How Do We Discern Dark Matter from Dark Energy in the Universe?

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How it's possible to discern dark matter from dark energy?
Why do we need both things? How we can tell so accuratelly that the universe
is made up 71.3% of dark energy and 27.4% of a combination of
dark matter and baryonic matter.
Thanks for answer.
 
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I find it in wikipedia:

The total amount of matter in the universe (including baryons and dark matter), as measured by the CMB, accounts for only about 30% of the critical density.

How it's possible to determine amount of matter from these measurements.
 
paweld said:
How it's possible to discern dark matter from dark energy?
Why do we need both things? How we can tell so accuratelly that the universe
is made up 71.3% of dark energy and 27.4% of a combination of
dark matter and baryonic matter.
Thanks for answer.
The behavior of the two is completely different.

Dark matter is a name for the missing matter we see in objects like galaxies and galaxy clusters. Basically, when we look at these objects, we find that most of the matter is in a non-visible component. Currently we've narrowed down the possibilities so that we're reasonably sure that dark matter is composed of some sort of massive particle that interacts only weakly with itself and with normal matter (somewhat like neutrinos, but neutrinos would have had too much kinetic energy when produced to explain our observations).

Dark energy, by contrast, is used to explain a very different sort of observation: the expansion of our universe after a few billion years ago has begun to accelerate. Right now it is much more speculative and open as to the possible explanations, but some of them have been eliminated, at least. Currently the prevailing explanations are some sort of modification of gravity at extremely large distances or an energy field that tends to stay constant or nearly constant in density as the universe expands.
 
paweld said:
How it's possible to discern dark matter from dark energy?
Why do we need both things? How we can tell so accuratelly that the universe
is made up 71.3% of dark energy and 27.4% of a combination of
dark matter and baryonic matter.
Thanks for answer.

The 71.3% is the negative pressure energy that's required for the accelerating expansion model of the universe to be complete.

Although Einstein believed the universe to be static at the time, GR had flexibility to accommodate "Dark Energy" known as The Cosmological Constant.

Or so I believe.
 
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https://en.wikipedia.org/wiki/Recombination_(cosmology) Was a matter density right after the decoupling low enough to consider the vacuum as the actual vacuum, and not the medium through which the light propagates with the speed lower than ##({\epsilon_0\mu_0})^{-1/2}##? I'm asking this in context of the calculation of the observable universe radius, where the time integral of the inverse of the scale factor is multiplied by the constant speed of light ##c##.
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