Compatibility of Einstein-Gauss-Bonnet inflation theory with non-minimal derivative coupling in the constant-roll

Naufal Aulia Adam, G. Hikmawan, F. P. Zen
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Abstract

Inflation is a theory in cosmology that explains that the early universe experienceda very fast expansion in a very short time and is able to explain some cosmological problemsand the presence of gravitational waves generated during the inflation period. Based on theevent GW170817, it was found that c2t = 1, which indicates that the speed of gravitationalwaves is nearly equal to the speed of light. This contradicts several modified theories of gravity,one of which is the Einstein-Gauss-Bonnet theory. This paper examines the compatibility ofEinstein-Gauss-Bonnet inflation theory with the GW170817 phenomenon, with the addition ofthe Non-minimal derivative coupling term and the constant-roll approach and its characteristics.The formulation of observational quantities is carried out using Horndeski theory and EffectiveField Theory with ADM formalism and the calculations are done numerically. The constantvalues are selected in such a way that the spectral index values and tensor-scalar ratios are closeto the 2018 Planck data. The results found that this theory is compatible with GW170817 withthe influence of Gauss-Bonnet term and constant-roll parameter β most dominant.
Einstein-Gauss-Bonnet膨胀理论与常滚非极小导数耦合的相容性
暴胀是宇宙学中的一种理论,它解释了早期宇宙在很短的时间内经历了非常快速的膨胀,并且能够解释一些宇宙学问题以及暴胀期间产生的引力波的存在。基于GW170817事件,发现c2t = 1,这表明引力波的速度几乎等于光速。这与一些修正的引力理论相矛盾,其中之一是爱因斯坦-高斯-邦纳理论。本文通过增加非极小导数耦合项和常滚方法,研究了爱因斯坦-高斯-邦纳暴胀理论与GW170817现象的相容性及其特性。利用Horndeski理论和有效场论的ADM形式进行了观测量的计算,并进行了数值计算。常数值的选择使光谱指标值和张量标量比接近2018年普朗克数据。结果表明,该理论与GW170817基本一致,其中高斯-博内项和常滚参数β的影响最大。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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