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![]() Carlip Quantum Gravity in 2+1 Dimensions † P. Hu Nonequilibrium Quantum Field Theory S. Brink Semi-Classical Methods for Nucleus-Nucleus Scattering † M. C´ el´ erier Structures in the Universe by Exact Methods: Formation, Evolution, Interactions D. Davies Quantum Fields in Curved Space † K. Broglia Oscillations in Finite Quantum Systems † N. Bernstein Kinetic Theory in the Expanding Universe † G. Henneaux The Cosmological Singularity † V. van Nieuwenhuizen Path Integrals and Anomalies in Curved Space † D. Talon Introduction to Classical Integrable Systems † F. Izquierdo Lie Groups, Lie Algebras, Cohomology and Some Applications in Physics † O. Anile Relativistic Fluids and Magneto-fluids: With Applications in Astrophysics and Plasma Physics J. Jonsson Quantum Geometry: A Statistical Field Theory Approach † A. Aarseth Gravitational N-Body Simulations: Tools and Algorithms † D. He is a member of the Royal Astronomical Society, specializes in gravitation and gravitational quantum physics, and is co-author of Gravitational Solitons (CUP, 2001).ĬAMBRIDGE MONOGRAPHS ON MATHEMATICAL PHYSICS S. E n r i c V e r d a g u e r is Professor of Physics at the University of Barcelona. His research in theoretical physics focuses on gravitation and quantum theory. He is a Fellow of the American Physical Society and co-authored Nonequilibrium Quantum Field Theory (CUP, 2008). H u is Professor of Physics at the University of Maryland. Covering over four decades of thematic development, this book is a valuable resource for researchers interested in quantum field theory, gravitation and cosmology. It explores the self-consistent description of both space-time and matter via the semiclassical Einstein equation of semiclassical gravity theory, exemplified by the inflationary cosmology, and fluctuations of quantum fields which underpin stochastic gravity, necessary for the description of metric fluctuations (spacetime foams). This book examines the effects of quantum field processes back-reacting on the background space-time which become important near the Planck time (10−43 sec). Combining the two yields quantum field theory in curved space-time, which is needed to understand quantum field processes in the early universe and black holes, such as the well-known Hawking effect. The two pillars of modern physics are general relativity and quantum field theory, the former describes the large scale structure and dynamics of space-time, the latter, the microscopic constituents of matter. S E M I C L A S S I C A L A N D S T O C H A S T I C G R AV I T Y Riemann tensor correlator in de Sitter -Įpilogue: Linkage with quantum gravity. ![]() ![]() Two-point metric perturbations in de Sitter. Stress-energy tensor fluctuations in de Sitter space. Structure formation in the early universe -īlack hole backreaction and fluctuations. Metric fluctuations in Minkowski spacetime -Ĭosmological backreaction with fluctuations. Metric correlations at one-loop : in-in and large N. Infrared behavior of interacting quantum fields -īackreaction of early universe quantum processes. Stress-energy tensor and correlation : point separation. Stress-energy tensor and correlators : zeta-function method. |
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