Formation of jets with accretion disks at black holes

In summary: Mmmm, yes, after some reference searching I get the feeling that my hope of a sketch of the physical process "on the back of an enevelope" is a bit naive.I was hoping to get some feeling of why there are jets in the first place, and how its direction(s) roughly are determined.This may not be so easy - I don't think the phenomenon is completely understood.At first order, things are simple. If the source is surrounded by an orbiting disk, you get absorbtion in the disk-ward direction and thus transmission perpendicular to that. The problem is that jets seem to be narrower and more energetic than that simple model.I don't think
  • #1
haushofer
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Looking for resources on the formation of jets at black holes
Dear all,

I'm going to give a course about black holes at an astrophysics association. The public will consist mainly of lay persons, perhaps wit a little bit of physics background. My background in General Relativity is good, but my background in astrophysics at bit less. My question is if you know about some good online resources/lecture notes about the formation of jets (and accretion discs) around black holes, and the mechanisms behind those jets launching charged particles. Is there an intuitive/easy way to understand how those jets form in the first place? Many thanks.
 
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This may not be so easy - I don't think the phenomenon is completely understood.

At first order, things are simple. If the source is surrounded by an orbiting disk, you get absorbtion in the disk-ward direction and thus transmission perpendicular to that. The problem is that jets seem to be narrower and more energetic than that simple model.

I don't think there is any model that reproduces all the observed features. Shock seems to be involved, ant multi-component fluids (electrons do this, ions do that). Certainly magnetic fields by themselves won't do the trick.

Wasn;t there an Annual Review on jets a few years back?
 
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  • #3
I concur that your task is far from simple. The only postulated mechanisms that I am aware of for formation of relativistic jets are the Penrose process and the Blandford-Znajek mechanism.

The first is based on frame-dragging, the second on a magnetized accretion disk with rotational contortions of the field lines.
 
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  • #4
Hyperfine said:
I concur that your task is far from simple. The only postulated mechanisms that I am aware of for formation of relativistic jets are the Penrose process and the Blandford-Znajek mechanism.

The first is based on frame-dragging, the second on a magnetized accretion disk with rotational contortions of the field lines.
Mmmm, yes, after some reference searching I get the feeling that my hope of a sketch of the physical process "on the back of an enevelope" is a bit naive. I was hoping to get some feeling of why there are jets in the first place, and how its direction(s) roughly are determined.
 
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  • #5
Vanadium 50 said:
This may not be so easy - I don't think the phenomenon is completely understood.

At first order, things are simple. If the source is surrounded by an orbiting disk, you get absorbtion in the disk-ward direction and thus transmission perpendicular to that. The problem is that jets seem to be narrower and more energetic than that simple model.

I don't think there is any model that reproduces all the observed features. Shock seems to be involved, ant multi-component fluids (electrons do this, ions do that). Certainly magnetic fields by themselves won't do the trick.

Wasn;t there an Annual Review on jets a few years back?
You mean

https://www.annualreviews.org/doi/pdf/10.1146/annurev-astro-081817-051948
?
That's behind a paywall, unfortunately.
 
  • #6
haushofer said:
behind a paywall
Unless you need it now, that's what libraries are for,

But why not just giove them the first order explanation perhaps adding "reality is far more complicated and not entirely understood".
 
  • #9
Vanadium 50 said:
Unless you need it now, that's what libraries are for,

But why not just giove them the first order explanation perhaps adding "reality is far more complicated and not entirely understood".
Yeah, sure, it's mostly for my own understanding. I'm just a bit surprised that my intuition falls short here, so I guess I learned something new :P
 
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  • #11
Neutron stars also have relativistic jets. A black hole is not a requirement. One may easily find images of the jets from the neutron star in the Crab Nebula. We know it has a neutron star because it is a pulsar. A black hole cannot be a pulsar.

I know that there is as yet no completely satisfactory explanation of relativistic jets. That is, an entirely successful model has yet to be built.
 
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  • #12
Old habits die hard - likewise old models. People still say that nothing can get out of a black hole but Hawking changed that many years ago (1970s).
 
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FAQ: Formation of jets with accretion disks at black holes

What are accretion disks around black holes?

Accretion disks are structures formed by diffused material in orbital motion around a central massive object, such as a black hole. The material in the disk gradually spirals inward due to gravitational forces and friction, heating up and emitting electromagnetic radiation, often in the form of X-rays and visible light.

How are jets formed in the vicinity of black holes?

Jets are formed when material from the accretion disk gets channeled along the black hole's magnetic field lines, which are twisted by the black hole's rotation. This process accelerates particles to near-light speeds and ejects them along the poles of the black hole, away from the accretion disk.

What role do magnetic fields play in jet formation?

Magnetic fields are crucial in jet formation as they provide the mechanism for extracting rotational energy from the black hole and the accretion disk. The twisted magnetic field lines act as a conduit, accelerating particles and collimating the jets, directing them away from the black hole along its rotational axis.

Why do some black holes have jets while others do not?

Not all black holes have jets because jet formation depends on several factors, including the presence and structure of the magnetic field, the spin of the black hole, and the rate at which material is accreted. If these conditions are not met, jets may not form or may be weak and difficult to detect.

What is the significance of studying jets from black holes?

Studying jets from black holes is significant because it helps scientists understand high-energy astrophysical processes, the behavior of matter under extreme conditions, and the role of black holes in galaxy evolution. Jets also serve as natural laboratories for studying relativistic physics and magnetic field interactions.

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