Quantum Coherence Arguments for Cosmological Scale

Lindesay, James

Stanford Linear Accelerator Center

关键词: Theory-Hep,Other;    Amplitudes;    Symmetry;    Cosmological Constant;    Universe Theory-Hep,Other;   

DOI  :  10.2172/890780
RP-ID  :  SLAC-WP-050
RP-ID  :  AC02-76SF00515
RP-ID  :  890780

美国|英语

来源: UNT Digital Library

【 摘 要 】

Homogeneity and correlations in the observed CMB are indicative of some form of cosmological coherence in early times. Quantum coherence in the early universe would be expected to give space-like phase coherence to any effects sourced to those times. If dark energy de-coherence is assumed to occur when the rate of expansion of the relevant cosmological scale parameter in the Friedmann-Lemaitre equations is no longer supra-luminal, a critical energy density is immediately defined. It is shown that the general class of dynamical models so defined necessarily requires a spatially flat cosmology in order to be consistent with observed structure formation. The basic assumption is that the dark energy density which is fixed during de-coherence is to be identified with the cosmological constant. It is shown for the entire class of models that the expected amplitude of fluctuations driven by the dark energy de-coherence process is of the order needed to evolve into the fluctuations observed in cosmic microwave background radiation and galactic clustering. The densities involved during de-coherence which correspond to the measured dark energy density turn out to be of the electroweak symmetry restoration scale. In an inflationary cosmology, this choice of the scale parameter in the FL equations directly relates the scale of dark energy decoherence to the De Sitter scales (associated with the positive cosmological constants) at both early and late times.