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

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 ultrarelativistic 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 that are damped, the circular polarization (V mode) of the gravitational wave (if present) is amplified by propagating through such a medium.

Automated summary

This paper introduces a new non-Markovian quantum Boltzmann equation by revising the application of the open quantum system approach to the early universe, extending it beyond the Markovian approximation, and studying irreversible processes at the macroscopic level. The equation is applicable to various processes in the early Universe, and specifically used to study the damping of gravitational waves in a medium of decoupled ultrarelativistic neutrinos. Interestingly, the intensity and linear polarization of the gravitational waves are damped, while the circular polarization is amplified in such a medium.