1(a).%20Milky%20Way%20 - PowerPoint PPT Presentation

About This Presentation
Title:

1(a).%20Milky%20Way%20

Description:

1(a) ... Large Magellanic Cloud (the same idea as 1(a)), period of ... acceleration between coordinates or Ephemeris time and International Atomic time; ... – PowerPoint PPT presentation

Number of Views:18
Avg rating:3.0/5.0
Slides: 38
Provided by: starst
Category:

less

Transcript and Presenter's Notes

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

3
  • 2(a).
  • 2(b).

circular 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
  • 4.

6
gt (0,0,-1.5) at this point, g(r)0
7
5.
8
6.
9
(No Transcript)
10
7.
a single Fermion has Phase space density
2 Fermions
maximum phase space density
11
8.
12
9.
13
when rgtgta,
14
10.
15
(No Transcript)
16
  • 11.

gtGravity is continuous at rr0 Beyond r0,
17
inside r0,
total mass
circular escape velocities at r0,
18
(No Transcript)
19
  • 12. Jeans eq. in spherical isotropic system

The self-gravitating isothermal system, Poisson
eq. is
20
(No Transcript)
21
12
Another singular isothermal sphere
trace population
asked to show
isotropic sphere Jeans eq.
plug in
22
consider a population,
static
f(E)f(v)Gaussian of zero mean and s dispersion
Gaussian
proved
0
23
Angular momentum
Energy change
gt
Tidal radius
24
change reduce by a factor of 2 if m-gtm/2
by a factor of 4 if
25
(No Transcript)
26
pmv, v//p, FFr, r//Fr gt
Angular momentum conserved
if
27
C9.4
isotropic Jeans Eq is
equilibrium, thus net velocity 0,
28
gt proved
same idea, to prove
we can always choose orthogonal axis of coordinate
when i ! j, dij 0
29
A 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,
30
gravity 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
31
for stellar
R1kpc, zlt0.1kpc, column density estimation ,
z2 ltlt R2
Msun/kpc3
32
Black hole
33
(No Transcript)
34
Roche Lobe
Here galaxies can be treated as point mass
objects
gt gGM/R2
same idea, easily prove
35
BH
When giant is close to the supermassive black hole
36
Link phase space quantities
r
f(r)
J(r,v)
d?/dt
E(r,v)
EKW-K
Vt
K(v)
vr

AS4021 Gravitational Dynamics

37
Link quantities in spheres
Vcir2 (r)
g(r)
M(r)
sr2(r) st2(r)
f(E,L)
f(r)
?(r)
vesc2(r)

AS4021 Gravitational Dynamics
Write a Comment
User Comments (0)
About PowerShow.com