Given gravitational time dilation, under what conditions will a test particle cross an event horizon before the black hole evaporates? Assume zero background radiation.
closed as unclear what you're asking by Chris White, Brandon Enright, Dimensio1n0, akhmeteli, tpg2114 Nov 26 '13 at 4:56
Please clarify your specific problem or add additional details to highlight exactly what you need. As it's currently written, it’s hard to tell exactly what you're asking. See the How to Ask page for help clarifying this question.If this question can be reworded to fit the rules in the help center, please edit the question.
There is no way to answer this question, as it is mixing up a classical picture with quantum effects.
If you have a classical black hole and a particle falling into it, it will freeze on the horizon, considered from the exterior viewpoint, and when the black hole is evaporating, you might conclude that it evaporates before the particle has a chance to cross. This is a classically allowed picture, it is consistent. It is found by considering the black hole horizon to be a white hole horizon. The white hole horizon recedes from any infalling matter at the speed of light, so you can't fall in, but then all the matter that ever fell in is just compressed to the final endpoint of the white hole and it hits this endpoint at finite time. In this picture, anything coming out of the hole comes from a back region which is sensible.
But this black hole picture is not compatible with the formation point of the black hole. This formation point is just the time reverse of the annihilation point, and near this point, you must think of the black hole as a proper black hole. The two extensions are classically incoherent at different places, one near the end and one near the beginning, which is why modern people accept Hawking's identification of white hole and black hole as the same object. Susskind clarified this with black hole complementarity, which says that both the black hole and white hole extension are correct in different basis.
This shows that while it is consistent to say the particle can't cross before the black hole evaporates, and it is equally consistent to say a particle can't leave in finite time from the black hole's formation, both consistent pictures are foolish hobgoblins. The right picture allows either continuation in the domain where the black hole is static, so it's been around for a while, and will continue to be around.
At the event horizon, a test particle will appear to be moving at the speed of light, however due to time dilation to an external observer that particle will appear to have its time slowed to the point it's time is not advancing at all. At this point it will neither appear to travel faster than the speed of light, nor continue to advance in time.
Accordingly the external observer will observe the black-hole evaporate before the particle appears to cross.