Cosmic Microwave Background Radiation II
Why Study the Cosmic Microwave Background Radiation (CMBR)?
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Test the Big Bang Theory
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The Big Bang Predicts a black body spectrum
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if the Universe is homogeneous and isotropic, then the CMBR
should be isotropic
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i.e. the same temperature in every direction
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Study the Universe when it was simple
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CMBR probes the Universe at t = 300,000 years
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current Universe is "messy"
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visible Universe is dominated by stars and galaxies
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stars and galaxies are complicated
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formation of stars and galaxies cannot be calculated in detail
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stars and galaxies are very much denser than the average
density of the Universe
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galaxies > 100 times denser than average
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stars > 1020 times denser than average
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At t = 300,000 years, the Universe was simpler
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density constant to better than 0.1%
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allows simple approximations
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perfectly uniform Universe with small corrections
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Learn the absolute velocity of the Sun through space
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Learn about the primordial density fluctuations which grew
to form galaxies
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Observations are difficult
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atmosphere (especially water vapor) is not transparent to
full spectrum of CMBR
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temperature variations are very small
CMBR Spectrum
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Test the Blackbody prediction
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deviations at short wavelengths can be caused by energetic
processes shortly after the Universe becomes transparent
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Example: stars of a million solar masses might have formed
and released lots of radiation
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mostly visible and ultra-violet radiation
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emitted at t = 1-10 million years
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generates some excess radiation at wavelengths shorter than
1 mm
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high T, smaller z -> shorter wavelength
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modified Big Bang might be able to live with small deviations
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Early tests focused on long wavelengths
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Here
is a plot of many spectrum measurements
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Short wavelength measurements were done from space
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Here's the current observed spectrum from the COBE-FIRAS
space mission:
Measurement Techniques and Problems
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At wavelengths of a few mm and longer
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use radio receivers
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radio wave radiation shakes electrons up and down in antenna
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creates electronic signal
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H2O vapor not a huge problem
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until very high sensitivity is required
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At wavelengths shorter than a few mm
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needed to confirm blackbody curve
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H2O vapor a big problem
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no atomic states at mm and sub-mm wavelengths
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molecular excitations
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rotational states
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vibrational states
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quantized just like atomic states
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How to get away from H2O vapor
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hot and dry location: say Yuma, AZ?
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NO! hot air holds a lot of moisture
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cold and dry location:
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YES!
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Saskatoon
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South Pole:

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high altitude:
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White Mt., California (14,000 ft)
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Chile's high desert (17,000 ft.):

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problems: altitude sickness - altitude stupidity
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balloons (> 100,000 ft):

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U2 spy plane (~100,000 ft):

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sub-orbital rockets
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flights last a few minutes
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rocket exhaust may travel with instrument
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detectors for
< a few mm
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radio receivers don't work
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Bolometers do:

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a bolometer's temperature will increase when it absorbs radiation
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must be cold
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cooled to T = 4K with liquid Helium at first
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now, state of the art is T = 0.1K with "adiabatic demagnetization"
refrigerator
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problem:
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bolometers can absorb all types of radiation
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non CMBR radiation (visible, infrared) must be excluded
CMBR Anisotropy
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Big Bang predicts approximate isotropy
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Universe is homogeneous and isotropic on large scales
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First deviation from Isotropy
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recall the following formulae:
if
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The first equation is valid when z << 1
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and the 2nd equation is valid for all z
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we can combine them to get
for 
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So the doppler effect gives a temperature shift
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This was first measured by the U2 flight led by Smoot:

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Here's their temperature map:

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This is a full sky map in Earth based coordinates
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Note the missing part of the map in the Southern Hemisphere.
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The velocity of the Sun with respect to the CMBR is about
0.001c or 300 km/sec.
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This is the motion of the Sun with respect to the "cosmic
rest frame."
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This is thought to be caused by the gravitational attraction
of nearby galaxies, clusters of galaxies and even superclusters of galaxies
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Here's a graphical representation of this result:
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Here's a more recent, and more accurate map from the COBE
mission: