Cosmology Flashcards

1
Q

What is the cosmological principle?

A
  • universe is isotopic and homogeneous
  • laws of physics are universal
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2
Q

What does homogeneous mean?

A
  • the universe is of a constant matter density
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3
Q

What does isotropic mean?

A
  • universe appears the same in all directions
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4
Q

What is the formula for red shift factor?

A
  • v/c
  • v: speed of recession
  • c: speed of light
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5
Q

What is stellar parallax?

A

Apparent shift of position of a nearby star against the background of distance stars.

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6
Q

What is the maximum distance that can be measured using stellar parallax?

A

100 pc

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7
Q

How is stellar parallax used to measure the distance to stars?

A
  • star is observed twice, six months apart
  • angular displacement between positions is calculated
    • halved to find parallax angle in arc seconds
  • find distance in parsec
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8
Q

What is the formula for finding distances using stellar parallax?

A

d = 1/p
- d: distance in Pc
- p: angle in arcseconds

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9
Q

What is Hubble’s Law?

A
  • recession speed of a galaxy is directly proportional to its distance from Earth
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10
Q

What is the equation for Hubble’s Law?

A
  • v = H0d
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11
Q

What is the value of Hubble’s Constant?

A
  • SI: 2.27×10−18 S-1
  • non SI: 69.8 km/s/Mpc
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12
Q

How to calculate the age of the universe?

A
  • in seconds
  • 1/H0
  • H0 in SI
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13
Q

What happened as soon as the Big Bang happened?

A
  • time and space created
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14
Q

When were the first hadrons made?

A
  • 10-3 seconds
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15
Q

What happened after the Big Bang?

A
  • time and space created
  • universe rapidly expands in period of inflation
  • first fundamental particles gain mass
  • quarks bind to create hadrons
  • universe cools as it expands
    • allows for formation of atoms
  • nuclei capture electrons
    • EM radiation from this stage forms CMBR
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16
Q

How was CMBR created?

A
  • When nuclei captured electrons, resulted in transition of electrons down energy levels
  • released energy in form of photons
  • giving rise to EM radiation, initially Gamma
    • stretched to microwaves as universe has expanded
17
Q

What evidence is there of dark matter?

A
  • discrepancy between observed rotational speed of galaxies and the predicted rotational speed
    • prediction was for observed speed to drop with increased diameter
    • instead observed speed was higher than prediction
  • suggested a halo of matter to be present around the galaxy
18
Q

What forces does dark matter interact through?

A
  • seems to be gravitational
19
Q

What is dark energy?

A
  • energy of empty space
  • used for the continuous expansion of the universe