Sentences with phrase «of microwave background»

These include observations of the microwave background radiation — the relic radiation of the early universe — and surveys of astronomical objects — galaxies, quasars, supernovae, gamma - ray bursters,... — over large fractions of the sky out to large fractions of the radius of the observable universe.

Pen, N. Turok, Polarization of the Microwave Background in Defect Models, Physical Review Letters 79, 1997, 1615, astro - ph / 9704231

AMiBA, a millimeter interferometer like ALMA, was constructed by ASIAA (Academia Sinica Institute of Astronomy and Astrophysics) and National Taiwan University for polarimetry of microwave background radiation and detection of distant clusters of galaxies using the Sunyaev Zeldovich effect.

What we can potentially see is the signature that they imprint into the pattern of the microwave background at about 400,000 years after the beginning.

Three observational «pillars» drive most cosmologists towards the big bang: the expansion of the Universe, the existence and character of the microwave background radiation, and the primordial abundances of the light elements.

Harrison believes his model can explain the smoothness of the microwave background, the afterglow of the big bang.

That simple model should generate strong gravitational waves, which would leave their own distinctive imprint on the polarisation of the microwave background.

These gravitational waves we will to detect will almost be the size of visible universe, but we mean, they'll produce signatures, temperature — well, in this case, the polarization of the microwave background — signatures which are at the level, well, the next generation, the best we can imagine doing is getting a 1 [percent] admixture of a signal from gravitational waves compared to the signal of the temperature fluctuations that we, kind of, measure in the universe.

It is thought to be the first look at a previously unseen period of the universe — between the release of the microwave background and the formation of the earliest known galaxies, about a billion years later.

At radio frequencies greater than 10 gigahertz the radio emission matched that of the microwave background, but at lower frequencies it was several times stronger.

Finkbeiner speculates the source may be electrons given off by dark matter in our galaxy or extraneous emission that accompanied the release of the microwave background in the primordial universe.

Not exact matches

It was theory decades ago, but has since been proven, in part by the existence of the Cosmic Microwave Background (CMB), but also by astronomical observations and by particle accelerator experiments.

Since 1965 and the discovery of the Cosmological Microwave background (CMB) by Penzias and Wilson, we know that Lemaître was wrong.

Recent cosmic microwave background (CMB) measurement not only demonstrate the existence of the cosmological constant, but the value of the constant.

It also confirms more than any other evidence that the universe had a beginning and expanded at a rate faster than the speed of light within less than a trillion of a trillion of a trillion of a second — less than 10 ^ -35 of a second — of the Big Bang by detecting the miniscule «light polarizations» called B - Modes caused by the Gravitational Waves — which were theorized in 1916 by Albert Einstein in his Theory of General Relativity but never detected before — of the Inflation of the Big Bang which are embedded in the Cosmic Microwave Background Radiation — CMB or CMBR that was discovered by American scientists back in 1964.

The Big Bang has been settled science for over 50 years, ever since the discovery of the cosmic microwave background radiation.

The big bang and the current iteration of the Universe having a «beginning» has been generally accepted since Penzias and Wilson stumbled upon the uniform background microwave radiation in 1964.

Red shift, the cosmic microwave background radiation... we've had confirmation of the big bang before.

@justageeker, The Big Bang model is bases on evidence such and the Cosmic Microwave Background Radiation and the «Hubble flow» of all distant objects away from the observer.

4s) then photons erupted from this energy cloud (detectable today as the microwave background radiation) 5s) photons and other particles form the bodies of the early universe (atoms, molecules, stars, planets, galaxies) 6s) it rained on the early earth until it was cool enough for oceans to form 7s) the first life form was blue green bacteria.

The value of the original energy field is unknown, but if the field had just the right strength, and the orresponding distortion in the cosmic microwave background appears, it would suggest that the Big Bounce and space - time quantum loops are real.

How about cosmic microwave background radiation, time dilation in supernovae light curves, the Hubble deep field, the Sunyaev - Zel «dovich effect, the Integrated Sachs - Wolfe effect, the hom.ogeneity of stars and galaxies, etc, etc...

The universe is expanding in all directions)-- 1965: discovery of microwave cosmic background radiation (the echo's of the big bang)-- 1998, two independent research groups studying distant supernovae were astonished to discover, against all expectations, that the current expansion of the universe is accelerating (Reiss 1998, Perlmutter 1999).

Because it can be proven mathematically and also because the background microwave radiation can be found in all directions of the sky.

4) then photons erupted from this energy 4) let there be LIGHT (1 - 4 all the first day) cloud (detectable today as the microwave background radiation) 5) photons and other particles form the 5) God next creates the heavens (what we call the sky) above bodies of the early universe (atoms, (2nd day) molecules, stars, planets, galaxies) 6) it rained on the early earth until it was 6) dry land appears as the oceans form (3rd day) cool enough for oceans to form 7) the first life form was blue green bacteria.

A team of astrophysicists had used the BICEP2 South Pole telescope to identify a pattern in the polarisation maps of the cosmic microwave background radiation (rather like an echo of the Big Bang).

The results are consistent with those from the cosmic microwave background — light emitted billions of years earlier.

Studies of the cosmic microwave background have delivered a peerlessly accurate picture of the cosmos — but dark spectres haunt it

Using the cosmic microwave background, cosmologists find a slower expansion rate than they do from measurements of supernovas.

They had accidentally discovered the cosmic microwave background, the afterglow of the Big Bang.

And measurements of cosmological parameters — the fraction of dark energy and matter, for example — are generally consistent, whether they are made using the light from galaxies or the cosmic microwave background.

Dark matter also plays a central role in structure formation and galaxy evolution, and has measurable effects on the anisotropy of the cosmic microwave background.

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.

The puzzle emerged after astronomers measured the cosmic microwave background — a bath of radiation, left over from the Big Bang — and found only slight variations in its temperature across the entire sky.

The first suggestion that the flow existed came in 2008, when a group led by Alexander Kashlinsky of NASA's Goddard Space Flight Center in Greenbelt, Maryland, scrutinised what was then the best map of the cosmic microwave background radiation, the big bang's afterglow.

The latest search is based on a new, higher - resolution map of the cosmic microwave background from Planck.

[6] Cosmic - infrared background radiation, similar to the more famous cosmic microwave background, is a faint glow in the infrared part of the spectrum that appears to come from all directions in space.

The BICEP2 experiment used 512 detectors, which sped up observations of the cosmic microwave background by 10 times over the team's previous measurements.

COBE's discovery of tiny variations in the temperature of the cosmic microwave background and the subsequent confirmation by WMAP that these are in excellent agreement with the predictions of inflation.

In the case of the cosmic microwave background, light scattered off particles called electrons to become slightly polarized.

Telltale signs of this early chapter in our universe's history are imprinted in the skies, in a relic glow called the cosmic microwave background.

Even more intriguing, the theoretical characteristics of that explosion closely matched the observed properties of the Big Bang — including the cosmic microwave background, the afterglow of the universe's fiercely hot early days.

For the past few years, a NASA spacecraft called the Wilkinson Microwave Anisotropy Probe, or WMAP, has been studying the cosmic microwave background radiation, which is a relic of the Microwave Anisotropy Probe, or WMAP, has been studying the cosmic microwave background radiation, which is a relic of the microwave background radiation, which is a relic of the Big Bang.

These photons fly uniformly through space from all directions, with an average temperature of 2.7 kelvins (° 455 degrees Fahrenheit), composing a cloud of radiation called the cosmic microwave background (CMB).

WMAP detects photons of the cosmic microwave background, the «echo» of the big bang, and these measurements are used...

The next decade, studies of the cosmic microwave background (the relic radiation from the Big Bang) by the Wilkinson Microwave Anisotropy Probe, or WMAP, provided a new way to measure the total amount of dark matter; this is the same technique that the Planck spacecraft built upon to come up with its more precise cosmic bmicrowave background (the relic radiation from the Big Bang) by the Wilkinson Microwave Anisotropy Probe, or WMAP, provided a new way to measure the total amount of dark matter; this is the same technique that the Planck spacecraft built upon to come up with its more precise cosmic bMicrowave Anisotropy Probe, or WMAP, provided a new way to measure the total amount of dark matter; this is the same technique that the Planck spacecraft built upon to come up with its more precise cosmic breakdown.

The initial fireball expands and cools, with the ripples of the membrane leading to the small temperature fluctuations in microwave background radiation observed in our universe.

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.

THE MEANING «Recently the Wilkinson Microwave Anisotropy Probe measured the age of the universe to be 13.7 billion years from the cosmic microwave background,» FreMicrowave Anisotropy Probe measured the age of the universe to be 13.7 billion years from the cosmic microwave background,» Fremicrowave background,» Frebel says.

Along with the familiar cosmic microwave background — the afterglow of the big bang — the distant universe is suffused with an infrared background, thought to come from galaxies and stars too faint and far away to see.