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| * <<la(L06-Small-Oscillations.pdf,"Lecture 6, Oct. 11")>>: Small oscillations (free and damped) ([[/L06/Qs|Qs]]) | * Lecture 7, Oct. 13: Driven oscillations+. ([[/L07/Qs|Qs]]) * <<la(L06-Small-Oscillations.pdf,"Lecture 6, Oct. 11")>>: Small oscillations, free or damped. ([[/L06/Qs|Qs]]) |
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| * <<la(L04-Lorentz-Force.pdf,"Lecture 4, Oct. 4")>>: Lorentz force ([[/L04/Qs|Qs]]) | * <<la(L04-Lorentz-Force.pdf,"Lecture 4, Oct. 4")>>: Lorentz force. ([[/L04/Qs|Qs]]) |
Lecture notes
Lecture 7, Oct. 13: Driven oscillations+. (Qs)
Lecture 6, Oct. 11: Small oscillations, free or damped. (Qs)
Lecture 5, Oct. 6: Conservation principles and 1D motions.
Lecture 4, Oct. 4: Lorentz force. (Qs)
- Read footnote 3, to clear up the confusion for the number of integration constants.
When we consider the time-reversal symmetry of this problem, we do not reverse the direction of $\vec{B}$, taking it as given. If we can reverse the direction of $\vec{B}$ as well as the direction of the particle's motion, then the time reversal symmetry would be valid. Read end of page 4, to see why sometimes $\vec{B}$ is not reversible.
Lecture 3, Sep. 29: Perturbation. Air resistance. (Qs)
Page 8, a new box on perturbation expansion. 2/3 → 1/3 in 3 lines above the box. — Sam, 1:04PM, Oct 04, 2011
Lecture 2, Sep. 27: Newton's laws. Air resistance. (Qs)
Lecture 1, Sep. 22: What to learn? Particles, dimensions. Vectors and (orthogonal) matrices.
Appendices
A1: Perturbation. Page 5 and examples are important.