Примери за използване на Very early universe на Английски и техните преводи на Български
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That's because in the very early universe, there were no metals.
We are the product of quantum fluctuations in the very early universe.
All dimensions in the very early universe may have been wrapped up by string loops.
We are the product of quantum fluctuations in the very early universe.
However, for this to happen, the very early universe must have been a bit lumpy.
We are the product of quantum fluctuations in the very early universe.
Presumably, in the very early universe all the dimensions would have been very curved.
The Big Bang theory states that the very early Universe was hot.
What's more, data on light from the very early universe show that everything just after the big bang was a fairly uniform temperature.
So galaxies must have been born, they must have formed, out of that very early universe.
The first results on the Big Bang and very early universe will not come for another year.
New model explains the formation of supermassive black holes in the very early Universe.
A new window on the very early universe will be opened when we can detect gravitational waves by accurately measuring the distances between space craft.
Physicists create ultra-hot drops of'quark soup' that dominated the very early universe.
There was a time in the very early universe when it was so hot that the particle energies would have been high enough for these transformations to take place.
And that's how we can tell how old the star is, because the very early Universe had no metals at all.
The axion particle presumably appeared in the very early universe, but has been"lurking" in the background while other forces and particles controlled the direction of the universe, .
And that's how we can say how old the star is because there were no metals in the very early Universe.
Further he argues that tiny quantum fluctuations in the very early universe became the seeds from which galaxies, stars, and ultimately human life emerged.
Computer simulations suggest that stars like this must have formed in the very early Universe.
The theory of eternal inflation is quite similar: the very early Universe was dominated by exponential growth, and at some point the growth needed to stop and the energy needed to be converted into matter and radiation.
NASA's Wilkinson Microwave Anisotropy Probe,known as WMAP… has measured the radiation left over from the very early universe.
Since one measurement comes from the very early universe, and another comes from more relatively recent time, the thinking is that maybe some new ingredient in the cosmos is altering the expansion rate of the universe in a way that we didn't already capture in our models.
Later work has also cast doubt on whether there could be a phase transition in the very early universe of the kind required.
Since one measurement comes from the very early universe, and another comes from more relatively recent time, the thinking is that maybe some new ingredient in the cosmos is altering the expansion rate of the universe in a way that we didn't already capture in our models.
In an environment of extremely high energy, the team said that the quark-gluon plasma would have been an ideal environment for rapid flux tube formation in the very early universe.
By studying patterns imprinted in that light today,scientists hope to understand the Big Bang and the very early universe, as it appeared long before galaxies and stars first formed.
Scientists realized that a higher energy version of the quark-gluon plasma would have been an ideal environment for flux tube formation in the very early universe.
Strong theoretical evidence suggests that an episode in the very early universe, perhaps during one of the force splits, endowed the universe with a remarkable asymmetry, in which particles of matter barely outnumbered particles of antimatter by a billion-and-one to a billion.
Because of the great distances to the farthest quasars and the finite velocity of light, we see them andtheir surrounding space as they existed in the very early universe.