #20
Exidor said:
Does the edge of a black hole show blue shifting of light in astronomical observations?
I'm not aware of one being directly imaged. Why would you expect it to blueshift? We're not infalling observers. And what are you actually looking at? Light from the accretion disc (would be redshifted) or grazing light from stars behind (no effect for a non-rotating hole)?
Exidor said:
I was thinking inside a black hole C is exceeded but time becomes imaginary.
I'm afraid this makes no sense.
 
  • #21
"My calculations suggest stars are blueshifted for an infalling observer." - Ibex

Consider two free falling objects, one after the other. As they fall, the distance between them constantly increases due to the first object always falling faster than the second. To the first object, the second is receding from it, so it would appear to be red shifted. To a stationary observer, yes, the stars would appear blueshifted, but not to an infalling observer.
 
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  • #22
Well your saying that light coming towards a black hole is blue shifted. If this is the case then some of it would escape and appear at the edge of a black hole in an actual observation?

I am rusty but if you let v exceed c:
1/((1-(v^2/c^2))^(1/2))
The result is imaginary.
 
  • #23
Ibix said:
My calculations suggest stars are blueshifted for an infalling observer.

You should check your calculations. Ingoing light is redshifted for infalling observers.

Ibix said:
the infalling light gains energy from the gravitational potential so is blue shifted

Relative to static observers (observers hovering at a constant altitude).

Ibix said:
apparently more than the kinematic redshift from the observer's increasing infall speed.

No. See above.
 
  • #24
Ibix said:
My calculations suggest stars are blueshifted for an infalling observer.

I wrote down a tangent vector to the worldline of a radially infalling massive observer and a radially infalling light pulse. The inner product should be proportional to the measured energy of the light, and hence its frequency. This appears to be an increasing quantity, at least as far as the horizon.
As noted, I made a sign error (accidentally switched to -+++ for the metric) and missed a sanity check (my energy was negative everywhere) that would have detected it. Incoming light is redshifted for an observer free-falling from infinity.

This isn't quite true for observers released from rest close to the hole, who see light blue shifted at rest. Light doesn't instantly become redshifted compared to its source frequency when the observer is released, but it is redshifted compared to the at-rest observation and the redshift grows as they infall.
 
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  • #25
Ibix said:
Incoming light is redshifted for an observer free-falling from infinity.

Yes, agreed.

Ibix said:
This isn't quite true for observers released from rest close to the hole

Yes, that's correct; an observer released from rest at a finite height will see a decreasing blueshift, then a switch to redshift and an increasing redshift. How long it takes them to see the switch depends on how close they are to the horizon.
 
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  • #26
Exidor said:
Well your saying that light coming towards a black hole is blue shifted. If this is the case then some of it would escape and appear at the edge of a black hole in an actual observation?
For an observer hovering near the hole, light is blueshifted. But it would be redshifted by the same amount as it climbs back out of the hole's gravitational field. So stars observed past a (non-rotating) black hole are neither red nor blue shifted if you are far from the hole. If you are near the hole they may be blueshifted if you are hovering or redshifted if you are moving fast enough.
Exidor said:
I am rusty but if you let v exceed c:
1/((1-(v^2/c^2))^(1/2))
The result is imaginary.
But as already noted, nothing is exceeding c.
 
  • #27
Grinkle said:
If there were a pinging beacon outside the EH (say in some stable orbit around the black hole) that the traveler was monitoring, will the ping frequency combined with knowledge of the beacon orbit and the mass of the black hole tell the traveler when they have crossed the EH? I am thinking, perhaps incorrectly, that the traveler will observe the ping frequency increasing as they go deeper into the gravity well.
The frequency will decrease, as per my correction in #24 to my claim in #12, and discussion with PeterDonis.
 
  • #28
You don't know if the rules apply inside a black hole. And what about tachyons? Some people think they exist. Quantum entanglement?
 
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  • #29
skeptic2 said:
"My calculations suggest stars are blueshifted for an infalling observer." - Ibex

Consider two free falling objects, one after the other. As they fall, the distance between them constantly increases due to the first object always falling faster than the second. To the first object, the second is receding from it, so it would appear to be red shifted. To a stationary observer, yes, the stars would appear blueshifted, but not to an infalling observer.
Please clarify.
If the object is released from infinity, and the light is released from a source at infinity, would not both be in free fall, so no red shift nor blue shift would be noted in this case.
 
  • #30
Exidor said:
You don't know if the rules apply inside a black hole. And what about tachyons? Some people think they exist.
Note that this site is for discussion of mainstream science only. If you want to discuss alternate models of black hole interiors, please provide a peer-reviewed reference for the model you wish to discuss, as per site rules. I'm afraid that "the rules don't apply" and applying the Lorentz gamma factor (one of those very rules) seem contradictory to me, so I need to see such a reference before I can comment meaningfully.
 
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  • #31
Exidor said:
You don't know if the rules apply inside a black hole.

If the rules don't apply, we can't say anything at all, which makes discussion pointless. So as a basis for discussion here, we're assuming the same rules apply inside a black hole that apply outside. No other basis for discussion is practical.

Exidor said:
And what about tachyons? Some people think they exist. Quantum entanglement?

All of these are irrelevant to this discussion. Please stick to the topic of the thread.
 
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  • #32
Close mindedness makes discussion pointless also.
 
  • #33
Exidor said:
Close mindedness makes discussion pointless also.
Agreed. (yours, not ours). Thread is closed.
 
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1. What is a conundrum?

A conundrum is a complex problem or puzzle that is difficult to solve. It often involves conflicting or contradictory factors that make it challenging to find a clear solution.

2. What does it mean to cross an event horizon?

Crossing an event horizon refers to the point of no return in a black hole, where the gravitational pull is so strong that nothing, including light, can escape. It is a theoretical boundary that marks the beginning of the black hole's singularity.

3. How does conundrum thinking apply to crossing an event horizon?

Conundrum thinking can be applied to crossing an event horizon by considering the various factors and complexities involved in this phenomenon. It requires critical thinking and problem-solving skills to understand and potentially find solutions to the mysteries of black holes and their event horizons.

4. What are some potential consequences of crossing an event horizon?

One potential consequence of crossing an event horizon is the phenomenon known as spaghettification, where the extreme gravitational forces stretch and elongate objects as they approach the singularity. Another consequence is the distortion of time and space, making it difficult to understand or predict what happens within the event horizon.

5. Can we ever truly understand what happens beyond an event horizon?

As of now, it is impossible to directly observe or study what happens beyond an event horizon. However, through mathematical and theoretical models, scientists can make predictions and gain some understanding of this mysterious phenomenon. With advancements in technology and further research, we may one day have a better understanding of what lies beyond an event horizon.

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