Seminario di Nicolai Rothe (U. Wuppertal)

We will discuss some newly found solutions to the full massless semiclassical Einstein equation (SCE) in a cosmological setting (Λ=0).

After a short introduction to the relevant notions we present the SCE in a particular shape which allows for the construction of a Minkowski-vacuum-like states. In this setting, solving the SCE breaks down into solving a certain ODE which can be approached numerically and, at least generically, we obtain solutions that well fit physical expectations. Moreover, these solutions indicate dark energy as a quantum effect on cosmological metrics and, since in our model m=Λ=0, this may not be traced back to the usual, obvious dark-energy/cosmological constant effect of a quantum field. Also we will shortly discuss some more physical problems that can be solved by our model. To close the talk, we will briefly speak about de Sitter solutions of the model and thereby foreshadow another talk taking place at the University of Genova later in the week.