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Quantum Mechanics Lecture Notes for
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Contents 0 Introduction 8 0.1 Essen
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5.3.1 Harmonic Oscillators and Nucl
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List of Figures 1.1 Tangent field f
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List of Tables 3.1 Location of node
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exactly on paper and move on to dis
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- What is Quantum Mechanics?, Trans
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0.3 2003 Course Calendar This is a
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Chapter 1 Survey of Classical Mecha
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Taking time derivatives ˙x(t) =
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Since δ ˙x = dδx/dt and integrat
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The equations of motion are d ∂L
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This example also illustrates anoth
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Our goal is to write this Hamiltoni
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Now, let’s take a time average of
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Chapter 2 Waves and Wavefunctions I
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We can also use the |φ(k)〉 = |k
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0.75 0.5 0.25 -3 -2 -1 1 2 3 -0.25
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Figure 2.3: Go for fixed t as a fun
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Since ψ(x) must vanish at x = 0 an
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We will choose the coefficients c1
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symêasym 4 3 2 1 -1 -2 -3 -4 2 4 6
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1 0.95 T 0.9 0.85 10 En 20 30 -10 4
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Im@yD 4 2 0 -2 -4 -10 x 0 10 -5 0 F
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30 20 10 DOS Quantum well vs. 3d bo
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12 10 5 -5 -10 -15 -20 -25 8 6 4 2
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Exercise 2.4 Consider a particle wi
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Exercise 2.8 Consider the Hamiltoni
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Chapter 3 Semi-Classical Quantum Me
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for circular orbits, then the theor
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Substituting Eq. 3.17 into χ = ¯h
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If we make the approximation that
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where a and b are the turning point
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This gives us the transmission prob
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and the WKB wavefunction becomes:
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15 10 5 -5 -10 2 4 6 8 10 Figure 3.
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Thus, where we use the fact that y
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Thus, once we know χ(b) for a give
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Exercise 3.5 The impact parameter,
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We transform this into an integral
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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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- Page 173 and 174: To solve this equation, we first ha
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- Page 177 and 178: with and The closure, or idempotent
- Page 179 and 180: 6.10 Problems and Exercises Exercis
- Page 181 and 182: 2. Express the stationary states as
- Page 183 and 184: solve with some additional complexi
- Page 185 and 186: 7.2.1 Expansion of Energies in term
- Page 187 and 188: So that the time evolution of the s
- Page 189 and 190: Thus, |+〉 = |+ (0) 〉 − µE |
- Page 191 and 192: i.e. Likewise: where |ψ (1) n 〉
- Page 193 and 194: where e 2 = q 2 /4πɛo. Now, let
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- Page 197 and 198: = Escs(t) + � VsnAn(t)e −i/¯hE
- Page 199 and 200: In other words: We can also define
- Page 201 and 202: is the unperturbed (atomic) hamilto
- Page 203 and 204: atom acquires a time-dependent dipo
- Page 205 and 206: Thus, the integral we need to perfo
- Page 207 and 208: R HarbL 0.8 0.6 0.4 0.2 0.5 1 1.5 2
- Page 209 and 210: The number of atoms going from 2 to
- Page 211 and 212: = 4 ω 3 3 ¯hc3 e2 r 4πɛo 2 . (7
- Page 213 and 214: other. The tunneling rate can be es
- Page 215 and 216: where 1F1(a, b, z) is the Hypergeom
- Page 217 and 218: Integrating over the electronic deg
- Page 219 and 220: 3. At t = 0, the initial classical
- Page 221: where b = � (Fj(0) − Fi(0)) 2
- Page 225 and 226: These states obey analogous rules f
- Page 227 and 228: where the columns represent the par
- Page 229 and 230: The remaining two must be construct
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- Page 233 and 234: the J integral for the 1s1s configu
- Page 235 and 236: where the sum is over the nuclei an
- Page 237 and 238: where Sij is the overlap between th
- Page 239 and 240: Exercise 8.2 Verify the expressions
- Page 241 and 242: Appendix: Creation and Annihilation
- Page 243 and 244: 8.5 Problems and Exercises Exercise
- Page 245 and 246: Figure 8.4: Setup calculation dialo
- Page 247 and 248: Figure 8.5: HOMO-1, HOMO and LUMO f
- Page 249 and 250: Appendix A Physical Constants and C
- Page 251 and 252: Appendix B Mathematical Results and
- Page 253 and 254: Figure B.1: sin(xa)/πx representat
- Page 255 and 256: B.2 Coordinate systems In each case
- Page 257 and 258: B.2.3 Cylindrical x φ • Coordina
- Page 259: Ground-state Configuration Protacti