Stability of Accelerating Cosmology in Two Scalar-Tensor Theory: Little Rip <em>versus</em> de Sitter

We develop the general reconstruction scheme in two scalar model. The quintom-like theory which may describe (different) non-singular Little Rip or de Sitter cosmology is reconstructed. The number of scalar phantom dark energy models (with Little Rip cosmology or asymptotically de Sitter evolution)...

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Main Authors: Yusaku Ito, Shin’ichi Nojiri, Sergei D. Odintsov
Format: Article
Language:English
Published: MDPI AG 2012-08-01
Series:Entropy
Subjects:
Online Access:http://www.mdpi.com/1099-4300/14/8/1578
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author Yusaku Ito
Shin’ichi Nojiri
Sergei D. Odintsov
author_facet Yusaku Ito
Shin’ichi Nojiri
Sergei D. Odintsov
author_sort Yusaku Ito
collection DOAJ
description We develop the general reconstruction scheme in two scalar model. The quintom-like theory which may describe (different) non-singular Little Rip or de Sitter cosmology is reconstructed. The number of scalar phantom dark energy models (with Little Rip cosmology or asymptotically de Sitter evolution) is presented. Stability issue of such dark energy cosmologies as well as the flow to fixed points are studied. The stability of Little Rip universe which leads to dissolution of bound objects sometime in future indicates that no classical transition to de Sitter space occurs. The possibility of unification of inflation with Little Rip dark energy in two scalar theory is briefly mentioned.
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spelling doaj.art-c9bf2f59b1dc445d984a776d309f43fb2022-12-22T04:22:18ZengMDPI AGEntropy1099-43002012-08-011481578160510.3390/e14081578Stability of Accelerating Cosmology in Two Scalar-Tensor Theory: Little Rip <em>versus</em> de SitterYusaku ItoShin’ichi NojiriSergei D. OdintsovWe develop the general reconstruction scheme in two scalar model. The quintom-like theory which may describe (different) non-singular Little Rip or de Sitter cosmology is reconstructed. The number of scalar phantom dark energy models (with Little Rip cosmology or asymptotically de Sitter evolution) is presented. Stability issue of such dark energy cosmologies as well as the flow to fixed points are studied. The stability of Little Rip universe which leads to dissolution of bound objects sometime in future indicates that no classical transition to de Sitter space occurs. The possibility of unification of inflation with Little Rip dark energy in two scalar theory is briefly mentioned.http://www.mdpi.com/1099-4300/14/8/1578dark energyscalar tensor theorylittle rip
spellingShingle Yusaku Ito
Shin’ichi Nojiri
Sergei D. Odintsov
Stability of Accelerating Cosmology in Two Scalar-Tensor Theory: Little Rip <em>versus</em> de Sitter
Entropy
dark energy
scalar tensor theory
little rip
title Stability of Accelerating Cosmology in Two Scalar-Tensor Theory: Little Rip <em>versus</em> de Sitter
title_full Stability of Accelerating Cosmology in Two Scalar-Tensor Theory: Little Rip <em>versus</em> de Sitter
title_fullStr Stability of Accelerating Cosmology in Two Scalar-Tensor Theory: Little Rip <em>versus</em> de Sitter
title_full_unstemmed Stability of Accelerating Cosmology in Two Scalar-Tensor Theory: Little Rip <em>versus</em> de Sitter
title_short Stability of Accelerating Cosmology in Two Scalar-Tensor Theory: Little Rip <em>versus</em> de Sitter
title_sort stability of accelerating cosmology in two scalar tensor theory little rip lt em gt versus lt em gt de sitter
topic dark energy
scalar tensor theory
little rip
url http://www.mdpi.com/1099-4300/14/8/1578
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AT shinichinojiri stabilityofacceleratingcosmologyintwoscalartensortheorylittleripltemgtversusltemgtdesitter
AT sergeidodintsov stabilityofacceleratingcosmologyintwoscalartensortheorylittleripltemgtversusltemgtdesitter