On Viability of Inflation in Nonminimal Kinetic Coupling Theory

被引:9
作者
Avdeev, N. [1 ,2 ]
Toporensky, A. [2 ,3 ]
机构
[1] Lomonosov Moscow State Univ, Fac Phys, Dept Astrophys & Stellar Astron, Leninskie Gory 1-2, Moscow 119991, Russia
[2] Lomonosov Moscow State Univ, Sternberg Astron Inst, Univ Sky Prospekt 13, Moscow 119991, Russia
[3] Kazan Fed Univ, Kazan 420008, Russia
关键词
UNIVERSE SCENARIO; FLUCTUATIONS; FLATNESS; HORIZON;
D O I
10.1134/S0202289321030038
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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, (phi)over dot. 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. (phi)over dot. 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. (phi)over dot 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.
引用
收藏
页码:269 / 274
页数:6
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