1. Spacetime: just when you thought it was it throws you a

2. On one hand mass seems to encourage acceleration. On the other hand, it resists it. Another conundrum Einstein just could not ignore.

3. PRINCIPLE OF EQUIVALENCE No experiment in an isolated space can distinguish between a gravitational field and an equivalent uniform acceleration.

4. No experiment would help you distinguish between being weightless far out in space and being in free-fall in a gravitational field.

5. GR POSTULATES PRINCIPLE OF EQUIVALENCE: IN THE VICINITY OF ANY POINT, A GRAVITATTIONAL FIELD IS EQUIVALENT TO AN ACCELERATED FRAME OF REFERENCE IN THE ABSENCE OF GRAVITTATIONAL EFFECTS THE LAWS OF NATURE HAVE THE SAME FORM IN ANY FRAME OF REFERENCE, WHETHER ACCELERATED OR NOT

6. A new way to look at why the Earth rotates around the Sun.

7. Two people are walking in parallel lines at the equator. They continue along lines of constant longitude, until, much to their surprise, they meet. They conclude they must have been attracted by a force. You see that they were actually walking on a curved surface.

9. Lensing

10. Gravitational Lensing

12. Why do we think there is dark matter? Isn’t obvious that most of the matter in the Universe is in Stars?Isn’t obvious that most of the matter in the Universe is in Stars? Spiral Galaxy

13. Clusters produce distinctive tangential patterns

14. Distortions of our view of the sky

16. Gravitational Lensing

17. Measuring the energy in the Universe We can measure the mass of clusters of galaxies with gravitational lensingWe can measure the mass of clusters of galaxies with gravitational lensing These measurements give  mass ~0.3These measurements give  mass ~0.3 We also know (from the primordial deuterium abundance) that only a small fraction is nucleons  nucleons < ~0.04We also know (from the primordial deuterium abundance) that only a small fraction is nucleons  nucleons < ~0.04 Gravitational lensing

18. Dark Matter

19. Another Consequence: GRAVITATIONAL WAVES Particular kind of phenomena (e.g. orbiting stars) produce ripples in the space-time curvature… Ripples travel at speed of light through space These are called gravitational waves.

20. Early instrumentation to detect gravity waves,, “Weber bars”, were pioneered by UMD professor, Joseph Weber! Go Terps!

21. LIGO - Laser Interferometer Gravitational Wave Observatory Like Michelson Morley, but each arm is kilometers long!