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Group Name: Back Bencher
Group Members
S M Manna (14203083)
Sumon Kumar Ghosh (14203098)
Imam Uddin (14203071)
MD. Sayham Khan (14203123)
MD. Yousuf Hassan (14203100)
Presentation Day: 12 March 2015
2The Big Bang
Contents
• The Big Bang Theory
• The Big Bang Phase
• Expanding Universe
• Testing Big Bang Model
• Dark matter & Dark energy
• Evidence of dark matter
• After time period of Big Bang
• Life cycle of star
The Big Bang 3
The Big Bang
• 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.
Image 1: Beginning of Big Bang
4The Big Bang
The Big Bang: Phase
Phase 1
At the beginning of time, from
Complete nothingness, a cosmic
Explosion ignites.
Phase 2
The thrust from the explosion sends
Billions of tons of energy through space
And the elements begin to cool.
Image 2: Phase 1
Image 3: Phase 2
5The Big Bang
The Big Bang: Phase
Phase 3
Galaxies begin to take shape while
Still moving away from the initial
Point of ignition.
Phase 4
The universe continues to expand to
This very day.
Image 4: Phase 3
Image 5: Phase 4
6The Big Bang
Ever Expanding Universe
According to the
Big Bang model,
the
universe expande
d from an
extremely dense
and hot state and
continues to
expand today.
Image 6: Ever Expanding Universe
7The Big Bang
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)
Image 7: Left over heat from early universe
8The Big Bang
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
Image 8: The Sun: 74.5% H, 24% He by mass
Image 9: Cecilia Payne
9The Big Bang
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.
Image 11: Vera Rubin
Image 10: Testing Big Bang
10The Big Bang
Expansion is accelerating
A recent discovery
and of unknown
origin, the concept of
Dark Energy is
actually an integral
part of Einstein’s
theory of gravity.
Image 12: Science Magazine
11The Big Bang
Dark Energy
73%
Normal Matter
4%
Dark Matter
23%
Figure 1: Materials of Universe 12The Big Bang
Evidence for Dark Energy -
supernovae as distance
indicators - step 1
Image 12: A dying star becomes a white dwarf.
13The Big Bang
Evidence for Dark Energy -
supernovae as distance
indicators - step 2
Image 13: The white dwarf strips gas from
its stellar companion….
14The Big Bang
Evidence for Dark Energy -
supernovae as distance
indicators - step 3
Image 14: ….and uses it to become a hydrogen bomb. Bang!
15The Big Bang
Evidence for Dark Energy -
supernovae as distance
indicators - step 4
Image 15: The explosion is as bright as an entire galaxy of stars….
16The Big Bang
Evidence for Dark Energy -
supernovae as distance
indicators - step 5
Image 16: and can be seen in galaxies across the universe.
17The Big Bang
How Everything Began
~ Several hundred thousand years
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.
Figure 2: Atom Formation.
18The Big Bang
~200 to 400 million years after Big Bang
• 1st stars and
galaxies
form
Image 17: ~200 to 400 million years after Big Bang
19The Big Bang
~ 4.6 billion years ago
• Our Solar
system
forms
Image 18: Our Solar system forms
20The Big Bang
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.
21The Big Bang
Figure 3: Life cycle of a star
22The Big Bang
Big Bang evidence
1) Universal expansion and Hubble’s Law
2) 3 degree background radiation
3) Quasars
4) Radioactive decay
5) Stellar formation and evolution
6) Speed of light and stellar distances
23The Big Bang
Conclusions – Till Now
• 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.
24The Big Bang
The Future of Cosmology:
Beyond Einstein
• What powered the Big Bang?
• What Is Dark Energy?
• How did the Universe begin?
25The Big Bang
LASTLY – we are pretty sure everything
has a beginning, right?
Image 20: Funny picture about Big Bang
26The Big Bang
Thanks
The Big Bang 27

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The Big Bang

  • 1.
  • 2. Group Name: Back Bencher Group Members S M Manna (14203083) Sumon Kumar Ghosh (14203098) Imam Uddin (14203071) MD. Sayham Khan (14203123) MD. Yousuf Hassan (14203100) Presentation Day: 12 March 2015 2The Big Bang
  • 3. Contents • The Big Bang Theory • The Big Bang Phase • Expanding Universe • Testing Big Bang Model • Dark matter & Dark energy • Evidence of dark matter • After time period of Big Bang • Life cycle of star The Big Bang 3
  • 4. The Big Bang • 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. Image 1: Beginning of Big Bang 4The Big Bang
  • 5. The Big Bang: Phase Phase 1 At the beginning of time, from Complete nothingness, a cosmic Explosion ignites. Phase 2 The thrust from the explosion sends Billions of tons of energy through space And the elements begin to cool. Image 2: Phase 1 Image 3: Phase 2 5The Big Bang
  • 6. The Big Bang: Phase Phase 3 Galaxies begin to take shape while Still moving away from the initial Point of ignition. Phase 4 The universe continues to expand to This very day. Image 4: Phase 3 Image 5: Phase 4 6The Big Bang
  • 7. Ever Expanding Universe According to the Big Bang model, the universe expande d from an extremely dense and hot state and continues to expand today. Image 6: Ever Expanding Universe 7The Big Bang
  • 8. 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) Image 7: Left over heat from early universe 8The Big Bang
  • 9. 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 Image 8: The Sun: 74.5% H, 24% He by mass Image 9: Cecilia Payne 9The Big Bang
  • 10. 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. Image 11: Vera Rubin Image 10: Testing Big Bang 10The Big Bang
  • 11. Expansion is accelerating A recent discovery and of unknown origin, the concept of Dark Energy is actually an integral part of Einstein’s theory of gravity. Image 12: Science Magazine 11The Big Bang
  • 12. Dark Energy 73% Normal Matter 4% Dark Matter 23% Figure 1: Materials of Universe 12The Big Bang
  • 13. Evidence for Dark Energy - supernovae as distance indicators - step 1 Image 12: A dying star becomes a white dwarf. 13The Big Bang
  • 14. Evidence for Dark Energy - supernovae as distance indicators - step 2 Image 13: The white dwarf strips gas from its stellar companion…. 14The Big Bang
  • 15. Evidence for Dark Energy - supernovae as distance indicators - step 3 Image 14: ….and uses it to become a hydrogen bomb. Bang! 15The Big Bang
  • 16. Evidence for Dark Energy - supernovae as distance indicators - step 4 Image 15: The explosion is as bright as an entire galaxy of stars…. 16The Big Bang
  • 17. Evidence for Dark Energy - supernovae as distance indicators - step 5 Image 16: and can be seen in galaxies across the universe. 17The Big Bang
  • 18. How Everything Began ~ Several hundred thousand years 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. Figure 2: Atom Formation. 18The Big Bang
  • 19. ~200 to 400 million years after Big Bang • 1st stars and galaxies form Image 17: ~200 to 400 million years after Big Bang 19The Big Bang
  • 20. ~ 4.6 billion years ago • Our Solar system forms Image 18: Our Solar system forms 20The Big Bang
  • 21. 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. 21The Big Bang
  • 22. Figure 3: Life cycle of a star 22The Big Bang
  • 23. Big Bang evidence 1) Universal expansion and Hubble’s Law 2) 3 degree background radiation 3) Quasars 4) Radioactive decay 5) Stellar formation and evolution 6) Speed of light and stellar distances 23The Big Bang
  • 24. Conclusions – Till Now • 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. 24The Big Bang
  • 25. The Future of Cosmology: Beyond Einstein • What powered the Big Bang? • What Is Dark Energy? • How did the Universe begin? 25The Big Bang
  • 26. LASTLY – we are pretty sure everything has a beginning, right? Image 20: Funny picture about Big Bang 26The Big Bang