Inflection point of coupled quintessence

IF 4.2 3区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
Jaskirat Kaur , S.D. Pathak , Vikash Kumar Ojha , Maxim Yu Khlopov
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引用次数: 0

Abstract

In this paper, we investigate the behavior of coupled quintessence at inflection point in the accelerated expansion of the universe. We consider spatially homogeneous quintessence coupled with the matter with two coupling parameters as Q=3αHρm and Q=3βρṁ. We obtain the inflection point for the power law form of potential V(ϕ)=V3(ϕϕ0)3 and its generalized form in two coupled quintessence models.

耦合精粹的拐点
在本文中,我们研究了宇宙加速膨胀拐点处耦合五子星的行为。我们考虑了与物质耦合的空间均质五子星,其两个耦合参数分别为 Q=3αHρm 和 Q=3βρṁ。我们得到了两个耦合五芒星模型中幂律形式的势 V(ϕ)=V3(ϕ-ϕ0)3 及其广义形式的拐点。
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来源期刊
Astroparticle Physics
Astroparticle Physics 地学天文-天文与天体物理
CiteScore
8.00
自引率
2.90%
发文量
41
审稿时长
79 days
期刊介绍: Astroparticle Physics publishes experimental and theoretical research papers in the interacting fields of Cosmic Ray Physics, Astronomy and Astrophysics, Cosmology and Particle Physics focusing on new developments in the following areas: High-energy cosmic-ray physics and astrophysics; Particle cosmology; Particle astrophysics; Related astrophysics: supernova, AGN, cosmic abundances, dark matter etc.; Gravitational waves; High-energy, VHE and UHE gamma-ray astronomy; High- and low-energy neutrino astronomy; Instrumentation and detector developments related to the above-mentioned fields.
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