Cosmic Background Imager |
Click on the thumbnail image for a bigger version.
Image credit: CBI / Caltech / NSF
The Cosmic Background Imager consists of 13 separate radio
antennas on a single mount that can be pointed to a particular
direction in space. Each antenna is a 90-cm parabolic reflector
enclosed in a shield can and protected by a teflon cover that is
transparent to radio radiation. The signals from each pair of antennas
are combined in a correlator which rejects the constant part of the
microwave background and radiation from the ground and the
atmosphere. The resulting numbers are processed to make images and
further analyzed in supercomputers to extract the power
spectrum. To minimize the effects of Earth's atmosphere, the CBI is located at 5080 m (16,700 feet) on the Llano
de Chajnantor in the Andes of northern Chile
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Seeds of galaxy clusters. The CBI polarization results
provide clear evidence of the motion of the remotest seeds of galaxy
clusters in the very early universe. These polarization results
combine high resolution with high sensitivity which allows us to see
fine details of the radiation from that epoch and to compare in detail
the total intensity with the polarization results. We find that the
polarization is “out of step” with the total intensity,
which is an indication of the motion of these seeds. At the upper
left is shown a total intensity CBI image of the microwave background
in which the variations in color indicate variations in temperature,
and hence in density, at this remote epoch, 13.8 billion years ago and
just 400,000 years after the Big Bang. These variations in density
are the seeds that gave rise to clusters of galaxies and all the
variety of structures that we see in the nearby universe, including
galaxies, stars and planets. At the lower right is shown an image of
the universe after galaxies had formed (Hubble Space Telescope image,
courtesy of NASA). | |
Polarization. The new results of the CBI are based on a property of light called
“polarization.” This is a property that can be demonstrated easily with a
pair of Polaroid sunglasses. If one looks at light reflected off water
(such as on a fish pond) through such sunglasses and then rotates the
sunglasses, one sees the reflected light varying in brightness. This is
because the reflected light is polarized, and the Polaroid sunglasses
only transmit light whose polarization is properly aligned with the
Polaroid.
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Power spectra. The CBI polarization results are found to fit
the predicted polarization curve (green line) which is out of step
with the total intensity curve (red line): the peaks in the total
intensity curve line up with valleys in the polarization curve, and
vice versa. The patterns in the temperature were more sensitive to the
compression of matter when the “first light” was released,
while those in the polarization were more sensitive to how it was
flowing. The two are predicted to be intimately related and
confirmation of this was one of the main findings if the CBI team,
lending support to the inflationary paradigm. The curves are not on
the same scale: the polarized power is a hundred times weaker than the
total intensity, so the polarized curve has been magnified for
clarity. |