Linguofreak
Well-known member
Radiation pressure from Hawking radiation, or "Do black holes ever actually form?"
When reading scientific literature on black holes, one generally hears the collapse process and the release of Hawking radiation discussed separately, though this article:
http://xxx.lanl.gov/abs/gr-qc/0304042
seems to indicate that Hawking radiation is actually driven by the collapse process itself, and that an object that does not collapse completely will radiate until it reaches its final radius (as seen by outside observers). But even the above article doesn't discuss the interaction of Hawking radiation and infalling matter beyond its relation to the production of Hawking radiation in the first place.
Near the horizon, without much gravitational redshift, or in the case of small black holes, Hawking radiation is extremely intense, according to one calculator I found, a 100 million metric ton hole would radiate 25 gigawatts from a surface area of 0.4 square femtometers, which is about a tenth the mass of Earth (times c^2) crossing every square meter of horizon area every second (of course, it has nowhere near a square meter of horizon area).
So can the radiation pressure from Hawking radiation prevent infalling matter from crossing the event horizon? Even if not, a black hole has a finite mass, and it seems to me that an infalling observer is likely to see that mass of Hawking radiation pass by them before they cross the horizon (in other words, they'll observe the hole to radiate itself away to nothing below them).
So would a black hole ever actually form? That is to say, would the interior part of the Schwarzschild geometry ever actually form, or would we just get an object that looks asymptotically like a black hole from the outside (collapsing to a radius asymptotically close to the Schwarzschild radius for the mass involved and radiating itself away in approximately the right timeframe), but with no actual event horizon or singularity?
When reading scientific literature on black holes, one generally hears the collapse process and the release of Hawking radiation discussed separately, though this article:
http://xxx.lanl.gov/abs/gr-qc/0304042
seems to indicate that Hawking radiation is actually driven by the collapse process itself, and that an object that does not collapse completely will radiate until it reaches its final radius (as seen by outside observers). But even the above article doesn't discuss the interaction of Hawking radiation and infalling matter beyond its relation to the production of Hawking radiation in the first place.
Near the horizon, without much gravitational redshift, or in the case of small black holes, Hawking radiation is extremely intense, according to one calculator I found, a 100 million metric ton hole would radiate 25 gigawatts from a surface area of 0.4 square femtometers, which is about a tenth the mass of Earth (times c^2) crossing every square meter of horizon area every second (of course, it has nowhere near a square meter of horizon area).
So can the radiation pressure from Hawking radiation prevent infalling matter from crossing the event horizon? Even if not, a black hole has a finite mass, and it seems to me that an infalling observer is likely to see that mass of Hawking radiation pass by them before they cross the horizon (in other words, they'll observe the hole to radiate itself away to nothing below them).
So would a black hole ever actually form? That is to say, would the interior part of the Schwarzschild geometry ever actually form, or would we just get an object that looks asymptotically like a black hole from the outside (collapsing to a radius asymptotically close to the Schwarzschild radius for the mass involved and radiating itself away in approximately the right timeframe), but with no actual event horizon or singularity?