To paraphrase a well known aphorism “All explanations are inaccurate, but some are useful”. And the picture of Hawking radiation as tunneling of one particle from the pair through the horizon while possibly “not entirely accurate” is certainly useful.
Note, that when Hawking suggested this tunneling picture it was indeed a “heuristic only” (and it remained such when his book was published), but since then a formalism was developed that put this explanation on a much firmer ground and linked it with a well known technique of quantum theory, the WKB approximation. So nowadays, this explanation not only helps with the intuition, but also produces quantitative predictions including Planck's spectrum of radiation (with the temperature coinciding with one obtained by QFT methods).
The original work establishing the mathematical formulation of tunneling for Hawking radiation is:
An essay explaining the main ideas, while omitting technical details:
And a review covering the first dozen years of further development of the tunneling methods:
Specific criticisms:
- The radiation arises not from the event horizon exclusively, but from the entirety of the curved space around it. (up to around 10–20 Schwarzschild radii)
It is possible to construct a static spacetime that fully coincides with the Schwarzschild metric outside event horizon for all $r>r_s+\epsilon$ for some small length $\epsilon$, yet does not have an event horizon. Such spacetime would not be emitting Hawking radiation.
On the other hand, we can imagine a black hole completely surrounded by a static screen impenetrable to radiation placed a small distance above the horizon. Inside this cavity a “thermal atmosphere” would emerge, consisting mostly of photons being emitted by horizon and falling back into it. If the walls of this cavity absorb some of the radiation and are thermally conductive then the black hole would be losing energy through vibrational degrees of freedom of the wall material. Theoretically it would be possible co construct a “heat sink” around the black hole that would remove energy from black hole much more efficiently than Hawking radiation in an empty space.
So the role of “entirety of the curved space” around the black hole is similar to the role of a lampshade around a lamp: it does affect radiation but as a passive element. The “active element” in the Hawking radiation is the horizon.
(Situation is more complicated for rotating black holes, where there are negative energy states strictly outside horizon. In this case tunneling overlaps with superradiance).
- There are no virtual particles (or antiparticles) with negative energy falling into the black hole. …
The flux of negative energy inside the black hole horizon is a real thing and could be obtained by a variety of methods. How this flux can be partitioned into particles is observer dependent, but once we chose consistent procedure there would be a particle stream falling toward singularity. Also note, that for a hypothetical observer inside the black hole horizon those particles would be perfectly ordinary photons, their “negative energy” would be apparent only in reference to how time flows outside the horizon.
… The curved space around the black hole is constantly emitting radiation due to the curvature gradient around it
The logic is backward. Curvature gradient is responsible for the black hole having an event horizon with nonzero surface gravity. Event horizon produces radiation.
- Black holes are not decaying because there’s an infalling virtual particle carrying negative energy... Instead, black holes are decaying, and losing mass over time, because the energy emitted by this Hawking radiation is slowly reducing the curvature of space in that region.
There is no “instead” here, energy conservation means that the flux of negative energy into the black hole equals up to the sign the flux of energy carried away by radiation and so we cannot have one without the other.
Overall remarks
It is good to have multiple ways to derive the same thing. This offers a way to check for consistency of other methods, some methods may be easier to use in some situations than the others and different methods might provide more insights for unsolved problems.
Here are some features of tunneling framework that might make it preferable to other (such as Bogoliubov transform) methods:
it incorporates gravitational backreaction from the start, so it might work better in situations where black hole quickly radiates away considerable fraction of its mass;
it is local in character, so just from the existence of this description we can conclude that the Hawking temperature of e.g. $\mathbb{RP}^3$ geon (a solution differing from Schwarzschild black hole by nontrivial topology of the interior) would be the same as Schwarzschild black hole;
calculating a tunneling rate might be possible even in spacetimes with pathologies posing difficulties for constructing QFT (such as spacetimes with closed timelike curves)…
So the tunneling framework for Hawking radiation has its place.