19 - Dark Matter Halos

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17 Terms

1
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What counters cosmic expansion?

Gravity

2
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Far from a halo, matter moves _____. Near a halo, matter _______ towards the halo.

Apart, collapses

3
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What is the divine line between matter collapsing and moving apart called?

The turnaround radius

4
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If there is more mass, it needs more _______ _________ to hold itself up.

Velocity dispersion

5
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What happens when smaller halos merge in?

They contribute their angular momentum to the main halo, speeding up the spin.

6
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How do you quantify spin?

Spin parameter I measures the amount of rotation support, typically around 3%

7
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Halos are not entirely dispersion-supported; there is a tiny amount of _______ support too.

Rotational

8
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The closer to the middle of a halo you go, the more the ________, so matter is denser.

pressure

9
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Simulations in the 1990s showed that all halos have broadly a similar _______ _____

density profile

10
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A common representation of the scale radius is the __________.

Concentration

11
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A halo with larger mass will have a ____ radius and a ______ concentration

Larger, smaller

12
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The first halos are tiny, formed from tiny CMB __________.

Fluctuations

13
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Halos grow by eating other halos, i.e. _______. This is known as __________ growth.

Merging, hierarchical

14
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What is growth by mergers represented by?

Merger trees

15
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After a smaller halo is merged in, for a while it still retains some identity as its own unit, known as a ________, eventually mixing in with the main halo.

Sub-halo

16
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Based on a merger tree, how do you define the age of a halo?

The time when half its main progenitor mass assembled

17
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Concentration is ______ at lower halo mass. Halos remember the density of the universe when it was formed: Smaller halos formed ______, with higher concentration.

Higher, earlier