“New Inflation” for a Bianchi Type IX Cosmological Model with Rotation and Dark Energy
IF 1.2
4区 物理与天体物理
Q3 ASTRONOMY & ASTROPHYSICS
引用次数: 0
Abstract
The first inflationary stage of the Bianchi type IX metric is considered for the case of inflation near the maximum potential according to the old terminology, “new inflation.” The evolution of rotation is studied with dark energy modeled by an anisotropic fluid.
包含旋转和暗能量的Bianchi IX型宇宙学模型的“新暴胀”
根据旧术语“新通货膨胀”，在通货膨胀接近最大潜力的情况下，考虑比安奇IX型指标的第一个通货膨胀阶段。用各向异性流体模拟暗能量，研究了暗能量的旋转演化。
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来源期刊
Gravitation and Cosmology
ASTRONOMY & ASTROPHYSICS-
CiteScore
1.70
自引率
22.20%
发文量
31
审稿时长
>12 weeks
期刊介绍：
Gravitation and Cosmology is a peer-reviewed periodical, dealing with the full range of topics of gravitational physics and relativistic cosmology and published under the auspices of the Russian Gravitation Society and Peoples’ Friendship University of Russia. The journal publishes research papers, review articles and brief communications on the following fields: theoretical (classical and quantum) gravitation; relativistic astrophysics and cosmology, exact solutions and modern mathematical methods in gravitation and cosmology, including Lie groups, geometry and topology; unification theories including gravitation; fundamental physical constants and their possible variations; fundamental gravity experiments on Earth and in space; related topics. It also publishes selected old papers which have not lost their topicality but were previously published only in Russian and were not available to the worldwide research community
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