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Strong equivalence principle
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Classroom Contents
Extraordinary Physics with Millisecond Pulsars - Scott Ransom
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- 1 Introduction
- 2 What are millisecond pulsars
- 3 Where do they come from
- 4 Pulsar timing
- 5 Timing residuals
- 6 Asking the right questions
- 7 First indirect detection of gravitational waves
- 8 Famous plots
- 9 Timing noise
- 10 NanoGrav
- 11 Comparing Telescopes
- 12 Data Release
- 13 Arrival Time Measurements
- 14 Gravitational Waves
- 15 Radio Galaxy
- 16 J 287
- 17 Stochastic Background
- 18 Hellings Curve
- 19 Results
- 20 Modeling
- 21 Combining Data
- 22 Preliminary Results
- 23 Improving Instruments
- 24 Finding New Pulsars
- 25 Time Baseline
- 26 More Pulses
- 27 Fermi
- 28 Black widows
- 29 Triple system
- 30 Pulse delay
- 31 Threebody effects
- 32 Strong equivalence principle
- 33 Best upper limits
- 34 What about the future
- 35 We need big telescopes
- 36 Chinas 500m spherical telescope
- 37 Square Kilometre Array
- 38 Arecibo vs GT
