Black Holes and the Evolution of Galaxies - PowerPoint PPT Presentation

1 / 35
About This Presentation
Title:

Black Holes and the Evolution of Galaxies

Description:

Objects the size of the solar system that outshine the galaxy. ... important as stars in early phases of galaxy. Some fraction of BH luminosity is mechanical ... – PowerPoint PPT presentation

Number of Views:100
Avg rating:3.0/5.0
Slides: 36
Provided by: DRich6
Category:

less

Transcript and Presenter's Notes

Title: Black Holes and the Evolution of Galaxies


1
Black Holes and the Evolution of Galaxies
2
Summary
  • Quasars and Evolution the universe becomes
    interesting
  • How we do it things invisible to see.
  • Demographics the inverse dinosaur problem.
  • M-? relation, bh mass spectrum.
  • Emerging developments
  • The energy budget for galaxy formation
  • Extension to very low masses
  • spins
  • Possibility of gravitational wave observation of
    BH mergers.

3
  • In 1963 the universe became more interesting
  • Quasars
  • Evolution
  • The initial conditions

4
(No Transcript)
5
3c175
6
Universe baby picture WMAP 5 year image.
7
(No Transcript)
8
(No Transcript)
9
Mysterious properties of quasistellar objects
  • Rapid variability minutes.
  • Light travel time across inner solar system.
  • Directed energy output (collimated beams of
    high-energy particles.
  • Superluminal motion.
  • Enormous luminosities 1011 suns.
  • Objects the size of the solar system that
    outshine the galaxy.
  • Quasars were populous in the youthful universe,
    but are rare now.

10
Quasars and Black Holes
  • Small size, large luminosity and apparent
    stability suggest that quasars are gravity
    powered.
  • Ultimate gravitational engine is a bh. Some
    fraction of accreted energy is radiated (can
    greatly exceed thermonuclear energy).
  • BH turns off when fuel is cut off.

11
Inverse dinosaur problem
  • The light radiated by quasars is proportional to
    mc2 of accreted matter.
  • The mass of order m of the accreted matter.
  • The density of quasars mandates a density of bh
    of about 2 x 105 solar masses/Mpc3.
  • Where are the relics?

12
(No Transcript)
13
Cavendish experiment
14
(No Transcript)
15
(No Transcript)
16
M84
17
(No Transcript)
18
(No Transcript)
19
(No Transcript)
20

21
Orbit Superposition (Schwarzschilds method)
  • Assume a mass distribution (light BH).
  • Compute the gravitational forces.
  • Follow all the orbits.
  • Sum the orbits to match the observed light
    distribution and velocities.
  • Failure rules out the mass distribution.

22
(No Transcript)
23
(No Transcript)
24
Results of 20 year effort
  • Most bulges have BH (97 so far).
  • BH mass tracks main-body parameters
  • (L, ?).

25
Gultekin et al.
26
Aller Richstone
27
  • Bulge M/L 3x10-3 h
  • Density
  • - 2.5x105 Msun/Mpc-3 for h.65 (Yu
    Tremaine)
  • - 4.8x105h2 Msun/Mpc-3 (Aller Richstone)
  • consistent results from different datasets.
  • S 2.2x105 Msun/Mpc3

28
Only gas will produce the correct Soltan number
  • Accreting matter
  • Stars
  • Degenerate objects
  • Dark matter
  • Gas

29
Implications
  • BH growth spurt during quasar era (is this the
    epoch of bulge formation?).
  • What is the pedigree of BH and galaxies?
  • Co-Evolution! --- feeding, bar disruption, core
    scouring, mergers --- bh growh connected to
    galaxy evolution.
  • Is any of this observable?

30
(No Transcript)
31
Thermodynamics of the protogalaxy
  • QSO emits Xrays 0.1m.c2 in 108yr
  • Galaxy has stars 0.01Mc2 in 1010yr
  • QSO light/starlight 103 m./M 1
  • bh is as important as stars in early phases of
    galaxy.
  • Some fraction of BH luminosity is mechanical -
    may be sufficient to blow gas out of galaxy.

32
(No Transcript)
33
(No Transcript)
34
(No Transcript)
35
(No Transcript)
Write a Comment
User Comments (0)
About PowerShow.com