New observations of the cosmic microwave
background radiation show that the early universe resounded with harmonious oscillations
Not exact matches
The balloon - borne microwave telescope (called «Boomerang») examined the cosmic
background radiation left over from the Big Bang.The angular power spectrum
showed a peak value at exactly the value predicted by the inflationary hot Big Bang model dominated by cold dark matter.
Their discovery of the cosmic microwave
background radiation won them the Nobel Prize because the remnant heat
showed that the universe must have begun with a violent explosion.
Experts say the dose from the backscatter is negligible when compared with naturally occurring
background radiation, but a linear model
shows even such trivial amounts increase the number of cancer cases
Now, one team of cosmologists has used the oldest
radiation there is, the afterglow of the big bang, or the cosmic microwave
background (CMB), to
show that the universe is «isotropic,» or the same no matter which way you look: There is no spin axis or any other special direction in space.
The first results from the FIRAS experiment, using only 9 minutes of data,
showed that the cosmic
background radiation has exactly the black - body spectrum expected in the hot big bang theory, with a temperature of 2.735 + / - 0.060 kelvin.
But apart from this, by the 1980s experiments
showed that the
background radiation temperature was embarrassingly smooth.
The first is the pattern of hot and cold spots in the cosmic microwave
background radiation, which
shows what the Universe looked like just 380,000 years after the Big Bang.
Working with a tough mentor named Yakov Zel «dovich, Sunyaev
showed that the tiny acoustic vibrations in the universe moments after the Big Bang could be observed as temperature and density variations in the cosmic microwave
background (CMB)
radiation, the faint afterglow of the Big Bang that suffuses the universe.
A statistical analysis of the weight loss of each leaf litter sample after those nine months
showed that higher
background radiation was associated with less weight loss.
A full - sky map produced by the Wilkinson Microwave Anisotropy Probe (WMAP)
showing cosmic
background radiation, a very uniform glow of microwaves emitted by the infant universe more than 13 billion years ago.
Trained as a theoretical physicist, Wolfe and Rainer Kurt Sachs first
showed how density fluctuations in an expanding universe affect the thermal
radiation left by the Big Bang, the cosmic microwave
background radiation.
Images taken by NASA's Cosmic
Background Explorer indicate that the featureless sea of cosmic particles and
radiation now
showed the first signs of structure.
We
show that the
background radiation can be well understood only in terms of the spontaneous emission of the molecules.
I hope it is not since this LNT - hypothesis kills more people then
radiation itself, as has once again been
shown in Chernobyl (or any other place where
radiation is much higher then average
background).