This course gives a broad introduction to numerical algorithms used in scientific computing. It covers classical methods to solve Ordinary and Partial Differential Equations such as spectral, finite difference and finite volume methods. A brief introduction to finite element methods is given. Explicit and implicit time integration using various high-order methods are discussed. We review basic methods to solve linear and non-linear systems of equations. Issues related to the implementation of efficient algorithms on modern high-performance computing systems are discussed. Hyperbolic systems of conservations laws are covered in detail.

This course, whose subject matter covers the entire universe, targets the frontiers of modern astrophysics. Topics include the planets of our solar system; the search for extrasolar planets and extraterrestrial life and intelligence; the birth, life, and death of stars; black holes; the zoo of galaxies and their evolution; the Big Bang and the expanding universe; and dark matter, dark energy, and the large-scale structure of the universe. This course is designed for the non-science major and has no prerequisites past high school algebra and geometry. High school physics would be useful, but is not required.

The solar system and planets around other stars; the structure and evolution of stars; supernovae, neutron stars, and black holes; gravitational waves; the interstellar matter; the formation and structure of galaxies; cosmology, dark matter, dark energy, and the history of the entire universe. Compared to AST 203, this course employs more mathematics and physics. Intended for quantitatively-oriented students.

Black holes are amazing: so much mass is contained in such a small region of space that nothing, not even light, can escape. In this class, we will learn to understand what black holes are, and (equally importantly) what they are not (sorry, science fiction!). We will grapple with the seeming simplicity of black holes and their weirdness. We will also study how black holes are discovered and how they give rise to some of the most astonishing phenomena in the Universe. We will cover concepts at the forefront of modern astronomy and physics and highlight the power of quantitative thinking (algebra only) and the scientific method.

Astronomy is in an amazing period of discovery. The Webb Space Telescope is enabling stunning discoveries about the formation of planets around other stars and first stars and galaxies. This course will open the curtain on astronomical discovery, examining astronomical telescopes and detectors, statistical methods, and astronomical computing. Students will also get a taste of what it means to be a professional astronomer by reading both popular and astronomical literature. Finally, as part of the final project, we will practice given public-level talks.

The Space Physics Laboratory course provides undergraduates at all levels the opportunity to participate in a laboratory developing NASA space flight instrumentation. The courses teach space physics laboratory skills, including ultrahigh vacuum, space instrument cleanroom, mechanical, electrical, and other laboratory skills, which then allow students to propose and carry out a significant group research project in the Laboratory. The class sequence comprises two semesters with AST 250 as a prerequisite for AST 251, a credit bearing (P/F) course.

Power from the nucleus offers a low-carbon source of electricity. Fission power is well developed, but carries risks associated with safety, waste, and nuclear weapons proliferation. Fusion energy research, which presents less such risk, is making important scientific progress and progress towards commercialization. We will study the scientific underpinnings of both of these energy sources, strengthening your physical insight and exercising your mathematical and computational skills. We will also ask ourselves the thorny ethical questions scientists should confront as they contribute to the development of new technologies.

Stars form from interstellar gas, and eventually return material to the interstellar medium (ISM). Nuclear fusion powers stars, and is also the main energy source in the ISM. This course discusses the structure and evolution of the ISM and of stars. Topics include: physical properties and methods for studying ionized, atomic, and molecular gas in the ISM; dynamics of magnetized gas flows and turbulence; gravitational collapse and star formation; the structure of stellar interiors; production of energy by nucleosynthesis; stellar evolution and end states; the effects of stars on the interstellar environment.

Theoretical and numerical analysis of the structure of stars and their evolution. Topics include a survey of the physical process important for stellar interiors (equation of state, nuclear reactions, transport phenomena); and the integrated properties of stars and their evolution.

Selected astrophysical applications of electrodynamics, special and general relativity, nuclear and particle physics. Topics may include synchrotron radiation, comptonization, orbits and accretion in black-hole metrics, radio sources, cosmic rays, and neutrino astrophysics.

Students will present talks and discussion on select topics in Astrophysics and Cosmology.

This is an introductory graduate course in plasma physics, focusing on magnetohydrodynamics (MHD) and its extension to weakly collisional or collisionless plasmas. Topics to be covered include: the equations of MHD and extended MHD, the structure of magnetic fields, static and rotating MHD equilibria and their stability, magnetic reconnection, MHD turbulence, and the dynamo effect. Applications are drawn from fusion, heliophysical, and astrophysical plasmas.

Introduction to theory of fluctuations and transport in plasma. Origins of irreversibility. Random walks, Brownian motion, and diffusion; Langevin and Fokker-Planck theory. Fluctuation-dissipation theorem; test-particle superposition principle. Statistical closure problem. Derivation of kinetic equations from BBGKY hierarchy and Klimontovich formalism; properties of plasma collision operators. Classical transport coefficients in magnetized plasmas; Onsager symmetry. Introduction to plasma turbulence, including quasilinear theory. Applications to current problems in plasma research.

Introduction to plasma diagnostics methods, including those used to measure high-temperature plasmas for fusion in both magnetic and inertial confinement systems. Also included are measurement methods used in low-temperature plasmas for industrial applications, in space and solar plasmas (or heliophysics), and astrophysical plasmas (or astronomy). Example plasma diagnostic techniques are magnetic measurements, Langmuir probes, microwave techniques, spectroscopic techniques, electron cyclotron emission, Thomson scattering, neutron measurements. Vacuum technology and associated diagnostics will be also introduced.

Advances in experimental and theoretical studies or laboratory and naturally-occurring high-temperature plasmas, including stability and transport, nonlinear dynamics and turbulence, magnetic reconnection, selfheating of "burning" plasmas, and innovative concepts for advanced fusion systems. Advances in plasma applications, including laser-plasma interactions, nonneutral plasmas, high-intensity accelerators, plasma propulsion, plasma processing, and coherent electromagnetic wave generation.

Analysis of methods for the numerical solution of the partial differential equations of plasma physics, including those of elliptic, parabolic, hyperbolic, and eigenvalue type. Topics include finite difference, finite element, spectral, particle-in-cell, Monte Carlo, moving grid, and multiple-time-scale techniques, applied to the problems of plasma equilibrium, transport and stability. Basic parallel programming concepts are discussed.

Develop skills, knowledge, and understanding of basic and advanced laboratory techniques used to measure the properties and behavior of plasmas. Representative experiments are: cold-cathode plasma formation and architecture; ambipolar diffusion in afterglow plasmas; Langmuir probe measurements of electron temperature and plasma density; period doubling and transitions to chaos in glow discharges; optical spectroscopy for species identification; microwave interferometry and cavity resonances for plasma density determination; and momentum generated by a plasma thruster.

What makes Earth habitable? How have we unraveled the mysteries of planetary interiors? Using a physics-centered approach, we'll explore a range of captivating subjects in earth and planetary science, including the origin of solar systems, tectonic plates, mantle convection, earthquakes, and volcanoes. You will learn methods to study the inner structures and dynamics of planets, not just Earth, but also celestial neighbors like Mars, Venus, Mercury, the Moon, and even exoplanets.

Ultrafast lasers are widely used as probes for chemistry, material science, biology, flow dynamics, and environmental science, as well as for generating ultra-intense light, relativistic particle beams, and attosecond light bursts. This course explores the technology and applications of ultrafast lasers, which produce pulses shorter than 1 picosecond. Ultrashort pulse generation techniques - including mode-locked oscillators, chirped pulse amplification, and optical parametric amplification - and pulse measurement methods such as frequency-resolved optical gating and high-order autocorrelations are discussed.

The course provides an introduction to modern statistics and data analysis. It addresses the question, "What should I do if these are my data and this is what I want to know"? The course adopts a model based, largely Bayesian, approach. It introduces the computational means and software packages to explore data and infer underlying parameters from them. An emphasis will be put on streamlining model specification and evaluation by leveraging probabilistic programming frameworks. The topics are exemplified by real-world applications drawn from across the sciences.