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https://doi.org/10.3938/NPSM.68.147
Dynamical Analysis in Nonlocal Gravity
New Phys.: Sae Mulli 2018; 68: 147~154
Published online January 31, 2018;  https://doi.org/10.3938/NPSM.68.147
© 2018 New Physics: Sae Mulli.

Seoktae KOH*

Department of Science Education, Jeju National University, Jeju 63243, Korea
Correspondence to: kundol.koh@jejunu.ac.kr
Received September 15, 2017; Revised October 28, 2017; Accepted November 10, 2017.
cc This is an open-access article distributed under the terms of the Creative Commons Attribution Non-Commercial License (http://creativecommons.org/licenses/by-nc/3.0/) which permits unrestricted non-commercial use, distribution, and reproduction in any medium, provided the original work is properly cited.
Abstract
We consider nonlocal gravity to explain the late time acceleration of the Universe without introducing dark energy. In this work, we use the localized form of the action for nonlocal gravity by introducing two scalar fields and investigate the attractor solutions for an accelerating Universe. If an atteractor solution exists the stability of that attractor is checked through a dynamical analysis. Firstly, we find the fixed points by assuming de Sitter solutions and then check the stability of the fixed points. We then extend the results to more general cases to find the fixed points, after which we check the stability of those fixed points; we also looked for accelerating solutions.
PACS numbers: 98.80.Cq, 04.62.+v
Keywords: Nonlocal gravity, Accelerating universe, Dynamical analysis


January 2018, 68 (1)
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