Chapter 22- Makeup of the Universe Flashcards

1
Q

what does “the universe was very dense and hot” mean

A

that the universe was full of particles and radiation

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2
Q

cosmic microwave background

A
  • electromagnetic radiation as a remnant from an early stage of the universe in Big Bang cosmology
  • evidence of BBT
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3
Q

what does it mean that we needed to wait of universe to become transparent

A

-the time of Recombination: the universe cooled enough for neutral atoms to form

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4
Q

ho long did we wait for the microwave background to start

A

380,000 years

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5
Q

cosmological redshift

A

-photons were stretched

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6
Q

isotropic

A

same in all directions

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7
Q

we know that cosmic microwave background is isotropic, so what can we infer

A

that Big Bang evidence is everywhere in the sky

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8
Q

closed (sphered) universe geometry

A
  • positive curvature

- mass density exceeds critical limit

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9
Q

flat universe geometry

A
  • zero curvature

- mass density equals critical limit

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10
Q

open universe geometry

A
  • negative curvature

- mass density less than critical limit

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11
Q

what suggests that the universe is flat

A

angular separation of temp fluctuations

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12
Q

what are the two problems with our universe

A

1) isotropy problem

2) Flatness problem

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13
Q

what is the isotropy problem within the universe

A
  • the uniform appearance of cosmic microwave background creates a problem
  • how did all parts of the observable universe achieve a common temp
  • to have a common temp things have to touch and some parts of the universe are just now coming in contact
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14
Q

what is the flatness problem within the universe

A
  • if the density is greater than 1 then the universe would end in a Big Crunch
  • if the density is less than 1 then the universe wouldn’t have enough matter to form
  • how did the density magically equal one
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15
Q

inflation in the universe

A

universe expands by rapid factor (faster than the speed of light)

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16
Q

planck epoch

A
  • unknown physics
  • need a theory of everything to describe this epoch
  • all 4 forces of nature would have been unified
17
Q

dark matter

A

-an undirected form of mass that emits little or no light. but whose existence we infer from its gravitational influence

18
Q

dark energy

A

an unknown form of energy that seems to be the source of a repulsive force

19
Q

evidence of dark matter

A
  • galactic rotation curves
  • gravitational lensing
  • cosmic microwave background
20
Q

makeup of universe

A

73% dark energy
22% dark matter
4% He/H
other stuff is stars and radiation

21
Q

what we DO know about dark energy

A
  • there is more of it than anything else

- it acts like antigravity