Jeans' length Flashcards

1
Q

What is the Jeans’ length (λJ)?

A

The length at which the gravitational attraction and gas pressure are balanced (right hand side of matter of growth of fluctuation eq is equal to zero)

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2
Q

What happens if λ&raquo_space; λJ?

A

Gravity wins (big things)

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3
Q

What happens if λ&laquo_space;λJ?

A

Pressure wins (small things)

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4
Q

If π is assumed to be 3, what is the relationship between 𝝀J and 𝝀H?

A

they are close in size due to free streaming of gravitational dominant photons and neutrinos

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5
Q

Why are there no pressure effects above horizon?

A

As the horizon is linked to speed of light

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6
Q

What is is the first term in the brackets (4πGρ) represent in the fluctuations formula?

A

Self-gravity

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7
Q

What is the second term in the brackets (k^2c^2/a^2) represent in the fluctuations formula?

A

pressure

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8
Q

When can cold dark matter fluctuations grow on all scales?

A

After matter-radiation equality

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9
Q

When do baryons grow on scales smaller than horizon at matter radiation equality?

A

At recombination

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10
Q

What happens to baryonic matter after recombination?

A

It can fall into the gravitational potential wells that the cold dark matter has been forming since the matter radiation equality

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11
Q

What happens to the baryon fluctuations after recombination?

A

The baryon fluctuations can be significantly larger than the fluctuations in the CMB

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12
Q

After recombination, what does baryon pressure effect?

A

Small scale structures only as Jean’s length is small (size of globular cluster)

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13
Q

What does the Jean’s length set?

A

The split between wavelengths where fluctuations can grow under the influence of their own self gravity and those where pressure dominates and no growth is possible

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14
Q

When do fluctuations stop growing?

A

Once universe behaves as if it were empty

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