How to calculate the Bremsstrahlung Background?

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Hi everybody,

first I like to thank you for this nice forum :smile:
I tried the search function and found no answer to my question, so here it is:
How can I calculate the Bremsstrahlungs background for TEM EDX spectras (Intensity vs. Energy)?
I found several formulas, for example the oldest Kramers/Small, but they all have
a 1/E dependecy, which of course go to ∞ approaching 0. But since I am interested in
the Oxygen peak, that doesn´t help much...
If anyone have an idea or can give me some directions (link to a paper maybe?)
I would really appreciate.

Thanks
 
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nevermind, problem solved :smile:
 
From the BCS theory of superconductivity is well known that the superfluid density smoothly decreases with increasing temperature. Annihilated superfluid carriers become normal and lose their momenta on lattice atoms. So if we induce a persistent supercurrent in a ring below Tc and after that slowly increase the temperature, we must observe a decrease in the actual supercurrent, because the density of electron pairs and total supercurrent momentum decrease. However, this supercurrent...
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