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This course examines general relativity. Topics include: The principle of equivalence; inertial observers in a curved space-time; vectors and tensors; parallel transport and covariant differentiation; the Riemann tensor; the stress-energy tensor; the Einstein gravitational field equations; the Schwarzschild solution; black holes; gravitational waves detected by LIGO, and Freidmann equation.
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This is a two-semester course on the classical interactions of light and matter (electromagnetism), and the relationship between space and time (special relativity). The focus of the course is similarly twofold; there is emphasis on developing skills to solve physical problems, and on the close interplay between mathematical results and physical laws.
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This course covers the theoretical foundations of the standard model of particle physics and its possible extensions. Among topics covered are the building blocks of the standard model, strong and electroweak interactions, CP violation, neutrino oscillations, and grand unification and supersymmetry.
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This course provides an introduction and overview of the physics of strong and electroweak interactions and their experimental foundation. These fundamental forces underlie the rich phenomenology of nature's smallest components: elementary particles and atomic nuclei. The course outlines the theoretical and experimental advances which have led to the current understanding of physics at the subatomic scale. These topics are covered at a mathematical level appropriate for undergraduates students of physics. The focus is more on the understanding of phenomena rather than their rigorous mathematical description. The course touches upon selected topics of current interest, including: symmetries and conservation laws in nuclear and particle physics; relativistic kinematics and applications in high-energy reactions; the Standard Model theory: fundamental matter particles and their interactions by strong and electroweak forces; the Higgs mechanism and the origin of mass; neutrino oscillations and masses; effective nucleon-nucleon interactions and models of nuclear physics; alpha, beta, and gamma decay and fission; form factors and structure functions; and selected applications of nuclear and particle physics.
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This course introduces the foundations of classical mechanics based on the principle of least action with emphasis on symmetries and conservation laws as well as special relativity with emphasis on relativistic kinematics. In particular the following is included: the Lagrange formalism, the principle of least action, Euler Lagrange's equations; conservation laws and generalized coordinates; introduction to the Hamilton formalism; constraints and Lagrange multipliers; general treatment of the two-body problem and Kepler's laws; Lorentz transformations; and four-vectors and relativistic kinematics.
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This is a special studies course involving an internship with a corporate, public, governmental, or private organization, arranged with the Study Center Director or Liaison Officer. Specific internships vary each term and are described on a special study project form for each student. A substantial paper or series of reports is required. Units vary depending on the contact hours and method of assessment. The internship may be taken during one or more terms but the units cannot exceed a total of 12.0 for the year.
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The course gives a brief introduction to all fields of astronomy. Overview of general fundamental concepts. The night sky and its motion. Astronomical instruments and observation techniques. The sun and the planetary system, exoplanets. The distances to the stars and their motion. The structure and evolution of stars. The space between the stars. The Milky Way and other galaxies. Theories of the origin and development of the universe.
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This course examines the observational aspect of astronomy (including constellations and planets), the physics of our solar system, and our own Sun, stars and their evolution, galaxies, blackholes, and cosmology.
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This course introduces calculus techniques to the study of the range of principles and applications presented. Topics include: fluids such as water and air pressure, breathing, hydraulics, flight (pressure in fluids, buoyancy, fluid flow, viscosity, surface tension); electricity and magnetism such as electrical devices, lightning, household electricity and electrical safety, electric motors, power generation and transmission, Earth’s magnetic field, particle accelerators, communications (electric charge and field, conductors and insulators, electric potential, capacitance, resistance, electric circuits, magnetic field, Faraday’s law of induction, Maxwell’s equations, electromagnetic waves); Quantum and atomic physics such as spectroscopy, lasers (photon, blackbody radiation, matter waves, quantization in atoms, interaction of light with matter, x-rays); and nuclear physics and radiation such as: nuclear energy, radiation safety, formation of atoms in stars, carbon dating (the atomic nucleus, radioactive decay, half-life, ionizing radiation, nuclear fission and fusion).
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This course explores whether the chemical and biological evolutions on the Earth could be a universal phenomenon in the galaxy. From an astronomical point of view the course examines the evolution of cosmic matter up to heavy elements, which are essential ingredients for forming biological creatures.
Topics include: modern search techniques, their limitations, and potential search technologies of the future; the formation of terrestrial planets as distinguished from Jovian; how orbits of the exo-planets are analyzed for evidence that they may be solar terrestrial planets; the evolutionary path of Earth over the last 4.6 billion years; the Goldilocks problem of atmospheric evolution; birth and growth of civilization; parameterization of human ignorance by Drake's equation; Gaia, and Ohn-Saeng Myung; interstellar communication; terraformation of Mars; heavens and hells.
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