An original theory or New Hypothesis regarding the Expansion of the Universe.
The universe is expanding at the velocity of light.
The universe is not expanding as a result of the Big Bang.
Gravity does not affect Universe Expansion.
There is only the observable universe.
An original theory and new hypothesis of the universe.
The universe is closed, positively curved, and asymptotically flat. [1]
"Space and time have a real existence independent of the matter
and energy that exist within them." (Jim Al-Khalili)
This means that mass (and gravity) do not affect the overall
Space and Time. This is an after-the-fact explanation.
What are stars made of?
It was astronomer Cecilia Payne who
found the answer. In her 1925 doctoral dissertation, she showed
that stars are primarily composed of hydrogen and helium.
This illustrates how important it is to understand the properties
of the hydrogen atom.
[2]
Who discovered the radial velocities of galaxies?
In 1912, astronomer Vesto Slipher
performed the first measurements of the radial velocity of the
Andromeda Galaxy, and to observe the shift of spectral lines
of many galaxies discovering their galactic redshifts.
[3]
Who discovered the pulsation-period-luminosity distance relationship
for galaxies?
It was the work of astronomer Henrietta Leavitt
to find the distance using her discovery of the period‑luminosity
relationship, where the absolute magnitude of Cepheid variables varied
with their brightness/dim period. By knowing the luminosity of a source
it is possible to measure the distance to that source by measuring how
bright it appears to us: the dimmer it appears, the farther away it is.
[4]
Who discovered the distance to galaxies?
Giving the distance to Cepheid stars by comparing its known luminosity
to its observed brightness, calibrated by directly observing the
parallax distance to the closest Cepheids. It has now been one hundred
years since astronomer Edwin Hubble
found the distance to the Andromeda nebula in 1924.
[5]
Who discovered the velocity-distance relationship with respect to galaxies
?
Using Slipher's work on redshifts
Hubble found a consistent velocity‑
distance relationship in other distant objects.
In 1929, Hubble published his
velocity‑distance diagram. Later, Hubble
himself publicly recognized the extremely important role of
Slipher, and he later wrote to
Slipher of the importance of
"Your velocities and my distances".
[6]
What is the Cosmological Principle?
On the largest scales, the universe is homogeneous and isotropic.
When physicist Arno Penzias
and radio‑astronomer Robert Wilson
discovered the Cosmic Microwave Background in 1964, this was the first
modern confirmation of this principle, which states that the universe
is the same everywhere. The Cosmic Microwave Background (CMB) snapshot
shows a near‑uniform distribution. If each part of the cosmos has
always been expanding uniformly at the velocity of light, then they have
very similar conditions across the universe.
[7]
Is the universe radiation background totally uniform?
?
Theoretical physicist Werner Heisenberg's
proposal of uncertainty, a principle that is basic to
quantum theory, comes into play. The uncertainty principle asserts that
it is physically impossible to measure the exact position as well as the
exact momentum of a particle at the same time. The more precisely one
quantity is measured, the less precisely the other is known. This
quantum fluctuation manifests as small discrepancies and not an
absolutely uniform CMB.
[8]
Can far‑flung galaxies affect us
gravitationally?
They already have. From the Big Bang onward, for each nucleon,
the curvature of space‑time tells matter how to move and has
expanded outward at the velocity of light, in the form of gravitational
waves known as the cosmic gravitational wave background.
All matter is connected, then and now.
[9]
Does each volume of space have the same temperature
?
At the scale of the universe, the concept of thermodynamic equilibrium
says so. Now, like gravity and light, and again from the Big Bang onward,
all of space‑time is connected, as heat‑carrying light
expands with the universe. The universe expands at the velocity of light.
[10]
Soon after the Big Bang, we have recombination, which marks the beginning of the Cosmic Dark Ages where light absorption was maximal, with mostly HI atoms prevailing. Photons can be absorbed by the electron cloud around each atom rendering HI clouds opaque. At redshift z≈1089, or about 13 million years, re‑ionization began, eliminating a major photon absorption line. This was done by removing the electron cloud around hydrogen atoms and began the widespread emergence of ionized hydrogen. These early stars helped ionize hydrogen atoms H+, which allowed for universe‑wide transparency. [11]
Gravitation pulled matter together which led to the early formation of stars and then galaxies. [12]
NASA's Wilkinson Microwave Anisotropy Probe (WMAP) announced in 2003 that the first stars were formed at redshift z≈20, or about 690 million years old. At about one billion years the Cosmic fog had lifted at redshift z=13.5, as the universe gradually transitioned into our visible sky. Now with denser, hotter, more intense star formation, the universe was richer in smaller spiral and irregular galaxies as opposed to the giant elliptical galaxies we see today. [13]
Is there a definitive redshift-distance relationship?
Yes. Now, consider that we have a linearly expanding universe, where an
object with a specific redshift implies a
perimeter(circumference)
distance to that object, using the following arguments.
We consider the perimeter(circumference)
P of a
circle that represents our universe at age UAge.
We come up with two equations describing the expansion of the universe.
[14]
Massive stars (at least with a mass over eight times that of our sun), create neutron stars, and as such massive stars are often created in pairs, which are likely to create neutron stars in pairs enhancing the likelihood of neutron‑star mergers.
Are the ad hoc expansion forces of cosmic inflation and dark energy
related in some way?
Yes, neither exists nor has ever existed.
What were the contributions of physicist
Albert Einstein and mathematician
Alexander Friedmann
?
It was the General Relativity equations, which
has correctly explained the contents of the universe. And yet, General
Relativity still needs a separate theory of inflation to explain the
evenness of the universe. It cannot solely be used to account for an
expanding universe.
[15]
Now Special Relativity alone can be used to account for such an expansion. The velocity of light c is profoundly tied to the Fine Structure Constant α and as such is a true constant. My calculations have shown that the value of α can be described by the following formula, which is an exact real number.
How long have neutrinos been around?
Presumably for 14.57 billion years. My Special Relativity calculations
have shown that time dilation can be described by the following equation.
[16]
If neutrinos travel no less than v/c=0.9999999999995, then this implies
t'/t=sin cos-1(0.9999999999995) = 0.000000999999999999875 or
a million to one, implying the oldest neutrinos have only experienced
14,570 years! Note: this means neutrinos travelling from our sun to
earth experience 1/2000 seconds and not 500 seconds.
While early stars have not been observed, some galaxies have been
observed from about 736 million years cosmic time
z=18.7 and were identified in 2023 by
the James Webb Space Telescope (JWST).
Note: In millions of years, cosmic time is determined by the ratio
14570/(z+1). As well, we have had spectroscopic confirmation of these
metal‑poor galaxies e.g. z=2.5(4.142 billion years),
z=3.9(2.959 billion years), z=8(1.611 billion years),
z=10.38(1.274 billion years), z=10.6(1.25 billion years),
z=11.3(1.178 billion years), z=11.58(1.152 billion years),
z=12.63(1.063 billion years) and z=13.2(1.021 billion years).
[17]
The universe will continue to appear very similar for many billions of years into the future. Our Solar System formed about 4.6 billion years ago with the earliest traces of life on Earth emerging about 3.7 billion years ago.
At some time the Stelliferous Era (the age of stars) will end where
matter is organized into stars, planets, nebulae, galaxies and galactic
clusters. This era is thought to run from about 106 to
1039 years, as stars are no longer being born, and the
expansion of the universe will mean that the easiest galaxies to see
are our local galaxies. There are various scenarios for the far future
and the ultimate fate of our universe. Don't worry, in the future,
there will be no Big Rip, no Big Crunch, and no Big Bounce.
The Hubble-Slipher constant can be computed directly assuming that
the Universe expands at exactly the velocity of light.
It as thought that the Type Ia category of supernova produced a fairly
consistent peak luminosity because of the fixed critical mass at which
a white dwarf will explode.
We now have something called the double-detonation supernovae of
sub-Chandrasekhar mass white dwarfs that no longer needs such a thing
as a fixed critical mass.
[18]
The universe is now an age of 14.57 billion years where its
perimeter(circumference)
is Pm = 4467 megaparsecs.
Note that HD 140283 is estimated to be 14.46±0.8 billion years old.
In four dimensions the volume(surface) is given by
2π2r3
where Perimeter(circumference) =
2πr, giving the volume to be V =
P3/4
π.
The universe contains 1080 protons, so the Universe completely
filled with protons occurs three hours after the big bang,
and the Universe completely filled with hydrogen atoms occurs
three years after the big bang
The volume of the universe is now seven cubic gigaparsecs, which equates
to 2.05454×1077 cubic metres.
Given a universe energy density of 411 photons/cc, it follows that there
are 8.44416×1085 CMB photons in the whole universe.
∗
This table includes redshift values previously discussed.

The Cosmic Redshift Table ∗ | |||
---|---|---|---|
z Redshift |
Age in megayears |
Pm Perimeter in megaparsecs |
Volume in Cubic gigaparsecs. |
0 | 14,570 | 4467 | 7.093 |
0.057 | 13784 | 4226 | 6.006 |
0.123 | 12974 | 3977 | 5.006 |
0.21 | 12041 | 3691 | 4.001 |
0.332 | 10938 | 3353 | 3.000 |
0.525 | 9554 | 2929 | 2.000 |
0.921 | 7585 | 2325 | 1.000 |
1089 | 13 | 3 | 0.000 |
∞ | 0 | 0 | 0 |
In the long term (after many trillions of years of cosmic time), the age of stars will end. Beyond this, all objects in the universe will cool and decompose progressively back to their fundamental particles, by a variety of possible processes.
What is the velocity of light?
What is the velocity of gravity?
They have the same value, the expansion rate of the Universe.
The universe is finite and ever‑expanding. It is not cyclic. The whole universe is observable.
∗ All calculation errors are my own.