Planck star

Short description: Hypothetical astronomical object

In loop quantum gravity theory, a Planck star is a hypothetical astronomical object, theorized as a compact, exotic star, that exists within a black hole's event horizon, created when the energy density of a collapsing star reaches the Planck energy density. Under these conditions, assuming gravity and spacetime are quantized, a repulsive "force" arises from Heisenberg's uncertainty principle. The accumulation of mass–energy inside the Planck star cannot collapse beyond this limit because it violates the uncertainty principle for spacetime itself.[1]

The key feature of this theoretical object is that this repulsion arises from the energy density, not the Planck length, and starts taking effect far earlier than might be expected. This repulsive "force" is strong enough to stop the star's collapse well before a singularity is formed and, indeed, well before the Planck scale for distance: for a stellar mass black hole the Planck star would be of the order of 10−12 m \- for a primordial black hole, the order of 10−16 m.[2] whilst tiny, these scales are many orders of magnitude larger than the Planck length of 10−35 m. Then too, this allows adequate room for all the information captured inside a black hole to be encoded in the star, thus avoiding information loss.[1]

While it might be expected that such a repulsion would act very quickly to reverse the collapse of a star, it turns out that the relativistic effects of the extreme gravity of such an object slow down time for the Planck star to a similarly extreme degree. Seen from outside the star's Schwarzschild radius, the rebound from a Planck star takes approximately fourteen billion years, such that even primordial black holes are only now starting to rebound from an outside perspective. Furthermore, the emission of Hawking radiation can be calculated to correspond to the timescale of gravitational effects on time,[clarification needed] such that the event horizon that "forms" a black hole evaporates as the rebound proceeds.[1]

Carlo Rovelli and Francesca Vidotto, who first proposed the existence of Planck stars, theorized in 2014 that Planck stars form inside black holes[3] as a solution to the black hole firewall and the black hole information paradox. Confirmation of emissions from rebounding black holes could provide evidence for loop quantum gravity. Recent work demonstrates that Planck stars may exist inside black holes as part of a cycle between black and white holes.[clarification needed][4]

A somewhat analogous object theorized under string theory is the fuzzball, which similarly eliminates the singularity within a black hole and accounts for a way to preserve the quantum information that falls into a black hole's event horizon.

## See also

* List of nearest black holes
* Supermassive black hole
* Intermediate-mass black hole
* Stellar black hole
* Micro black hole
* Neutron star

## References

1. ↑ 1.0 1.1 1.2 "New Type of Star Emerges From Inside Black Holes". Physics arXiv Blog. 5 February 2014. https://medium.com/the-physics-arxiv-blog/6cf7ec0ed28b.
2. ↑ Carlo Rovelli & Francesca Vidotto (8 February 2014). "Planck stars". Physics 23 (12). doi:10.1142/S0218271814420267. Bibcode: 2014IJMPD..2342026R.
3. ↑ Rovelli, Carlo; Vidotto, Francesca (2014). "Planck stars". International Journal of Modern Physics D 23 (12): 1442026. doi:10.1142/S0218271814420267. Bibcode: 2014IJMPD..2342026R.
4. ↑ Carlo Rovelli (10 December 2018). "Viewpoint: Black Hole Evolution Traced Out with Loop Quantum Gravity". Physics 11. https://physics.aps.org/articles/v11/127. Retrieved 11 December 2018.

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Black holes

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