Q-reeus
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Unless diffuse scattering is significant (hugely unlikely imo), what matters is the relative size of that diameter - i.e. beam angle remains small. [Whoops: on second thoughts, all that matters is the probability of absorption - and photons in a spherical pulse has essentially the same chance of survival as for those in a narrow laser beam]skippy1729 said:Even a high quality laser (small divergence) will spread to an enormous diameter at cosmological distances.
Why would you conclude non-absorption would be minute in deep space directions, rather than the other way around? Astonomers have no trouble seeing in sharp detail (limited only by instrument resolution) distant galaxies back to 13 odd billion years ago. And that from times when dust and gas was far more concentrated than now or especially into the distant future.Still, averaging over this area which might contain spots of no absorption which might show minute power discrepancies versus the complete absorption of the sun.
Making the reasonable assumption that absorption this side of horizon crossing is statistically unlikely, in #17 was provided a modified version of OP's experimental test in #1 that is rediculously easy to implement. One that should give an easily observable positive if that 2nd conjecture: "Emission probabilities in the directions of absorbers increase to compensate for the dark spots." is correct. Even moderately powered laser pointers are now illegal to own where I live, but having kept an old, low power one, I can confirm there is zero visual evidence for the above conjecture, based on the 'test' of #17. But let's have feedback from various 'labs' - like independent corroboration to confirm things.Absent such experimental evidence...
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