Consider a „Rindler observer“ hovering close to the event horizon of a black hole, whereby flat spacetime is assumed locally.
Does this observer see the same Unruh radiation like a Rindler observer accelerating with the same proper acceleration in flat Minkowski spacetime?
What follows from the fact that these two scenarios differ due to the locality condition?
Does it make sense - and if yes why - to distinguish between Unruh- and Hawking-radiation regarding the radiation our hovering observer sees?