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This course focuses on 1-Dimensional Waves. Key points of this lecture are: Schrodinger Wave Equation, Wave Function, Eigenstates and Energy Eigenvalues, Ket Notation, Dispersion Relation, Phase Velocity, Time Dependent Schrƶdinger Equation, Energy Eigenvalue Equation, Eigenstates
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Schrƶdinger Wave Equation
Ė H Ļ ( x , t ) = i ļØ
āĻ ( x , t )
ā t
(both images from
Wikipedia.com)
Schrƶdinger Wave Equation
Ė H Ļ ( x , t ) = i ļØ
āĻ ( x , t )
ā t
Schrƶdinger Wave Equation:
More-or-less āgod-givenā, just like Newtonās law F(x) = d p /d t.
It works, and if we can show that it fails, weāll refine or discard.
You learned in PH425 that the solution to the time-dependent SE is,
in terms of the eigenstates of the Hamiltonian:
Ļ (^) ( x , t ) = Ļ
n
n
ā ( x ) e
ā iE n
t / ļØ
Ļ (^) ( t ) = Ļ n
ā iE n
t / ļØ
n
ā
n
n
n
n
( x ) =^ E n
n
( x )
where
where
Notice the parallels to the rope problem we solved last week?
Schrƶdinger Wave Equation
Ļ ( x , t ) = c n
( t )Ļ n
( x )
n
ā
What follows is cast in terms of wave functions to give you
practice, but in fact the ket notation can be used just as easily.
The ket version of this discussion is in your text (Ch. 3) and
was discussed in PH425.
Expand wave function in energy basis; time dependence
comes from coefficients:
Substitute
Ė H Ļ ( x , t ) = i ļØ
āĻ ( x , t )
ā t
Ė H c n
( t )Ļ n
( x )
n
ā
= i ļØ
ā
ā t
c n
( t )^ Ļ n
( x )
n
ā
c n
( t ) E n
Ļ n
( x )
n
ā
= i ļØ
ā
ā t
c n
( t )^ Ļ n
( x )
n
ā
Schrƶdinger Wave Equation
Ļ ( x , t ) = c n
( t )^ Ļ n
( x )
n
ā
Expand wave function in energy basis; time dependence
comes from coefficients:
Substitute
c n
( t ) E n
Ļ n
( x )
n
ā
= i ļØ
ā
ā t
c n
( t )Ļ n
( x )
n
ā
ā
iE n
ļØ
ā
ā
ā
ā
ā
ā
c n
( t )Ļ n
( x ) =
ā c n
( t )
ā t
Ļ n
( x )
c n
( t ) =^ e
ā
iE n
ļØ
t
Ļ ( x , t ) = e
ā
iE n
ļØ
t
Ļ n
( x )
n
ā
Schrƶdinger Wave Equation
There are usually many functions that
solve the eigenvalue problem, each
function with its own associated
eigenvalue. Label them with index n.
n
( x ) = E n
n
( x )
Ė H Ļ n
= E n
Ļ n
ĪØ( x , t ) = Ļ n
( x ) Ae
ā i
E n
ļØ
t
n
ā
In general, the state of particle is NOT an eigenstate of the
Hamiltonian, but a superposition of eigenstates ā¦
Very important that the energy in the exponent
matches the corresponding eigenstate.
Schrƶdinger Wave Equation
Example: V ( x ) = 0 (free particle)
n
( x ) = E n
n
( x )
Ļ( x ) = C ' e
i
2 mE
ļØ
x
ā i
2 mE
ļØ
x
1st term is traveling wave (to right) and 2nd is traveling to
left. Same eigenvalue E - ādegenerateā
ā
ļØ
2
2 m
d
2
Ļ( x )
dx
2
= E Ļ( x )
Ļ ( x , t ) = C ' e
i
2 mE
ļØ
x ā
E
ļØ
t
ā
ā
ā
ā
ā
ā
ā i
2 mE
ļØ
x +
E
ļØ
t
ā
ā
ā
ā
ā
ā
Schrƶdinger Wave Equation
Now solve the TISE for different potentials and find
examples where there are many solutions with different
energies
-a a ā x
ā
Energy
0
V 0
E
V (^) ( x ) =
V 0
x > a
0 x < a
ā§
āØ
āŖ
ā©
āŖ
Schrƶdinger Wave Equation
Schrƶdinger Wave Equation
What shall we call the separation constant?
T ( t )
T ( t )
T ( t )
Schrƶdinger Wave Equation
Eigenvalue problem! Solutions (and there
are many in general) depend on particular
V ( x ). E represents the energy of a particle
in that particular eigenstate, and there are
many E values.
= ā i
T ( t )
T ( t ) = Ae
ā i
E
ļØ
t
T ( t ) = Ae
ā i Ļ t
Most general solution is:
n
n
ā iE n
t / ļØ