Gravitational non linearity: the glue of Black Holes

In summary, the conversation discusses the effects of gravitational non-linearity (GNL) on the formation and stability of black holes. It is noted that at low levels of spacetime curvature, gravity is weak, but at the formation of a black hole, GNL becomes the dominant force. This is compared to the formation of the great red spot on Jupiter, which also relies on non-linearities to hold itself together. It is also mentioned that the current causal event horizon of a black hole can be affected by future growth, which is also explained by GNL.
  • #1
Naty1
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Any comments on the following description from Kip Thorne, BLACK HOLES AND TIME WARPS, 1994, Box 10.1 would be appreciated. It seems odd to me that at some given curvature, gravity would become self sustaining...if that is what he is saying.

...When spacetime curvature is weak [as in the solar system]... [gravity] is weak...Einsteins general relativistic laws predict the curvature ...of BH and at the Big Bang.. should be among the most non linear phenomena in the Universe...as yet we possesses almost no experimental or observational data to show us the effects of gravitational non linearity [GNL] and we are so inept at solving Einsteins equation that our solutions have taught us about the non linearity only in simple situations...for example around a quiescent spinning BH.

A quiescent BH owes its existence to gravitational non linearity [GNL]; without the GNL the hole could not hold itself together just as without gaseous non linearities the great red spot on the plant Jupiter could not hold itself together. When the imploding star that creates a BH disappears through the hole's horizon the star loses it ability to influence the hole in any way; most important, the star's gravity can no longer hold the hole together. The hole then continues to exist solely because of GNL without the aid of the star and the self generated curvature acts as a nonlinear glue to bind itself together.

We have previously discussed in these forums that the current causal event horizon is affected by any future growth of the black hole... and the causal event horizon grows in anticipation or a BH merger or in-falling mass-energy. Can those effects be reconciled with the above description or do you think Thorne's 'quiescent' discussion is too simple to account for any accretion?? [that's my take]
 
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  • #2
Naty1 said:
It seems odd to me that at some given curvature, gravity would become self sustaining...if that is what he is saying.

It is. But note that it's not "at some given curvature", because the curvature at the hole's horizon varies inversely with its mass. For a large enough hole, curvature at the horizon is negligible, so the formation of a horizon, which I think is basically what Thorne means by "the hole holding itself together", can't be a function of curvature.

Naty1 said:
We have previously discussed in these forums that the current causal event horizon is affected by any future growth of the black hole... and the causal event horizon grows in anticipation or a BH merger or in-falling mass-energy. Can those effects be reconciled with the above description

Sure. Any time additional matter falls into the hole, it works similarly to the collapse of the matter that intially formed the hole. Once the matter falls through the horizon, it can't hold the hole together at its new, larger mass. So the hole holding together at its new, larger mass must be due to GNL, just as the hole holding together at its original, smaller mass was. It's the same thing.
 

1. What is gravitational non-linearity?

Gravitational non-linearity refers to the phenomenon in which the gravitational force between objects is not directly proportional to their masses or distances. This is a key concept in understanding the behavior of black holes.

2. How does gravitational non-linearity affect black holes?

In black holes, the intense gravitational pull causes the fabric of spacetime to become highly curved and distorted, resulting in non-linear gravitational effects. This is what gives black holes their unique properties, such as the event horizon and singularity.

3. What is the "glue" of black holes?

The "glue" of black holes refers to the strong gravitational force that holds the singularity at the center of a black hole together. This force is a result of the extreme non-linearity of gravity within a black hole.

4. How does gravitational non-linearity impact our understanding of the universe?

Gravitational non-linearity is a crucial aspect of general relativity, the theory of gravity that has been successful in explaining many astronomical phenomena. It allows us to understand the behavior of massive objects like black holes and their effects on the surrounding space.

5. Is there any evidence for gravitational non-linearity in the real world?

Yes, there is strong evidence for gravitational non-linearity in the form of gravitational lensing, which is the bending of light around massive objects due to their gravitational pull. This effect has been observed and studied extensively by scientists and provides strong support for the theory of general relativity.

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