Classical Physics Review
Newtonian Mechanics
Electric and Magnetic fields
Electromagnetic Radiation
- Basics: speed, amplitude, phase
- linear superposition -> interference
Classical Relativity
Newtonian Mechanics
Newton's Laws of Motion:
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For a constant mass we have the familiar forms:
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-> Conservation of momentum (equal and opposite forces acting over the same time).
Important Application: Simple Harmonic Oscillator
Force opposite and prop. to displacement, e.g. a pendulum or a spring:
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General Solutions:
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where the Angular frequency ![]()
Frequency ![]()
Energy:
= force applied x distance:
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Particle: Total Energy = Kinetic Energy + Potential Energy:
E = K + U
Principle of Relativity:
Examples of Inertial Reference Frames:
Counter-examples (non-inertial frames):
Rotation:
Centripetal acceleration ![]()
Electric & Magnetic Fields
Electric fields:
Electrostatic force between point charges:![]()
Charge
q is measured in Coulomb ( C). Charge of electron e =-1.6x10-19 CElectric field = force per unit charge: ![]()
e.g. field around a point charge ![]()
Potential Energy = work required to move a charge into an electric field from infinity, e.g. for two point charges ![]()
Electrical Potential = potential energy per unit charge, e.g. around a point charge ![]()
So "Work done" = charge x potential difference = qV
-> new unit of energy: 1electron-Volt (1 eV) = work done when a charge of 1 electron crosses a potential difference of 1V. 1eV = 1.6x10-19 J.
Magnetic Fields:
-> Perpendicular to velocity and field direction - causes charge to rotate around field lines. Moving charges = a current!
Electromagnetic Radiation
(Krane 3.1)Solution of Maxwell's Equations - electric and magnetic fields propagate together as an electromagnetic wave (demonstrated by Hertz, 1887).
Speed of light in vacuo: ![]()
Measured by Romer (moons of Jupiter), and Fizeau (cogs on wheel)
General Properties of Waves
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(i) Observer moving (
vO): changes perceived frequency or wave velocity(ii) Source moving (
vS): changes actual wavelength-> different results depending on who does the moving (try it!).
i.e. The wave-carrying medium defines the reference frame!
Classical (Galilean) Relativity
(Krane 2.1)Transforming between Inertial Frames:
Q. How do observers in different inertial frames relate measurements?
A. Principle of Relativity states that all physical laws are the same
(N.B. not just Newton's Laws can use the same thermometers & barometers too!)
BUT: coordinates of events different - we need a coordinate transformation.


Two observers at rest in their frame of reference, but moving relative to
each other with velocity u. Synchronize clocks and origins at
t=0, andmake the x-axis the direction of motion.
Galilean Transformation: ![]()
Consequences:
Velocities:
Accelerations:
-> Newton's Laws hold for both observers (as long as
u is constant).e.g. O' tosses an apple straight up: ![]()
O observes a parabolic trajectory: ![]()
but both agree that O' catches the apple.
See also this week's Homework (on the WWW, solutions next week!)