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 />
● 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