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PHYS 30101 Quantum Mechanics PHYS 30101 Quantum Mechanics Dr Jon Billowes Nuclear Physics Group (Schuster Building, room 4.10)

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Presentation on theme: "PHYS 30101 Quantum Mechanics PHYS 30101 Quantum Mechanics Dr Jon Billowes Nuclear Physics Group (Schuster Building, room 4.10)"— Presentation transcript:

1 PHYS 30101 Quantum Mechanics PHYS 30101 Quantum Mechanics Dr Jon Billowes Nuclear Physics Group (Schuster Building, room 4.10) j.billowes@manchester.ac.uk These slides at: www.man.ac.uk/dalton/phys30101 Lecture 3

2 Plan of action 1.Basics of QM 2.1D QM Will be covered in the following order: 1.1 Some light revision and reminders. Infinite well 1.2 TISE applied to finite wells 1.3 TISE applied to barriers – tunnelling phenomena 1.4 Postulates of QM (i) What Ψ represents (ii) Hermitian operators for dynamical variables (iii) Operators for position, momentum, ang. Mom. (iv) Result of measurement 1.5 Commutators, compatibility, uncertainty principle 1.6 Time-dependence of Ψ

3 Re-cap: Wavefunctions for a bound particle in a finite well (1-D) V0V0 V=0 E Two types of solution: Cosine-like tan ka = μ/k Sine-like cot ka = -μ/k exp(-μx)

4 Finite square well: solutions for tan ka = μ/k where thus In graph below, y = ka

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6 Compare with wavefunctions for an infinite square well: n=3 n=2 n=1

7 Useful formulae TDSE – time dependent Schrödinger Equation TISE – time independent S.E. Vector operators in spherical polar coordinates Angular momentum operators in spherical polars

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9 1.3 QM tunnelling through a barrier A e ikx B e -ikx F e ikx V=0 V=V 0 Consider a flux of particles, momentum ħk, energy E= ħ 2 k 2 /2m approaching a barrier, height V 0 (V 0 > E), width a. 0a x We assume that some flux emerges on the far side…


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