PHYSICS 7546 - Statistical Mechanics
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Elements of Nonequilibrium Statistical Mechanics. The course covers the principles and practical applications of macromolecular crystallography and NMR in contemporary structural biology research. Besides the key issues in macromolecular structure determination, students will also learn practical aspects of the design and performance of experiments, and will process and analyze experimental data. Principles and practical applications of biophysical methods in biological research, with an emphasis on macromolecular structure and function.
This course allows students to work on a specific topic not covered by any lecture courses under the guidance of a faculty member of the Department of Physics and Astronomy. This course carries the same credit as a lecture course. At most half of the courses taken by a first-year student can be A student enrolls in when he or she is working in a research group.
The student should enroll in the corresponding to the faculty member leading that research group. Students not enrolled in letter-grade courses should enroll in at least one unit of Survey of radio astronomy, emphasizing technical aspects; radiation, antennas, receivers, radio spectroscopy, interferometer arrays and aperture synthesis; radio emission mechanisms and cosmic rays.
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Astronomy Astrophysical Radiative Processes and Transport. Radiative processes important in astrophysics and the methods to model the propagation of radiation. Synchrotron and bremsstrahlung emission. Compton scattering. Plasma effects. Basic atomic and molecular processes. Example astronomical applications. Methods of exoplanet detection. The observed architecture of exoplanetary systems. The formation and evolution of planetary systems. Modeling exoplanet interiors and atmospheres.
Exoplanet habitability and the search for biosignatures. Dynamics of fluids as applied to astrophysical bodies. Topics include hydrostatics, shocks, waves, instabilities, and magnetohydrodynamics. Applications include atmospheres, stars, accretion disks, stellar winds, and galactic disks. Geometric optics applied to the design of optical and X-ray telescopes. Diffraction and the Airy disk, radio and optical interferometry and aperture synthesis, adaptive optics, recent developments in detector technology, quantum and thermal noise in astronomy.
Includes independent research projects using the CCD camera and inch refractor in Dearborn Observatory. Physics of stellar interiors, stellar atmospheres, and star formation. Specific topics covered include: simple stellar models, nuclear energy generation, overview of evolutionary phases, degenerate stars white dwarfs, neutron stars , radiative transfer, continuous and line opacities, interstellar gas and dust grains, gravitational collapse and protostars. Big bang cosmology, Friedman model, thermal history of the Universe, primordial nucleosynthesis, microwave background, dark matter, inflation, large-scale structure, galaxy formation, spiral and elliptical galaxies, groups and clusters of galaxies.
Thermodynamics of stellar interiors, equations of stellar structure and radiation transfer, stellar atmospheres, thermonuclear reactions, weak interactions and nucleosynthesis, stellar stability and pulsation, evolution of binaries. Special topics may include novae and supernovae, stellar rotation, stellar magnetic fields, and cooling of neutron stars, white dwarfs, and brown dwarfs.
Prerequisite: Astr or consent of the instructor.
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Interstellar gas phases, absorption and emission lines, masers, bremsstrahlung, synchrotron radiation, excitation of atoms and molecules, thermal balance and cooling lines, equations of hydrodynamics, shocks, ionization fronts, supernova remnants, magnetohydrodynamic processes and turbulence, gravitational collapse and star formation, protostars, accretion disks, outflows. Gravitational potential theory, regular and chaotic orbits, equilibrium and stability of collisionless stellar systems, galactic nuclei and supermassive black holes, galactic disk dynamics and spiral structure, interactions of stellar systems, kinetic theory of collisional systems, evolution of galaxies and star clusters, dark matter.
This course covers a wide range of topics in modern high-energy astrophysics, focusing on the physics of compact objects and their observational manifestations across the electromagnetic spectrum, from the radio to gamma-ray bands, and through gravitational waves and neutrinos. The course includes a computational component, focusing on the numerical simulations of black hole accretion and outflows.
Physics Classical Mechanics Review of Newtonian mechanics, conservation laws and rigid-body dynamics. Physics Methods of Theoretical Physics The topics covered include: techniques for the solution of differential equations; approximations such as the method of steepest descent; techniques for integration; complex analysis; the special functions of mathematical physics; usage of Greens functions and eigenfunctions to solve differential equations; introduction to probability and statistics.
Physics ,2,3 Quantum Mechanics First quarter : Vector spaces and linear operators, postulates of quantum mechanics, observables and Hermitian operators, state vectors and quantum dynamics, stationary states, bound states, the harmonic oscillator, statistical interpretation and the Uncertainty Principle, symmetry and conservation laws, quantization of angular momentum, intrinsic spin, the Stern-Gerlach experiment, spherically symmetric potentials.
Physics ,2 Electrodynamics First quarter : Electrostatics, boundary-value problems, Green's functions, multipoles, electrostatics of macroscopic media, conductors and dielectrics, magnetostatics, Maxwell's equations, electromagnetic waves and gauge transformations, conservation laws. Physics Introduction to Statistical Mechanics Statistical mechanics and probability.
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Physics Statistical Physics Correlation functions, measurement, and response theory. Physics Introduction to Superconductivity Lectures and experimental demonstrations on the basic theory and phenomenology of superconductivity and its applications. Physics ,2,3 Condensed-Matter Physics First quarter : Periodic potentials, crystal lattices, x-ray diffraction. Physics ,2 Particle Physics First Quarter : Overview of modern particle physics and experimental techniques, the quark model, particle production, quantum chromodynamics, quark density functions.
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Physics Nonlinear Optics Nonlinear optical susceptibilities, wave propagation and coupling in nonlinear media. Physics Quantum Optics Review of quantum fields.
Physics ,2,3 Quantum Field Theory First quarter : Lagrangian field theory, relativistic Lagrangians and relativistic wave equations, symmetries and conservation laws, canonical quantization, covariant perturbation theory, the S-Matrix, cross sections and lifetimes, and elementary processes of quantum electrodynamics. The information below is provided as a guide to assist students in engaging appropriately with the course requirements.
The University's policy on Assessment for Coursework Programs is based on the following four principles: Assessment must encourage and reinforce learning. Assessment must enable robust and fair judgements about student performance. Assessment practices must be fair and equitable to students and give them the opportunity to demonstrate what they have learned. Assessment must maintain academic standards.
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Grades for your performance in this course will be awarded in accordance with the following scheme:. Grade Descriptors are available which provide a general guide to the standard of work that is expected at each grade level. More information at Assessment for Coursework Programs. Final results for this course will be made available through Access Adelaide.
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