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The Big Bang Theory

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Title: The Big Bang Theory


1
The Big Bang Theory
2
Time begins
  • The universe begins 13.7 Billion years ago
  • The universe begins as the size of a single atom
  • The universe began as a violent expansion
  • All matter and space were created from a single
    point of pure energy in an instant

3
3 minutes after big bang
  • The universe has grown from the size of an atom
    to larger than the size a grapefruit
  • Emc2
  • energy froze into matter according to Albert
    Einsteins equation.
  • This basically says that like snowflakes
    freezing, energy forms matter into clumps that
    today we call protons, neutrons and electrons.
  • These parts later form into atoms

4
Several hundred thousand years 380,000 after
Big Bang
  • ATOMS form (specifically Hydrogen and its
    isotopes with a small amount of Helium.)
  • The early Universe was about 75 Hydrogen and 25
    Helium. It is still almost the same today.

5
200 to 400 million years after Big Bang
  • 1st stars and galaxies form

6
4.6 billion years ago
  • Our Solar system forms

7
Misconceptions about the Big Bang
  • there was no explosion there was (and continues
    to be) an expansion
  • Rather than imagining a balloon popping and
    releasing its contents, imagine a balloon
    expanding an infinitesimally small balloon
    expanding to the size of our current universe
  • we tend to image the singularity as a little
    fireball appearing somewhere in space
  • space began inside of the singularity. Prior to
    the singularity, nothing existed, not space,
    time, matter, or energy - nothing.

8
Big Bang evidence
  • Universal expansion and Hubbles Law
  • 3 degree background radiation
  • Quasars
  • Radioactive decay
  • Stellar formation and evolution
  • Speed of light and stellar distances

9
Testing the Big Bang model
Prediction The universe is expanding
Observation Galaxies are moving apart from
each other (1929)
10
1. Universal expansion and Hubbles Law
  1. Hubble observed the majority of galaxies are
    moving away from us and each other
  2. The farther, the faster they move
  3. Red Shift

11
Testing the Big Bang model
Prediction If the universe was denser, hotter,
in past, we should see evidence of left-over
heat from early universe.
Observation Left-over heat from the early
universe. (Penzias and Wilson, 1965)
12
2. Back ground radiation
  1. Noise radiation (static) is evenly spread across
    space
  2. The amount of radiation matched predictions
  3. C.O.B.E satellite confirmed for the entire
    universe that noise radiation (static) is evenly
    spread
  4. Law of conservation of energy (energy can neither
    be created or destroyed) energy remains
    constant over time

13
Testing the Big Bang model
Prediction A hot, dense expanding universe,
should be predominantly hydrogen, helium.
Observation Universe is 75 hydrogen, 25
helium by mass
Cecilia Payne
The Sun 74.5 H, 24 He by mass
14
Testing the Big Bang model
Prediction An expanding universe is evolving
over time. If we look at the early universe, it
should appear different.
Observation Distant galaxies less evolved,
physically and chemically.
15
Testing the Big Bang model
Observation 90 of matter is an unknown form
Dark Matter.
Refine A new and unknown form of matter exists.
But its gravity works the same way, and its
presence is needed to explain how the universe
looks.
Vera Rubin
16
Testing the Big Bang model
Observation Expansion is accelerating.
Refine Extra energy content. A recent
discovery and of unknown origin,the concept of
Dark Energy is actually an integral part of
Einsteins theory of gravity.
17
3. Quasars - super large (solar system size)
galactic cores that put out more light than whole
galaxies
  • Only found 10-15 billion light years away
  • Found nowhere else
  • Nothing exists past them

18
Conclusions
  • Big Bang model describes our current
    understanding of the universe.
  • New discoveries, such as dark matter and
    accelerating
  • expansion (Dark Energy), lead us to refine our
    model,
  • but there is no crisis in our understanding
    (yet).
  • Science is an ongoing process - forcing us to
    test
  • our model through prediction and observation.
    The
  • more tests it passes, the greater is our
    confidence in it.

19
The Future of Cosmology Beyond Einstein
  • What powered the Big Bang?
  • What is Dark Energy?
  • How did the Universe begin?

20
LASTLY we are pretty sure everything has a
beginning, right?
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