ar X iv : g r - qc / 9 90 60 45 v 2 1 5 Ju n 19 99 FRW - TYPE UNIVERSE WITH VARIABLE G AND Λ Arbab
نویسنده
چکیده
We have considered a cosmological model with a cosmological term of the form Λ = 3α ˙ R 2 R 2 + β ¨ R R , α, β = cont. The cosmological term is found to decrease as t −2 and the rate of particle creation is smaller than the Steady State value. Solutions with β = 3α in the radiation dominated era and β = 6α in the matter dominated era are equivalent to the FRW results. We have found an inflationary solution of the de-Sitter type with β = 3 − 3α. The model is found to resolve the problems of the Standard Model. Very recent results [1] suggest that the age of the universe is about 11 − 14 billion years. However results obtained from Standard Model of cosmology are not consistent with these findings. Numerous models have been presented to reconcile these contradiction with observations. Only few of these models have given a satisfactory solution. The presence of a cosmological constant (Λ) in a given cosmology prolongs the age of the universe. The inflationary paradigm requires the Universe to have a critical density but observations do not support this. One of the motivations for introducing Λ term is to reconcile the age parameter and the density parameter of the universe with current observational data. In an attempt to resolve these problems with current observations, we suggest a variation law for the cosmological constant of the form Λ = 3α ˙ R 2 R 2 + β ¨ R R , α, β = const. Observational data indicate that Λ ∼ 10 −55 cm −2 while particle physics prediction for Λ is greater than this value by a factor of order 10 120. This discrepancy is known as the cosmological constant problem. It is interesting that this decay law helps to resolve this problem. The entropy problem which exists in the Standard Model can be solved by the proposed decay law. The success of the inflationary model in extending the Big Bang model strengthen the theoretical prejudice toward a flat universe. In this paper we will consider a flat universe. Therefore this model preserves the spirit of the inflationary scenario. This inflationary solution is built in the model. The present model resolves many, if not all, of Standard Model
منابع مشابه
ar X iv : g r - qc / 0 60 81 07 v 1 2 3 A ug 2 00 6 FRW UNIVERSE WITH VARIABLE G and Λ - TERMS
A new class of exact solutions of Einstein’s field equations with a perfect fluid source, variable gravitational coupling G and cosmological term Λ for FRW spacetime is obtained by considering variable deceleration parameter models for the universe. The nature of the variables G(t), Λ(t) and the energy density ρ(t) have been examined for three cases : (i) exponential (ii) polynomial and (iii) s...
متن کاملar X iv : g r - qc / 9 90 70 03 v 1 1 J ul 1 99 9 Cosmological models with variable ” constants ”
The behavior of the ”constants”, G, c, h̄, a, e, mi and Λ, considering them as variable, in the framework of a flat cosmological model with FRW symmetries described by a bulk viscous fluid and considering mechanisms of adiabatic matter creation are investigated. Within two models; one with radiation predominance and another of matter predominance, this behavior are studied.
متن کاملar X iv : a st ro - p h / 98 10 23 9 v 1 1 5 O ct 1 99 8 Cosmological Implications of The Bulk Viscous Model With Variable G And Λ ARBAB
We have investigated the cosmological implications of the bulk viscous cosmological model with variable G and Λ. These results are found to be compatible with the present observations. The classical cosmological tests for this model encompass the Freese et al. ones. The model has some spirits of the Standard Model. The inflationary solution which solves the Standard Model problems is obtained a...
متن کاملar X iv : g r - qc / 0 30 50 41 v 1 1 1 M ay 2 00 3 Brane - Universes with Variable G and Λ ( 4 )
We investigate the cosmological consequences of a brane-world theory which incorporates time variations in the gravitational coupling G and the cosmological term Λ (4). We analyze in detail the model where ˙ G/G ∼ H and Λ (4) ∼ H 2 , which seems to be favored by observations. We show that these conditions single out models with flat space sections. We determine the behavior of the expansion sca...
متن کاملar X iv : g r - qc / 0 51 11 56 v 1 2 9 N ov 2 00 5 Adiabatic Particle Production with Decaying Λ and Anisotropic Universe
The inclusion of cosmological constant into Einstein field equation was done primarily by Einstein himself with a view to model a static universe. Later he discarded the cosmological constant (and commented [1] “...... the biggest blunder of my life”), on the basis of the observational data supporting the expansion of the universe. Subsequently, it was reintroduced and then omitted to match wit...
متن کامل