Does Gravitational Lensing Cause Red Shift in Light?

Tanelorn
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Does light get red shifted during lensing, when it passes by an object with great mass such as a galaxy or cluster?

If so then what are the effects on measurements of the CMBR and most distant red shifted galaxies?

If true then presumably some light would be red shifted more than others resulting in frequency dispersion?
 
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Think about shining a laser horizontally along a road from point A to point B, one mile apart and each one foot off the ground. Now put a 2 foot diameter beach ball in the middle of the path and require that the light beam go from point A to a point just above the beach ball and then on to point B. I don't think the added length of the path would cause any significant red shifting.

I think the CMB measurements ignore any lensing, and since lensing really is only used to show the effects of GR, it's irrelevant to measurements of distant galaxies (assuming I'm right about the added red shift being insignificant).

All of this is just what I hope is an educated guess. I haven't done any math on this and if I'm off, I'm sure someone more knowledgeable will jump in and let us know.
 
What if the light bends around an object and significantly changes direction?
 
Tanelorn said:
What if the light bends around an object and significantly changes direction?
That might make very slightly more difference, but that is not what happens with galactic lensing.
 
Tanelorn said:
What if the light bends around an object and significantly changes direction?
Doesn't really matter. Lensing just changes the direction of light beams. It doesn't impact their wavelength. It does change light travel time and distance, which may have some impact on the redshift, but it's a very minor impact. I doubt it is measurable.
 
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Light gets blueshifted as it approaches a massive body then redshifted by the same amount as it departs. The net effect is zero - re: http://curious.astro.cornell.edu/ab...hen-it-is-gravitationally-lensed-intermediate. There is, however, a special case called the Sachs-Wolfe effect that occurs when photons pass through a massive extended body. Those photons are slightly less redshifted when they exit such a region.
 
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Chronos said:
Light gets blueshifted as it approaches a massive body then redshifted by the same amount as it departs. The net effect is zero - re: http://curious.astro.cornell.edu/ab...hen-it-is-gravitationally-lensed-intermediate. There is, however, a special case called the Sachs-Wolfe effect that occurs when photons pass through a massive extended body. Those photons are slightly less redshifted when they exit such a region.
Just to expand upon the Sachs-Wolfe effect, this occurs as a result of the gravitational potential well changing over the time the photon passes through it. Obviously this will only be a significant effect for extremely large systems, where the dominant cause of changing gravitational potential wells is dark energy, which causes the gravitational potential of large systems to decay slowly over time.
 
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