Accretion Discs in Non-Rotating Black Holes: A Closer Look at Sagittarius A*

In summary, an idealised non rotating black hole is unlikely to exist as they are formed from objects with angular momentum. While it is impossible to observe black holes, we are able to observe accretion disks outside of the event horizon. While accretion disks are common, there are also cases where no disk is present. In the case of Sagittarius A*, the supermassive black hole at the center of our galaxy, there is no prominent or permanent accretion disk. This was originally inferred from the orbiting of stars around the black hole.
  • #1
RoDnSuE
5
0
Does a non rotating BH have an accretion disc?
 
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  • #2
An idealised non rotating black hole would be an unlikely occurance, since black holes are formed from objects which do have angular momentum.
It's impossible to observe black holes, but it is possible to observe accretion disks which are outside of the event horizon.
Accretion disks seem commonplace, but there are also cases where no disk is apparent.
The black hole along with perturbation caused by other massive objects has probably resulted in all nearby matter falling into the hole and nothing significant remaining in the vacinity of the black hole.
 
  • #3

Related to Accretion Discs in Non-Rotating Black Holes: A Closer Look at Sagittarius A*

1. What is an accretion disc?

An accretion disc is a structure formed by swirling matter around a central object, such as a black hole or a young star. The matter in the disc is gradually pulled towards the center by gravity, causing it to spin faster and heat up due to friction.

2. How are accretion discs related to black holes?

Accretion discs are commonly observed around black holes. As matter falls towards the black hole, it forms an accretion disc around it. The intense gravitational pull of the black hole causes the matter in the disc to heat up and emit radiation, making it visible to telescopes.

3. Do all black holes have accretion discs?

Not all black holes have accretion discs. Smaller black holes, known as stellar-mass black holes, are more likely to have accretion discs compared to supermassive black holes that reside in the center of galaxies. However, even supermassive black holes can have accretion discs if they are actively feeding on surrounding matter.

4. Why do accretion discs form around black holes?

Accretion discs form around black holes because of the intense gravitational pull of the black hole. As matter falls towards the black hole, it gets caught in its gravitational field and begins to orbit around it. Over time, the matter in the disc loses angular momentum and falls towards the black hole, causing it to grow in size.

5. Can we observe accretion discs around black holes?

Yes, we can observe accretion discs around black holes using various telescopes and instruments. The radiation emitted from the accretion disc can be detected in different wavelengths, such as X-rays, infrared, and radio waves. By studying the properties of the radiation, we can learn more about the structure and behavior of the accretion disc and the black hole at its center.

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