Cosmic Background Radiation
Cosmic Background RadiationCosmologists—those who study the nature of the universe—struggle between two competing theories of the origin of the universe. One theory, the Steady State theory, maintains that the universe has always been in the same state as it is now, that new matter is made in order to fill space created by the expansion of the universe so that the density of matter in the universe remains unchanged. The opposing opinion, The Big Bang theory, maintains that about 13 billion years ago the universe began with an explosion that caused the initial highly compressed state to expand and evolve in the universe as it is today.
The CMB was discovered and measured in 1965 by radio astronomers Arno Penzias and Robert Wilson, who had been studying the “sky temperature.” Sky temperature describes the level of noise at different radio frequencies. It is required in the planning of satellite and other wireless communication systems because it enters receiving antennas along with communication signals. The measurement system devised by Penzias and Wilson consisted of antennas designed to minimize the radiation picked up from the ground, a traveling-wave maser amplifier, and helium-cooled terminations to minimize the noise level of the measurement system.
Measurements taken by Penzias and Wilson showed the presence of a background noise level equivalent to thermal radiation at 3 °K. Since there was no apparent source for this radiation, they concluded that the radiation is a “fossil” left behind by the big bang. This information gave increased weight to the Big Bang theory. Penzias and Wilson were awarded the 1978 Nobel Prize in Physics for their discovery.As a result of the large-scale dissimilarity in the distribution of matter in the universe, the cosmological theories require that the intensity (and hence the “temperature”) of the cosmic microwave background radiation vary with direction in the sky. That is, if you fix your location at one point in space and look towards different directions (as you do when you turn your head from side to side, for example) the universe will vary and there will be more radiation coming from some directions than from others.
microwave radiometer (DMR) used to map the cosmic radiation precisely. The third instrument was a non-microwave instrument called a Diffuse Infrared Background Experiment (DIRBE).
COBE was launched in November 1989 and enabled the microwave background radiation spectrum to be measured about 1000 times more precisely than was previously possible. [In July of 2001, the Microwave Anisotropy Probe (or MAP) satellite was launched to find out more about cosmic microwave background with even more precision than COBE]. The data collected by COBE showed that the cosmic microwave background has an intrinsic anisotropy of the order of 1 part in 100,000. In other words, the measured intensity (or “temperature”) of the radiation does not have the same value in all directions, but varies very slightly from place to place. These tiny variations in the intensity of the cosmic microwave background over the sky show how matter and energy were distributed when the universe was still very young.
Numerous cosmological explanations have been put forth to explain this observed anisotropy, and many conclusions drawn from the resulting models of the universe. In particular, the observations support the hypothesis that the geometry of the universe is flat, the initial perturbations in the density of mass in the universe are scale invariant, and the density is dominated by a form of matter other than ordinary matter.