Lecture 7 Flashcards

1
Q

what did vesto slipher do and when

A

measured redshifts of other galaxies (and velocities)
Andromeda in 1913
25 more in 1917

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2
Q

how did slipher measure redshifts

A

spent weeks measuring individual galaxy spectra, identified patterns of lines in them from known elements, finding redshifts

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3
Q

what did Edwin Hubble and Georges lemaitre do?

A

combined Hubbles measurements of galaxy distances with silphers measurements of galaxy velocities

found more distant galaxies travelled faster

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4
Q

how did the Hubble parameter measurements change over time since 1929

A

they became more accurate over time

in recent times value of the parameter has not changed much but the scatter and uncertainty has

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5
Q

what does Hubbles law imply

A

the universe is expanding

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6
Q

are galaxies moving?

A

no, the space between them is expanding

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7
Q

since the universe is NOT expanding into anything, what is actually happening

A

space is internally getting larger, this stretches light on its path, the expansion is uniform there is no centre

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8
Q

how does gravity effect expansion/vice versa

A

expansion is a gravitational effect

galaxies stars and planets do not get larger

anything that is gravitationally bound together stays together (clusters and galaxies)

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9
Q

what are peculiar velocities

A

components of velocities that deviate from hubble flow

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10
Q

on average what is happening to galaxies due to expansion

A

moving apart but some can move towards each other (andromeda and the Milky Way)

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11
Q

what does the Hubble space telescope do

A

measures cepheids out to 25 Mpc using 800 cepheids, this is 5 times further than previous measurements

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12
Q

why is their a conflicting measurement of H0

A

measured h0 to be 72 via the Hubble space telescope, 68 from earlt universe such as CMB , it is either 68 or 72 so there is a tension

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13
Q

what is tired light

A

an alternative proposed to the universe expanding - suggested that light gradually lost energy as it travelled

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14
Q

explain the specifics of tired light

A

lower energy light meant redder photons which could explain Hubbles law, could happen if light interacts with other light very slightly

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15
Q

why is tired light wrong

A

would have been detectable within our galaxy and In distant radio and optical source behaviour

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16
Q

what are the two possibilities for the past if the universe is expanding

A

matter was all denser - big bang
matter has been gradually created during expansion - steady state model

17
Q

who created steady state model

A

fred Hoyle, Hermann bondi, thomas gold

18
Q

explain the steady state model

A

theory adding a new source called c-field to relativity that gradually generated new matter

generated at 1 atom per cubic meter every 100k years so not detectable

einstein explored similar but didn’t publish

perfect cosmological principle - universe would look the same at any point in space or time

19
Q

why was the steady state theory ruled out

A

despite being fully realised and mathematical cosmological model, based on relativity with a small tweak. it was ruled out with observations

20
Q

what happened after steady state was ruled out

A

creators kept working on it, updated model had periods and regions of expansion and contraction

not taken seriously

21
Q

over view of the Big Bang

A

early matter was denser and hotter, near uniform with no structures
it occurred everywhere in space at once
it is a process/era not a point

22
Q

what is the CMB

A

a microwave signal that is uniform across the sky
if interpreted as a black body then temperature about 3 kelvin
had to work carefully to remove other known signals
exactly as big bang predicted

23
Q

why are most gasses transparent

A

photons are scattered by the free electrons

24
Q

how do you get plasma and what is it

A

hot gas, free elections and protons, scatters photons so it is opaque

25
what is the CMB plasma
before 380k years from the start, universe hot enough to be in plasma state photons bounced around inside plasma so had short paths causing opaque
26
what is recombination
the universe cooling enough for elections to bound to protons, the universe became transparent
27
what happened when the universe became transparent
photons escaped and travelled, this is the CMB. Afterglow of first photons
28
what temp and wavelength were cmb photons released at
3000k, 1 micrometre
29
what factor has the universe expanded out by since photons were released and what has wave length stretched to
factor of 1000, 1mm this is exactly as detected
30
what did the COBE project do
measured CMB spectrum to high accuracy perfect black body spectrum nothing else produces as clean of a signal these measurements killed any other alternative, big bang definitely happened