Synchrotron function
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In mathematics the synchrotron functions are defined as follows (for x ≥ 0):
- First synchrotron function
- <math>F(x) = x \int_x^\infty K_{\frac{5}{3}}(t)\,dt</math>
- Second synchrotron function
- <math>G(x) = x K_{\frac{2}{3}}(x)</math>
where Kj is the modified Bessel function of the second kind. These functions are shown on the right, as the output from a plot in Mathematica.
Use in Astrophysics
In astrophysics, x is usually a ratio of frequencies, that is, the frequency over a critical frequency (critical frequency is the frequency at which most synchrotron radiation is radiated). This is needed when calculating the spectra for different types of synchrotron emission. It takes a spectrum of electrons (or any charged particle) generated by a separate process (such as a power law distribution of electrons and positrons from a constant injection spectrum) and converts this to the spectrum of photons generated by the input electrons/positrons.
For further information, see High Energy Astrophysics, Malcolm S. Longair, CUP, 1990.
