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Scale-free density-potential component
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Astrophysics
Galaxy
Galaxy dynamics
Stellar dynamics
Galactic distribution function
Constant-anisotropy distribution function
2026-09-28
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For
f
=
f
0
L
−
2
β
E
n
,
velocity
integration gives
ρ
=
A
r
−
2
β
Ψ
n
+
3/2
−
β
.
(1)
Thus
a
scale-
free
monomial
in
radius
and
relative potential
corresponds directly to
a
power-law
constant-anisotropy
distribution
function
.
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Constant-anisotropy distribution function
Galactic distribution function
Stellar dynamics
Galaxy dynamics
Galaxy
Astrophysics
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Physics
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(1)
Past exam of the mathematics course of the University of Cambridge
/
2023
/
iii
/
Paper 320
/
2
/
a
/
Solution
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