rot.qm.3d.part1
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Angular momentum in classical physicsAngular momentum in classical physics
Consider a particle at the position r
i
k
j
rv
Where
r = ix + jy + kz
The velocity of this particle is given by
v = drdt = i
dxdt + j
dydt + k
dzdt
Classical Angular Momentum
Classical Angular MomentumThe linear momentum of the particle with mass m isgiven by
p = mv where e.i px = mvx = mdxdt
The angular momentum is defined as
L = rXp
L
L = r X p
Φ
| | | | r p sinΦ
r
p
The angular momentum is perpendicular to the plane .defined by r and p
Classical Angular Momentum
We have in addition
L = rXp = (ix +jy + kz)X (ipx + jpy +kpz)
L = (rypz -rzpy)i + (rzpx -rxpz)j + (rxpy - rypx)k
or
i j k
rXp = r x ry rz
px py pz
Classical Angular Momentum
Why are we interested in the angularmomentum ?
Consider the change of L with time
dLdt =
drdt Xp + rX
dpdt
dLdt = mvXv + rX
dpdt = rX
dpdt
dLdt = rX
ddt [m
drdt ] = mrX
d2rdt2
dLdt = mrXF F = force
r
F
Classical Angular Momentum
Examples :
movement of electron around nuclei movement of planets around sun
For such systems L is a constant of motion, e.g. doesnot change with time since
dLdt = 0
In quantum mechanics an operator O representing aconstant of motion will commute with the Hamiltonianwhich means that we can find eigenfunctions that areboth eigenfunctions to H and O
rF
Quantum mechanical representation of angular momentumQuantum mechanical representation of angular momentumoperatoroperatorWe have
L = rXp = iLx + jLy + kLz
where
Lx = rypz - rzpy ; Ly = rzpx - rxpy ; Lz = rxpy - rypx
In going to quantum mechanics we have
x --> x ; y --> y ; z --> z
px --> -ihδδx ; p y --> -ih
δδy ; p z --> -ih
δδz
:Thus
L x = -ih( yδδz - z
δδy ) ; L y = -ih( z
δδx - x
δδz )
L z = -ih( xδδy - y
δδx )
Rotation..Quantum Mechanics 3D
We have
L = iLx + jLy + kLz
thus
L.L = L2 =(iLx + jLy + kLz).(iLx + jLy + kLz)
L2 = Lx2 + Ly2 + Lz2
Rotation..Quantum Mechanics 3D
Can we find common eigenfunctions to
L2 , Lx , Ly , Lz ?
Only if all four operators commute
We must now look at the commutationrelations
The two operators L x and L y will
commute if
[L xL y - L yL x] f(x,y,z) = 0
Rotation..Quantum Mechanics 3D
Rotation..Quantum Mechanics 3D
We have
Lxf = -ih( yδfδz - z
δfδy ) = -ih ux
Ly = -f ih( zδfδx - x
δfδz ) = -ih uy
Next
LxLy = -f ih Lxuy
LxLy = -f ih [ -ih( yδuyδz - z
δuyδy ) ]
LxLy = -f h2 [ yδuyδz - z
δuyδy ]
We have
δuyδz =
δδz (z
δfδx - x
δfδz )
δuyδz =
δfδx + z
δ2fδzδx - x
δ2fδz2
Rotation..Quantum Mechanics 3D
Further
δ u
y
δ y
= δδy (z
δfδx - x
δfδz )
δuyδy = z
δ2fδyδx - x
δ2fδyδz
combining terms
Thus
LxLyf = -h2[ yδfδx + yz
δ2fδzδx - yx
δ2fδz2 - z2
δ2fδyδx +zx
δ2fδyδz ]
LxLy = -f h2[ yδfδx + yz
δ2fδzδx - yx
δ2fδz2 - z2
δ2fδyδx +zx
δ2fδyδz ]
It is clear that LxLy f can be evaluated by :interchanging x and y We get
LyLx = -f h2[ xδfδy + xz
δ2fδzδy - xy
δ2fδz2 - z2
δ2fδxδy +zy
δ2fδxδz ]
Rotation..Quantum Mechanics 3D
Rotation..Quantum Mechanics 3Dusing the relations
δ2fδzδy =
δ2fδyδz .etc
We have
[ LxL y - LyLx] = -f h2[ yδfδx - x
δfδy ] = -h2[ y
δδx - x
δδy ]
f
We have: Lz = -i h[ xδδy - y
δδx ]
Thus: [ LxLy - LyLx] f = ihLz f ; [Lx,Ly] = ihLz
We have shown [Lx,Ly] = ihLz
Rotation..Quantum Mechanics 3DBy a cyclic permutation
[ Ly,L z] = ihLx
[ Lz,Lx] = ihLy
We have shown that the three operators L x,L y,L zare non commuting
What about the commutation between Lx,Ly,Lz and L2
Y
Z X
X
Y
z
X
Yz
C3
Let us examine the commutation relation
between L2 and Lx
We have:
[ L2,Lx]=[Lx2 +Ly
2 +Lz2,Lx]
[ L2,Lx]=[Lx2,Lx]+[Ly
2,Lx]+[Lz2,Lx]
[Lx2,Lx]=Lx
2Lx −LxLx2 =Lx
3 −Lx3 =0
For the first term
Rotation..Quantum Mechanics 3D
For the second termRotation..Quantum Mechanics 3D
[Ly2,Lx]=Ly
2Lx −LxLy2
=Ly2Lx −LyLxLy +LyLxLy −LxLy
2
=Ly[LyLx −LxLy]+[LyLx −LxLy]Ly
=−ihLyLz −ihLzLy
Y
Z X
For the third termRotation..Quantum Mechanics 3D
[Lz2,Lx]=Lz
2Lx −LxLz2
=Lz2Lx −LzLxLz +LzLxLz −LxLz
2
=Lz[LzLx −LxLz]−[LzLx −LxLz]Lz
=ihLzLy +hLyLz
Y
Z X
[ L2,Lx]=[Lx2 +Ly
2 +Lz2,Lx]
Rotation..Quantum Mechanics 3D
In total
−ihLyLz −ihLzLy=0 +ihLzLy +hLyLz =0
Y
Z X
We have shown[L2,Lx] = [Lx2+Ly2+Lz2,Lx] = O
now by cyclic permutation
[Ly2+Lz2+Lx2,Ly] = [L2,Ly] = 0
[Lz2+Lx2+Ly2,Lz] = [L2,Lz] = 0
Thus Lx,Ly,Lz all commutes with L 2
and we can find common eigenfunctions for
L2 and Lx or L 2 and Ly or L 2 and Lz
the normal convention is to obtain eigenfunctions that areat the same time eigenfunctions to Lz and L2.
How do we find the eigenfunctions ?
Y
Z XRotation..Quantum Mechanics 3D
How do we find the eigenfunctions ?
The eigenfunctions f must satisfy
Lzf = af and L 2f = bf
The function f must in other wordssatisfy the differential equations
Lzf = af
as well as
L2f = bf
Rotation..Quantum Mechanics 3D
It is more convenient to solve the equations in
spherical coordinates
Θ
φ
r
(x,y,z)→
(r, Θ,φ )
We find after some tedious but straight forward
manipulations
Lz = -ih [ddφ
]
L2 = -h2[ d2
dΘ2 +cotΘ
d dΘ
+ 1
sin2Θ d2
dφ2 ]
Rotation..Quantum Mechanics 3D
We must now solve
L̂ zY(Θ,φ) = (b YΘ, φ )
and
L̂ 2 (Y Θ,φ) = (c YΘ, φ )
First let us solve
L̂ z (Y Θ , φ ) = -ihδδφ Y(Θ, φ ) = b Y(Θ, φ )
We shall try a solution of the form
Y(Θ, φ ) = S( Θ)T( φ )
as L̂ z only depends on φ
Rotation..Quantum Mechanics 3D
Rotation..Quantum Mechanics 3DWe have
-ihδδφ S(Θ)T(φ) = b S( Θ)T(φ)
or
- ihS(Θ)δ
δφ T(φ)= b S( Θ)T(φ)
multiplying with 1/ S( Θ) from left
δT(φ)
δφ =
ib
hT(φ)
The general solution is
T(φ) = AExp[
ib
hφ]
A general point in 3-D space is given by ( r,Θ, φ)
Θ
φ
r
( , , )x y z → ( ,r Θ,φ )
X
Y
ZrcosΘ
rsinΘ
We have the following relation = x rsinΘ cosφ = y rsinΘ sinφ = z rcosΘ
( ,The same point is represented by rΘ,φ+2π)
We must thus have
Exp[
ibh
φ] = Exp[
ibh
(φ+2π) = Exp[
ibh
φ] Exp[
ibh
2π]
A general point in 3-D space is given by ( r,Θ, φ)
Θ
φ
r
( , , )x y z → ( ,r Θ,φ )
X
Y
ZrcosΘ
rsinΘ
We have the following relation = x rsinΘ cosφ = y rsinΘ sinφ = z rcosΘ
( ,The same point is represented by rΘ,φ+2π)
We must thus have
Exp[
ibh
φ] = Exp[
ibh
(φ+2π) = Exp[
ibh
φ] Exp[
ibh
2π]