Astrophysical Jets from accreting Black Holes
Astrophysical Jets from accreting Black Holes
Astrophysical Jets from accreting Black Holes
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II.2 Diffusive shock acceleration<br />
● We again obtain a power law, but unlike other Fermi processes the<br />
slope is fixed<br />
● to verify the slope a, we can look at the synchrotron emission<br />
if the initial spectum is a power law, the synchrotron spectrum<br />
will be a power law with slope<br />
= a−1<br />
2 =0.5
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