As we learn about particle spins, we will talk about brain imaging studies enabled by Nobel winning physics research. Examples include wave-particle duality and its relevance for technological applications, behavior of spin particles in a magnetic field to explain magnetic resonance imaging, ion flow through ion channels and ohm's law to explain electrical signal flow in our body, and other examples within the core of physics and bridging to interdisciplinary areas of material science and devices, biology and neuroscience. The course content is mostly physics, although we link it to cognitive sciences, but the main focus is on motivating and explaining the basic physical laws behind new phenomena and related technologies. We will explore the basic classical and quantum physics concepts, and link themto newly observed physical phenomena and technologies, as well as to brain research, in the context of tools that physicists helped bring about like the seminal magnetic resonance imaging. No previous study of physics is assumed.Įxperiments in electromagnetism and optics. We will examine a number of alternative modes of energy generation - fossil fuels, biomass, wind, solar, hydro, and nuclear - and study the physical and technological aspects of each, and their societal, environmental and economic impacts over the construction and operational lifetimes. We describe the physical principles of energy, its production and consumption, and environmental consequences, including the greenhouse effect. The developed world's dependence on fossil fuels for energy production has extremely undesirable economic, environmental, and political consequences, and is likely to be mankind's greatest challenge in the 21st century. Students with AP or Transfer Credit for PHYS 091 or 093 who complete PHYS 0008 will thereby surrender the AP or Transfer Credit. Credit is awarded for only one of the following courses: PHYS 0008, PHYS 0101, PHYS 0150, or PHYS 0170. Enrollment restricted to graduate students.Īn introduction to the classical laws of mechanics, including static equilibrium, elasticity, and oscillations, with emphasis on topics most relevant to students in architecture. Models and observations of galaxy formation and evolution. Galaxies: Structure, Dynamics and Formation Application is made to the observed features of planetary motion, the atmospheres and stars and planets, and the structure and evolution of stars. The course provides fundamental knowledge of Newtonian gravity and the properties of light and matter as they are relevant for understanding astrophysical objects. Fulfills quantitative data analysis requirement.Ī basic course for majors in physical sciences and engineering required for the astrophysics concentration. Topics will include the solar system, stars, black holes, galaxies, and the structure, origin and future of the Universe itself. Fulfills quantitative data analysis requirement.Īn introductory course for students who do not intend to major in a physical science or engineering, covering theories of the Universe ranging from the ancient perspective to the contemporary hot big bang model, including some notions of Einstein's special and general theories of relativity. Engineering students receive no credit for this course. This course is not recommended for physical-science majors or engineering students. Elementary algebra and geometry will be used. Topics include planets, satellites, small objects in the solar system, and extraterrestrial life stars, their evolution, and their final state as white dwarfs, neutron stars, or black holes galaxies, quasars, large structures, background radiation, and big bang cosmology. A general survey, designed for the non-major, of the facts and theories of the astronomical universe, from solar system, to stars, to galaxies and cosmology.
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