This is what I don't understand.
Who cares what en external observer sees? The particle DIDN'T come from the black hole, therefore the black hole can't lose energy.
I know I'm wrong, 'cause Hawking is right, but HOW am I wrong![]()
Your question is a good one.
First of all, where does the Black Hole end? Its gravitational field extends to infinity. The external observer Cuddles mentioned is actually the asymptote, someone situated at infinity.
More importantly: the picture of a particle-antiparticle being created on the horizon is just a story. Actual calculations of Hawking radiation do not represent these pairs. The idea is often repeated because it is simple and we think that, once we get a full quantum description of the process, something similar will arise. But we lack a microscopic description. Our treatment of BH thermodynamics is only semiclassical at this point.
With more detail, to get particle creation you need quantum field theory. QFT is very well understood for flat spacetimes and we can handle it even for static curved spacetimes. With static I mean that the geometry is given and the processes we study do not change it (because they have too low an energy). Even static curved spacetimes are complicated. In them the concept of particle is not well defined, for example. But if we want to study things like BH evaporation, we will eventually reach a point were the quantum processes and the gravitational ones are both important, so we must handle dynamic curved spacetimes. We do not know how to do this.
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