COSMOLOGY (THE BIG BANG)

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  • Created by: CPev3
  • Created on: 02-12-20 14:23

Define astronomical unit (AU)

  • Mean distance from the Earth to the Sun

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  • 150 million km
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Define light-year (ly)

  • Distance travelled by light in a vacuum in a time of one year

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  • Distance = speed x time

= (3 x 108) x (365 x 24 x 60 x 60)

= 9.46 x 1015 m

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Define arcsecond

  • A second of arc

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  • 1 arcsecond = 1 / 3600o

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  • 60 arcseconds = 1 arcminute
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Define arcminute

  • A minute of arc

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  • 60 arcminutes = 1o
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Define parsec (pc)

The distance at which a radius of 1 AU subtends an angle of 1 arcsecond

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1 pc = 1 AU /  tan (1 arcsecond)

= (1.5 x 1011) / tan (1 / 3600) 

= 3.1 x 1016 m

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If the point is at a distance of d pc, then the angle subtended by the radius is 1 / d arcsecond

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Define stellar parallax

A technique used to determine the distance to stars

......that are relatively close to the Earth (less than 100 pc)

............by comparing their apparent positions against distant stars

..................at times 6 months apart

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Distance to the nearby star equation

Distance to nearby star in parsecs = 1 / parallax angle in arcseconds

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Define doppler effect

The change in the frequency and wavelength of waves recieved from an object

......moving relative to an observer

............compared with what would be observed without relative motion

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Source moving from A to B

Waves recieved by B are compressed

Shorter wavelength

Higher frequency

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Waves recieved by A are stretched out

Longer wavelength 

Lower frequency

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Greater speed = greater effect

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Doppler shifts in starlight

1. Absorption spectrum of a specific element determined in the laboratory

2. Same spectrum observed in light from a distant galaxy

3. Difference in observed wavelengths of absorption lines caused by relative motion between galaxy and Earth

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Blue-shifted

  • Galaxy moving towards Earth
  • Absorption lines move towards blue end of spectrum
  • Shorter wavelength

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Red-shifted

  • Galaxy moving away from Earth
  • Absorption lines move towards red end of spectrum
  • Longer wavelength
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Doppler equation

When speed of galaxy << speed of light

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Δλ / λ  Δf / f  v / c

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Δλ = change in wavelength recorded by observer

λ = source wavelength

Δf = change in frequency recorded by oberver

f = source frequency

v = magnitude of relative velocity between source and observer

c = speed of light through vacuum (3 x 108 ms-1)

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Hubble's law

The recessional speed of a galaxy is almost directly proportional to its distance from the Earth

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v-d graph

  • Straight line

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  • Through the origin

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  • Constant, positive gradient

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  • Gradient = Hubble constant
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Recessional speed equation

v = Hod

Ho = 2.2 x 10-18 s-1 or 67.80 ± 0.77 kms-1Mpc-1

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The model of the expanding Universe

The fabric of space and time is expanding in all directions

......∴ any point, in any part of the Universe, is moving away from every other point in the Universe

............Greater distance between points = faster relative motion away from each other

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Light from more distant galaxies is more red-shifted

......∴ they are moving faster than those nearer to us

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Define cosmological principle

When viewed on a sufficiently large scale, the Universe is:

Homogeneous

  • Matter distributed uniformly

Isotropic

  • Looks the same in all directions
  • Has no centre or edge

The laws of Physics are universal

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Big Bang theory

At a moment in the past

......all the matter in the Universe was contained in a singularity (at a single point)

............(the beginning of space and time)

..................that expanded rapidly outwards

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Microwave background radiation

The microwave signal of uniform intensity detected from all directions of the sky, which fits the profile for a black body at a temperature of 2.7 K

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When Universe was young and extremely hot

......space saturated with high-energy gamma photons

............Expansion of Universe and thus space stretched their wavelength

..................Now observed as microwaves

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Universe extremely dense and hot when young

......Expansion of Universe and thus space reduced temperature to around 2.7 K

............Universe = black-body radiator

..................Peak wavelength  1 mm = in microwave region of EM spectrum

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Age of Universe equation

t = 1 / Ho

= 1 / (2.2 x 10-18)

= 4.5 x 1017 s

≈ 14 billion years

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Inaccurate as expansion of Universe is accelerating

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Define dark energy

  • Hypothetical form of energy

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  • Fills all of space

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  • Would explain the accelerating expansion of the Universe

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  • 68.3% of the Universe
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Define dark matter

  • Hypothetical form of matter

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  • Spread throughout the galaxy

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  • Neither emits nor absorbs light

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  • Could explain the differences between the predicted and observed velocities of stars in galaxies

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  • 26.8% of the Universe (matter = 4.9% of the Universe)
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Evolution of the Universe- part 1

The Big Bang

  • Time and space created
  • Universe is a singularity- infinitely dense and hot

10-35 s

  • Universe expands rapidly
  • Phase of incredible acceleration (inflation)
  • No matter, only high-energy gamma photons
  • 1028 K

10-6 s

  • First fundamental particles gain mass

10-3 s

  • Quarks combine to form hadrons
  • Pair production (high-energy gamma photons transform into particle-antiparticle pairs)
  • Most of mass in Universe created by now
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