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The Big Bang Theory

The Big Bang Theory. Galaxies: islands of stars making up the universe. Edwin Hubble. First to realize that galaxies lie outside the Milky Way … … by measuring their distances using Cepheid variables as ‘standard candles’ .

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The Big Bang Theory

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  1. The Big Bang Theory

  2. Galaxies: islands of stars making up the universe

  3. Edwin Hubble • First to realize that galaxies lie outside the Milky Way … • … by measuring their distances using Cepheid variables as ‘standard candles’ Edwin P. Hubble (1889-1953) was trained as a lawyer, before boredom made him turn to astronomy instead Cepheid variables oscillate in brightness with a regular period that depends on their luminosity. By measuring this period, they can be used as standard candles.

  4. Cosmic Speedometer • When a galaxy is receding, light waves travelling to us are red-shifted • Hubble measured the spectrum of these galaxies and found the spectral lines to be red-shifted • The faster the recession, the greater the red-shift

  5. Hubble’s Law • Hubble noticed a correlation between the distance of the galaxies and the speed at which they are moving away from us

  6. Hubble constant graph

  7. Expansion of the Universe … ‘winding’ backwards, the universe must have had a beginning

  8. Georges Lemaître • Proposed that the universe began with the explosion of a ‘primeval atom’ • His model was improved by George Gamow and others, who proposed that elements were forged during this hot and dense stage • Known as the Big Bang theory today; coined by Fred Hoyle who proposed a rival theory ... Georges Lemaître (1894-1966) was a Belgian Catholic priest who was fond of saying there is no conflict between science and religion

  9. Steady State Model • Universe is expanding, but maintainsa constant average density • Matter is continually being created in the voids to form new stars, galaxies • Universe has no beginning and no end • But disproved with the discovery of …

  10. Cosmic Microwave Background (CMB) • Background radiation from the sky that is isotropic (same strength in all directions) • Corresponds to a temperatureof just 2.7 Kelvins • Identified as the radiation left over from the Big Bang explosion Arno Penzias (right) and Robert Wilson of Bell Laboratories, next to the horn antenna with which they discovered the CMB in 1965

  11. Cosmic Background Explorer (COBE) The COBE was the world’s most sensitive thermometer, built to probe the heat radiation left over from the Big Bang. In 1992, it detected fluctuations of just a few millionths of a degree in the CMB.

  12. CMB Maps by COBE of the Entire Sky 1) This dipole signal is due to the motion of the Earth through space. The CMB is blue-shifted in the direction of Earth’s motion, and red-shifted in the opposite direction 2) After the dipole signal has been subtractedout, we are left with a hot central bandrunning across the sky, which is due to ourown Milky Way 3) The final CMB map is obtained after both the dipole and galaxy signals have been removed. The resultis a map of regions that are a few millionths of a degree hotter (pink) or colder (blue) than average

  13. These tiny fluctuations have evolved into clusters of galaxies today

  14. Tests of the Big Bang Theory • Expansion of the universe • Cosmic microwave background • Relative abundances of hydrogen, deuterium, helium and lithium

  15. Obtaining the Age of the Universe • Extrapolate the current expansion rate (Hubble constant) back to the Big Bang • 10 to 20 billion years old • Look for the oldest stars (in globular clusters) • 11 to 18 billion years old • Best current estimate is 13.4 ± 1.6 billion years M10 Globular Cluster

  16. Problems with the Big Bang Theory • Flatness problem • why is the geometry of universe so close to being flat? • Horizon problem • why is the universe so isotropic? • Smoothness problem • why is the universe so • homogeneous? Why does the universe appear so uniformeven on opposite sides of the sky, whichcould never have been in causal contactwith each other?

  17. Alan Guth: Inflation Alan Guth of MIT was only 32 when he developed the theory of inflation in 1979 • Lasted between 10-35 and 10-32 seconds after the Big Bang • Universe expanded by a factor of 1050, from smaller than an atom to bigger than a galaxy • It was driven by vast amounts of energy released when a ‘symmetry breaking’ phase transition occurred

  18. Inflation to the Rescue • Flatness problem • Horizon and smoothness problems In each successive frame, the sphere is inflated by a factor of three. By the fourth frame, it looks like a flat plane. Thus, inflation drives the geometry of the universe toward flatness Without inflation, the universe today would consist of a patchwork of different regions. Instead, it is very uniform Inflation had the effect of expanding a small region to a very large one. Since we are inside such a region, our neighborhood appears uniform

  19. Summary: Timeline of the Universe

  20. Timeline of the Universe 2

  21. Possible Fates of the Universe

  22. Will the Universe Recollapse? • Gravitational pull of the galaxies on each other is slowing down the rate of expansion • Required density for the universe to recollapse is 4.5 x 10-30 g/cm3 • Observed density of luminous material (stars, galaxies) is about 3 x 10-31 g/cm3

  23. Dark Matter • But there may be about 10 times this amount in the form of ‘dark matter’ • So the universe is very close to the threshold for recollapse! (This is related to the flatness problem) Measurements of the velocities of stars ina galaxy show that there must be morematter in the galaxy than is apparent.This ‘dark matter’ is known to form aninvisible halo around the galaxy

  24. Possible forms of dark matter

  25. If the universe recollapses ...

  26. If the universe expands forever ... “Some say the world will end in fire, others say in ice.” – Robert Frost

  27. Your Research Presentation Groups must do more extensive research into the following topics: • Red Shift/Doppler Effect • Cosmic Microwave Background Radiation • Inflation • Steady State Model • Cepheid Variables and Hubble Constant • Fates of the Universe

  28. Project RequirementsThursday Meet in Computer Lab 322 1) 8 Minute (minimum) Power Point Presentation • Each Group Member must speak • Each slide must be labeled by the creator of the slide 2) Each group must create one paper poster summarizing their topic 3) Draft slides (one per student) due Thursday, September 15th (50 classwork points) 4) 2nd Draft Slides due Tuesday, September 20th (50 classwork points) 5) Presentations next Thursday, SEPTEMBER 22nd (100 project points)

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