Modern Introductory Physics Part II — Daily Schedule Term 5
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See also Daily Schedule-Term 4
Week 8 — Continue Wave Functions
- Tuesday, Mar. 12 — Finish Q9 and start Q10 — Study Moore through p. 154 — Sx , Sy , and Sz cannot be simultaneously specified — Position and momentum cannot be simultaneously specified! — The momentum operator in position space (one of the brilliant leaps of de Broglie and Schrödinger) — Review of a couple super-useful integral calculus techniques: changes of variables in integrals (nowadays, people are calling this “u-substitution”) and integration by parts — The Heisenberg Uncertainty Principle (a long and important supplement that rigorously states what Moore only briefly states in Section Q9.4) — Problem Set 10 for Tuesday
- Friday, Mar. 15 — Finish Q10 (except save Q10.4 until Tuesday, Mar. 19) — Presentations: Brian, The time-independent Schrödinger Equation; Hexi, Ethan, and Miles, Building a simple oscillator out of the 0th and 1st harmonic oscillator wave functions introduced in Section Q10.5; Emma and Trey, The fundamental quantum mechanics behind lasers — Course feedback discussion — Debate and decision of what we will do in weeks 11-14 (it was decided that we will do more quantum mechanics and nuclear physics, rather than switching to special relativity) — Problem Set 11 for Friday
Week 9 — Observed Properties of the Hydrogen Atom, Atomic Spectra, and the Schrödinger Equation
- Tuesday, Mar. 19 — Q10.4 and Q11.1 to Q11.5 — Presentations: Brian, The 3-D Schrödinger Equation; Ren and Rebecca, Using the Pauli Exclusion Principle to discover the energy of a Fermion Gas (ignoring Coulomb repulsion) — Problem Set 12 for Tuesday
- Friday, Mar. 22 — Study Q11.6 and Q12.1 to Q12 — Problem Set 13 for Friday — Presentations: Emma, Applying the ideas of Example 11.1 to other molecules (caffeine?!); Brian, Continuation of the quantum tunneling ideas started in Problem Set 13
Week 10 — Continue Schrödinger Equation Examples — Exam 3
Week 11 — Numerical Methods for Solving Schrödinger’s Equation — Theory of the Hydrogen Atom — Spherical Harmonics — The Dawn of Nuclear Physics, 1896-1911
- Tuesday, Apr. 2 — Finish Q12 — Problem Set 14 — Discussion of 12.6 and 12.7, qualitative graphical solutions of Schrödinger’s equation and the application of qualitative methods to ramp and barrier wave functions — The two-dimensional and three-dimensional rotationally-symmetric potential, which is especially important for understanding hydrogen, and also a gateway to being able to converse with chemists who often think in terms of probability densities and electron clouds — Another, possibly or even probably, better write-up of the what I wrote up, see especially the state-naming conventions at the end which need to be second nature if you want to be able to converse with chemists — In a year-long, junior-level quantum mechanics course, you would spend lots more time studying these solutions — In our semester-long, sophomore-level course, we are being quite ambitious to have even discussed them at all
- Friday, Apr. 5 — Nuclear Physics from 1896-1911, the discovery of radioactivity, exponential decay and the nucleus following pp. 19-40 of Reed — Please jump on the historical reading because I would like three groups of two people to springboard from that into class presentations for Friday — Start Q13: Sections Q13.1, Q13.2 and Q13.6 — Problem Set 15
Week 12 — Continue Nuclear Physics
- Tuesday, Apr. 9 — Finish your study of Q13 — Presentations: (1) Brian will present the relativistic kinematics that forced the hypothesis of the neutron; (2) We had a five-part presentation on mass spectrometry! — We looked ahead to Section 14.1 and discussed how neutron decay is understood in terms of quarks — Problem Set 16
- Friday, Apr. 12 — Study Q14 — The reasoning behind the mass-deficit formulae — The traditional definition of the amu (atomic mass unit) — The traditional definitions of the meter and the kilogram (the distance from the north pole to the equator on a line passing through Paris as 10,000,000 meters was the first definition of the meter) — The modern definitions of SI Units and especially of the gram in terms of Avogadro’s number and Carbon-12, which is now defined to have an amu of 12.0000 — Reading decay-chain diagrams (e.g. those in Moore in Fig. Q14.15, p. 237) — Why are β decays so slow — Why is an α-particle emission a decay mode? — How is fission induced? — Problem Set 17
Week 13 — Nuclear Physics Applications (Fission and Fusion) — Intro to Magnetic Resonance
- Tuesday, Apr. 16 — Study Q15 — Problem Set 18 — Some Q15 topics: (1) Nuclear stability (and in particular, why we plot binding energy per nucleon rather than just binding energy) (2) High-energy neutrons (mostly captured) vs. thermal neutrons (the ones that are likely to cause new fissions) in a reactor — Choose the remaining special topics (you will have homeworks on the special topics but not be tested on them) — We started our introduction to MRI by considering the behavior of a magnetic moment in the large constant axial magnetic field of an MRI machine
- Friday, Apr. 19 — Prepare by studying Part I of the Introduction to MRI — Presentation by Miles: How are atoms or electrons or ions counted so as to make 1 mole (abbreviated mol), in practice; and in particular, how is the gram which is now defined as 1/12 of the mass of an Avogadro’s number (602,214,076,000,000,000,000,000) of Carbon-12 atoms counted in practice (or is it Silicon-29 that is now the definition!?) — Optional Exam Review Q&A scheduled for 11am Sunday (bring anything you want to ask about) — Part II of the Introduction to MRI — We did not get to the off-resonance response and the Lorentzian function — Problem Set 19
MRI Scanner Cutaway (from the National MagLab website)
Week 14 — Exam 4 — Special Topic: Introduction to Special Relativity
- Tuesday, Apr. 23 — Exam 4 Covering Problem Sets 14-18 — For your convenience when reviewing, here are Problem Sets 14-18 combined — You will need to use a calculator on this exam, unlike Exams 1-3 — I will bring some spare calculators
Einstein’s thought experiment: lightning striking both ends of a train, “simultaneously”
Einstein and Oppenheimer