Примери за използване на Cosmic inflation на Английски и техните преводи на Български
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Cosmic inflation is a winner.
This period is known as cosmic inflation.
The theory of cosmic inflation, which attempts to.
This was the period known as Cosmic Inflation.
Cosmic inflation takes place right after a pop from nothing into something.
Quantum fluctuations Cosmic inflation Flatness problem.
Most scientists solve this problem with a theory called cosmic inflation.
The Big Bang is here, along with cosmic inflation, dark matter and dark energy.
Cosmic inflation is the exponential expansion of space in the early universe.
Joao's theory solves the homogeneity problem just as effectively as cosmic inflation.
The theory of cosmic inflation, first proposed in the 1980s by MIT's Alan Guth, the V.F.
Recent observations have independently supported theories for both the Big Bang and cosmic inflation.
In 1979, Guth proposed the cosmic inflation theory, which predicts the existence of an infinite number of universes.
Instead, his mathematical modeling suggests that dark matter could have been a product of cosmic inflation.
And, if cosmic inflation occurred before the Big Bang, dark matter could have been around before the rest of the stuff in the primordial Universe Soup.
Instead, his mathematical modelling suggests that dark matter could have been a product of cosmic inflation.
And, if cosmic inflation occurred before the Big Bang, dark matter could have been around before the rest of the stuff in the primordial Universe Soup.
Most often attacked are the parts of standard cosmology that include dark matter,dark energy, and cosmic inflation.
This problem is also resolvable by cosmic inflation, which removes all point defects from the observable universe in the same way that it drives the geometry to flatness.
We owe him insights into black holes, but also into quantum physics behind phenomena such as the Big Bang or cosmic inflation.
After the big bang,in an event known as cosmic inflation, the observable universe expanded from the size of a small ball to billions of kilometers, all in fractions of a second.
Approximately 10 -35 seconds after the Planck epoch,the universe expanded exponentially during a period called cosmic inflation.
These are particles with a spin of zero, andthe inflaton theory- whereby a scalar field drove cosmic inflation- suggests that they were produced in abundance during this eyeblink of time.
The main idea was that our part of the world emerged as a result of an exponentially rapid stretching of space called cosmic inflation.
Such a multiverse may be a consequence of cosmic inflation, the widely accepted idea that the early universe expanded exponentially in the slimmest fraction of a second after the big bang.
Approximately 10-35 seconds after the Planck epoch a phase transition caused the universe to experience exponential growth during a period called cosmic inflation.
Although cosmic inflation is well known for resolving some important mysteries about the structure and evolution of the universe, other very different theories can also explain these mysteries.
We normally delineate four distinct levels of Multiverse, andthis first one- in the context of cosmic inflation- most definitely occurs.
The simulation's initial conditions were based on a particular inflationary model-- a set of predictions for how the early universe's distribution of matter may have behaved during cosmic inflation.
These are particles with a spin of zero, andthe inflaton theory- whereby a scalar field drove cosmic inflation- suggests that they were produced in abundance during this eyeblink of time.