On Viability of Inflation in Nonminimal Kinetic Coupling Theory

IF 1.2 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
N. Avdeev, A. Toporensky
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引用次数: 5

Abstract

We consider the initial conditions for inflation in the nonminimal kinetic coupling theory. If inflation is driven solely by the kinetic term with no potential, the resulting number of e-folds depends only on the initial velocity of the scalar field, \(\dot{\phi}\). We write down the expression for the number of e-folds explicitly, and show that for physically reasonable values of the coupling constant, we can get 60 e-folds only for an exponentially big initial \(\dot{\phi}\). When the scalar field potential is taken into account, a double inflation scenario arises, where the first inflation is kinetic term driven, while the second one is potential term driven. In this case, we need not a very large \(\dot{\phi}\) to start with for 60 e-folds, on the other hand, some initial conditions lead to a physically inadmissible eternal inflation. We show numerically that in the measure used in the present paper only a smaller part of initial conditions leads to eternal inflation for reasonable values of the coupling constant.

Abstract Image

论非极小动力学耦合理论中暴胀的生存能力
我们考虑了非极小动力学耦合理论中暴胀的初始条件。如果暴胀仅由没有势能的动力学项驱动,则得到的e折叠数仅取决于标量场的初始速度\(\dot{\phi}\)。我们明确地写出了e-fold数目的表达式,并表明,对于物理上合理的耦合常数值,我们只能在初始值呈指数级大\(\dot{\phi}\)时得到60个e-fold。当考虑标量场势时,出现了双重膨胀情景,其中第一次膨胀是动能项驱动的,而第二次膨胀是势项驱动的。在这种情况下,我们不需要一个非常大的\(\dot{\phi}\)来开始60个e-fold,另一方面,一些初始条件导致物理上不可接受的永久暴胀。我们在数值上表明,在本文所使用的测度中,只有一小部分初始条件会导致耦合常数合理值的永久膨胀。
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来源期刊
Gravitation and Cosmology
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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