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Components of the Milky Way. The light from galaxies is centrally concentrated. But is the mass also centrally concentrated? Does Mass follow Light in Galaxies?. Examples of Rotation Curves. Expected Versus Observed Rotation Curves for Our Galaxy.

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Components of the milky way
Components of the Milky Way

The light from galaxies is centrally concentrated. But is the mass also centrally concentrated?

Does Mass follow Light in Galaxies?



Expected versus observed rotation curves for our galaxy
Expected Versus ObservedRotation Curves for Our Galaxy


The maybe correct way to think about our galaxy
The Maybe Correct Way to Think about Our Galaxy

The “Mass Size of the Galaxy is 10 times larger (1000 times more volume) than the “Light Size” of the galaxy  this seems weird?

Shouldn’t there be “DarkGalaxies”  appearance of light (baryons) in the DM halo is random?




Dark matter in elliptical galaxies evidence from x ray gas
Dark Matter in Elliptical Galaxies – Evidence from X-ray Gas

NGC 4697 optical

NGC 4697 Chandra


X ray evidence for dark matter in clusters of galaxies
X-ray Evidence for Dark Matter in Clusters of Galaxies Gas

Need enough gravity

to keep the X-ray gas

from “boiling off” into

intergalactic space.


Possible dark matter candidates
Possible Dark-Matter Candidates Gas

Dark Matter is material that emits low light per unit mass



What about ordinary low mass stars: Clearly ruled out by Space Telescope observations. Left picture shows simulation if these stars dominate stellar clusters at the level required for being DM candidates  observations strongly fail to confirm their existence at the required number density.


Gravitational lensing in abell 2218
Gravitational Lensing in Abell 2218 Space Telescope observations. Left picture shows simulation if these stars dominate stellar clusters at the level required for being DM candidates


Gravitational microlensing
Gravitational Microlensing Space Telescope observations. Left picture shows simulation if these stars dominate stellar clusters at the level required for being DM candidates


Microlensing light curves
Microlensing Light Curves Space Telescope observations. Left picture shows simulation if these stars dominate stellar clusters at the level required for being DM candidates

Length of the lensing event is determined by the mass of the lensing object.


Wimps weakly interacting massive particles left over from early big bang now filling the universe
Wimps: Weakly Interacting Massive Particles left over from early big bang now filling the Universe

  • Dark matter elastically scatters off nuclei

  • Nuclear recoils detected by phonons, scintillation, ionization, …, …

DM

e, g

Attisha


Three real choices
Three Real Choices early big bang now filling the Universe

  • DM is baryonic  most likely ruled out

  • DM is a particle  hasn’t been detected despite 30 years of experiments and expectation that detection is just around th corner.

  • Maybe its gravity that is broken (covered in the third homework assignment).

  • Until DM is actually detected, it remains just like an epicycle.


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