A Mechanism for a small but nonzero cosmological constant · arXivDesk
gr-qc/9602030Feb 14, 1996uuencoded, gzipped Latex 7 pages including 4 postscript figures using epsf.sty; to appear in Proceedings of RESCEU Symposium "Cosmological Constant and the Evolution of the Universe," 7-10 November 1995, University of Tokyo
A Mechanism for a small but nonzero cosmological constant
Based on a thoeretical model in which scalar fields play crucial roles, we propose a mechanism to better understand a cosmological constant expected to be small (nearly comparable with the critical density) but nonzero as suggested strongly by the recent observations. We emphasize that a step further is needed beyond the simplest scenario of a decaying cosmological constant, according to which the effective Λ is not a true constant but decays like t−2, thus explaining why any effect of Λ which is assumed to be of the Planckian order of magnitude in the earliest Universe is at most 120 orders smaller today (t∼1060
Nearby in the stack
in units of the Planck time), without any extreme fine-tuning of the parameters. In addition to the overall smooth fall-off
∼t−2
, the total energy density, the sum of the contributions from the ordinary matter and the scalar fields, must show some leveling-off behavior, hence mimicking a truly constant
Λ
to fit the observations. We find that the desired behavior can be obtained by introducing two scalar fields interacting with each other in a specific manner. Many aspects of this model are discussed in detail, including the real origin of the whole mechanism, and how the parameters and the initial conditions of the theory can be determined by the cosomological parameters at the present epoch as well as the past history of the Universe.