The creation of a quantum Universe is described by a density matrix which yields an ensemble of universes with the cosmological constant limited to a bounded rangeThe lower bound is defined by a cosmological bootstrap requirement (the self-consistent back reaction of hot matter). The upper cutoff results from the quantum effects of vacuum energy and the conformal anomaly mediated by a special ghost-avoidance renormalization. The Euclidean path integral formalism used for the construction of the fundamental density matrix for a mixed state of the Universe is justified by proving its correspondence to the microcanonical ensemble in quantum cosmology. The cosmological evolution starting with these initial conditions also have some new features: the stage of cosmic acceleration can be followed by a big boost singularity -- a rapid growth up to infinity of the scale factor acceleration parameter. From the developed approach it follows that the notion of the density matrix plays a more fundamental role than that was traditionally prescribed to it.
A.O., B., A.Yu., K. (2009). The problem of initial conditions in cosmology. MELVILLE : American Institute of Physics.
The problem of initial conditions in cosmology
KAMENCHTCHIK, ALEXANDR
2009
Abstract
The creation of a quantum Universe is described by a density matrix which yields an ensemble of universes with the cosmological constant limited to a bounded rangeThe lower bound is defined by a cosmological bootstrap requirement (the self-consistent back reaction of hot matter). The upper cutoff results from the quantum effects of vacuum energy and the conformal anomaly mediated by a special ghost-avoidance renormalization. The Euclidean path integral formalism used for the construction of the fundamental density matrix for a mixed state of the Universe is justified by proving its correspondence to the microcanonical ensemble in quantum cosmology. The cosmological evolution starting with these initial conditions also have some new features: the stage of cosmic acceleration can be followed by a big boost singularity -- a rapid growth up to infinity of the scale factor acceleration parameter. From the developed approach it follows that the notion of the density matrix plays a more fundamental role than that was traditionally prescribed to it.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.