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Quantum Mechanics and Atomic Physics

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Title: Quantum Mechanics and Atomic Physics


1
Quantum Mechanics and Atomic Physics
  • Lecture 14
  • Angular Momentum Operators
  • http//www.physics.rutgers.edu/ugrad/361
  • Prof. Eva Halkiadakis

2
Last time
  • Solved for S.E. in 3D using particle in a box
    example
  • Using separation of variables we found that the
    total wavefunction is
  • Quantization of energy is
  • And found that energy degeneracy increases with
    energy

3
Spherical Coordinates
  • One of our goals is to solve S.E. in 3D for the
    Coulomb potential (1/r) which describes the
    hydrogen atom (next week)
  • To do this we need to use spherical coordinates

Reed Chapter 6
4
Angular Momentum
  • Recall that angular momentum is
  • It can be easily shown that in Cartesian
    coordinates

Note No x appears in Lx, No y appears in
Ly, And no z appears in Lz.
5
Commutators of x,y,z components of L
  • For example

6
(No Transcript)
7
What does this mean?
  • The components of L do not commute with each
    other!
  • No simultaneous eigenstates!
  • If you measure Lx ? get a certain value
  • Next, measure Ly ? get a certain value
  • Measure Lx again ? in general, you wont get the
    same value as before!
  • We will revisit this in Chapter 8

8
L operator in spherical coordinates
9
Now the x,y,z components in spherical coordinates
  • First the z component

10
  • Similarly,
  • I leave it for you as an exercise to derive these
  • Later, we will need to use the expression for Lz

11
What about important quantity Lop2 ?
12
Lets relate this to the Hamiltonian
13
Central Potentials V( r )
  • The S.E. for a particle of mass ? moving in a
    central potential V( r)
  • Ive replaced m with ???to not be confused with
    new variable I will introduce shortly ml, and in
    reality it should be expressed as the reduced
    mass ??
  • Again, lets use separation of variables, like we
    did last time

14
  • Some things to note about this equation

15
Separation of variables
  • (we will come back to this equation)
  • Lets call the constant

16
  • Lets rewrite the RHS

So, full wavefunction is ?(r,???) R(
r)????????
17
  • Lets call the constant (-ml2)
  • We will discover later that this is called the
    mangetic quantum number

18
Solutions to ????
You will see later that we dont need the e-im?
term
19
  • Single-valuedness requires that
  • We find that the mangnetic quantum number is
    quantized!

? is cyclic
20
Lets go back to separated S.E.
  • RHS depends on ?
  • LHS depends on r
  • Equal to a constant
  • Lets call it l(l1) . Which is also equal to
    what weve been calling ?!

21
  • Solutions to ????
  • They are associated Legendre Polynomials (see
    Chapter 6 for full expression)
  • A few of them are
  • Note special cases of ml0 are called Regular
    Legendre Polynomials

22
Spherical Harmonics
  • We usually deal with a combined angular
    dependence
  • Y(?????????????
  • These are called Spherical Harmonics (see Chapter
    6 for full expression)
  • And is l called the orbital angular momentum
    quantum number

23
Radial Solutions
  • Solutions to R( r), depend on the potential
    energy
  • We will revisit this next week

24
Lets go back to
  • Recall

25
Total angular momentum is quantized!
26
What about Lz?
  • So, solutions exist only if l is an integer and l
    ml

27
Space Quantization
  • The magnetic quantum number ml expresses the
    quantization of direction of L
  • So L can assume only certain angles, given above,
    with respect to the z-axis.
  • This is called space quantization.

28
Example
  • For a particle with l2, what are the possible
    angels that L can make with the z-axis?

29
Plot of Spherical harmonics
  • 3D plots of
  • ? is vertically up
  • Independent of ?
  • So rotationally symmetric around z-axis
  • We will see later these will manifest themselves
    as the probability distributions

30
Summary/Announcements
  • Next time Central Potentials
  • Next homework due on Monday Oct 27.
  • You will have a quiz next week on Wed!
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