1020
Introductory Physics I
(F)
is a non-calculus based introduction to mechanics.
CO: Mathematics 1090
LH: 3
PR: Level III Advanced Mathematics or Mathematics 1090. It is recommended that students have completed at least one of level II and level III high school physics courses, however this course may be completed by someone who has no physics background provided some extra effort is made.
1021
Introductory Physics II
(W)
is a non-calculus based introduction to fluids, wave motion, light, optics, electricity and magnetism.
CO: Mathematics 1000
LH: 3
OR: optional tutorials will be available, on average one hour per week
1050
General Physics I: Mechanics
(F)
is a calculus based introduction to mechanics. The course will emphasize problem solving.
CO: Mathematics 1000
LH: 3
PR: Mathematics 1000, which may be taken concurrently
1051
General Physics II: Oscillations, Waves, Electromagnetism
is a calculus based introduction to oscillations, wave motion, physical optics and electromagnetism.
CO: Mathematics 1001
CR: Physics 1021
LH: 3
PR: Physics 1050 or Physics 1021 or Physics 1020 (with a minimum grade of 65%) and Mathematics 1001.
2056
General Physics VI: Modern Physics
(W)
is special relativity, quanta of light, atomic structure and spectral lines, quantum structure of atoms and molecules, nuclei and elementary particles.
CO: Mathematics 1001 and Physics 1051
CR: Physics 2750
LH: 3
PR: Mathematics 1001, Physics 1050 (or Physics 1020 and Physics 1021), and Physics 1051.
2065
Experimental and Computational Physics
is laboratory techniques, including experimental method and design. Data analysis, including application of statistics to experimental physics. Numerical analysis using Maple, and an introduction to modelling in physics. Topics are introduced through experiments, complementary lectures, and library research of some of the great experiments of physics.
CO: Mathematics 2050
LH: 3
PR: Physics 1051 (or Physics 2054), Mathematics 1001, and Mathematics 2050. Students who have completed Physics 1020/1021 will be allowed to register for Physics 2065 with the permission of the Instructor and the Program Chair.
2151
Stellar Astronomy and Astrophysics
(W)
is atomic structure and spectra. The sun: radiation, energetics, magnetic field. Stars: distance, velocity, size, atmospheres, interiors. Variable stars, multiple stars, clusters and stellar associations. Stellar evolution, interstellar matter, structure of the Milky Way Galaxy. Exterior galaxies, quasi-stellar objects, pulsars. Cosmology.
PR: six credit hours in Mathematics at the first year level
3060
Electricity and Magnetism
is point charges; Coulomb's law; electrostatic field and potential; Gauss' law; conductors; magnetostatics; Ampere's law; Biot-Savart law; dielectric and magnetic materials; electrostatic and magnetostatic energy; Lorentz force; time varying fields; Faraday's law; Lenz's law; Maxwell's equations.
CO: Applied Mathematics 3260
LH: 3
3160
Stellar and Galactic Astronomy
is the physics and mathematics of stars and galaxies. Orbits and the two-body problem, radiation and matter, theory of stellar atmospheres, structure and evolution of stars. Galaxies: Morphology and kinematics. Milky Way kinematics and structure, large-scale star formation, the distribution of interstellar matter in galaxies. Starburst and active galaxies. An introduction to cosmology.
CR: Physics 3150 and Physics 3151
PR: Physics 2056, 2151 and Mathematics 2000. Physics 3220 is recommended.

