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Chapter
2
Time-independentSchrödinger
EquationStationary
States
24The
infinite
Square
well
30The
Harmonic
Oscillator
40The
Free
Particle
59The
Delta-Function
Potential
68The
Finite
Square
Well
782.1
Stationary
StatesHow
to
get
wave
function?To
solve
the
Schrödinger
Equationwhere
V
is
a
specified
potential
and
independent
of
t.In
this
case
the
Schrödinger
Equation
can
be
solved
bythe
method
of
separation
of
variables,
looking
forthefollowing
solutions:Substituting
above
equations
into
the
Schrödinger
Equation:and,
dividing
through
bySeparation
of
variables
has
turned
a
partial
differentialequation
into
two
ordinary
differential
equations.②①Called
time-independentSchrödinger
Equation.The
rest
of
this
chapter
will
be
devoted
to
solving
the
time-independent
Schrödinger
Equation,
for
a
variety
of
simplepotentials.What
are
the
solutions
and
why
the
solutions
of
time-independent
Schrödinger
Equation
is
so
important.Three
properties
of
the
solutions:①:②:(1)
They
are
stationary
states.solutions:The
probability
density
is
time-independent.Every
expectation
value
is
constant
in
time.(2)
They
are
states
of
definite
total
energyIn
classical
mechanics,
the
total
energy
(kinetic
andpotential
energy)
is
called
the
Hamiltonian:Conclusion:A
separable
solution
has
the
property
that
everymeasurement
of
the
total
energy
is
certain
to
return
thevalue
E.(3)
The
general
solution
is
a
linear
combination
of
separablesolutions.A
more
general
solution
can
be
constructed
by
alinear
combination:Determine
the
constantsc
to
match
the
specifiedinitial
conditions:Example
2.1:2.2
The
Infinite
Square
WellOutside
the
well:Inside
the
well:whereSimple
harmonicoscillator
equationSolutionBoundary
conditions:
Both
and are
continuous.But
if
the
potentialgoes
toinfinity,
only
the
is
continuous.
(2.5)Boundary
points:0and
aAt
point
a:Discrete
energyTo
find
A,
using
the
normalization
condition:Phase
has
no
physical
significancen
=
3n
=
2n
=
10x0xGround
stateExcited
statesThe
functions have
some
interesting
andimportant
properties:They
are
alternately
even
and
odd,
with
respect
to
the
center
ofthe
well:
ψ1
is
even,
ψ2
is
odd,
ψ3
is
even,
and
so
on.Each
successive
state
has
one
more
node:
ψ1
has
0,
ψ2
has
one,
ψ3
has
two,
and
so
on.(3).
They
are
mutually
orthogonal,
in
the
sense
thatKronecker
deltaare
orthonormal.Proof:
see
the
book
as
a
homework.(4).
They
are
complete,
in
the
sense
that
any
other
function
cabe
expressed
as
a
linear
combination
of
them:Fourier
’s
seriesThe
stationary
states
of
the
infinite
square
well
areThe
most
general
states
of
the
infinite
square
well
arewhere
theyield
the
value
Enis
the
probability
that
a
measurement
of
the
energyThereforeThe
expectation
value
of
the
energy
must
beProof:Which
is
independent
of
time,
and
is
manifestation
of
conservation
of
E2.3
The
Harmonic
OscillatorClassical
harmonic
oscillator:mxkoThe
motion
is
governed
by
Hooke’s
Law:The
solution:The
potential
energy:Of
course,
there’s
no
perfect
harmonic
potential,
but
practically
anypotential
is
approximately
parabolic,
that
isWhich
describes
simple
harmonic
oscillation
aboutthe
point
x0,
with
aneffective
spring
constant
k=V”
(x0)
.Therefore
any
oscillatorymotion
is
approximately
simple
harmonic,
aslong
as
the
amplitude
is
small.The
quantum
problem
is
to
solve
the
Schrödinger
Equation
for
thepotentialTwo
approaches:Power
series
methodAlgebraic
technique:
using
ladder
operators2.3.1
Algebraic
MethodRewrite
Equation
:We
define
:Then
:Commutator
of
x
andpIn
general,
the
commutator
of
operators
A
and
B
is
defined
by?That
is:Canonical
commutation
relationSimilarly:Then
:(1)
IfTherefore
the
operators
a-
and
a+
are
called
ladder
operators.Raising
operatorLowering
operatorLowest
rungDetermineground
stateDifferential
equation:Determine
A:
normalizeSoGround
statewhere
An
is
the
normalization
constant.Therefore,
we
haveDetermine
A1
by
normalizingBut
the
method
to
determine
An
by
normalizing
is
so
difficult!To
develop
an
algebraic
method
to
find
AnExample2.4:We
suppose
thatFor
any
functions
f(x)
and
g(x)Proof:In
particular:(1):(2):
SimilarlyHenceThusThe
stationary
state
of
theharmonic
oscillator
areorthogonalExample2.5:
Find
the
expectation
value
of
the
potential
energy
in
the
nthstate
of
the
harmonic
oscillator.Solution:Evaluating
the
integral
!2.3.2
Analytic
MethodWe
return
to
the
Schrödinger
Equation
of
the
harmonic
oscillatorSolveit
directly
by
series
method:First,
we
introduce
a
dimensionless
variable:Then
the
equation
reads:where
K
is
the
energy,
in
unit
of:Approximation
solution:
whenAsSoTherefore,
we
suppose
the
form
of
the
solution
iswhere
we
supposeis
a
power
series
inSubstituting
above
solution
into
the
differential
equation,
we
haveSecond,
we
look
forby
series
method,
in
whichis
a
power
series
in,
that
isWe
have
thefollowing
equations:Putting
above
equations
intoWe
findItfollowsthat
the
coefficient
of
each
power
ofmust
be
zero.And
henceThis
is
a
recursion
formulawhich
can
generates
allcoefficients.(1)
Generates
the
even-numbered
coefficient
from
a0Then
we
have:(2)
Generates
the
odd-numbered
coefficient
from
a1TwoarbitraryconstantAnalysis
of
the
solution:Question:
If
the
sum
is
infinite
series?If
j
is
large
enough,
that
isThe
approximate
solution
will
be:Above
asymptotic
solution
is
not
the
physical
one
which
will
be
infinite
asTherefore
j
will
not
be
so
large,
that
is
the
power
series
must
terminateat
certain
value
j=n.Analysis
of
the
solution:Above
conditionrequiresthatThereforeQuantization
of
energy:For
allowed
values
of
K,
the
recursion
formula
readsFor
certain
n,
we
consider
the
solutions:(1)
For
n=0(2)
For
n=1(3)
For
n=2Conclusion
of:Hermite
polynomials
:By
tradition,
an
arbitrary
multiplicative
factor
is
chosen
forthe
coefficient
of
the
highest
power
of
is
2n,
that
isso
thaNormalize
to
determine
CnFigure
of
solutions-3
-2
-1
0
1
2
3E0
E1E2n
=
0n
=
1n
=
22-4
-24|10|2Example
2.1Problem
2.1Problem
2.2Example
2.2normalizing:the
nth
coefficient:wave
function
attimet:conservation
of
energy:Example
2.3Problem
2.3Problem
2.4Problem
2.5(homework)Problem
2.6(homework)Problem
2.7Problem
2.8
?Problem
2.9Example
2.5Problem
2.10Problem
2.11Problem
2.12Problem
2.13Problem
2.14Problem
2.15Problem
2.16Problem
2.172.4
The
Free
ParticlewhereThe
general
solution
of
above
equation
can
be
written
in
exponentialform:everywhereAbove
function
represents
a
combination
of
two
waves:Represents
a
wave
traveling
positive
in
the
x-directionRepresents
a
wave
traveling
in
the
negative
x-directionWe
can
cover
all
the
above
waves
by
letting
k
run
from
negative
to
positive:traveling
to
the
rigwheretraveling
to
the
lefSolution
whenk
is
fixed:The
“stationary
states”
of
the
free
particle
are
propagating
waves.The
wave
length
is:The
speed
of
these
waves
is
:The
classical
speed
of
a
free
particle
with
energyis1.
Properties
of
the
Solution
of
free
particle(1)
Normalization
of
separable
solution
with
certain
k
:This
wave
function
is
not
normalizable.That
means
the
separable
solutions
do
not
represent
physicalrealizable
states.
A
free
particle
cannot
in
a
stationarystate;
or,toput
it
in
another
way,
there
is
no
such
thing
as
a
free
particle
with
adefinite
energy.(2)
General
solution:As
a
free
particle can
carry
any
energy,
that
means
k
can
takecontinues
values.
Therefore
the
sum
of
the
separable
solutionsshould
be
replaced
by
integral
of
k.The
final
general
solution
of
a
free
particle:The
final
solution
of
a
free
particle
is
a
wave
packet
which
is
asuperposition
of
propagating
waves.
If
we
choose
proper
Φ(k)
,
thewave
function
can
be
normalized!Question:Plancherel’s
theorem:Inverse
Fouriertransformation
of
F(k)Fourier
transformation
of
f(x)Generic
quantum
problem:ThereforeExample
2.6:Solution:(1)
Normalization
to
determine
A:(2)
Calculate:(3)
Calculate:The
integral
can
not
be
solved
in
terms
of
elementary
functions,
thoughit
can
be
evaluated
numerically.(3)
DiscussionWhen
a<<1:When
a>>1:2.
Paradox:
speed
(phase
velocity
and
group
velocity)A
realphysicalstate
is
a
wave
packet
which
is
a
superposition
ofOn
sinusoidal
state
,
we
haveHow
to
determine
the
group
velocity
of
any
wave
packet
?as
a
function
of
,Generally,
dispersion
relation
is
a
formula
forthat
is
.For
example,
for a
wave
packet
of
free
particle:where
is
a
dispersion
relation.For
anywave
packet:(1)
Let
us
assume
thatvalue
.is
a
narrowly
peaked
about
some
particularor(2)
Changing
variables
fromto,
we
haveAt
t=0At
tThe
total
wave
packet
evidently
moves
along
x
at
a
speedthat
is
actuallythe
group
velocity
of
whole
wave
packet:,In
our
case
offree
particle:the
group
velocity:the
phase
velocity:Example
2.6Phase
velocity
and
group
velocityProblem
2.18Problem
2.19Problem
2.20(homework)Problem
2.21Problem
2.22(homework)2.5
The
Delta-Function
Potential2.5.1
Bound
states
and
scattering
statesDifferent
potentials:Infinite
square
wellHarmonic
oscillatorsolutionsFreeparticleNormalizableDiscrete
nNon-normalizableContinuous
kTwo
different
solutionsSumIntegralRead
book
!Properties
of
Delta-function:2.5.1
The
Delta-Function
Well1.
Delta-Function:2.
A
potential
of
Delta-Function:A
well
potential
of
Delta-Function:(1)
Bound
statesIn
the
region
x<0,
V(x)=0,
soThe
general
solution
to
above
equation
isAsThereforeIn
the
regionx>0,
V(x)=0,
so
Stitch
these
two
functions
togetherby
using
theboundary
conditions
as
folderivativeNow
we
use
it:The
first
condition:
the
function
is
continuous
at
any
pointThen,
we
haveThe
second
condition:
the
derivative
of
function
is
continuous
exceptis
not
continuous
at
point
x=0Generally,
integrate
the
Schrödinger
EquationIf
we
setIfWe
haveBy
using
it
on
delta-potentialThereforeThe
allowed
energy
is:NormalizationAtlast,
the
bound-state
solution
isone
bound-state
solution(2)
Scattering
statesIn
the
region
x<0,
V(x)=0,
soThe
general
solution
to
above
equation
isSimilarly,
in
the
region
x>0,
V(x)=0,
soStitch
these
two
functions
together
at
x=0
by
using
the
boundary
conditiThe
continuity
of
at
x=0
requires
thatThe
second
condition:
the
derivative
of
function
is
continuous
exceIntegrate
the
Schrödinger
EquationUnknown
variable:Two
equations,
and
the
scattering
states
can
not
be
normalized.How
to
determine
the
5
unknown
variablesIn
a
realizable
scattering
experiment,particles
are
fired
in
from
onedirection.
Here
we
suppose
a
leftcoming.Therefore:is
the
amplitude
of
the
incident
wave.is
the
amplitude
of
the
reflected
wave.is
the
amplitude
of
the
transmitted
wave.By
usingWe
findReflection
rate
and
transmission
rate:
R
and
TThe
probability
that
an
incident
particlewillbereflected
back
is
defined
byReflectioncoefficientMeanwhile,
the
probability
that
an
incidentparticle
will
be
transmitted
is
defined
byTransmissioncoefficientA
barrier
potential
of
Delta-Function:Read
the
book:2.6
The
Finite
Square
WellFinite
square
well:Bound-state
Solutions:
E<0In
the
region
of
:Or
:Where(1)(2)
In
the
region
of:Or
:WhereAsThe
general
solution
is(2)(3)
In
the
region
of:Or
:Where(3)Symmetric
problem:The
advantage
of
the
symmetry
is
that
we
need
only
imposethe
boundary
conditions
on
one
side
(say,
at
+a);
the
otherside(say,
at
–a)
is
then
automatically
satisfied.Even
solutions(Or
odd
solutions)Therefore
the
following
form
ofsolutionis
looking
forEven
solutionsIf
E
can
be
determined,
then
the
k
and
l
will
be
obtained,
and
the
wavefunction
will
be
plotted.EQuantum
m
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