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Regarding Laura and Harald's paper:
DR. Vidotto: Hi Tashja, ours was a "friendly citation" as we both think that there is no singularity at the center of a collapsing region, but then opinions and results diverges...
Paddoboy, Tashja: If Black holes don't form according to Mersini & Pfeiffer's recent paper, then... What are these unseen companions we see in apparent binary systems? Or the polar jets we see emanating from around apparent BH's? What do we put down these other observations to, that give results for objects with an apparent escape velocity at or exceeding "c." What do you think the dark, massive compact object (Sag A*) at the core of the Milky Way is?
Dr. Vidotto: I totally agree with you. Yes, we observe things that behave exactly as black holes, soon we will also be able to directly observe the event horizon with the new Event Horizon Telescope... so yes, I think that a theory of non-singular black hole should be compatible with such observation.
In the case of our work on Planck Stars, the singularity at the center of the black hole is removed by quantum effects, and a collapsing shell would bounce back approximately when it reaches a size comparable with the Schwarzschild radius (this calculation is the Fireworks' paper by Rovelli and Haggard). But the key point is that, even if such a bounce for a "bouncing observer" would last a millisecond, for a far-away observer it would take about a time comparable with the age of the universe. So everything goes for us as if there are standard black holes, and observation are not contradicted.
RJBeery: Do you agree that QM, as a theory, forbids black holes?
Dr. Vidotto: QM should forbids curvature singularity to form. Also, adding quantum effects convert event horizons into trapping surfaces, i.e. horizons that do not last forever. This is what Hawking also meant, when it was reported that BH do not exists: the asymptotic definition of a BH do not holds, BH are object with a limited life. THis was true because Hawking's evaporation cause their death, and it is even more true if internal quantum effects are turned on.
What Mersini & Pfeiffer is a different story. They notice that, during a collapse, there is already Hawking evaporation, and this was known. They says that the backreaction of this radiation is so strong to prevent the Schwarzschild horizon to form. I think this should be better understood. It could very well be that this backreaction was previously underestimated, but it think it is more likely that there is a flaw in the calculation they are doing. For instance the way they plug the Hawking energy density into the Friedmann equation for the interior of a star that is a non-vacuum and non-static spacetime, looks pretty suspicious...
RJBeery: And would you agree that QM is incomplete or even wrong if black holes do "exist"?
Dr. Vidotto: No, not at all, see above.
You're welcome! Cheers,
Francesca
Dr. Francesca Vidotto
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Institute for Mathematics, Astrophysics and Particle Physics
Radboud University Nijmegen - The Netherlands"
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