Title: 1(a).%20Milky%20Way%20
1- 1(a). Milky Way M31 a roughly estimation, M31
is on a circular orbit, both MW and M31 are point
mass objects, and period of the M31 orbit is 12
times of Hubble time (eg. 20Gyr).
2- 1(b). Large Magellanic Cloud (the same idea as
1(a)), period of circular orbit is Hubble
time/5 3Gyr
3circular velocity is much smaller than observed
200km/s, which implies dark matter required
4- 3(a).
- 3(b). Observational errors.
- Real deceleration not accounted Kuiper belt or
dark matter dust, solar winds, cosmic rays gas
leaks radiation pressure electromagnetic
forces... - New physics clock acceleration between
coordinates or Ephemeris time and International
Atomic time MOND... - http//en.wikipedia.org/wiki/Pioneer_anomaly
5 6gt (0,0,-1.5) at this point, g(r)0
75.
86.
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107.
a single Fermion has Phase space density
2 Fermions
maximum phase space density
118.
129.
13when rgtgta,
1410.
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16gtGravity is continuous at rr0 Beyond r0,
17inside r0,
total mass
circular escape velocities at r0,
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19- 12. Jeans eq. in spherical isotropic system
The self-gravitating isothermal system, Poisson
eq. is
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2112
Another singular isothermal sphere
trace population
asked to show
isotropic sphere Jeans eq.
plug in
22consider a population,
static
f(E)f(v)Gaussian of zero mean and s dispersion
Gaussian
proved
0
23Angular momentum
Energy change
gt
Tidal radius
24change reduce by a factor of 2 if m-gtm/2
by a factor of 4 if
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26pmv, v//p, FFr, r//Fr gt
Angular momentum conserved
if
27C9.4
isotropic Jeans Eq is
equilibrium, thus net velocity 0,
28gt proved
same idea, to prove
we can always choose orthogonal axis of coordinate
when i ! j, dij 0
29A toy galaxy
first term of potential,
the first term of potential predicts flat
rotation curve, while the dark matter does the
same.
second of potential,
30gravity decreases fast when rgt1kpc, and the
stellar component, plays an important role at
small radii but gravity decreases fast when radii
gt core radius
v_cir 141km/s
for an estimate of total mass, at R10kpc,
spherical simplify
31for stellar
R1kpc, zlt0.1kpc, column density estimation ,
z2 ltlt R2
Msun/kpc3
32Black hole
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34Roche Lobe
Here galaxies can be treated as point mass
objects
gt gGM/R2
same idea, easily prove
35BH
When giant is close to the supermassive black hole
36Link phase space quantities
r
f(r)
J(r,v)
d?/dt
E(r,v)
EKW-K
Vt
K(v)
vr
AS4021 Gravitational Dynamics
37Link quantities in spheres
Vcir2 (r)
g(r)
M(r)
sr2(r) st2(r)
f(E,L)
f(r)
?(r)
vesc2(r)
AS4021 Gravitational Dynamics