- Page 1 and 2: Quantum Mechanics Lecture Notes for
- Page 3 and 4: Contents 0 Introduction 8 0.1 Essen
- Page 5 and 6: 5.3.1 Harmonic Oscillators and Nucl
- Page 7 and 8: List of Figures 1.1 Tangent field f
- Page 9 and 10: List of Tables 3.1 Location of node
- Page 11 and 12: exactly on paper and move on to dis
- Page 13 and 14: - What is Quantum Mechanics?, Trans
- Page 15 and 16: 0.3 2003 Course Calendar This is a
- Page 17 and 18: Chapter 1 Survey of Classical Mecha
- Page 19 and 20: Taking time derivatives ˙x(t) =
- Page 21 and 22: Since δ ˙x = dδx/dt and integrat
- Page 23 and 24: The equations of motion are d ∂L
- Page 25 and 26: This example also illustrates anoth
- Page 27 and 28: Our goal is to write this Hamiltoni
- Page 29 and 30: Now, let’s take a time average of
- Page 31: Chapter 2 Waves and Wavefunctions I
- Page 35 and 36: 0.75 0.5 0.25 -3 -2 -1 1 2 3 -0.25
- Page 37 and 38: Figure 2.3: Go for fixed t as a fun
- Page 39 and 40: Since ψ(x) must vanish at x = 0 an
- Page 41 and 42: We will choose the coefficients c1
- Page 43 and 44: symêasym 4 3 2 1 -1 -2 -3 -4 2 4 6
- Page 45 and 46: 1 0.95 T 0.9 0.85 10 En 20 30 -10 4
- Page 47 and 48: Im@yD 4 2 0 -2 -4 -10 x 0 10 -5 0 F
- Page 49 and 50: 30 20 10 DOS Quantum well vs. 3d bo
- Page 51 and 52: 12 10 5 -5 -10 -15 -20 -25 8 6 4 2
- Page 53 and 54: Exercise 2.4 Consider a particle wi
- Page 55 and 56: Exercise 2.8 Consider the Hamiltoni
- Page 57 and 58: Chapter 3 Semi-Classical Quantum Me
- Page 59 and 60: for circular orbits, then the theor
- Page 61 and 62: Substituting Eq. 3.17 into χ = ¯h
- Page 63 and 64: If we make the approximation that
- Page 65 and 66: where a and b are the turning point
- Page 67 and 68: This gives us the transmission prob
- Page 69 and 70: and the WKB wavefunction becomes:
- Page 71 and 72: 15 10 5 -5 -10 2 4 6 8 10 Figure 3.
- Page 73 and 74: Thus, where we use the fact that y
- Page 75 and 76: Thus, once we know χ(b) for a give
- Page 77 and 78: Exercise 3.5 The impact parameter,
- Page 79 and 80: We transform this into an integral
- Page 81 and 82: 1. Assume that ψo and ψ1 are solu
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Figure 4.1: Gaussian distribution f
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Figure 4.3: Constructive and destru
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4.0.1 The description of a physical
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4.0.5 The Superposition Principle L
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Similarly for P2. Part of our job i
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Thus, Thus, Let’s see if ˆx and
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Now, we reinsert the definitions of
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Therefore, and 〈µ|a〉 = � 〈
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The matrix A is Hermitian if A = A
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Thus, we can show that F ( Â)|φa
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4.3 Bohr Frequency and Selection Ru
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We can also compute: 〈p 2 〉 =
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ack to the ground state or some low
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Solution: You can either do this th
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Exercise 4.8 For this section, cons
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For Domain 1 we have: For Domain 2
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and ∂y ′ ∂α = ∂η ∂x we
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the pivot point. In any case, the g
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5.2.3 Variational method applied to
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Thus, we can expand any state |ψ
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φo(x) = φo(x) = 1 φo(x) = � φ
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Since What happends if I do the sam
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eigenstate withe energy En − ¯h
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〈φm|p|φn〉 = i � mω¯h 2
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Since we know that a † acting on
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5.3.2 Classical interpretation. In
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Figure 5.4: Quantum and Classical P
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Figure 5.5: London-Eyring-Polanyi-S
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Figure 5.7: Model potential for pro
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5.4.2 Numerical Diagonalization A m
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Table 5.1 lists a the first few of
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V[x_] := a*(x^4 - x^2); cmm = 8064*
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1. Express the total Hamiltonian as
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Figure 5.10: Ammonia Inversion and
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(d) Since the ψL and ψR basis fun
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Bibliography [1] C. A. Parr and D.
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6.1 Quantum Theory of Rotations Let
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Which we can summarize as = i¯hLz
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Thus, L 2 = − 1 � 1 ∂ sin θ
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6.4 Eigenfunctions of L 2 The wavef
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For the case of m = 0, Yl0 = i l
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We can use this to write � Y ∗
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i.e. (x = cos θ) and satisfy Pl(x)
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When l is very large the sin 2 ((l
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Table 6.2: Relation between various
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To solve this equation, we first ha
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The proceedure is to substitute thi
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with and The closure, or idempotent
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6.10 Problems and Exercises Exercis
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2. Express the stationary states as
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solve with some additional complexi
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7.2.1 Expansion of Energies in term
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So that the time evolution of the s
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Thus, |+〉 = |+ (0) 〉 − µE |
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i.e. Likewise: where |ψ (1) n 〉
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where e 2 = q 2 /4πɛo. Now, let
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as the interaction between a dipole
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= Escs(t) + � VsnAn(t)e −i/¯hE
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In other words: We can also define
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is the unperturbed (atomic) hamilto
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atom acquires a time-dependent dipo
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Thus, the integral we need to perfo
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R HarbL 0.8 0.6 0.4 0.2 0.5 1 1.5 2
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The number of atoms going from 2 to
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= 4 ω 3 3 ¯hc3 e2 r 4πɛo 2 . (7
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other. The tunneling rate can be es
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where 1F1(a, b, z) is the Hypergeom
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Integrating over the electronic deg
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3. At t = 0, the initial classical
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where b = � (Fj(0) − Fi(0)) 2
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energy level for R = 1fm and compar
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These states obey analogous rules f
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where the columns represent the par
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The remaining two must be construct
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Not too bad, the actual result is
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the J integral for the 1s1s configu
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where the sum is over the nuclei an
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where Sij is the overlap between th
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Exercise 8.2 Verify the expressions
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Appendix: Creation and Annihilation
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8.5 Problems and Exercises Exercise
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Figure 8.4: Setup calculation dialo
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Figure 8.5: HOMO-1, HOMO and LUMO f
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Appendix A Physical Constants and C
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Appendix B Mathematical Results and
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Figure B.1: sin(xa)/πx representat
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B.2 Coordinate systems In each case
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B.2.3 Cylindrical x φ • Coordina
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Ground-state Configuration Protacti