PHY 311 — Modern Physics

Fall 2026 · Klamath Falls / Portland-Metro (Zoom-linked) · TuTh, 3:00–4:20 p.m.

Instructors David Johnston Jesse Kinder
Office 208 H SE 214 or SE 204
Office hours TBD Mon/Wed 3:30–5:30 p.m., Tue/Thu 4:30–5:30 p.m.

Required Text: Six Ideas That Shaped Physics, Units R (Relativity) and Q (Quantum) — Moore
Supplement: Exploring Black Holes (Taylor & Wheeler) — selected sections for the GR unit
Recommended: Spacetime Physics (Taylor & Wheeler) — relativity problem source

Grades and assignments live on Canvas. Everything else is here.

Learning Objectives

By the end of this course, you should be able to:

  • Think like a physicist. Apply relativity and quantum mechanics to explain, analyze, and predict real phenomena.
  • Think critically. Identify where relativity and quantum mechanics defy common sense, and trust evidence over instinct. Nature is always right.
  • Solve problems. Apply problem-solving heuristics in relativity and quantum mechanics. Communicate your reasoning clearly, on paper and at the board.
  • Connect theory to experiment and application. Describe key experiments that shaped modern physics. Explain technologies — MRI, GPS, semiconductors — that depend on them today.

Format

This course is co-taught by David and Jesse.

Physics education research is consistent on one point — you learn physics by doing it, not by watching someone talk about it — so most of our time together is discussion, problem solving, and chalk talks at the board, not lecture.

Come prepared: read the assigned material before class, and bring pencil, a calculator, and your laptop or tablet.

We will use a leapfrog method as we work through the text.

  • Read the chapter and attempt a few practice problems before class.
  • Ask questions. Discuss and apply the new concepts during class.
  • Attempt challenging problems after class.
  • Repeat.

Grading

There are no exams in this course. Your grade comes from problem sets, chalk talks, and two projects.

Component Percentage
Problem Sets 50
Chalk Talks 15
Midterm Project 15
Final Project 20

Problem Sets include practice problems due before class each day and challenge problems due each week. Solutions to the challenge problems will be available for self-assessment and corrections. Most of your grade on problem sets (30 points) comes from completion. The remaining points will be assigned at the end of the term by looking at the overall quality of your body of work: effort, clarity, accuracy, critical thinking, and reflection.

Chalk talks. Much of class time is discussion — of problems, of your questions. You’ll occasionally share your own work informally at a chalkboard. Regular attendance and visible, steady effort earns full credit here. You don’t need the right answer to get credit for a chalk talk. There’s a difference between being confused and being unprepared, though.

Midterm project. Research a key experiment in the development of modern physics and present it as we discuss the topic in class. These will be spread throughout the term.

Final project. Research a technology application of relativity or quantum physics. Prepare a written report and peer-review classmates’ reports.

Academic Integrity

Work with others, use outside resources, learn from peers and tutors — but submit your own original work. What you turn in should show your own reasoning, your own calculations, your own conclusions. Generative AI is useful for composing text and as a tutor — you are welcome to use it. But don’t ask it to do your assignments for you. You do the thinking, you ask the questions. If AI contributes substantially to your work, acknowledge it, like any other source you would cite.

Presenting someone else’s work — human or AI — as your own is academic dishonesty. Confirmed plagiarism or cheating earns zero credit for the assignment in question, and reporting to the Student Affairs Office is mandatory. Review Oregon Tech’s Student Academic Integrity Policy if you’re not already familiar with it.

Accessibility

If you need accommodation because of a disability, contact us at the start of the term and reach out to Disability Services — we rely on them to coordinate accommodations.

University Policies

Oregon Tech’s Commission on College Teaching syllabus statements and the “Campus-Wide Syllabus Information” document on Canvas are part of this syllabus. Where they conflict with this document, this document takes precedence.

Tentative Schedule

  • Leapfrog through Unit R (Relativity, ~3 weeks)
  • Quick survey of general relativity (selections from EBH, ~2 weeks)
  • Leapfrog through Unit Q (Quantum, ~5 weeks)
Date Reading Topic Experiments Problems
Oct 1 — Course intro
Oct 6 R1 & R2 Coordinate time Michelson–Morley, Hafele–Keating R1: T1, T2, B1, B2, B5 — M2+R2, M7
R2: T1, B1, B3, B5, B11 — M6, R3, A1
Oct 8 R3 Spacetime interval Kennedy–Thorndike T1, T2, B1, B3, B9 — M5, R2
Oct 13 R4 & R5 Proper time; coordinate transformations Rossi–Hall (muons) R4: T1, T8, B2, B4 — M6, R1, A3
R5: T1, T2, T3, T9, B1 — M3, D4
Oct 15 R6 Lorentz contraction T1, T3, T7, B1, B8 — M4, R1, D4, A2
Oct 20 R7 & RB Cosmic speed limit; Doppler effect Bertozzi · Ives–Stillwell R7: T1, T8, T9, B1, B8 — M2, R1, D7
RB: B1, B2 — M1, D3
Oct 22 R8 & R9 Four-momentum, and its conservation Anderson (positron) · Compton scattering R8: T6, T9, T10, B1, B6 — M10, R1
R9: T4, T5, T10, B2, B4 — M11+R1, M13
Oct 27 EBH 1 & 2 SR review → the curvature bridge to GR
Oct 29 EBH 3 & 4 Schwarzschild map; GPS Pound–Rebka
Nov 3 EBH 6, 7 & 16 Falling in; gravitational waves LIGO · Cygnus X-1 · EHT
Nov 5 EBH 10 & 11 GR’s classic confirmations Eddington · Mercury’s perihelion · 2020 Nobel Prize
Nov 10 Q1, Q2, Q3 Waves, interference, diffraction
Nov 12 Q4 & Q5 Photons; matter waves Compton / Bothe–Geiger · Davisson–Germer
Nov 17 Q6 & Q7 Spin; rules of QM Stern–Gerlach · Franck–Hertz
Nov 19 QA & Q8 Complex numbers; quantum weirdness Bell tests (2022 Nobel Prize)
Nov 24 Q9 & Q10 Wavefunction; simple quantum models Jönsson (electron double-slit)
— — No class — Thanksgiving
Dec 1 Q11 & Q12 Spectra; the Schrödinger equation Lamb shift
Dec 3 Q13 & Q14 Nuclei; nuclear stability Rutherford · Cowan–Reines
Dec 8 — Guest speaker: Jaime Evers, medical physics
Dec 10 Q15 Nuclear technology

Attempt the italicized problems BEFORE class.

Attempt the bold problems AFTER we discuss the chapter in class. Solutions will be available the following Thursday, for self-assessment and corrections. (You can substitute a different problem of the same category from the same chapter and request a solution.)

All “A” and “D” problems are optional — difficult, but worth the effort.