Over the decades since he was first hailed by critics and filmmakers around the world, Sergei Eisenstein has assumed many identities. Originally cast as a prophet of revolution and the maestro of montage, and later seen as both a victim of and apologist for Stalin's tyranny, the scale and impact of Eisenstein's legacy has continued to grow. If early research on Eisenstein focused on his directorial work – from the legendary Battleship Potemkin and October to the still-controversial Ivan the Terrible – with time scholars have discovered many other aspects of his multifarious output. In recent years, multimedia exhibitions, access to his vast archive of drawings, and publication of his previously censored theoretical writings have cast Eisenstein in a new light. Deeply engaged with some of the leading thinkers and artists of his own time, Eisenstein remains a focus for many of their successors, contested as well as revered. Over half a century since his death in 1948, an ambitious treatise that he hoped would be his major legacy, Method, has finally been published. Eisenstein's lifelong search for an underlying unity that would link archaic art with film's modernity, individuals with their historic communities, and humans as a species with the universe, may have more appeal than ever today. And among his many thwarted film projects, those set in Mexico and what were once the Soviet Central Asian republics reveal complex and still-intriguing realms of speculation. In this ground-breaking collection, sixteen international scholars explore Eisenstein's prescient engagement with aesthetics, anthropology and psychology, his roots in diverse philosophical traditions, and his gender politics. What emerges has surprising relevance to contemporary media archaeology, intermediality, cognitive science, eco-criticism and queer studies, as well as confirming Eisenstein's prestige within present-day film and audiovisual media.

This book is concerned with discontinuous groups of motions of the unique connected and simply connected Riemannian 3-manifold of constant curva ture -1, which is traditionally called hyperbolic 3-space. This space is the 3-dimensional instance of an analogous Riemannian manifold which exists uniquely in every dimension n :::: 2. The hyperbolic spaces appeared first in the work of Lobachevski in the first half of the 19th century. Very early in the last century the group of isometries of these spaces was studied by Steiner, when he looked at the group generated by the inversions in spheres. The ge ometries underlying the hyperbolic spaces were of fundamental importance since Lobachevski, Bolyai and Gauß had observed that they do not satisfy the axiom of parallels. Already in the classical works several concrete coordinate models of hy perbolic 3-space have appeared. They make explicit computations possible and also give identifications of the full group of motions or isometries with well-known matrix groups. One such model, due to H. Poincare, is the upper 3 half-space IH in JR . The group of isometries is then identified with an exten sion of index 2 of the group PSL(2,

A gripping first-person account of how scientists came to understand our universe's mysterious structure J. Richard Gott was among the first cosmologists to propose that the structure of our universe is like a sponge made up of clusters of galaxies intricately connected by filaments of galaxies—a magnificent structure now called the "cosmic web" and mapped extensively by teams of astronomers. Here is his gripping insider's account of how a generation of undaunted theorists and observers solved the mystery of the architecture of our cosmos. The Cosmic Web begins with modern pioneers of extragalactic astronomy, such as Edwin Hubble and Fritz Zwicky. It goes on to describe how, during the Cold War, the American school of cosmology favored a model of the universe where galaxies resided in isolated clusters, whereas the Soviet school favored a honeycomb pattern of galaxies punctuated by giant, isolated voids. Gott tells the stories of how his own path to a solution began with a high-school science project when he was eighteen, and how he and astronomer Mario Jurič measured the Sloan Great Wall of Galaxies, a filament of galaxies that, at 1.37 billion light-years in length, is one of the largest structures in the universe. Drawing on Gott’s own experiences working at the frontiers of science with many of today’s leading cosmologists, The Cosmic Web shows how ambitious telescope surveys such as the Sloan Digital Sky Survey are transforming our understanding of the cosmos, and how the cosmic web holds vital clues to the origins of the universe and the next trillion years that lie ahead.

Complex analysis nowadays has higher-dimensional analoga: the algebra of complex numbers is replaced then by the non-commutative algebra of real quaternions or by Clifford algebras. During the last 30 years the so-called quaternionic and Clifford or hypercomplex analysis successfully developed to a powerful theory with many applications in analysis, engineering and mathematical physics. This textbook introduces both to classical and higher-dimensional results based on a uniform notion of holomorphy. Historical remarks, lots of examples, figures and exercises accompany each chapter.

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"Volume 209, number 985 (fourth of 5 numbers)."

Distilling into concise and focused formulations many of the main ideas that Mari Ruti has sought to articulate throughout her writing career, this book reflects on the general state of contemporary theory as it relates to posthumanist ethics, political resistance, subjectivity, agency, desire, and bad feelings such as anxiety. It offers a critique of progressive theory's tendency to advance extreme models of revolt that have little real-life applicability. The chapters move fluidly between several theoretical registers, the most obvious of these being continental philosophy, psychoanalytic theory, Butlerian ethics, affect theory, and queer theory. One of the central aims of Distillations is to explore the largely uncharted territory between psychoanalysis and affect theory, which are frequently pitted against each other as hopelessly incompatible, but which Ruti shows can be brought into a productive dialogue.

Animators work within a strictly defined, limited space that requires difficult artistic decisions. The blank frame presents a dilemma for all animators, and the decision of what to include and leave out raises important questions about artistry, authorship, and cultural influence. In Animating Space: From Mickey to WALL-E, renowned scholar J. P. Telotte explores how animation has confronted the blank template, and how responses to that confrontation have changed. Focusing on American animation, Telotte tracks the development of animation in line with changing cultural attitudes toward space and examines innovations that elevated the medium from a novelty to a fully realized art form. From Winsor McCay and the Fleischer brothers to the Walt Disney Company, Warner Bros., and Pixar Studios, Animating Space explores the contributions of those who invented animation, those who refined it, and those who, in the current digital age, are using it to redefine the very possibilities of cinema.

Detailed exposition of automorphic representations and their relation to string theory, for mathematicians and theoretical physicists.