UNDER RECONSTRUCTION BELOW
But what does the cosmological constant mean physically?
In the Einstein field equations, Lambda just appears as a modification to how gravity affects spacetime. It is a "just-so" modification.
The cosmological constant is sort of an anti-gravity, but we do NOT call it that and it is NOT symmetric with gravity in any simple way.
In modern physics, there is a strong preference to interpret Lambda as representing a constant dark energy. The dark energy just grows with the expansion of space adding a balanced amount of relative kinetic energy and gravitational potential energy such as to keep the space growing at a constant relative rate (a time-constant Hubble constant) if there were no other mass-energy forms in the observable universe.
The dark energy is often said to have NEGATIVE PRESSURE, but this is so far just a formal NEGATIVE PRESSURE since the NEGATIVE PRESSURE does NOT pull on anything. The NEGATIVE PRESSURE is, in fact, a formal thermodynamics effect if you want to think of the dark energy in a certain hypothetical way.
Now constant dark energy has a constant energy density in time and space. It is about the simplest kind of dark energy imaginable.
That the cosmological-constant dark energy density is constant in time is UNUSUAL. For example, matter density must decrease because of the expansion of the universe. In fact, as cosmic scale factor a(t) increases, volumes increase by a(t)**3, and matter density falls as a(t)**(-3).
The cosmological-constant dark energy density can be treated as a contribution to Omega: we denote this contribution by Omega_Lambda.
Answer 2 and 3 are right. But answer 3 is best in this context.
But the dark energy
need NOT have constant density in either time or space and
it may interact with other forms of mass-energy
in ways we do NOT know.
Until circa
2018,
nothing in the observations told us to go beyond the simple theory of
cosmological-constant dark energy.
But currently, there is
Hubble tension:
see the discussion in the figure below
(local link /
general link: hubble_constant_problem.html).
Yes, quantum field theory
(i.e., relativistic quantum mechanics) suggests there could be
cosmological-constant dark energy,
but alas
predicts its density to be 10**120 times bigger than needed to fit the
observed acceleration
(e.g.,
Carroll, S. 2003, p. 3, Why is the Universe Accelerating?).
This remarkable OVERESTIMATE suggests that the
dark energy
is more complex than the simple
cosmological-constant dark energy
with a density which is constant in time and space.
Another remarkable thing about
dark energy is
that
the cosmological-constant dark energy density
from the analysis of the
CMB data
is
Omega_Lambda
= 0.6853(74),
which is COMPARABLE to the
matter density
Omega_matter
= 0.3147(74).
The reference for these values is
Planck 2018 results. I. Overview and the cosmological legacy
of Planck 2018.
There may be some deep reason why the
dark energy
and matter should be COMPARABLE in which case the
dark energy
CANNOT be simply a
cosmological-constant dark energy.
On the other hand, possibly the COMPARABILITY of
Omega_Lambda
= 0.6853(74)
and
Omega_matter
= 0.3147(74)
(Planck 2018 results. I. Overview and the cosmological legacy
of Planck 2018)
is explained
by the anthropic principle.
(See IAL 0:
A Philosophical and Historical Introduction to Astronomy: The Anthropic Principle.)
Say there are an infinity or a quasi-infinity of
pocket universes
in a multiverse
with different parameters set by some probability distribution of parameters.
Those NOT somewhat like our own
in mass-energy
contents
may NOT be able to support life.
Too small a
cosmological-constant dark energy density
and the universe may NOT have formed the right
kind of galaxies
and stars.
Too large a
cosmological-constant dark energy density
and the universe would have expanded too quickly
ever to form galaxies and
stars.
So the ratio of
dark energy
and matter may just be a roll of the
pocket universe
parameter
dice.
Now it is very hard to prove an argument based on the
anthropic principle.
But such an argument could be falsified if the
dark energy density
and matter density
(the sum of dark matter density
and
baryonic matter density)
were fine-tuned beyond
the needs (so far as we can tell) of making our
pocket universes
suitable for us to be here.
For example, the ratio is now of
dark energy density
to matter density is approximately 2 to 1.
If the ratio were exactly 2 to 1, that is more exactness
than is needed for a
pocket universe
to that can support life like us,
and strongly suggests
dark energy
and matter---NOT
just that random throw of the
pocket universe
parameter
dice.
But there is NOT such exactness, and
so the multiverse
passes this significant
falsification test.
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Is there any reason for believing there could be
just a
cosmological-constant dark energy
from physical theory?