Non-Markovian open quantum system approach to the early universe: I. Damping of gravitational waves by matter

Abstract

By revising the application of the open quantum system approach to the early universe and extending it to the conditions beyond the Markovian approximation, we obtain a new non-Markovian quantum Boltzmann equation. Throughout the paper, we also develop an extension of the quantum Boltzmann equation to describe the processes that are irreversible at the macroscopic level. This new kinetic equation is, in principle, applicable to a wide variety of processes in the early universe. For instance, using this equation one can accurately study the microscopic influence of a cosmic environment on a system of cosmic background photons or stochastic gravitational waves. In this paper, we apply the non-Markovian quantum Boltzmann equation to study the damping of gravitational waves propagating in a medium consisting of decoupled ultra-relativistic neutrinos. For such a system, we study the time evolution of the intensity and the polarization of the gravitational waves. It is shown that, in contrast to intensity and linear polarization which are damped, the circular polarization (V-mode) of the gravitational wave (if present) is amplified by propagating through such a medium.

Relativistic viscous effects on the primordial gravitational waves spectrum

“…Among the effects regarding the non-free evolution of pGW, i.e. Π TT ij = 0, we mention the damping due to free-streaming particles [5][6][7][8][9][12][13][14][15] and the absorption of GW while propagating in a viscous medium [16][17][18][19][20][21][22][23][24][25][26][27][28]. We also remark the studies on the angular anisotropies of GW background [29,30].…”