Quantum Noise in Gravitation and Cosmology

We begin by enumerating the many processes in gravitation and cosmology where quantum noise and fluctuations play an active role such as particle creation, galaxy formation and entropy generation. Using the influence functional we first explain the origin and nature of noise in quantum systems interacting with an environment at a finite temperature. With linear coupling to nonohmic baths or at low temperatures, colored noise and nonlocal dissipation would appear and for nonlinear coupling multiplicative noise is generally expected. We derive a generalized fluctuation- dissipation relation for these systems. Then using a model of quantum Brownian motion in a bath of parametric oscillators, we show how noise and dissipation can be related to the Bogolubov coefficients of parametric amplification, which in the second-quantized sense, depicts cosmological particle creation in a dynamic background. We then calculate the influence functional and study the noise characteristics of quantum fields as probed by a particle detector. As examples, we show that an uniformly- accelerated observer in flat space or an inertial observer in an exponentially expanding (de Sitter) universe would see a thermal particle spectrum, recovering the well-known results of Unruh and Gibbons and Hawking , as inspired by the Hawking effect in black holes. We show how this method can be effectively used for treating the backreaction of particle creation and other quantum field processes on the