How Do Black Holes Emit Radio Waves if They Only Suck Things In?

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Discussion Overview

The discussion revolves around the mechanisms by which black holes emit radio waves and other forms of radiation, despite their nature as objects that supposedly only absorb matter. Participants explore concepts related to event horizons, accretion disks, and the nature of black holes, raising questions about their formation and behavior.

Discussion Character

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

Main Points Raised

  • Some participants note that while black holes have event horizons where matter cannot escape, they can emit radiation due to the heating of material in the accretion disk surrounding them.
  • There is a suggestion that black holes grow larger as they consume matter, leading to questions about the nature of this matter and whether it is truly annihilated.
  • Participants discuss the concept of gravity in relation to black holes, with some describing it as "gravity gone wild" and others referencing different types of degenerate stars.
  • One participant emphasizes that black holes do not "spit stuff out," but rather emit radiation due to the intense gravitational forces acting on nearby material.
  • Questions arise regarding the behavior of photons near the event horizon, including whether they can escape if not emitted perpendicularly.
  • There is a discussion about the definition of the event horizon and how it relates to the trajectories of photons, with some participants expressing confusion over the concept.

Areas of Agreement / Disagreement

Participants express a range of views on the nature of black holes and their emissions, with no clear consensus reached. Some agree on the role of accretion disks in radiation emission, while others question the implications of matter being absorbed by black holes.

Contextual Notes

Participants highlight the complexity of black hole physics, including the unresolved nature of certain phenomena like Hawking radiation and the behavior of light near the event horizon. Discussions also touch on the definitions and assumptions surrounding black holes and their properties.

Who May Find This Useful

This discussion may be of interest to those exploring astrophysics, particularly concepts related to black holes, radiation, and gravitational effects in extreme environments.

Siadeug
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From my limited understanding, black holes supposedly have "event horizons" where everything near them just falls inside the black hole and becomes nothingness, totally anhilated. If this is the case then how is it that black holes emit stuff, like radio waves? If they suck things in and then spit things back out, isn't that the opposite of what a black hole is really supposed to do? I would really like to gain a better understanding of black holes. Thank you!
 
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Anything that crosses the event horizon of a black hole is gone for good.
However all the material that is attracted to a black hole can't immediately fall in. Because of conservation of angular momentum it forms a disk around the black hole at large a distance from the event horizon. It is the heating of the material in the disk from the attraction of the black hole and the acceleration of new material arriving that creates the x-rays and radio waves

But yes it is a little odd that 'black' holes are the among the brightest sources of energy in the sky!
 
Well that makes sense.. I have some more newbie questions. I've read that black holes grow larger as they consume more things. Doesn't that mean that the matter is not getting anhilated? Is a black hole actually made of some sort of matter then? I don't see how "nothingness" can really grow. And, of course, a most basic question: why does a black hole even happen? I understand that the gravity of a black hole is very strong and that it's basically an imploded star but why do black holes form when stars die?
 
Siadeug said:
Well that makes sense.. I have some more newbie questions. I've read that black holes grow larger as they consume more things. Doesn't that mean that the matter is not getting anhilated?
The matter degenerates to a form that we don't yet understand. But it is still there. As is its mass.

Siadeug said:
And, of course, a most basic question: why does a black hole even happen? I understand that the gravity of a black hole is very strong and that it's basically an imploded star but why do black holes form when stars die?
It is quite simply gravity gone wild.

There are various lesser forms of degenerate stars: white dwarf, neutron star.

A neutron star is gravity gone almost wild. There is just enough gravity to crush the matter of the star to the point where the electron and protons combine into neutrons and the neutrons get packed almost edge-to-edge.
 
First, black holes don't 'spit stuff out". They only emit waves (radio,infared etc.) The reson they do that is because of their intense gravity. I suggest that you google black holes and see what you find out about them.
 
Ultrastar 1 said:
First, black holes don't 'spit stuff out". They only emit waves (radio,infared etc.) The reson they do that is because of their intense gravity. I suggest that you google black holes and see what you find out about them.

Be cautious with the word emit. Most people define the object "a black hole" to be everything contained within the event horizon, and this region certainly doesn't emit anything. The only candidate would be the proposed Hawking radiation that happens at the event horizon. The common x-ray emissions are, like mgb says, created by accreting gas, which really doesn't have anything to do with the black hole itself. The same happens any compact object accreting gas, say, a neutron star.
 
As others have already mentioned, the black hole itself doesn't emit anything (except perhaps hawking radiation).

The radio jets and x-ray/gamma ray emissions are due to infall of material from nearby stars and clusters of stars as it forms a massive accretion disk of gas around the black hole. This matter, as it slowly gets pulled in by gravity is obviously increasing in temperature due to the acting gravitational force from the black hole. In turn, the increase in energy of these atoms and subatomic particles results in the emission of high energy radiation. Radio jets are also formed from similar reactions but that radiation "travels" along the magnetic poles of the BH (hence the jet).
 
i am venturing a guess that anything that radiates from the surface of the event horizon must do so perfectly perpendicular to the surface? at the speed of light? (the escape velocity AT the event horizon is the speed of light, yes?) what would happen if the radiated wave or particle had a velocity that was not perpendicular? would it "fall" back in?

also, this might be another topic, but since when is gravity so "intense"? it's the weakest of the four (or three) forces; would it ever be possible to have a large gathering of, let's say, electrons, all negatively charged, so collectively together as if in a black hole?
 
Unit said:
i am venturing a guess that anything that radiates from the surface of the event horizon must do so perfectly perpendicular to the surface? at the speed of light? (the escape velocity AT the event horizon is the speed of light, yes?) what would happen if the radiated wave or particle had a velocity that was not perpendicular? would it "fall" back in?
You're looking at it backwards. The radius within which light cannot escape defines the event horizon.

If some photons are on a trajectory [say, that is not directly away from the centre of the BH] and they fall back in, then the EH is above that. If, OTOH, there are photons that are able to escape, that the EH is below that.

So, the question is: looking at a given photon, did it escape or did it fall back in?
 
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  • #10
to be honest i don't quite understand how I'm seeing it backwards, but maybe it's because I'm tired and sleepy. either way, i hope I'm not being redundant in asking this:

i imagine the event horizon to be a sphere, a very large sphere, without a tangible surface of course. let's say it is 10 km from the centre of the black hole. if a photon, whose velocity is radially outward away from the centre of the black hole, is placed just outside the edge of this event horizon (let's say, 10.00001 km from the centre of the black hole), will it escape? what would happen if the photon's velocity was NOT perpendicular to the "surface" of the event horizon sphere, and instead had an angle of 80 degrees to it. that would mean that the vertical, "escaping" component would be 0.98c. would it escape then?

also,
The radius beyond which light cannot escape defines the event horizon.
By this, I assume you mean the radius within which, yes?
 
  • #11
Unit said:
also, By this, I assume you mean the radius within which, yes?
Why, whatever are you talking about? :biggrin:
 
  • #12
Unit said:
to be honest i don't quite understand how I'm seeing it backwards, but maybe it's because I'm tired and sleepy.
Because you're defining the EH first, then asking what the photons will do second.
You can only define the EH by determining what the photons did.

Unit said:
either way, i hope I'm not being redundant in asking this:

i imagine the event horizon to be a sphere, a very large sphere, without a tangible surface of course. let's say it is 10 km from the centre of the black hole. if a photon, whose velocity is radially outward away from the centre of the black hole, is placed just outside the edge of this event horizon (let's say, 10.00001 km from the centre of the black hole), will it escape? what would happen if the photon's velocity was NOT perpendicular to the "surface" of the event horizon sphere, and instead had an angle of 80 degrees to it. that would mean that the vertical, "escaping" component would be 0.98c. would it escape then?

also, By this, I assume you mean the radius within which, yes?
Observe your photon. Did it escape? Then the EH is defined as below that point. If it didn't, escape, the EH is defined as above that point.


Imagine the black hole is not symmetrical, even for a moment, say while it's absorbing an extra helping of matter (this may or may not be realistic, let's just pretend). The point is, the EH is not mathematically defined as a radius or any other predetermined shape or formula. At this or that point, photons may or may not escape. The EH depends on whether photons escaped or not.
 
  • #13
DaveC426913 said:
The point is, the EH is not mathematically defined as a radius or any other predetermined shape or formula. At this or that point, photons may or may not escape. The EH depends on whether photons escaped or not.

isn't the Schwarzschild radius defined as r_s = \frac{2GM}{c^2}? i think I'm wrong, though, because of general relativity and the way how spacetime bends in the presence of gravity. the radius cannot be thought of like a pretty little sphere in plain, 3d cartesian coordinates. plus, what if the black hole is spinning? then it gets messier.

i totally understand your explanation though, thanks a bundle
 

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