Kramers-Kronig relation for refractive index

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The discussion centers on the Kramers-Kronig relations and their application to refractive index calculations. It highlights the differences between various expressions for refractive index, specifically Δn(ω), n(ω) - 1, and n(ω) - n∞. The conversation explains that the Kramers-Kronig relations arise from the spectral theorem and are linked to the properties of retarded Green's functions, which are analytic in the upper complex frequency half-plane. Subtracted dispersion relations are introduced for cases where the integral does not converge due to the behavior of the imaginary part at infinity. The focus remains on the refractive index and its connection to the permittivity ε(ω) as per the Kramers-Kronig framework.
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I don't understand why sometime
kk 1.png
for paper : Kramers-Kronig relations and sum rules of negative refractive index media
kk 2.png
for paper : A Differential Form of the Kramers-Kronig Relation for Determining a Lorentz-Type of Refractive Index*
kk 3.png
for paper : Comparison Among Several Numerical Integration Methods for Kramers-Kronig Transformation

I know maybe ##\omega = \nu ##

What different between ##Δn(\omega)##, ##n(\omega) - 1## and ## n(\omega)-n_{∞} ##
 
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The formulae given are all socalled "subtracted dispersion relations". It's making use of the spectral theorem aka. Kramers-Kronig relations which are very general relations resulting from retarded Green's functions and causality.

The retardation condition for a Green's function means that it's Fourier transform wrt. time leads to a function that is analytic in the upper complex frequency half-plane and from this you can derive the relations between real and imaginary part of ##\tilde{G}_{\text{ret}}(\omega)##.

If you have a function, for which the integral is not convergent, because the imaginary part doesn't vanish at infinity quickly enough you can derive subtracted dispersion relations. In your example that's applied to the refractive index, which usually goes to a constant for ##\omega \rightarrow \infty##. In this case of the refractive index (though I'm a bit puzzled, because the KK relations refer to ##\epsilon(\omega)## rather than ##n(\omega)##).
 
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