Why can't a static spacetime have an ergosphere?An ergoregion is

In summary, static spacetimes cannot have an ergosphere because they are invariant under time reversal, resulting in a null surface where the event horizon and ergosurface coincide. This is due to the Killing vector field being hypersurface orthogonal in static spacetimes, as shown by Carter and Vishveshwara's arguments. Additionally, the Penrose process can only produce negative energy in the ergoregion under specific conditions.
  • #1
latentcorpse
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Why can't a static spacetime have an ergosphere?

An ergoregion is just a region outside the event horizon where k can become negative (k being a Killing vector field that is timelike near infinity). Both stationary and static spacetimes have such a KVF so surely static spacetimes could also have regions where k can become spacelike.

I know that the answer is they can't - but I don't understand why? I'm assuming it has something to do with rotation of event horizon?
 
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  • #2


In a stationary spacetime you also have a Killing vector field ξ which is timelike near spatial infinity. So what is the exact difference between static and stationary?
 
  • #3


grey_earl said:
In a stationary spacetime you also have a Killing vector field ξ which is timelike near spatial infinity. So what is the exact difference between static and stationary?

static spacetimes are stationary spacetimes that are invariant under time reversal. but the killing vector field still exists in the static case! does that mean they do admit an ergoregion?
 
  • #4


Invariant under time reversal, I see. You then have to show that this implies your Killing vector field is irrotational, [tex] \xi_{[a} \nabla_b \xi_{c]} = 0 [/tex], i.e. that it is hypersurface orthogonal. (shouldn't be too hard, in fact I think it's a one-liner)

Then there are two classical articles by Carter "Killing Horizons and Orthogonally Transitive Groups in Space‐Time" and Vishveshwara "Generalization of the Schwarzschild Surface to Arbitrary Static and Stationary Metrics" showing this implies there cannot be an ergosurface. If you want to read them (they are quite technical), check if your university has access to the Journal of Mathematical Physics (where they we published), or drop me a private mail.

Basically, their argument shows that an ergosurface is a timelike surface where the Killing vector becomes null, but that in a static spacetime the length of the normal vector of a "would-be" ergosurface is proportional to the length of the Killing vector there, so this must be a null surface. Ergosurface and event horizon therefore coincide in a static spacetime, so there is no ergoregion between them.
 
  • #5


grey_earl said:
Invariant under time reversal, I see. You then have to show that this implies your Killing vector field is irrotational, [tex] \xi_{[a} \nabla_b \xi_{c]} = 0 [/tex], i.e. that it is hypersurface orthogonal. (shouldn't be too hard, in fact I think it's a one-liner)

Then there are two classical articles by Carter "Killing Horizons and Orthogonally Transitive Groups in Space‐Time" and Vishveshwara "Generalization of the Schwarzschild Surface to Arbitrary Static and Stationary Metrics" showing this implies there cannot be an ergosurface. If you want to read them (they are quite technical), check if your university has access to the Journal of Mathematical Physics (where they we published), or drop me a private mail.

Basically, their argument shows that an ergosurface is a timelike surface where the Killing vector becomes null, but that in a static spacetime the length of the normal vector of a "would-be" ergosurface is proportional to the length of the Killing vector there, so this must be a null surface. Ergosurface and event horizon therefore coincide in a static spacetime, so there is no ergoregion between them.

Thanks for your reply. Interesting!

I have a related question concerning the Penrose process. Consider equation (4.50) in these notes
http://arxiv.org/PS_cache/gr-qc/pdf/9707/9707012v1.pdf
He claims that it needn't be positive in the ergoregion since p is timelike or null and k is spacelike meaning -p.k can be negative.

But timelike times spacelike is negative e.g. consider (1,0,0,0) and (1,1,1,1) in the minkowski metric. they have scalar product -1 so -p.k would be positive again!

I see no way in which -p.k will ever be negative?

Cheers.
 
  • #6


And what do you think of (1,1/2,0,0) and (0,1,1,1) ?
 
  • #7


grey_earl said:
And what do you think of (1,1/2,0,0) and (0,1,1,1) ?

I see. The point being that it CAN be negative BUT won't always, right?
 
  • #8


Yes, exactly. You have to shoot in a particle at the right angle (namely, against the rotation, if I remember correctly) for this to work.
 

FAQ: Why can't a static spacetime have an ergosphere?An ergoregion is

Why can't a static spacetime have an ergosphere?

A static spacetime is defined as one in which the metric does not change with time. This means that there is no concept of rotation or angular momentum in a static spacetime, and therefore there cannot be an ergosphere. The ergosphere is a region of spacetime where the rotation of a black hole is strong enough to drag spacetime along with it, creating a region of spacetime that rotates with the black hole. Since a static spacetime has no concept of rotation, it cannot have an ergosphere.

What is an ergoregion?

An ergoregion is a region of spacetime surrounding a rotating black hole where the rotation is so strong that even light cannot escape from it. This region is created by the strong gravitational pull of the black hole, which warps spacetime and causes it to rotate along with the black hole. The ergoregion is often referred to as the "zone of no return" because once matter or light enters it, it cannot escape.

How is an ergoregion different from an event horizon?

An ergoregion and an event horizon are both regions of spacetime surrounding a black hole, but they serve different functions. The ergoregion is a region of extreme rotation where even light cannot escape, while the event horizon is the point of no return for anything that enters it. Once an object crosses the event horizon, it is pulled into the black hole and cannot escape. The ergoregion, on the other hand, allows matter and light to escape, but it is extremely difficult to do so due to the strong gravitational pull.

Can an ergoregion exist without a black hole?

No, an ergoregion can only exist in the presence of a black hole. The extreme rotation and strong gravitational pull of a black hole are necessary to create an ergoregion. In the absence of a black hole, there is no source of extreme rotation or strong gravitational pull to create an ergoregion.

What is the significance of the ergoregion in black hole physics?

The ergoregion plays a crucial role in understanding the behavior of black holes. It is the region where the effects of strong gravity and extreme rotation are most pronounced, and it is also the region where the black hole's spin energy can be extracted. The ergoregion is also important in the study of black holes' interaction with their surrounding environments, as it can influence the dynamics of matter and energy in the vicinity of the black hole.

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