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211 - 220 of 258 results for: all courses

OSPPARIS 163: Advanced Biochemistry

Examine the biochemical bases of fundamental regulatory processes at the protein/enzyme level. Prerequisites: BIO 41 or HUMBIO 2A/3A or permission of instructor.
Terms: Win | Units: 3 | UG Reqs: WAY-SMA
Instructors: Simoni, R. (PI)

OSPSANTG 58: Living Chile: A Land of Extremes

Physical, ecological, and human geography of Chile. Perceptions of the Chilean territory and technologies of study. Flora, fauna, and human adaptations to regional environments. Guest lectures; field trips; workshops.
Terms: Aut, Spr, Sum | Units: 5 | UG Reqs: GER:DB-EngrAppSci, WAY-SMA
Instructors: Reid, S. (PI)

PEDS 51N: How Discovery and Innovation Have Transformed Medicine

Topics include the science behind vaccines and why some refuse vaccination, how antibiotics are discovered and what can be done about increasing resistance to antibiotics, stem cells and their potential use, the role of genomics in modern medicine, development of drugs to treat HIV/AIDS, discovery of surfactant, personal responsibility in health and wellness and how technology relates to the "cost conundrum" of healthcare in the U.S. Appreciate important connections between science, discovery and human health and think critically about the potential impact of new discoveries on life and death, and their ethical and spiritual boundaries.
Last offered: Spring 2016 | UG Reqs: WAY-SMA

PHIL 165: Philosophy of Physics (PHIL 265)

Graduate students register for 265.) TOPICS: Absolute and relational theories of space, time, and motion: the problem of motion from Descartes, Newton and Leibniz to Einstein and beyond. The principle of relativity leads from space and time to space-time. Mach¿s attempt to `relativize¿ inertia and its influence on Einstein in formulating the general theory of relativity. Space-time substantivalism and relationism. The problem of determinism in Einstein¿s ¿Lochbetrachtung¿, and the physical meaning of general covariance. Background independence as a requirement for fundamental physical theory, including quantum gravity. May be repeated for credit if content is different.
Terms: Aut | Units: 4 | UG Reqs: GER:DB-Hum, WAY-A-II, WAY-SMA | Repeatable for credit

PHYSICS 14N: Quantum Information: Visions and Emerging Technologies

What sets quantum information apart from its classical counterpart is that it can be encoded non-locally, woven into correlations among multiple qubits in a phenomenon known as ¿entanglement.¿ Will discuss paradigms for harnessing entanglement to solve hitherto intractable computational problems or to push the precision of sensors to their fundamental quantum mechanical limits. Will also examine challenges that physicists and engineers are tackling in the laboratory today to enable the quantum technologies of the future.
Terms: Spr | Units: 3 | UG Reqs: WAY-FR, WAY-SMA

PHYSICS 15: Stars and Planets in a Habitable Universe

Is the Earth unique in our galaxy? Students learn how stars and our galaxy have evolved and how this produces planets and the conditions suitable for life. Discussion of the motion of the night sky and how telescopes collect and analyze light. The life-cycle of stars from birth to death, and the end products of that life cycle -- from dense stellar corpses to supernova explosions. Course covers recent discoveries of extrasolar planets -- those orbiting stars beyond our sun -- and the ultimate quest for other Earths. Intended to be accessible to non-science majors, material is explored quantitatively with problem sets using basic algebra and numerical estimates. Sky observing exercise and observatory field trips supplement the classroom work.
Terms: Aut, Sum | Units: 3 | UG Reqs: GER: DB-NatSci, WAY-SMA

PHYSICS 16: The Origin and Development of the Cosmos

How did the present Universe come to be? The last few decades have seen remarkable progress in understanding this age-old question. Course will cover the history of the Universe from its earliest moments to the present day, and the physical laws that govern its evolution. The early Universe including inflation and the creation of matter and the elements. Recent discoveries in our understanding of the makeup of the cosmos, including dark matter and dark energy. Evolution of galaxies, clusters, and quasars, and the Universe as a whole. Implications of dark matter and dark energy for the future evolution of the cosmos. Intended to be accessible to non-science majors, material is explored quantitatively with problem sets using basic algebra and numerical estimates.
Terms: Win, Sum | Units: 3 | UG Reqs: GER: DB-NatSci, WAY-SMA

PHYSICS 17: Black Holes and Extreme Astrophysics

Black holes represent an extreme frontier of astrophysics. Course will explore the most fundamental and universal force -- gravity -- and how it controls the fate of astrophysical objects, leading in some cases to black holes. How we discover and determine the properties of black holes and their environment. How black holes and their event horizons are used to guide thinking about mysterious phenomena such as Hawking radiation, wormholes, and quantum entanglement. How black holes generate gravitational waves and powerful jets of particles and radiation. Other extreme objects such as pulsars. Relevant physics, including relativity, is introduced and treated at the algebraic level. No prior physics or calculus is required, although some deep thinking about space, time, and matter is important in working through assigned problems.
Terms: Spr | Units: 3 | UG Reqs: GER: DB-NatSci, WAY-SMA

PHYSICS 18N: Frontiers in Theoretical Physics and Cosmology

Preference to freshmen. The course will begin with a description of the current standard models of gravitation, cosmology, and elementary particle physics. We will then focus on frontiers of current understanding including investigations of very early universe cosmology, string theory, and the physics of black holes.
Terms: Aut | Units: 3 | UG Reqs: GER: DB-NatSci, WAY-SMA

PHYSICS 19: How Things Work: An Introduction to Physics

Introduction to the principles of physics through familiar objects and phenomena, including airplanes, cameras, computers, engines, refrigerators, lightning, radio, microwave ovens, and fluorescent lights. Estimates of real quantities from simple calculations. Prerequisite: high school algebra and trigonometry.
Last offered: Autumn 2014 | UG Reqs: GER: DB-NatSci, WAY-SMA
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