Mean Free Path

“Lerner [is] among the most promising young poets now writing.”—Publishers Weekly “Sharp, ambitious, and impressive.” —Boston Review National Book Award finalist Ben Lerner turns to science once again for his guiding metaphor. “Mean free path” is the average distance a particle travels before colliding with another particle. The poems in Lerner’s third collection are full of layered collisions—repetitions, fragmentations, stutters, re-combinations—that track how language threatens to break up or change course under the emotional pressures of the utterance. And then there’s the larger collision of love, and while Lerner questions whether love poems are even possible, he composes a gorgeous, symphonic, and complicated one. You startled me. I thought you were sleeping In the traditional sense. I like looking At anything under glass, especially Glass. You called me. Like overheard Dreams. I’m writing this one as a woman Comfortable with failure. I promise I will never But the predicate withered. If you are Uncomfortable seeing this as portraiture Close your eyes. No, you startled Ben Lerner is the author of three books of poetry and was named a finalist for the National Book Award for his second book, Angle of Yaw. He holds degrees from Brown University, co-founded No: a journal of the arts, and teaches at the University of Pittsburgh.

University Physics is designed for the two- or three-semester calculus-based physics course. The text has been developed to meet the scope and sequence of most university physics courses and provides a foundation for a career in mathematics, science, or engineering. The book provides an important opportunity for students to learn the core concepts of physics and understand how those concepts apply to their lives and to the world around them. Due to the comprehensive nature of the material, we are offering the book in three volumes for flexibility and efficiency. Coverage and Scope Our University Physics textbook adheres to the scope and sequence of most two- and three-semester physics courses nationwide. We have worked to make physics interesting and accessible to students while maintaining the mathematical rigor inherent in the subject. With this objective in mind, the content of this textbook has been developed and arranged to provide a logical progression from fundamental to more advanced concepts, building upon what students have already learned and emphasizing connections between topics and between theory and applications. The goal of each section is to enable students not just to recognize concepts, but to work with them in ways that will be useful in later courses and future careers. The organization and pedagogical features were developed and vetted with feedback from science educators dedicated to the project. VOLUME II Unit 1: Thermodynamics Chapter 1: Temperature and Heat Chapter 2: The Kinetic Theory of Gases Chapter 3: The First Law of Thermodynamics Chapter 4: The Second Law of Thermodynamics Unit 2: Electricity and Magnetism Chapter 5: Electric Charges and Fields Chapter 6: Gauss's Law Chapter 7: Electric Potential Chapter 8: Capacitance Chapter 9: Current and Resistance Chapter 10: Direct-Current Circuits Chapter 11: Magnetic Forces and Fields Chapter 12: Sources of Magnetic Fields Chapter 13: Electromagnetic Induction Chapter 14: Inductance Chapter 15: Alternating-Current Circuits Chapter 16: Electromagnetic Waves

This title is part of UC Press's Voices Revived program, which commemorates University of California Press’s mission to seek out and cultivate the brightest minds and give them voice, reach, and impact. Drawing on a backlist dating to 1893, Voices Revived makes high-quality, peer-reviewed scholarship accessible once again using print-on-demand technology. This title was originally published in 1964.

An Introduction to the Gas Phase is adapted from a set of lecture notes for a core first year lecture course in physical chemistry taught at the University of Oxford. The book is intended to give a relatively concise introduction to the gas phase at a level suitable for any undergraduate scientist. After defining the gas phase, properties of gases such as temperature, pressure, and volume are discussed. The relationships between these properties are explained at a molecular level, and simple models are introduced that allow the various gas laws to be derived from first principles. Finally, the collisional behavior of gases is used to explain a number of gas-phase phenomena, such as effusion, diffusion, and thermal conductivity.

In his bold second book, Ben Lerner molds philosophical insight, political outrage, and personal experience into a devastating critique of mass society. Angle of Yaw investigates the fate of public space, public speech, and how the technologies of viewing—aerial photography in particular—feed our culture an image of itself. And it’s a spectacular view. The man observes the action on the field with the tiny television he brought to the stadium. He is topless, painted gold, bewigged. His exaggerated foam index finger indicates the giant screen upon which his own image is now displayed, a model of fanaticism. He watches the image of his watching the image on his portable TV on his portable TV. He suddenly stands with arms upraised and initiates the wave that will consume him. Haunted by our current “war on terror,” much of the book was written while Lerner was living in Madrid (at the time of the Atocha bombings and their political aftermath), as the author steeped himself in the history of Franco and fascism. Regardless of when or where it was written, Angle of Yaw will further establish Ben Lerner as one of our most intriguing and least predictable poets.

First published in 1988, this book is a comprehensive survey of the astrophysical characteristics of the hot gas which pervades clusters of galaxies. In our universe, clusters of galaxies are the largest organised structures. Typically they comprise hundreds of galaxies moving through a region of space ten million light years in diameter. The volume between the galaxies is filled with gas having a temperature of 100 million degrees. This material is a strong source of cosmic X-rays. Dr Sarazin describes the theoretical description of the origin, dynamics, and physical state of the cluster gas. Observations by radio and optical telescopes are also summarised. This account is addressed to professional astronomers and to graduate students. It is an exhaustive summary of a rapidly expanding field of research in modern astrophysics.