Jarek Duda
Registered Senior Member
T/CPT symmetric analog of black hole in Kruskal–Szekeres coordinates is white hole, which only allows photons to cross horizon outside, hence pushing objects around with EM - act with positive radiation pressure p=<ExH>/c vectors outside, absorption equation increasing the number of excited atoms (N2).
If so, shouldn't black hole symmetrically act with negative radiation pressure - pull objects around with EM by p=<ExH>/c radiation pressure vectors pointing inside, act with stimulated emission equation decreasing the number of excited atoms (N2)?
Such looking necessary effect of black hole could be slightly easier to observe than Hawking radiation, maybe even look below the horizon - would need e.g. telescope with excited sensor, monitoring its population - testing if it doesn't deexcite faster than usual by stimulated emission e.g. from black hole.

If so, shouldn't black hole symmetrically act with negative radiation pressure - pull objects around with EM by p=<ExH>/c radiation pressure vectors pointing inside, act with stimulated emission equation decreasing the number of excited atoms (N2)?
Such looking necessary effect of black hole could be slightly easier to observe than Hawking radiation, maybe even look below the horizon - would need e.g. telescope with excited sensor, monitoring its population - testing if it doesn't deexcite faster than usual by stimulated emission e.g. from black hole.

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