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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MDPI AG
2012-08-01
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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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id | doaj.art-c9bf2f59b1dc445d984a776d309f43fb |
institution | Directory Open Access Journal |
issn | 1099-4300 |
language | English |
last_indexed | 2024-04-11T13:18:31Z |
publishDate | 2012-08-01 |
publisher | MDPI AG |
record_format | Article |
series | Entropy |
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 |
work_keys_str_mv | AT yusakuito stabilityofacceleratingcosmologyintwoscalartensortheorylittleripltemgtversusltemgtdesitter AT shinichinojiri stabilityofacceleratingcosmologyintwoscalartensortheorylittleripltemgtversusltemgtdesitter AT sergeidodintsov stabilityofacceleratingcosmologyintwoscalartensortheorylittleripltemgtversusltemgtdesitter |