Why was the cosmic
microwave background so smooth while all the stuff that came after it looked so lumpy?
Not exact matches
So said Dragan Huterer of the University of Michigan, Ann Arbor, the night before the European Space Agency released the highest - resolution map yet of the entire cosmic
microwave background (CMB), relic light from the primordial universe.
That light, the
so - called cosmic
microwave background (CMB), serves as a familiar hunting ground for astronomers who seek to understand the universe in its infancy.
The time asymmetry will then explain why in the beginning the universe was
so uniform, as evinced by the
microwave background radiation left over from the big bang, whereas the end of the universe must be messy.
Astrophysicists have predicted that this B - mode polarization pattern is recorded ever
so faintly in the cosmic
microwave background.
These numbers are corroborated by studies of the afterglow of the big bang — the
so - called cosmic
microwave background (CMB)-- which suggests that our universe is made of roughly 70 % dark energy, 23 % dark matter, and only 4.6 % of ordinary, or baryonic, matter.
The latest study of the afterglow of the big bang — the
so - called cosmic
microwave background radiation — confirms even more precisely the standard model of cosmology — and that's a victory for the theory — but it leaves researchers with no discrepancies that might point to a deeper understanding.
«We are measuring the expansion rate better than at any point since the afterglow of the Big Bang, known as the Cosmic
Microwave Background (CMB), and that precision is giving us a hint that maybe we aren't getting what we expected and
so maybe the universe isn't quite as we had thought.»
PRYKE: About a year ago, we announced that we had detected this
so called swirliness, this B - mode in the
microwave background polarization pattern.
Watching a lecture by the Physicist Lawrence Krauss, I was struck by the idea that in 100 billion years, there will be no cosmic
microwave background and you will look out into the sky with a telescope and only see our galaxy (all other galaxies now being
so far beyond the «horizon» as to be undetectable).
In the particular instance of
so - called back radiation the reality is that if you point an IR spectrometer up at the night sky photons of far higher energy than the cosmic
microwave background are hitting it.