Are superconductors perfect reflectors?

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    optics superconductors
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SUMMARY

Superconductors are not perfect reflectors, but they exhibit better reflective properties than non-superconducting materials. The reflection mechanism involves charge redistributions that generate electromagnetic waves, but superconductors experience exponential damping of electromagnetic radiation, characterized by the skin depth or London penetration depth. While superconductivity enhances reflection compared to metals, it does not significantly alter optical properties at room temperature. The discussion highlights the need for clarity on surface resistivity and its implications for energy dissipation in superconductors.

PREREQUISITES
  • Understanding of electromagnetic wave behavior
  • Familiarity with superconductivity principles
  • Knowledge of skin depth and London penetration depth
  • Basic grasp of surface resistivity concepts
NEXT STEPS
  • Research the relationship between surface resistivity and electromagnetic wave absorption
  • Explore the effects of temperature on superconductivity and reflection
  • Study the mathematical models for skin depth in superconductors
  • Investigate the optical properties of superconductors versus metals
USEFUL FOR

Students, physicists, and engineers interested in superconductivity, electromagnetic theory, and materials science will benefit from this discussion.

Tazerfish
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To my current(somewhat pathetic:wink:) knowledge the reflection off metal surfaces happens because
the changing electric and magnetic fields cause "mini currents" or charge redistributions
which produce their own electromagnetic waves identical to the incoming ones or in other words the reflection.

My guess is that resistance and the fact that metals really aren't a continuous sea of charge (but more like a few electrons moving fairly freely in a crystal lattice) make the reflective abilities of metals less than perfect.

But how close do you get with a superconductor?
Maybe it was just the condensation due to the cold temperatures or a little oxidant layer or protective coating but i can't remember superconductors being particularly bright or shiny.:confused:
And if there is no fundimental misconception about that model of reflection then i would be interested to know where it breaks down.
The thought that very high gamma ray photons should be reflected off a superconductor is absurd.
So why doesn't it happen ?
 
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Electromagnetic radiation does penetrate a superconductor, but is damped exponentially. The distance over which energy is lost is called the skin depth (london penetration depth). So no, they would not be perfect reflectors.

See https://cas.web.cern.ch/cas/ZEUTHEN/Zeuthen-talks/170903/Schmueser-sc_cav.pdf
 
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Thanks for the answer.
I am just a 11 grade student in germany (i would be in high school in america) so i didn't understand very much of that pdf...
Consequently my question isn't completely resolved.
I changed my question a little:
Superconductors aren't perfect reflectors, but they are the better reflectors than any non-superconducting surface.
Is the statement correct now ?

In the paper you linked a formula for surface resistivity is derived from page 16 to 18.
What does that formula imply ?
Is the absorbed power per reflection proportional to the surface resistivity ?
And if the resistance of the copper pairs does not arise from interactions with the crystal lattice then where does the dissipated energy go.
And is the formula only valid in the microwave regime or does the surface resistivity keep rising to the second power of the frequency ?

Additionaly i assume that the superconductivity has little to no influence on the reflective "abilities" in the optical spectrum.
When cooling down high temperature superconductors they don't start to look different when they pass their transition temperature.
Why is that?

It might be that i am asking the wrong questions... but i am still quite confused.
I am very much in the dark concerning this topic so i would be glad about a "beginner"-friendly explanation :smile:.
 

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