Evidence of Rotating Black Holes?

Click For Summary

Discussion Overview

The discussion revolves around the evidence for rotating black holes, specifically focusing on the existence of spin in black holes and the implications of such spin on their properties and behavior. Participants explore theoretical frameworks, observational evidence, and speculative ideas related to black hole spin, including the effects of accretion disks and relativistic jets.

Discussion Character

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

Main Points Raised

  • Some participants question the direct evidence of black holes with spin, noting that while there are theoretical models, such as the Kerr black hole, these do not constitute proof of their existence.
  • Others propose that the Thirring-Lense effect could provide a method to evaluate a black hole's spin through the observation of thermal emission modulation from the inner accretion disk.
  • A few participants discuss the marginally stable orbit (MSO) in relation to rotating black holes, suggesting that the detection of X-rays and gamma rays around black hole candidates may imply high spin values.
  • There is mention of a theoretical upper limit of rotation for black holes, beyond which they could not possess an event horizon, although no such objects have been observed.
  • Speculative ideas are raised regarding exotic black hole types, such as the Kerr-Newman black hole and the concept of naked singularities, which are discussed in a more imaginative context.
  • Some participants explore the implications of large black holes on tidal forces and the potential for traversable wormholes, referencing theoretical work by Novikov.

Areas of Agreement / Disagreement

The discussion contains multiple competing views regarding the evidence and implications of black hole spin. Participants express uncertainty about the existence of direct evidence and the nature of theoretical constructs, indicating that the topic remains unresolved.

Contextual Notes

Participants reference various theoretical frameworks and observational claims, but there are limitations in the assumptions made about the nature of black holes and the interpretations of the data. The discussion also reflects a dependence on definitions and unresolved mathematical steps related to black hole physics.

cbd1
Messages
123
Reaction score
1
I would like to ask if there is any direct evidence of black holes with spin. I understand that there are formulas that would describe a black hole if it were to have spin, but this does not prove that they actually can. I also know there are accretion disks and relativistic jets around black holes. However, those only prove that matter revolves around black holes and that sometimes, if the conditions are right, matter and energy can be directed away from them in jets. In simpler terms, accretion disks and relativistic jets only decisively prove that there are accretion disks and relativistic jets. Is there any solid physical evidence of a black hole rotating?
 
Astronomy news on Phys.org
Black holes without spin curve spacetime, black holes with spin also distort it. This causes spacetime vibration which in turn causes thermal emission modulation (oscillations) from the inner part of the accretion disk, for more information see thirring-lense effect.
Observing these oscillations it's possible to evaluate black hole's spin (obviously this isn't a simple method).

If you are trying to connect relativistic jets and disk I have to quote Krolik (it's old but it's still pretty funny):
“In principle one could imagine that accretion onto a black hole occurs without any outflow at any point. Put another way, we don't know why jets exist.”
 
Spin is one of three theoretically possible variables for a black hole - mass, charge and angular momentum. Spin is the angular momentum component. One with spin is called a Kerr black hole, without spin it is called a Schwarzschild black hole.
 
cbd1 said:
I would like to ask if there is any direct evidence of black holes with spin.

According to the static solution (Schwarzschild metric) the marginally stable orbit (MSO) which normally also represents the inner edge of the accretion disk is at 6M, anything inside this radius quickly falls into the BH. For a rotating BH, due to frame dragging, there are two MSO, retrograde and prograde, the prograde MSO can reduce to simply M for an extremal BH where a/M=1. X-rays/gamma rays have been detected around BH candidates that hint at a MSO inside 6M, in some cases, close to where the event horizon would be, implying a very high spin (approx. a/M=0.98). Below are a couple of articles-

http://www.nytimes.com/2001/05/01/s...usive-spin-of-a-black-hole.html?pagewanted=1" NY Times

http://www.newscientist.com/article/dn10611-spinning-black-hole-is-fastest-on-record.html" New Scientist
 
Last edited by a moderator:
stevebd1 said:
According to the static solution (Schwarzschild metric) the marginally stable orbit (MSO) which normally also represents the inner edge of the accretion disk is at 6M, anything inside this radius quickly falls into the BH. For a rotating BH, due to frame dragging, there are two MSO, retrograde and prograde, the prograde MSO can reduce to simply M for an extremal BH where a/M=1. X-rays/gamma rays have been detected around BH candidates that hint at a MSO inside 6M, in some cases, close to where the event horizon would be, implying a very high spin (approx. a/M=0.98). Below are a couple of articles-

http://www.nytimes.com/2001/05/01/s...usive-spin-of-a-black-hole.html?pagewanted=1" NY Times

http://www.newscientist.com/article/dn10611-spinning-black-hole-is-fastest-on-record.html" New Scientist

That's what I love about Physics Forums! Learn something new every day!
 
Last edited by a moderator:
There is also a theoretical upper limit of rotation past which a Black Hole couldn't have an Event Horizon. No such object has been observed, but it's another limit on the system to consider.
 
Frame Dragger said:
There is also a theoretical upper limit of rotation past which a Black Hole couldn't have an Event Horizon. No such object has been observed, but it's another limit on the system to consider.

An extremal Kerr-Newman 'black hole'... quite an exotic beastie, if it could evolve naturally. A naked ring singularity would be quite a sight to see. Stephen Baxter imagines such in his Xeelee stories - the Xeelee create a vast spinning ring of cosmic-string to open up a ring singularity to escape the Photino birds' destruction of the stars.
 
qraal said:
An extremal Kerr-Newman 'black hole'... quite an exotic beastie, if it could evolve naturally. A naked ring singularity would be quite a sight to see. Stephen Baxter imagines such in his Xeelee stories - the Xeelee create a vast spinning ring of cosmic-string to open up a ring singularity to escape the Photino birds' destruction of the stars.

Hmmm, sounds like a book I need to read. A Kerr-Newmann BH that isn't 'Black. From my understanding it would be both inhaling matter, and blowing energy out of broad polar cones. Needless to say, a naked ring-singularity would be the ultimate aphrodesiac for sci-fi writers... other side of the galaxy here we come *sphagettification... pain*.
 
Frame Dragger said:
Hmmm, sounds like a book I need to read. A Kerr-Newmann BH that isn't 'Black. From my understanding it would be both inhaling matter, and blowing energy out of broad polar cones. Needless to say, a naked ring-singularity would be the ultimate aphrodesiac for sci-fi writers... other side of the galaxy here we come *sphagettification... pain*.

A large black hole or singularity has low tidal forces, thus 'spaghettification' is a minor hazard. We're talking an astrophysical object as large as a solar system or bigger, thus negligible tidal forces except right up close to the singularity itself. The Galactic Core black-holes are sufficiently large to be navigable too - the Milky Way's masses c. 4 million solar masses, thus has an event horizon 12 million km in radius. To go through it's Kerr-Newman wormhole you'd need to enter it via the poles and hope the dynamical tidal forces are forgiving.
 
  • #10
qraal said:
A large black hole or singularity has low tidal forces, thus 'spaghettification' is a minor hazard. We're talking an astrophysical object as large as a solar system or bigger, thus negligible tidal forces except right up close to the singularity itself. The Galactic Core black-holes are sufficiently large to be navigable too - the Milky Way's masses c. 4 million solar masses, thus has an event horizon 12 million km in radius. To go through it's Kerr-Newman wormhole you'd need to enter it via the poles and hope the dynamical tidal forces are forgiving.

Fair enough, but you're going to run into the singularity, not go through in all likliehood. Like an ERB, I think the whole mess wouldn't be traversable. It's fascinating to imagine however...
 
  • #11
Frame Dragger said:
Fair enough, but you're going to run into the singularity, not go through in all likliehood. Like an ERB, I think the whole mess wouldn't be traversable. It's fascinating to imagine however...

A polar trajectory takes you through the middle of the singularity ring, which is where the wormhole forms, thus you dodge the singularity - but that's for massless infalling trajectories. Any real object's gravity interacts with the singularity and causes dynamical tides... but it's hard to compute exactly how bad or for how long those tides occur. Novikov's own work on it suggests the wormhole is traversable, though where it exits is anyone's guess.
 
  • #12
qraal said:
A polar trajectory takes you through the middle of the singularity ring, which is where the wormhole forms, thus you dodge the singularity - but that's for massless infalling trajectories. Any real object's gravity interacts with the singularity and causes dynamical tides... but it's hard to compute exactly how bad or for how long those tides occur. Novikov's own work on it suggests the wormhole is traversable, though where it exits is anyone's guess.

Whichever physicist said that we'd find green slime and lost socks there is probably right. :wink:

Of course, Novikov also predicted that history would be consistent regardless of potential paradoxes arising from his traversable wormholes. An interesting notion, but it would seem to indicate that at some point history becomes deterministic once measured. I don't know about that.
 

Similar threads

  • · Replies 11 ·
Replies
11
Views
2K
  • · Replies 5 ·
Replies
5
Views
3K
  • · Replies 1 ·
Replies
1
Views
2K
  • · Replies 1 ·
Replies
1
Views
3K
  • · Replies 9 ·
Replies
9
Views
2K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 8 ·
Replies
8
Views
2K
  • · Replies 24 ·
Replies
24
Views
3K
  • · Replies 5 ·
Replies
5
Views
2K
  • · Replies 22 ·
Replies
22
Views
4K