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2. Solving Schr

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Title: 2. Solving Schr


1
2. Solving Schrödingers Equation
Superposition
  • Given a few solutions of Schrödingers equation,
    we can make more of them
  • Let ?1 and ?2 be two solutions of Schrödingers
    equation
  • Let c1 and c2 be any pair of complex numbers
  • Then the following is also a solution of
    Schrödingers equation
  • We can generalize this to an arbitrary number of
    solutions
  • We can even generalize to a continuum of
    solutions

2
2A. The Free Schrödingers Equation
We know a lot of solutions
  • Consider the free Schrödinger equation
  • We know a lot of solutions of this equation
  • By combining these, we can make a lot more
    solutions
  • The function c(k) can be (almost) any function of
    k
  • This actually includes all possible solutions

The factor of (2?)3/2 is arbitrary and inserted
here for convenience. In 1D, it would be (2?)1/2
3
We can (in principle) always solve this problem
Goal Given ?(r,t 0) ?(r), find ?(r,t) when
no potential is present
  • Set t 0
  • This just says that c(k) is the Fourier transform
    of ?(r)
  • Substitute it in the formula above for ?(r,t) and
    we are done
  • Actually doing the integrals may be difficult

4
Sample Problem
A particle in one dimension with no potential has
wave function at t 0 given by What is the wave
function at arbitrary time?
  • Need 1D versions of these formulas

From Appendix Find c(k)
5
Sample Problem (2)
A particle in one dimension with no potential has
wave function at t 0 given by What is the wave
function at arbitrary time?
  • Now find ?(x,t)

6
2B. The Time Independent Schrödinger Eqn.
Separation of Variables
  • Suppose that the potential is independent of time
  • Conjecture solutions of the form
  • Substitute it in
  • Divide by ?(r)?(t)
  • Left side is independent of r
  • Right side is independent of t
  • Both sides are independent of both! Must be a
    constant. Call it E

7
Solving the time equation
  • The first equation is easy to solve
  • Integrate both sides
  • By comparison with e-i?t, we see that E ?? is
    the energy
  • Substitute it back in

8
The Time Independent Schrödinger Equation
  • Multiply the other equation by ?(r) again

The Strategy for solving
  • Given a potential V(r) independent of time, what
    is most general solution of Schrödingers
    time-dependent equation?
  • First, solve Schrödingers time-independent
    equation
  • You should find many solutions ?n(r) with
    different energies En
  • Now just multiply by the phase factor
  • Then take linear combinations
  • Later well learn how to find cn

9
Why is time-independent better?
  • Time-independent is one less variable
    significantly easier
  • It is a real equation (in this case), which is
    less hassle to solve
  • If in one dimension, it reduces to an ordinary
    differential equation
  • These are much easier to solve, especially
    numerically

10
2C. Probability current
Probability Conservation
  • Recall the probability density is
  • This can change as the wave function changes
  • Where does the probability go as it changes?
  • Does it flow just like electric charge does?
  • Want to show that the probability moves around
  • Ideally, show that it flows from place to place
  • A formula from E and M can we make it like this?
  • To make things easier, lets make all functions
    of space and time implicit, not write them

11
The derivation (1)
  • Start with Schrödingers equation
  • Multiply on the left by ?
  • Take complex conjugate of this equation
  • Subtract
  • Rewrite first term as a total derivative
  • Cancel a factor of i?
  • Left side is probability density

12
The derivation (2)
  • Consider the following expression
  • Use product rule on the divergence
  • Substitute this in above
  • Define the probability current j
  • Then we have

13
Why is it called probability current?
  • Integrate it over any volume V with surface S
  • Left side is P(r ? V)
  • Use Gausss law on right side
  • Change in probability is due to current flowing
    out

V
  • If the wave function falls off at infinity (as it
    must) and the volume V becomes all of space, we
    have

14
Calculating probability current
  • This expression is best when doing proofs
  • Note that you have a real number minus its
    complex conjugate
  • A quicker formula for calculation is
  • Lets find ? and j for a plane wave

15
Sample Problem
A particle in the 1D infinite square well has
wave function For the region 0 lt x lt a. Find ?
and j.
16
Sample Problem (2)
A particle in the 1D infinite square well has
wave function For the region 0 lt x lt a. Find ?
and j.
  • In 1D

17
Sample Problem (3)
A particle in the 1D infinite square well has
wave function For the region 0 lt x lt a. Find ?
and j.
  • After some work

18
2D. Reflection from a Step Boundary
The Case E gt V0 Solutions in Each Region
I
  • A particle with energy E impacts a step-function
    barrier from the left

incident
transmitted
reflected
II
  • Solve the equation in each of the regions
  • Assume E gt V0
  • Region I
  • Region II
  • Most general solution
  • A is incident wave
  • B is reflected wave
  • C is transmitted wave
  • D is incoming wave from the right set D 0

19
Step with E gt V0 The solution
I
incident
transmitted
reflected
  • Schrödingers equation second derivative finite
  • ?(x) and ?(x) must be continuous at x 0

II
  • We cant normalize wave functions
  • Use probability currents!

20
Summary Step with E gt V0
I
incident
transmitted
reflected
II
21
Step with E lt V0
  • What if V0 gt E?
  • Region I same as before
  • Region II we have

I
II
incident
reflected
evanescent
  • Most general solution
  • A is incident wave
  • B is reflected wave
  • C is damped evanescent wave
  • D is growing wave, cant be normalized
  • ?(x) and ?(x) must be continuous at x 0
  • No transmission since evanescent wave is damped

22
Step Potential All cases summarized
  • For V0 gt E, all is reflected
  • Note that it penetrates, a little bit into the
    classically forbidden region, x gt 0
  • This suggests if barrier had finite thickness,
    some of it would bet through
  • Reflection probability

23
2E. Quantum Tunneling
Setting Up the Problem
V(x)
  • Barrier of finite height and width

V0
  • Solve the equation in each of the regions
  • Particle impacts from left with E lt V0
  • General solution in all three regions

III
II
I
- d/2
d/2
x
  • Match ? and ? at x -d/2 and x d/2

Why didnt I include e-ikx in ?III? Why did I
skip letter E?
  • Solve for F in terms of A

24
Skip this Slide Solving for F in terms of A
  • Multiply 1 by ik and add to 2
  • Multiply 3 by ? and add to 4
  • Multiply 3 by ? and subtract 4
  • Multiply 5 by 2? and substitute from 6 and 7

25
Barrier Penetration Results
  • We want to know transmission probability
  • For thick barriers,
  • Exponential suppression of barrier penetration

26
Unbound and Bound State
  • For each of the following, we found solutions for
    any E
  • No potential
  • Step potential
  • Barrier
  • This is because we are dealing with unbound
    states, E gt V(??)
  • Our wave functions were, in each case, not
    normalizable
  • Fixable by making superpositions
  • We will now consider bounds states
  • These are when E lt V(??)
  • There will always only be discrete energy values
  • And they can be normalized
  • Usually easier to deal with real wave functions

27
2F. The Infinite Square Well
Finding the Modes
V(x)
  • Infinite potential implies wave function must
    vanish there
  • In the allowed region, Schrödingers equation is
    just

x
a
0
  • The solution to this is simple
  • Because potential is infinite, the derivative is
    not necessarily continuous
  • But wave functions must still be continuous

28
Normalizing Modes and Quantized Energies
  • We can normalize this wave function
  • Note that we only get discrete energies in this
    case
  • Note that we can normalize these
  • Most general solution is then

29
The 3D Infinite Square Well
  • In allowed region
  • Guess solution
  • Normalize it
  • This is product of 1D functions
  • Energy is
  • This is sum of 1D energies

c
b
a
30
2G. The Double Delta-Function Potential
Finding Bound States
V(x)
a/2
-a/2
I
III
II
  • First, write out Schrödingers Equation

x
  • Bound states have E lt V(?) 0
  • Within each region we have
  • General solution (deleting the parts that blow up
    at infinity)

31
Dealing with Delta Functions
V(x)
a/2
-a/2
I
III
II
  • To deal with the delta functions, integrate
    Schrödingers equation over a small region near
    the delta function
  • For example, near x a/2
  • Do first term on right by fundamental theorem of
    calculus
  • Do second term on right by using the delta
    functions
  • Take the limit ? ? 0
  • Left side small in this limit

32
Simplifying at x ½a
V(x)
a/2
-a/2
I
III
II
  • Since there is a finite discontinuity in ?, ?
    must be continuous at this boundary

On the right side of the equation above, is that
?I, ?II, or ?III?
  • Write these equation out explicitly
  • Substitute first into second

33
Repeating at x ½a
  • Repeat the steps we did, this time at x ½a
  • Note these equations are nearly identical
  • The only numbers equal to their reciprocal are ?1

34
Graphical Solution
  • Right side is two curves, left side is a straight
    line
  • Black line always crosses red curve, sometimes
    crosses green curve, depending on parameters
  • Sometimes two solutions, sometimes one
  • Normalize to finish the problem
  • Note one solution symmetric, one anti-symmetric
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