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Astrophysical Jets from accreting Black Holes

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II.2 Diffusive shock acceleration<br />

● In reality p is a random variable, but for v >> U and initial<br />

momentum identically<br />

n<br />

pn~ i=1 p0[1 4<br />

3<br />

p 0<br />

U 1−U 2<br />

v i<br />

]⇒ ln pn ~<br />

p0 4<br />

3 U n<br />

1−U 2 i=1<br />

● The probability of crossing the shock front n times is<br />

n<br />

Pn~ i=11−<br />

4U 2<br />

n<br />

⇒ ln P<br />

v<br />

n~−4U 2 i=1 i<br />

⇒ P n= p −3U 2 /U 1−U 2 n<br />

=<br />

p0 p −3/r −1<br />

n<br />

<br />

p0 1<br />

v i<br />

1<br />

=−3<br />

vi U 2<br />

ln<br />

U1−U 2<br />

pn <br />

p0

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