Outline of the Lectures Lecture 1: The Einstein Equivalence Principle Lecture 2: Post-Newtonian Limit of GR Lecture 3: The Parametrized Post-Newtonian Framework Lecture 4: Tests of the PPN Parameters
Outline of the Lectures Lecture 1: The Einstein Equivalence Principle Lecture 2: Post-Newtonian Limit of GR Lecture 3: The Parametrized Post-Newtonian Framework Parametrizing the PN metric Conservation laws Equations of motion - photons Equations of motion - massive bodies Equations of motion - gyroscopes Locally measured gravitation constant G The Strong Equivalence Principle Lecture 4: Tests of the PPN Parameters
The PN metric in GR
Effect of a PN gauge change
Parametrizing the post-Newtonian metric
Effect of a Boost
The parametrized post-Newtonian (PPN) framework
Parameter What it measures, relative to general relativity Value in GR Value in scalar tensor theory Value in semi- conservative theories How much space curvature produced by unit mass? 1(1+ )/(2+ ) How “nonlinear’’ is gravity? 11 + Preferred-location effects? 00 Preferred-frame effects? 00 00 000 Is momentum conserved? 000 000 000 000 PPN Parameters and their Significance
PPN n-body equation of motion
Newtonian” part of the n-body acceleration
PPN n-body equation of motion
The problem of motion Geodesic motion Droste, De Sitter - n-body equations of motion Lense & Thirring - motion in field of spinning body Levi-Civita - center-of-mass acceleration Eddington & Clark - no acceleration EIH paper & Robertson application 1960s - Fock & Chandrasekhar - PN approximation the Nordtvedt effect& the PPN framework numerical relativity - BH head-on collision discovery of PSR
The Strong Equivalence Principle (SEP) All bodies fall with the same acceleration Weak Equivalence Principle (WEP) In a local freely falling frame, all physics is independent of frame’s velocity Local Lorentz Invariance (LLI) In a local freely falling frame, all physics is independent of frame’s location Local Position Invariance (LPI)
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