On thermodynamic and quantum fluctuations of cosmological constant
G. E. Volovik
Low Temperature Laboratory, Helsinki University of Technology, Box 2200, FIN-02015 HUT, Finland
L. D. Landau Institute for Theoretical Physics RAS, 119334 Moscow, Russia
PACS: 04.60.-m, 98.80.Cq
Abstract
We discuss from the condensed-matter point of view the recent idea
that the Poisson fluctuations of cosmological constant about zero could be a
source of the observed dark energy [Padmanabhan,Ahmed]. We argue
that the thermodynamic fluctuations of Λ are much bigger. Since
the amplitude of fluctuations is where V is the
volume of the Universe, the present constraint on the cosmological
constant provides the lower limit for V, which is much bigger than the
volume within the cosmological horizon.