The Standard Cosmological Model has introduced in physics two new concepts that didn't exist before:
- Dark
matter: It seems
to be five times more abundant than ordinary matter, but we don't know
what it is, what it's made of. We only know that it appears to be affected
by gravity, and so far, its existence has been concluded in two different
ways: a) By analyzing the rotational motion of galaxies, which seems to
require that there is more mass in them than what we can see. b) By
studying the cosmic microwave background radiation, which has served as
the basis for adjusting the standard cosmological model.
- Dark
energy: We
have no idea what it is. Some speak of a fifth fundamental interaction (or
force), the quintessence, which would join the four we know: gravitational,
electromagnetic, strong, and weak. Others offer different explanations,
none of which have received experimental confirmation. The hypothesis of
its existence is supported by two observations: a) Analyzing the expansion
rate of the universe, after the 1998 discovery that this rate is
accelerating. b) By studying the cosmic microwave background radiation,
which has served as the basis for adjusting the standard cosmological model.
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Alexander Friedmann (Александр Фридман) |
First of all, I must point out that in the two
cases cited above, we do not have discoveries, but rather hypotheses that
attempt to explain the data we know. As I explained in other
posts, scientific hypotheses are only considered confirmed when they make surprising
accurate predictions,
which so far have not been achieved by either the dark matter or the dark
energy hypothesis.
One of the most important recent instruments
developed to observe the cosmos is DESI (Dark
Energy Spectroscopic Instrument). It has been built to analyze millions of
galaxies, from the nearest to the most distant, to try and deduce the
properties of dark energy, the term in Einstein and Friedmann's cosmological
equation represented by the constant Λ.
The
first results of DESI have just been published, embodied in 270 terabytes
of data about galaxies and quasars whose light started towards us up to 11
billion years ago. And the first analyses of these results do not confirm the
predictions of the Standard Model. This has been considered a cosmological
bombshell. These results seem to indicate (it must be confirmed) that the
dark energy constant (Λ) is not
constant, as had been assumed, but rather varies over time according to a
process similar to the following:
- Initially, its value would have been relatively
low. The
universe was small, all its mass was compressed in a small volume, and
gravity was then the dominant interaction.
- After a certain point, dark energy overtook
gravity as the dominant interaction in an expanding cosmos. But this
happened because another type of dark energy, phantom
dark energy, had appeared, which at first did not exist but grew as the
universe expanded. At that point in time, the expansion of the universe
began to accelerate, as was discovered in 1998.
- About 4.5 billion years ago, basic dark
energy, along with phantom dark energy, reached its maximum density. Since
then, it has been decreasing, for phantom dark energy is disappearing. The
expansion of the universe is still accelerating, but not as rapidly as 4.5
billion years ago.
If these results are confirmed (their current
statistical significance is 4.2σ, and to be
considered confirmed, it should be at least 5σ),
we would find ourselves in the following situation:
•
The
dark energy constant (Λ) would not be constant, so Einstein and Friedmann's cosmological equations
would not be correct. The theory would have to be reworked.
•
The
quintessence hypothesis would
be ruled out.
•
Dark
energy, if it really exists, would be much more complex than previously thought.
•
As
dark energy diminishes, after its phantom version disappears, the universe will
decelerate its expansion, and its future would be unpredictable. It could
continue expanding forever, more and more slowly; reach a maximum size and stay
there; or begin to contract, ending in a Big Crunch.
The latest discoveries, therefore, increase the
mystery and put an end to the feeling, which many cosmologists tried to foster,
that we already know everything. As things stand, the standard cosmological model
cannot be considered validated, as I have said several times in these posts.
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