microwave background

See for yourself: Tune an old analog TV to an empty channel. Much of that "snow" is from the cosmic microwave background.

Those photons are still running loose, detectable as the cosmic microwave background, a microwave glow from all parts of the sky.

That noise turned out to be the cosmic microwave background, the afterglow of the big bang fireball.

The microwave background fluctuations indeed indicate that the average sum could be zero within the measurement uncertainties.

For instance, consider how cosmologists used the microwave background to rule out a finite spherical geometry.

But the groups who are critical of his work say that this is not what the cosmic microwave background is like.

The mottled look of the Cosmic Microwave Background radiation is the result of differences in temperature and density.

The cosmic microwave background is apparent as the grainy structure towards the top and bottom of the image.

If two universes had collided, the researchers say, it would have left a circular pattern behind in the cosmic microwave background.

One of these satellites, Planck, will look at the cosmic microwave background, a snapshot taken a mere 380, 000 years after the Big Bang.

This cosmic microwave background radiation, they said, represents the ancient afterglow of the big bang.

The Thomson scattering process ended, and the photons ceased interacting with matter so intensively , becoming the microwave background.

Fluctuations in the cosmic microwave background radiation probe the earliest moments of the universe.

However, measurements of the cosmic microwave background radiation temperature suggest that its structure may have some systematic order.

This is the famous cosmic microwave background (CMB) radiation, and a key target of the Planck mission.

Then on larger scales we have the measurements from the motions of clusters of galaxies and the cosmic microwave background.

In addition, the cosmic microwave background has some anomalous features that could potentially be explained by large-scale inhomogeneity.

Would the cosmic microwave background allow them to probe the dynamics of the universe?

For their discovery of the blackbody form and anisotropy of the cosmic microwave background radiation.

During that time, the radiation diffused across short distance scales, smearing the fine print in the microwave background sky.

The pattern of spots in the cosmic microwave background has a suspicious deficiency: there are surprisingly few big spots.

Many of the recent studies in cosmology focus on the cosmic microwave background (CMB).

We've shown that it can fit all of the data that we have about the formation of galaxies, the fluctuations in the microwave background.

And the prime evidence for dark energy doesn't come from the cosmic microwave background, either.

While the microwave background supports both of these, it isn't the foundation of a house of cards.

This is the WMAP microwave background that we see.

But we couldn't do it as accurately as we can from the fluctuations in this microwave background.

Anisotropy and polarization of the microwave background radiation, and the reionization of the universe

An Approximate Analytic Formula for Polarization of Cosmic Microwave Background Radiation

Effect of the cosmic microwave background Radiation to the flux of the Superhigh Energetic Cosmic Ray

Cosmic Microwave Background (CMB) Radiation

His work in black body form and anisotropy of the cosmic microwave background radiation