# Syllabus of descriptive physics csu

Early Universe Cosmology 3 Lecture - 3 hours. Introduction to observations of the night sky using small telescopes in nighttime laboratory.

## Csu physics 141 syllabus

Advanced topics in nuclear theory; theory of quantum-mechanical scattering processes. Potter Not open for credit to students who have completed course 2 or Theory of Mechanics and Electromagnetics Lecture - 3 hours; independent study - 1 hour. Renormalization theory and applications, including dimensional regularization, Ward identities, renormalization group equations, coupling constant unification, and precision electroweak calculations. Prerequisite: courses A, B C is corequisite or consent of instructor. Careers in Physics 1 Seminar - 2 hours. Introduction to Solid State Physics Lecture - 3 hours; extensive problem solving. Introduction to early universe cosmology: the Big Bang, inflation, primordial nucleosynthesis, dark matter, dark energy, and other topics of current interest. Oscillations and Waves: Simple harmonic motion SHM and Hookes law, elastic potential energy and kinetic energy of vibrating objects, vibration velocity, period and frequency, equation for SHM, description of waves, properties of waves superposition and interference , wave interactions, Fourier synthesis and analysis, wave phenomena, resonance. Introduction to Cosmology Lecture - 3 hours; extensive problem solving. Check with the department office for the current emphasis. Not open for credit to students who have completed course 9B or 9D. Continuation of course 9A. Collider Physics 3 Lecture - 3 hours.

Explores intrinsic unpredictability deterministic chaos and the emergence of structure in natural complex systems. Careers in Physics 1 Seminar - 2 hours. Prerequisite: courses B and A passed with a grade of C— or better, or consent of department.

Heat characteristics in x-ray tubes: Power rating of tubes, Stefans Law and cooling curves, relationship to I-V waveform. Basic x-ray circuit: Primary circuit, secondary circuit, I2R losses. Supplementary Work in Lower Division Physics Students with partial credit in lower division physics courses may, with consent of instructor, complete the credit under this heading.

Definition of the mathematical frame work for the description of the gravitational field, introduction of the dynamical equations of Einstein governing its evolution and review of the key solutions, including black holes and expanding universes. Basic Electronics: Semiconductors, diodes, transistors, thyristors and triacs, basic electronic circuits used in radiological applications eg switches, filters, detection, logic circuit elements.

## Csu online physics

Continuation of course 9A. High-Energy Physics 3 Lecture - 3 hours. Stellar Structure and Evolution 4 Lecture - 3 hours; extensive problem solving. Not open for credit to students who have taken Astronomy 2, the former Astronomy 10, any quarter of Physics 9 or 9H, or any upper-division physics course other than or Survey course covering measurement and signal analysis techniques for astrophysics and cosmology throughout the electromagnetic spectrum. Prerequisite: courses B, B, and C or the equivalent; course A concurrently. Properties and classification of elementary particles and their interactions. Presentation and discussion of topics of current research interest in joint theory physics. Physics 9 is a four-quarter sequence using calculus throughout and including laboratory work as an integral part. Introduction to classical and quantum statistical mechanics and their connections with thermodynamics. Either 1A alone or both quarters may be taken. Read the following information carefully if you are using Physics 7 to complete an introductory course you have already begun. Cosmic Structure Formation 3 Lecture - 3 hours. The theory is developed for the ideal gas model and simple magnetic models and then extended to studies of solids, quantum fluids, and chemical equilibria. Recent Syllabus and More Complete Descriptions

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