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Origin of the Universe Kenza Arraki 10/08/2009

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Page 1: Origin of the Universefaculty.washington.edu/ljrberg/AUT09_PHYS485-archive/... · 2009. 10. 13. · History of the Universe cosoc rays m Particle Data Group, LBNL, 2000. Inflation

Origin of the Universe

Kenza Arraki 10/08/2009

Page 2: Origin of the Universefaculty.washington.edu/ljrberg/AUT09_PHYS485-archive/... · 2009. 10. 13. · History of the Universe cosoc rays m Particle Data Group, LBNL, 2000. Inflation

Historical Overview

Size of the universe

1901 - Olber’s Paradox http://en.wikipedia.org/wiki/File:Olber%27s_Paradox_-_All_Points.gif

1920 - The Great Debate Shapely & Curtis

Page 3: Origin of the Universefaculty.washington.edu/ljrberg/AUT09_PHYS485-archive/... · 2009. 10. 13. · History of the Universe cosoc rays m Particle Data Group, LBNL, 2000. Inflation

Historical Overview

Einstein 1916 - General Relativity

Cosmological Constant Strong desire to find a static universe

Page 4: Origin of the Universefaculty.washington.edu/ljrberg/AUT09_PHYS485-archive/... · 2009. 10. 13. · History of the Universe cosoc rays m Particle Data Group, LBNL, 2000. Inflation

Historical Overview

Hubble 1925 - Cepheid Variable stars Solution to the Great Debate

1929 - Distance and radial velocity Expanding Universe

Page 5: Origin of the Universefaculty.washington.edu/ljrberg/AUT09_PHYS485-archive/... · 2009. 10. 13. · History of the Universe cosoc rays m Particle Data Group, LBNL, 2000. Inflation
Page 6: Origin of the Universefaculty.washington.edu/ljrberg/AUT09_PHYS485-archive/... · 2009. 10. 13. · History of the Universe cosoc rays m Particle Data Group, LBNL, 2000. Inflation

Big Bang

What does it successfully explain? •  Expansion of the Universe •  Abundance of the light elements •  Properties of the CMB

Page 7: Origin of the Universefaculty.washington.edu/ljrberg/AUT09_PHYS485-archive/... · 2009. 10. 13. · History of the Universe cosoc rays m Particle Data Group, LBNL, 2000. Inflation

Expansion of the Universe •  Hubble’s Law

v=HO*D

•  Preferred Reference Frame •  Center point

Big Bang

Page 8: Origin of the Universefaculty.washington.edu/ljrberg/AUT09_PHYS485-archive/... · 2009. 10. 13. · History of the Universe cosoc rays m Particle Data Group, LBNL, 2000. Inflation

Big Bang

Abundance of the light elements •  H, D, He, and Li abundances

Started 3 min after BB Ended 20 min after BB

•  Observations 1970’s - Not enough matter 1990’s - High redshift clouds 2000’s - Calculated values from CMB

Page 9: Origin of the Universefaculty.washington.edu/ljrberg/AUT09_PHYS485-archive/... · 2009. 10. 13. · History of the Universe cosoc rays m Particle Data Group, LBNL, 2000. Inflation

Big Bang

Page 10: Origin of the Universefaculty.washington.edu/ljrberg/AUT09_PHYS485-archive/... · 2009. 10. 13. · History of the Universe cosoc rays m Particle Data Group, LBNL, 2000. Inflation

Big Bang

Page 11: Origin of the Universefaculty.washington.edu/ljrberg/AUT09_PHYS485-archive/... · 2009. 10. 13. · History of the Universe cosoc rays m Particle Data Group, LBNL, 2000. Inflation

Ground Based Missions •  SDSS •  Two degree field

Page 12: Origin of the Universefaculty.washington.edu/ljrberg/AUT09_PHYS485-archive/... · 2009. 10. 13. · History of the Universe cosoc rays m Particle Data Group, LBNL, 2000. Inflation

Inflation

What does it successfully explain? •  Large size and uniformity of the universe •  Flatness of the universe •  Origin of lumpiness