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ASTR340 Spring 2002

THE ORIGINS OF THE UNIVERSE

Course description and syllabus

Lecture notes:

  • Lecture 1 - Course Introduction
  • Lecture 2 - Early Cosmologies and the Beginnings of Modern Astronomy
  • Lecture 3 - Newton's laws and reference frames
  • Lecture 4 - Newtonian gravity and the weak equivalence principle
  • Lecture 5 - Absolute time, and the speed of light problem
  • Lecture 6 - The extragalactic universe and distance measurement
  • Lecture 7 - Special Relativity I (Time dilation)
  • Lecture 8 - Special Relativity II (Simultaneity and Causality)
  • Lecture 9 - Special Relativity III (Mass and Energy)
  • Lecture 10 - General Relativity I (Strong Equivalence Principle)
  • Lecture 11 - General Relativity II (Curved space-time)
  • Lecture 12 - General Relativity III (Consequences of General Relativity)
  • Lecture 13 - Review
  • Lecture 14 - Mid-Term examination
  • Lecture 15 - General Relativity IV (Black Holes)
  • Lecture 16 - Discovery of the expanding universe
  • Lecture 17 - Cosmological Models I
  • Lecture 18 - Cosmological Models II
  • Lecture 19 - Non-Standard Cosmological Models
  • Lecture 20 - The Cosmic Microwave Background
  • Lecture 21 - Primordial Nucleosynthesis
  • Lecture 22 - Weighing the Universe, and Non-Baryonic Dark Matter
  • Lecture 23 - The Formation of Structure
  • Lecture 24 - Our Universe: the Cosmic Concordance
  • Lecture 25 - The Early Universe
  • Lecture 26 - Problems with the standard model
  • Lecture 27 - Inflation
  • Lecture 28 - Various Inflation models, and the anthropic principle

Homeworks:

Supplementary material

 
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