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CHEM 1301 | Introduction to Quantum Mechanics
Principles of CM
Classical mechanics describes how objects such as particles and waves behaves
It describes motion, position, velocity, mass, energy, acceleration etc. of the particle
Basic
Quantity Symbol Definition SI Unit
Position x m
Time t s
Mass m kg
Δ x x 1−x 2 d x
Velocity v v= = = = ẋ ms-1
Δ t t 1−t 2 d t
dv
Acceleration a a= = ẍ ms-2
dt
Momentum p p=mv=m ẋ m kg s-1
p2 1
Derived
2
Kinetic energy T T= = mv m2 kg s-2 = J
2m 2
Potential energy V J
Total energy E E=T +V J
−d v
Force F F= m kg s-2 = N
dx
Note: velocity, acceleration, momentum and force are vectors (both magnitude and
direction)
Force = rate of change of potential energy with position
A free particle refers to a particle which has no force acting upon it and is neither
accelerating nor decelerating
Thus, T > 0 (V = 0 or constant)
Harmonic Oscillator (spring)
1 2 p2
V x = Dx T=
( )
2 2m
0 x
Where D = spring constant (the larger the D, the stiffer the spring)
Object is moving the fastest at x = 0 (V=0 and E=T)
At extreme ends of the curve, T=0
−d v −d 1
F=
dx
=
dx 2 ( )
D x 2 =−Dx (Hooke’s Law)
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Newton’s Laws of Motion
1. A particle moves with constant velocity unless acted upon by a force
(If F=0, a=0, V is constant)
2. If acted upon by a force, a particle will change velocity (or momentum) (i.e.
accelerate)
(F = ma or F = dp/dt since p = mv and a = dv/dt)
Equations of Motion (EOM)
Describes the trajectory of particles (i.e. the position as time changes)
Solving the EOM gives the position of the particle after a time t
dp
Momentum ṗ= =F which when integrated gives p(t)
dt
dx p
Position ẋ= = which when integrated gives x(t)
dt m
Can be solved given suitable initial / boundary conditions
Free particle
Velocity is constant, so p = constant and dp/dt = 0 and dx/dt = p/m = constant
Let the initial conditions be p(t=0)=p0 and x(t=0)=x0
p0 t p
From EOM, p ( t ) =p 0 x ( t ) =x0 + (by integrating∫ dx=∫ dt )
m m
Harmonic Oscillator
Solutions are p ( t ) =−p 0 sin ( ωt ) x ( t )=x 0 cos (ωt)
D
Initial conditions: p0 = 0 and x0 where ω=
√ m
Wave Mechanics
Waves have wavelength which has period T
A wave can be described by the 2nd order partial differential equation wave equation
∂2 y 2
2 ∂ y
−c =0
∂ t2 ∂ x2
A general solution can be obtained by setting initial conditions (x0,y0) giving
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ω
y ( t ) = y 0 cos ( kx−ωt ) if c=
k
Important Equations
2 π where = wavelength
Wave vector k =
❑
2π
Angular frequency ω= where T = vibrational period
T
ω
Wave velocity c=
k
dx ωt
Since c= then x=
dt k
Direction of waves
y ( t ) = y 0 cos ( kx−ωt ) (travelling right)
y ( t ) = y 0 cos (−kx−ωt ) (travelling left)
Standing Waves
y ( t ) = y 0 [cos ( kx−ωt ) +cos (−kx−ωt ) ]=2 y 0 cos ( ωt ) cos (kx )
When cos(kx) = 0, there will be nodes (i.e. y = 0) for all values of t
❑
Nodes will be at (n+1)
2 where n = 0, +1, +2, ...
Standing Waves in Boxes
Boundary conditions are y(0) = 0 and y(L) = 0 (zero at both ends of the box)
Interference
Waves an constructively (in-phase) and destructively (out-of-phase) interfere and
may also be diffracted
The energy of the wave is proportional to its amplitude
Failure of CM
Black Body Radiation