Big Bang Cosmology Flashcards

1
Q

what does the cosmological principle state?

A

on sufficiently large scale, the properties of the Universe are the same for all observers

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2
Q

what causes the expansion of the Universe?

A

the expansion of SPACE

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3
Q

what is one proof that the expansion of universe has no center

A

no matter where you are in the universe you will measure the same Hubble Law

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4
Q

what measurement should we talk about rather than the SIZE of the universe?

A

the scale factor of the universe

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5
Q

what does the scale factor describe?

A

how the separation of galaxies change with time

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6
Q

what does the amount of stretching depend on?

A

the change in scale factor

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7
Q

redshift is equal to (z + 1 =)

A

scale factor of the universe today/scale factor when light was emitted

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8
Q

what does cosmological expansion imply?

A

that in the past galaxies were closer together

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9
Q

the cosmological principle does not state that the universe is ____ at all times

A

constant

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10
Q

what are two things that can help us determine the age of the universe?

A

1) separation of two galaxies

2) we know how fast these galaxies are moving apart due to expansion of universe

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11
Q

the combined gravity of the mass to slow the expansion of the universe tells us that expansion cannot be ___

A

constant

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12
Q

the mass contained w/in the volume exerts a _____ force that slows down expansion

A

gravitational

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13
Q

what does the geometry of the universe depend on?

A

mass and energy density of the universe

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14
Q

closed universe (>1)

A

positive curvature, spherical geometry…finite in size

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15
Q

flat universe (=1)

A

no curvature, flat geometry…infinite in size

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16
Q

open universe (<1)

A

negative curvature…infinite in size…..saddle shaped

17
Q

why is the sky dark at night?

A

the universe has a finite age, thus our view of the Universe is limited to the finite speed of light so we cannot see infinite number of stars

18
Q

what is the cosmic horizon

A

marks a limit to the observable universe and is limited by time and not space

19
Q

what did. Gamow, Alpher, and Herman predict in 1948?

A

the early universe was filled w/ visible radiation

20
Q

when was the universe opaque to light?

A

when the universe was hot and ionized

21
Q

when did the universe become transparent to light?

A

when it cooled below 3000 K…can now see microwave radiation

22
Q

who discovered cosmic microwave background and when was it?

A

1965 by Penzias and Wilson

23
Q

why are anisotropies important?

A

they represent the beginning of structure of the universe