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Big Bang (1)

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The Big
Bang
Theory
What is the Big Bang
Theory?
Big Bang Theory explains that the universe is
expanding, and if we reverse the expansion, there must
have been a singularity where everything is together.
The sudden separation and expansion of the singularity
is called the Big Bang.
Evidence
There are 3 main evidences
to the Big Bang: Red Shift,
Cosmic Microwave
Background Radiation
(CMBR), and Elemental
Abundances
Red Shift
Red Shift is a phenomenon where light is
shifted towards the red of the light spectra
the further away the source of the light is. It
is seen that all observable galaxies are red
shifting from us, meaning that the universe
is expanding. The "reddest" in the
spectra are known as microwaves
Cosmic Microwave Background
Radiation (CMBR)
CMBR is the microwaves that are detected all around us.
This shows that that the universe has expanded so far
since the big bang that the radiation of the big bang has
redshifted so far to the point where it turned to
microwaves. This was discovered by a satellite called
COBE. The pink spots on the left picture are the
microwaves.
Elemental
Abundnces
After the Big Bang, the universe was
too cold for fusion, therefore atoms
were broken up to one of the lightest
elements, Hydrogen and Helium.
There are about 70% H, 29% He, and
1% everything else, in the universe.
Limitations of the Big Bang
There are some problems that come with the Big Bang Theory, which are
called the Limitations of the Big Bang.
The Flatness Problem: WMAP (A satellite) has determined that the
geometry of the universe is flat, while the Big Bang Theory contradicts
this and states that curvature grows with time
The Horizon Problem: The distance in the region of space is so big that
the light-years of the distance between space exceed the age of the
universe.
Big Bang Theory (cont)
The Inflation Theory
The inflation theory theorizes that there was a
small period after the Big Bang where the
universe expanded rapidly called the Inflation,
unlike the gradual expansion currently.
How this solves the
Limitations
The Flatness Problem: The universe had
expanded so much during the Inflation, that it
became perceived as "flat"
As you can see from the picture, the circle is the Universe, round.
(not to scale) if we zoom in and in, (the stars are markers), by the
time we reach the purple star, the terrain seems flat. This is like
the universe: The universe is so big that in the field of our view (as
far as we can go), it will look flat because the universe is inflated
so much. Inflation stretches any initial curvature of the universe to
near flatness.
How it solves the Horizon
Problem
Because the Universe had expanded rapidly in
such as small period of time, it explains why
there are larger light-years of distances of space
between galaxies.
Structure of the
Universe
There is some speculation on how the
universe is shaped. There are 3 ways it
could be shaped, Closed, Flat, or Open.
Fun Fact
Dark Energy takes up 73% of the
universe, and Dark matter takes
up 23%, while atoms, or regular
things we see such as stars only
take up 4.6%. Astounding!
Dark Matter
Dark Matter is matter that does
not emit any radiation, nor can
we see it, but it does have
gravity.
Dark Energy
Dark Energy is a mysterious
energy that pushes the universe
faster and faster. This is why the
expansion of the universe is
slower a few billion years ago
than now.
Sources
NASA. (n.d.). WMAP inflation theory. NASA. Retrieved September 16, 2021, from
https://map.gsfc.nasa.gov/universe/bb_cosmo_infl.html.
NASA. (n.d.). WMAP big BANG CMB Test. NASA. Retrieved September 16, 2021, from
https://map.gsfc.nasa.gov/universe/bb_tests_cmb.html.
NASA. (n.d.). Wmap- big bang expansion: The hubble constant. NASA. Retrieved September
16, 2021, from https://map.gsfc.nasa.gov/universe/bb_tests_exp.html.
NASA. (n.d.). WMAP- content of the universe. NASA. Retrieved September 16, 2021, from
https://map.gsfc.nasa.gov/universe/uni_matter.html.
Greicius, T. (2016, August 31). The universe comes into sharper focus. NASA. Retrieved
September 16, 2021, from
https://www.nasa.gov/mission_pages/planck/multimedia/pia16874.html.
E=mc
2
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