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Tests of Relativity

By Charles Bailyn - Yale
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Lecture Description

The lecture begins with the development of post-Newtonian approximations from Newtonian terms. Several problems are worked out in calculating mass, force and energy. A discussion follows about how concepts like mass and velocity are approached differently in Newtonian physics and Relativity. Attention then turns to the discovery that space and time change near the speed of light, and how this realization affected Einstein's theories. Finally, the possibility of traveling faster than the speed of light is addressed, including how physicists might predict from laboratory conditions how this might occur. Muons, unstable particles that form at the top of the Earth's atmosphere, are used as an example.

Course Description

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Lecture Transcript and Reading Assignment   |  Transcript

Course Index

  1. Introduction to Introduction to Astrophysics
  2. Planetary Orbits
  3. Our Solar System and the Pluto Problem
  4. Discovering Exoplanets: Hot Jupiters
  5. Planetary Transits
  6. Microlensing, Astrometry and Other Methods
  7. Direct Imaging of Exoplanets
  8. Introduction to Black Holes
  9. Special and General Relativity
  10. Tests of Relativity
  11. Special and General Relativity (cont.)
  12. Stellar Mass Black Holes
  13. Stellar Mass Black Holes (cont.)
  14. Pulsars
  15. Supermassive Black Holes
  16. Hubble's Law and the Big Bang
  17. Hubble's Law and the Big Bang (cont.)
  18. Hubble's Law and the Big Bang (cont.)
  19. Omega and the End of the Universe
  20. Dark Matter
  21. Dark Energy and the Accelerating Universe and the Big Rip
  22. Supernovae
  23. Other Constraints: The Cosmic Microwave Background
  24. The Multiverse and Theories of Everything