@drskyskull I've been chatting to @robryk about coherence in starlight, and I'm stuck on something: up close, there's no phase coherence in starlight, but at a great enough distance it can be considered a point source, so multiple detectors on Earth can consider it in phase with itself (...says the internet...)
WHY? Even as a point source it's many photons with random phases, different ones hitting different detectors, surely?

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@_thegeoff @drskyskull

I think I figured it out in the meantime.

Assume a star is a collection of ideally monochromatic point sources. Then you can clearly see how they will interfere with each other at infinity in a particular direction. The net phase you observe there will be a function of phases of these sources, which avoids the "where does the timeshift asymmetry come from" problem. (Also, amusingly, the "you can't emit polarisationful wave in all directions" seems to still be the case, so there will be a line along which nothing gets emitted. If we allow the sources some bandwidth, this restriction disappears because it doesn't apply across different frequencies.)

Re "which photons we actually see": the question is ill-formed, because they interfere with each other.

@robryk @drskyskull Ah...you're saying the *resultant* light can be considered in phase, because the "non-average-phases" cancel and we're left with the average phase?
Analogy - particles in a gas cloud have random angular momentum, but by the time they collapse to a star only the average angular momentum is left?

@_thegeoff @drskyskull

Not exactly average phase, but something along these lines.

The reason I say along these lines instead of exactly that is quibbles around the difference between "there's literally no way to distinguish" and "our description considers these equivalent".

BTW. If the source is not monochromatic (as it never is), the notion of in phase becomes weird and complicated.

@_thegeoff @drskyskull

Yes, sum-up amplitudes and take argument of that. (And it might be brighter/dimmer in different directions. I haven't figured out what will happen if I e.g. take a bunch of sources with positions taken from a Gaussian and with polarisations picked uniformly from a sphere.)

The other thing I wanted to point out is that this is not the thermodynamic case, where the information on which particle went where is there, but unretrievable without investing lots of entropy. In this case the information about source of the particular photon you captured doesn't exist.

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