Formation of gravastars

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SUMMARY

The discussion centers on the dynamical formation of gravastars, horizonless black hole mimickers, as demonstrated in a recent paper by Luciano Rezzolla et al. The study shows that gravastars can form from the collapse of a uniform dust sphere via nucleation and expansion of a de Sitter region at the center, without invoking higher-curvature corrections. A critical compactness threshold of 𝒞 = 3/8 is identified, above which black hole formation is inevitable. The formation mechanism involves integrating backwards from a final static equilibrium state, but the exact physical origin of the de Sitter region during collapse remains unclear and is referenced to prior works on bouncing gravitational collapse. The discussion also references previous research by Rezzolla on gravastar ringdown signals, concluding that thick gravastars cannot model observed gravitational wave ringdowns such as GW150914.

PREREQUISITES

  • General Relativity and Schwarzschild solution
  • Oppenheimer-Snyder gravitational collapse model
  • de Sitter spacetime and vacuum energy concepts
  • Gravitational wave ringdown analysis and light ring phenomenology

NEXT STEPS

  • Study the papers on bouncing gravitational collapse (arXiv:2009.12057, arXiv:2301.01309, arXiv:2309.14912, arXiv:2412.02742) for detailed mechanisms of de Sitter region nucleation
  • Analyze the gravitational wave ringdown signatures of gravastars versus black holes, focusing on Rezzolla’s 2016 paper (arXiv:1602.08759)
  • Explore numerical relativity simulations of horizonless compact objects formation
  • Review the role of compactness thresholds in gravitational collapse outcomes

USEFUL FOR

The discussion benefits theoretical physicists, astrophysicists, and gravitational wave researchers investigating alternatives to classical black holes, specifically those studying gravastar models, gravitational collapse dynamics, and exotic compact objects in general relativity.

Sagittarius A-Star
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TL;DR
Big Bang inside a Star: How a Gravastar forms
The following paper was just published:
Abstract
Regular black holes and horizonless black hole mimickers offer mathematically consistent alternatives to address the challenges posed by standard black holes. However, the formation mechanism of these alternative objects is still largely unclear and constitutes a significant open problem since understanding their dynamical formation represents a first step to assess their existence. We here investigate, for the first time and without invoking higher-curvature corrections, the dynamical formation of a well-known horizonless black hole mimicker, namely, a gravastar. More specifically, starting from the collapse of a uniform dust sphere, as in the case of the Oppenheimer-Snyder collapse, we demonstrate that, under fine-tuned conditions, a gravastar can form from the nucleation and expansion of a de Sitter region with initial zero size at the center of the collapsing sphere. Furthermore, the de Sitter expansion naturally slows down near the Schwarzschild radius, where it meets the collapsing dust surface and gives rise to a static equilibrium. Interestingly, we also find a maximum initial compactness of the collapsing star of 𝒞 =3/8, above which the collapse to a black hole is inevitable.
Source:
https://journals.aps.org/prd/abstract/10.1103/c6lw-nx7k

preprint archive:
https://arxiv.org/abs/2509.15302

via:
https://www.uni-frankfurt.de/en/new...nern-eines-sterns-wie-ein-gravastern-entsteht
 
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From one of the authors of the paper:

Video: Seminar entitled "Three exotic (but not crazy) ideas in classical gravity", given by Luciano Rezzolla (Goethe University Frankfurt, Germany), September 24th, 2025, during the VII Amazonian Symposium on Physics:

 
I'm not quite sure where the de Sitter region comes from. The FLRW region is the star itself, but they just seem to add the de Sitter region by hand. They argue that it's plausible by integrating backwards from their final state and showing that the de Sitter region goes to a zero size volume, but I'm not clear on the causation before that event. Perhaps I missed something.
 
Ibix said:
they just seem to add the de Sitter region by hand. ... Perhaps I missed something.
The paper does not describe, how a dark energy vacuum region is created by the collapse. They refer to other papers:

In our case, since we eventually want to obtain a static gravastar, we need to add an expanding de Sitter region inside the collapsing FLRW spacetime, noting that the appearance of a de Sitter solution represents a common feature of most “bouncing” solutions in gravitational collapse (see, e.g., [11–13, 15]).

sources 11 to 13:
https://arxiv.org/abs/2009.12057
https://arxiv.org/abs/2301.01309
https://arxiv.org/abs/2309.14912

source 15:
https://arxiv.org/abs/2412.02742
 
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Hey, Luciano Rezzola is one of my favorite GR researchers! I’ll want to take a close look at these.
 
berkeman said:
Wow, yeah. I was about to it call it bunk but if you people think there's something there I guess I'll have to take it seriously. Weird indeed!
 
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  • #10
PAllen said:
Hey, Luciano Rezzola is one of my favorite GR researchers! I’ll want to take a close look at these.

I found an older paper from him:
we conclude it is not possible to model the measured ringdown of GW150914 as due to a rotating gravastar.
...
We conclude with two final remarks. First, there is no contradiction between our results and those of Ref. [32] as our conclusions refer to gravastars that are thick and have a surface at a small but not infinitesimal distance from the putative event horizon.
Source:
https://arxiv.org/abs/1602.08759

The reference [32] is:
In other words, universal ringdown waveforms indicate the presence of light rings, rather than of horizons.
Source:
https://journals.aps.org/prl/abstract/10.1103/PhysRevLett.116.171101
 
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