\( \newcommand{\d}{\mathrm{d}} \newcommand{\bomega}{\vec\omega} \newcommand{\half}{ {1\over 2} } \def\mathnot#1{\text{"$#1$"}} %operators \newcommand{\diag}{\mathrm{diag}} \newcommand{\sinc}{\mathrm{sinc}} \newcommand{\Sh}{ {\large\style{font-family:Times}{\text{Ш}}} } \newcommand{\res}{\mathrm{Res}} \)

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  • 4. Classical Mechanics, Special and General Relativity

4. Classical Mechanics, Special and General Relativity¶

  • 4.1. Gravitation and Electromagnetism as a Field Theory
    • 4.1.1. Gravitation
    • 4.1.2. Electromagnetism
    • 4.1.3. Relativistic Dust
    • 4.1.4. Equations of Motion
  • 4.2. Classical Mechanics
    • 4.2.1. Rigid Body Rotation
  • 4.3. Relativity
    • 4.3.1. Introduction: Why Tensors
    • 4.3.2. High School Formulation
    • 4.3.3. College Formulation
    • 4.3.4. Differential Geometry Formulation
    • 4.3.5. Metrics
    • 4.3.6. Conclusion About Metric
    • 4.3.7. Einstein’s Equations
    • 4.3.8. Continuous Distribution of Matter
    • 4.3.9. Obsolete Section
    • 4.3.10. Inertial frames
    • 4.3.11. Lorentz Group
    • 4.3.12. O(4) Group
    • 4.3.13. Proper Time
    • 4.3.14. FAQ
    • 4.3.15. Questions Without Answers (Yet)

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