Image 1 Caption: The expansion of the universe is a literal growth of space between gravitationally unbound systems according to general relativity. All the cosmological physical distances between the gravitationally unbound systems undergo a general, uniform scaling up with cosmic time.
Gravitationally bound systems and bound systems in general do NOT expand. So you and yours truly don't expand. Moons, planets and stars don't expand. Galaxies and galaxy clusters (if they are gravitationally bound systems which they mostly are) don't expand. Galaxy superclusters, though gravitationally interacting, seem to be mostly gravitationally unbound systems, and so will probably be mostly torn apart eventually by the expansion of the universe if it continues long enough.
In Image 1, we see the ideal scaling up in cosmological physical distances between 3 spiral galaxies 6 dwarf galaxies.
The expansion of the universe is really the expansion of the observable universe. Beyond the observable universe, there is probably expansion for a long way, but we do NOT know how far it extends.
There is NO center of expansion and nothing is being expanded into as far as we can see in the observable universe. There is just a scaling up. But maybe there is a center of expansion and a realm to expand into beyond the observable universe. But we do NOT know.
Note the animation gives the impression that
there is a center of expansion.
But everyone in the
observable universe
can take the perspective that they are at the center of expansion.
We and they actually just see the scaling up of the
observable universe.
The comoving frames,
in fact, form a continuum of
fundamental free-fall frames
throughout the
observable universe.
For cosmologically remote
astronomical objects,
recession velocities do exceed the
vacuum light speed c = 2.99792458*10**8 m/s ≅ 3*10**8 m/s =3*10**5 km/s ≅ 1 ft/ns.
But this is NOT a violation of
special relativity since
recession velocities
are NOT with respect to
inertial frames
Typically peculiar velocities
are relatively small for
cosmological physical distances
>∼ 10 Mpc
and typically become relatively large and even dominating for
cosmological physical distances
<∼ 1 Mpc.
Actually, several observers had partially anticipated
Hubble,
but he observationally discovered
Hubble's law which gave the
expansion behavior, and thus made the
expansion of the universe
a definite result.
Hubble's law (which holds
between points participating in the mean
expansion of the universe) is
where v is recession velocity,
r is cosmological physical distance,
and we have
Hubble constant H = 70 (km/s)/Mpc fiducial value accurate to within ∼ 10 %.
Willem de Sitter (1872--1934)
had predicted
expansion of the universe
in 1917
with his de Sitter universe
which was based on
general relativity plus
the assumptions of the
cosmological principle
and the cosmological constant
with NO matter.
The Friedmann equation
implies Hubble's law, but
it seems that the first to present Hubble's law
as mathematical result explicitly was
Lemaitre
in 1927
in a scientific article
in French
in the pretty obscure
Annals of the Scientific Society of Brussels.
No one seems to have noticed at this mathematical result in
1927 and
Lemaitre did NOT
draw much attention to it.
All the cosmologicalphysical distances r(t)
separating points participating
in the expansion of the universe
scale with a(t):
Note we define a_0 = a(t_0) = 1 by convention.
Thus, the
cosmological physical distances
at
cosmic present t_0
are also referred to as the
comoving distances
since they are the same for all
cosmic time.
Of course, for
Friedmann equation (FE) models
other than the Λ-CDM model
cosmic present t_0 may have
other values.
In fact, for those
Friedmann equation (FE) models
like the
de Sitter universe
and the Steady State Universe
which are eternal
in both
cosmic time directions,
t_0 is usually set to 0.
The Λ-CDM model
is the
standard model of cosmology (SMC, Λ-CDM model)
circa
1998--2025?.
The Einstein-de Sitter universe
(which is neither
the Einstein universe (1917)
nor the de Sitter universe)
was probably the most standard model of cosmology (SMC) for
circa 1965--circa
1998).
The positive-curvature universe
is formally a
closed universe:
i.e., finite, but unbounded.
It is a hyperspherical space: i.e.,
the curved 3-sphere space
which is the surface of a
4-dimensional
Euclidean geometry (AKA flat geometry)
sphere.
In fact, it is NOT clear that
FE models
can be extrapolated endlessly beyond the
observable universe.
If the observable universe
is embedded in a
pocket universe
of a eternal inflation universe,
then the FE models CANNOT be
extrapolated endlessly beyond the
observable universe.
There must be point at which the behavior of the
pocket universe changes in a way
we do NOT know.
v = Hr ,
r(t) = a(t)r_0 ,
where r_0 are the
cosmological physical distances
at
cosmic present t_0 which is
age of the observable universe = 13.797(23) Gyr (Planck 2018)
according to the Λ-CDM model