Global Arc

This is an introductory course in general relativity for undergraduates. Topics include the early universe, black holes, cosmic strings, worm holes, and time travel. Designed for science and engineering majors. Two 90-minute lectures. Prerequisites: MAT 201 and 202, OR MAT 203 and 204. Also PHY 205 or 207. PHY 304 is recommended.

How do we observe and model the universe? We discuss the wide range of observational tools available to the modern astronomer, with telescopes on the ground and in space, observing from gamma rays to radio, as well as gravitational waves. We review basic probability and statistics and introduce students to techniques used in analysis and interpretation of modern data sets containing millions of galaxies, quasars and stars, plus the analytic tools and numerical methods used by theoretical astrophysicists to model the data. The course is problem-set-based and aims to provide students with tools needed for independent research in astrophysics.

We develop the scientific ideas behind fission and fusion energy. For fission we move from elementary nuclear physics to calculations of chain reactions, understanding how both reactors and nuclear weapons work. We examine safety and waste concerns, as well as nuclear proliferation. We look at new reactor concepts. For fusion we address the physics of confining hot, ionized gases, called plasmas. We address the control of large-scale instabilities and small-scale turbulence. We examine progress and prospects, as well as challenges, for the development of economically attractive fusion power.

Topics include the properties and nature of galaxies, quasars, clusters, superclusters, the large-scale structure of the universe, dark matter, dark energy, the formation and evolution of galaxies and other structures, microwave background radiation, and the evolution of the universe from the Big Bang to today. Two 90-minute lectures. Prerequisites: MAT 201, 202; PHY 207, 208. Designed for science and engineering majors.

Stars form from the interstellar medium (ISM), and the nuclear fusion that powers stars is also the main energy source in the ISM. This course discusses the structure and evolution of the ISM and 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; structure of stellar interiors; radiation transport; production of energy by nucleosynthesis; stellar evolution and end states; effects of stars on interstellar environment. Prerequisites: MAT 201, 202; PHY 208, 301 or permission of instructor.

A broad overview of the discipline of architecture: its history, theories, methodologies, and its manners of thinking and working. Rather than a chronological survey, the course will be organized thematically, with examples drawn from a range of historical periods as well as contemporary practice. Through lectures, readings, precepts, and studio sessions, students will acquire a working knowledge of key texts, buildings, and architectural concepts. Two lectures, one preceptorial.

The first in a series of design studios offered to students interested in majoring in architecture. The course will introduce architecture as an "impure'' plastic art, inseparable from a network of forces acting upon it. The student will be confronted with progressively complex exercises involving spatial relations in two dimensions, three dimensions, and time. The course will stress experimentation while providing an analytical and creative framework to develop an understanding of structure and materials as well as necessary skills in drawing and model making. Two three-hour studios with lectures included.

The course focuses on the social forces that shape design thinking. Its objective is to introduce architectural and urban design issues to build design and critical thinking skills from a multidisciplinary perspective. The studio is team-taught from faculty across disciplines to expose students to the multiple forces within which design operates.

This course sets out two goals: the first is to understand the theories and techniques of geometry in architectural representation; the second is to develop the student's drawing sensibilities through 5 thematic drawing projects engaging both digital and manual techniques. Each new theme will be introduced through a lecture, tutorial, and discussion including a number of specific readings related to the topic at hand. The second class will be an individual desk crit to discuss the development of each drawing project. The third class will consist of a group pin-up review of each drawing experiment.

This course examines two places that play an outsized role in the American economy: Wall Street and Silicon Valley. They are distinct and similarly enduring locations. They embody a divide between urban and suburban, East Coast and West Coast, skyscrapers and office parks, tradition and innovation, conservative and liberal. Despite the ubiquity of electronic trading, firms still congregate in Lower Manhattan. Tech workers fight traffic to maintain a presence in Mountain View. What makes these places endure? How do their histories, architecture, economic dynamics, and distinct cultures shape them as places?