
explore modern physics as a shift from classical, continuous energy to quantized energy and quantum concepts, including wave-particle duality and early ideas behind blackbody radiation.
Explore blackbody radiation and how freely vibrating electrons absorb and reemit all em radiation in an idealized blackbody. Learn how classical theory fails, prompting Planck's quantized energy and Planck's constant.
Explore how light ejects electrons from materials via the photoelectric effect, with emission driven by photon energy and frequency, not light intensity.
Explore the photoelectric effect: light acts as photons with energy hf that eject electrons when hf exceeds the work function and threshold frequency, linking intensity, kinetic energy, and stopping potential.
Trace the atom's history from Thomson's cathode ray revealing the electron to Rutherford's gold foil showing a dense nucleus, then Bohr's quantized energy levels and photon-driven transitions.
Explore atomic history and the Bohr model to see how electrons move between energy levels, absorb and emit photons, and form hydrogen's emission spectra across ultraviolet, visible, and infrared.
Identify the fundamentals of nuclear physics, including protons, neutrons, electrons, and isotopes, and use atomic mass, atomic number, and mass number to explain binding energy via mass defect.
Explore nuclear physics as part of modern physics through AP and high school lessons, delivered as clearly marked video series to master the AP curriculum.
Explore the standard model by detailing the atom’s nucleus, protons, neutrons, and electrons. Understand mass-energy equivalence via E=mc^2, atomic mass units, MeV, and the strong, weak, EM, and gravity forces.
Explore the standard model of particle physics by examining antiparticles, hadrons and leptons, quark composition of protons and neutrons, and the Higgs boson as predicted by the model.
Explore the photoelectric effect by calculating photon energy from 400 nm light (hf), deducing the work function, kinetic energy, stopping potential, and electron emission behavior.
Determine the work function from the graph's x-intercept using hf = phi + KE max at threshold frequency, and relate stopping potential to kinetic energy and wavelength.
Analyze energy level transitions A, B, and C and the photoelectric effect to find emitted photon wavelengths, kinetic energy above work function, and the de Broglie wavelength of ejected electrons.
Compute a proton's momentum and de Broglie wavelength, then use energy conservation to find the turning point distance near a uranium nucleus and estimate the mass defect.
Analyze a modern physics style problem on atomic energy levels, transitions from level three to one and two, and determine the longest photon wavelength and ionization energy.
An exploration of the photoelectric effect, calculating stopping potential and work function from incident light and electron energies, and explaining how frequency, wavelength, and light intensity affect electron emission.
This course is one of several Mousseau Physics courses designed for students in high school physics, AP Physics, and introductory college physics. In this course we focus on modern physics, including the ideas that changed physics beyond classical mechanics, waves, and electricity. Students will study atomic models, light as photons, energy levels, spectra, the photoelectric effect, nuclear physics, radioactive decay, and related algebra based problem solving.
The videos and resources use clear lectures, diagrams, demonstrations, and worked out example problems. Students will learn how to connect conceptual models to equations, how to interpret what a quantum or nuclear model is saying, and how to solve problems involving energy, frequency, wavelength, photons, half-life, and nuclear reactions. The goal is to make modern physics approachable without hiding the important physical ideas.
This course is a strong fit for high school physics students, AP Physics students, and introductory college physics students working through algebra based modern physics. It does not require calculus. The course can be used as a full unit, a supplement to class, or a focused review when modern physics appears near the end of a school year.
By the end of the course, students should be more comfortable explaining why classical physics needed new models, using modern physics equations, interpreting atomic and nuclear processes, and solving the kinds of modern physics problems that appear in high school, AP, and introductory college physics courses.
Students can work straight through the course as a full unit or use individual lessons as targeted support alongside a class. The videos are built to be paused, rewound, and practiced with pencil and paper, so the course works well for homework help, test review, exam preparation, or rebuilding a topic that did not fully click the first time.