Office of the Registrar
Grenfell Campus (2016/2017)
13.23 Physics

Physics courses are designated by PHYS.


Introductory Physics I

is a non-calculus based introduction to mechanics.

CO: Mathematics 1090

CR: PHYS 1050

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.


Introductory Physics II

is a non-calculus based introduction to fluids, wave motion, light, optics, electricity and magnetism.

CO: Mathematics 1000

LH: 3

PR: Mathematics 1000, PHYS 1020 or PHYS 1050


General Physics I: Mechanics

is a calculus based introduction to mechanics. The course will emphasize problem solving.

CO: Mathematics 1000

CR: PHYS 1020

LH: 3

PR: Mathematics 1000, which may be taken concurrently


General Physics II: Oscillations, Waves, Electromagnetism

is a calculus based introduction to oscillations, wave motion, physical optics and electromagnetism.

CO: Mathematics 1001

LH: 3

PR: PHYS 1050 or PHYS 1021 or PHYS 1020 (with a minimum grade of 65%) and Mathematics 1001


Fluids and Thermal Physics

examines elasticity, fluid mechanics, thermodynamics, kinetic theory and statistical mechanics.

CO: Mathematics 1001 and PHYS 1051

LH: 3

PR: Mathematics 1001 and PHYS 1051


General Physics VI: Modern Physics

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 PHYS 1051

CR: PHYS 2750

LH: 3

PR: Mathematics 1001, PHYS 1050 (or PHYS 1020 and PHYS 1021), and PHYS 1051


Experimental and Computational Physics

i- inactive course.


Stellar Astronomy and Astrophysics

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: 6 credit hours in Mathematics at the first year level


Subatomic Physics

is an introduction to nuclear and particle physics. Topics include nuclear properties and models; radioactive dating; fission; nuclear reactors; accelerators; the detection, classification, and properties of subatomic particles. Applications in areas such as ecology, dosimetry, medical physics and nuclear astrophysics are discussed.

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.


Introduction to Analog and Digital Electronics

covers the basics of the analog and digital electronics; direct current circuits, capacitors and inductors, alternating currents, test equipment and measurement, transducers, diodes and transistors, introduction to operational amplifiers, digital basics, digital circuitry and digital analog I/O. This course is a combined lecture/laboratory course with two three-hour sessions scheduled per week.

PR: Mathematics 1000 or equivalent, PHYS 1021 or 1051


Computational Mechanics

covers newtonian dynamics and celestial mechanics, numerical differentiation and integration, numerical solutions to mechanics problems, data and spectral analysis, Fourier series and normal modes, oscillations and vibrations, linear and non-linear oscillators, nonlinear dynamics and chaos.

CO: Mathematics 2000

LC: 5

LH: 5

PR: Mathematics 2000 and PHYS 1051


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: Mathematics 2260 (or the former Mathematics 3260)

LH: 3

PR: PHYS 1051 and Mathematics 2260 (or the former Mathematics 3260)


Electromagnetic Theory

includes Maxwell’s equations, energy and momentum in electromagnetic systems, EM waves, potentials and fields, dynamical systems of charges, radiation, the interaction of EM fields with matter, and the relativistic formulation of electromagnetism and its applications.

PR: PHYS 3060


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: PHYS 3150 and PHYS 3151

PR: Mathematics 2000, PHYS 2056, PHYS 2151. PHYS 3220 is recommended.


Observational Astrophysics

covers theoretical topics including celestial mechanics, continuous and line spectra, stellar structure and nucleosynthesis, and stellar evolution. Observational topics include planning observations, acquisition of images with a CCD electronic camera, fundamentals of astronomical image processing, photometry, and stellar spectroscopy using a variety of software packages.

LH: 3

PR: Mathematics 2000, PHYS 2056. PHYS 2151 is recommended.


Classical Mechanics I

is kinematics and dynamics of a particle. Moving reference systems. Celestial mechanics. Systems of particles.

CO: Mathematics 2260 (or the former Mathematics 3260)

PR: PHYS 2820 and Mathematics 2260 (or the former Mathematics 3260)


Classical Mechanics II

covers rigid body motion. Lagrange's equations. Hamilton's equations. Vibrations. Special theory of relativity.

PR: PHYS 3220 and 3810 (or Mathematics 3202) and Mathematics 2260 or the former Mathematics 3260


Elementary Particles and Fields

includes the Standard Model, classification of elementary particles and forces of nature, symmetries, conservation laws, quark model, quantum electrodynamics, quantum chromodynamics, and the theory of weak interactions.

PR: Mathematics 3202, Mathematics 2260 (or the former Mathematics 3260), PHYS 2056, PHYS 2400



covers the first and second laws of thermodynamics. Entropy. Thermodynamics of real substances. Kinetic theory of matter. Introduction to statistical mechanics.

PR: Mathematics 2000, PHYS 2053 and PHYS 2750 or 2056


Quantum Mechanics I

includes a review of elementary quantum physics and covers topics such as wave functions, operators, expectation values, the Schrodinger equation in 1-dimension, states and operators in Hilbert space, coordinate and momentum representations, quantum mechanics in three dimensions, angular momentum, spherically symmetric potentials, and approximation methods.

PR: Mathematics 3202, PHYS 2056, PHYS 3220


Mathematical Physics II

examines the functions of a complex variable; residue calculus. Introduction to Cartesian tensor analysis. Matrix eigenvalues and eigenvectors. Diagonalization of tensors. Matrix formulation of quantum mechanics. Quantum mechanical spin. Vector differential operators in curvilinear coordinate systems. Partial differential equations of Mathematical Physics and boundary value problems; derivation of the classical equations, separation of variables; Helmholtz equation in spherical polar coordinates.

PR: Mathematics 2260 (or the former Mathematics 3260), and PHYS 3810 (or Mathematics 3202)


Senior Physics Seminar

is a review of current topics in Physics discussed in a seminar format. Seminars are presented by faculty, students, and guest speakers. Topics are normally drawn from the fields of sub-atomic & nuclear physics or astronomy & cosmology. This is a designated Writing course.

PR: normally restricted to Physics students who have completed 78 credit hours or more


Physics Laboratory

introduces the student to advanced laboratory work in several areas of physics.

PR: Physics students who have completed 60 credit hours or more


Research Experience in Physics

is an opportunity for students to participate in original research under the supervision of a faculty advisor. Students are required to present a written report and to give a seminar on their work.

PR: Physics students who have completed 78 credit hours or more and permission of the Physics Program Chair

AR = Attendance requirement; CH = Credit hours are 3 unless otherwise noted; CO = Co-requisite(s); CR = Credit can be retained for only one course from the set(s) consisting of the course being described and the course(s) listed; LC = Lecture hours per week are 3 unless otherwise noted; LH = Laboratory hours per week; OR = Other requirements of the course such as tutorials, practical sessions, or seminars; PR = Prerequisite(s); UL = Usage limitation(s).