Objects falling into a black hole

In summary: This is because the particle has crossed the event horizon and is no longer in contact with the outside universe.
  • #1
aademarco
11
1
I have a question pertaining to objects falling through the event horizon of a black hole.

It is my understanding that due to the immence gravity of a black hole and the way gravity affects the flow of time, that from the point of view of an observer at a safe distance from a black hole watching any object fall through the event horizon you can never see an object fall through due to how its flow of time changes relative to the observer. Its time will appear to become slower and slower until it appears to freeze infinitely close to the event horizon. From the point of view of the object falling through the event horizon it continues to fall all the way to the singularity. If that object could turn and look back out through the event horizon it would see time speed up infinitely.

Im having a hard time understanding, if the above is true, why black holes are not glowing bright with images of everything they have ever 'eaten' just above or at the event horizon. From our perspective, all the matter which has ever fallen into it had a clock which slowed to a stop the moment it hit the horizon despite the fact that from their own perspectives they went right through.
 
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  • #2
aademarco said:
Im having a hard time understanding, if the above is true, why black holes are not glowing bright with images of everything they have ever 'eaten' just above or at the event horizon. From our perspective, all the matter which has ever fallen into it had a clock which slowed to a stop the moment it hit the horizon despite the fact that from their own perspectives they went right through.

We do see them glow brightly at the event horizon, in the form of an accretion disk, as well as at the poles, where large quantities of x-rays can be emitted. Observing the actual black hole is not possible with visible light, but measuring the orbital speeds of visible matter and calculating the central mass about which they are falling towards is.
 
  • #3
aademarco said:
Im having a hard time understanding, if the above is true, why black holes are not glowing bright with images of everything they have ever 'eaten' just above or at the event horizon. From our perspective, all the matter which has ever fallen into it had a clock which slowed to a stop the moment it hit the horizon despite the fact that from their own perspectives they went right through.
The light from a collapsing object persists, but it becomes increasingly faint and increasingly redshifted. See this paper by Ames and Thorne for a complete analysis.

Ames and Thorne said:
The star is brightest and bluest at its rim, where the spectrum and intensity are independent of time; but the width of this time-independent region decays exponentially. Nearer the center of its disk, the star appears darker and redder; the redshift increases exponentially in time, and the intensity decays exponentially. The total, integrated radiation is dominated by the contribution from the rim: The spectrum is nearly time-independent and is peaked at its high-frequency end; but the total luminosity decays exponentially with time.
 
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  • #4
aademarco said:
If that object could turn and look back out through the event horizon it would see time speed up infinitely.
This is not quite correct, although it's a bit tricky to explain. Take a look at this earlier PF post https://www.physicsforums.com/showpost.php?p=2336347&postcount=4 which shows a Kruskal diagram copied from Misner, Thorne and Wheeler, the one labeled Fig 31.4(b).

The event horizon is the diagonal line labeled r = 2M, t = +∞. The falling particle is the curve with labels A, A', A''. As the particle approaches the event horizon, the coordinate time t runs through all its values and becomes infinite.

However the incoming light that the particle would see looking back is represented by left-sloping diagonal lines such as B, B', B''. Even when the particle hits the horizon, the incoming photons do not pile up. Although the retarded time as measured by the outgoing light rays becomes infinite, the "advanced time" as measured by the incoming rays remains finite.
 
  • #5


Your understanding is correct. According to Einstein's theory of general relativity, the gravitational pull of a black hole is so strong that it warps space and time around it. This means that the closer an object gets to the black hole, the slower time moves for that object according to an outside observer. This effect is known as gravitational time dilation.

As an object approaches the event horizon of a black hole, its time dilation becomes infinitely large. This means that from the perspective of an outside observer, time for the object appears to slow down and eventually stop at the event horizon. However, from the perspective of the object itself, it continues to fall into the black hole and experiences time normally.

So why don't we see a bright glowing image of everything that has fallen into a black hole at the event horizon? This is because as the object approaches the event horizon, it also becomes increasingly redshifted. This means that the light emitted from the object becomes stretched to longer wavelengths, making it difficult to detect. Additionally, the intense gravity of the black hole can also distort and bend light, making it difficult for us to see objects near the event horizon.

In summary, the extreme effects of gravity near a black hole, including time dilation and redshifting of light, make it impossible for us to see objects falling into the event horizon. Instead, we can only observe the effects of their presence on the surrounding environment.
 

FAQ: Objects falling into a black hole

1. What happens to an object when it falls into a black hole?

When an object falls into a black hole, it is pulled towards the singularity at the center of the black hole. As it gets closer to the singularity, the gravitational pull becomes stronger and the object is stretched and compressed, a process known as spaghettification. Eventually, the object will reach the event horizon and be pulled into the black hole, where it will be crushed into an infinitely small point.

2. Can anything escape from a black hole?

Once an object has crossed the event horizon of a black hole, it is impossible for it to escape. This is due to the immense gravitational pull of the black hole, which even light cannot escape from. However, there are some theoretical ways that particles and radiation can escape from a black hole, such as Hawking radiation.

3. How does the size of a black hole affect objects falling into it?

The size of a black hole, specifically the size of its event horizon, determines the distance from the singularity at which the gravitational pull is strong enough to trap objects. A larger black hole will have a larger event horizon, so objects can fall closer to the singularity before being pulled in. However, the strength of the gravitational pull at the event horizon is the same for all black holes, regardless of size.

4. Is there any way to survive falling into a black hole?

No, it is not possible for a human or any known object to survive falling into a black hole. The intense gravitational forces would destroy any physical object, and the laws of physics as we know them break down at the singularity. However, there are some theoretical ideas about white holes, which are the opposite of black holes, where objects may be able to survive falling into them.

5. Can black holes merge with each other?

Yes, black holes can merge with each other through a process called gravitational wave emission. As two black holes orbit each other, they emit gravitational waves which carry away energy. Eventually, the black holes will merge into one larger black hole. This process has been observed by scientists through the detection of gravitational waves.

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