1. Origin & Evolution of the Universe
The Big Bang Theory:
Origin & Evolution of the Universe
Su’dud Mayadmeh

2. . . . . Introduction Where did the Universe come from?
Where is it going?
How can we see the past?
How can we learn about the future from seeing the past? . . .

3. Newton’s Static Universe
Universe is static and composed of an infinite number of stars that are scattered randomly throughout an infinite space.
rse is infinitely old and will exist forever without any major changes.
Time and Space are steady and independent of one another and any objects in existence within them.
This made sense to Newton because the gravity of a finite number of stars would eventually cause the universe to fall together into a compact blob - clearly this isn’t/hasn’t happen[ing]/[ed]

4. Newton’s Error
If universe is as how Newton describes, then why is the sky dark at night?

5. Olber’s Paradox
If space goes on forever with stars scattered randomly throughout, then in any line of sight in any direction will eventually run into a star.
Using this logic, the sky should be the average brightness of all of these stars; the sky should be as bright as the sun, even at night.

6. But isn’t the sky dark at night…?
Yes, of course - that is what we observe now and have always observed.
Something is wrong with Newton’s idea of a static, infinite universe.

7. What is the Big Bang Theory?
The universe started as a single point.
That point was extremely dense.
It became unstable and exploded outward.
Today the universe continues to expand

9. 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

10. ~ 3 minutes after big bang
The universe has grown from the size of an atom to larger than the size a grapefruit
E=mc2
energy froze into matter according to Albert Einstein’s 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

11. The Doppler Effect

12. Universal expansion and Hubble’s Law
Hubble observed the majority of galaxies are moving away from us and each other
The farther, the faster they move
Red Shift

13. Galactic Red shifts l Z = [(1+ v/c)/(1+ v/c)]1/2 - 1 Z
Edwin Hubble ( ) and colleagues
measured the spectra (light) of many galaxies
found nearly all galaxies are red-shifted
Redshift (Z)
rest l - =
observed Z
Andromeda galaxy
(Doppler Effect) Z=V/C
(For speed approaching C
we’ll need a relativistic version
Of this equation.)
Z = [(1+ v/c)/(1+ v/c)]1/2 - 1

14. Do you know what Red Shift is?

15. In relativity the space between the galaxies
Quasars & Cosmology
Redshift
In relativity the space between the galaxies
is expanding.
Department of Physics, Applied Physics & Astronomy, RPI

16. Hubble’s Law Galaxies are moving away from us.
The farther away the faster they go.
V = Ho x D
v = recessional velocity of the galaxy
H0 = Hubble constant
D = distance of galaxy to earth

17. Hubble’s Constant Expansion rate measured using Type 1A Supernovae.
The age of the universe can be derived from Hubble’s constant:
T0 = d  T0 = 1
H0d H0
For example, if H0 = 73 km/s*Mpc, then
T0 = 13.4 Billion years old

18. Evidence for Expansion
The light from remote galaxies and other objects is red shifted.
This red shift is called cosmological red shift because it is caused by the expansion of the universe, not by the actual movement of the object (doppler red shift).
If galaxies are all moving away, then at some point they were all much closer.
Hubble’s Law implies the Universe is expanding.

19. Three Pieces of Evidence Supporting the Big Bang
The observation of the galaxies spreading away from the center of the universe (Red Shift)
The presence of Background Radiation
Heat in space 3°K

20. Center of Universe? There is NO CENTER to the universe
Expansion looks the same regardless of where you are in the universe.
Every point appears to be the center of the expansion, therefore no point is the center.
The universe is infinite.

21. What Happens Next?
Astronomers feel that the Big Bang theory leads to two possible futures for the Universe.

22. Open Universe Closed Universe
Galaxies will continue racing outward (continue to expand). All of the stars will die off as the last of their energy is released. There will be nothing left, total emptiness
Closed Universe
Gravitational attraction between the galaxies will cause the movement away from each other to slow and, eventually come to a halt. The gravitational pull will begin to pull the galaxies back to the center of the universe

23. The Shape of the Universe
According to Einstein, mass bends space. This means that the universe has a shape. This shape is related to the density of the universe.
Type
Shape of Universe
Open Universe
Closed Universe
Flat Universe

24. Cosmic Background Radiation
Discovered in 1965
Discovered by Arno Penzias & Robert Wilson
Their radio telescope detected faint radiation coming from all directions
Now believed to be leftover thermal energy from the big bang

25. Cosmic Background Radiation (or CBR)
George Gamow, Ralph Alpher and Robert Herman (1948) suggested that the Universe should have been filled with radiation shortly after the Big Bang. A remnant of this radiation should still be detectable today as low intensity background microwaves.
In an expanding Universe, the wavelength of radiation from the Big Bang would also expand, becoming red shifted and cooled.
 Therefore, we should be able to detect the red shifted cooled-off remnant of the Big Bang explosion all around us (pervading the entire Universe)!
 Furthermore, the remnant of the Big Bang explosion should have a blackbody spectrum.

37. Not The End
Just out of time

38. LASTLY – we are pretty sure everything has a beginning, right?

40. To be continue…