Physics courses are designated by PHYS.
1020
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.
1021
Introductory Physics II
is a non-calculus based introduction to fluids, wave motion, light, optics, electricity and magnetism.
CO: Mathematics 1000
LH: 3
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
1051
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
2056
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
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: Mathematics 1001, Mathematics 2050, PHYS 1051 (or the former PHYS 2054). Students who have completed PHYS 1020/1021 will be allowed to register for PHYS 2065 with the permission of the Instructor and the Program Chair.
2151
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
2400
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.
2553
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.
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: Mathematics 3260 (or 2260)
LH: 3
3061
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
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.
PR: Mathematics 2000, PHYS 2056, PHYS 2151. PHYS 3220 is recommended.
3180
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
3220
Classical Mechanics I
is kinematics and dynamics of a particle. Moving reference systems. Celestial mechanics. Systems of particles.
3250
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 3260, PHYS 2056, PHYS 2400
3650
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.
3820
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 3260 (or 2260), and PHYS 3810 (or Mathematics 3202)
4100
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
4880
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
4950
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

