scholarly journals Computing Dark Energy and Ordinary Energy of the Cosmos as a Double Eigenvalue Problem

2015 ◽  
Vol 06 (04) ◽  
pp. 384-395 ◽  
Author(s):  
Mohamed S. El Naschie
Symmetry ◽  
2021 ◽  
Vol 14 (1) ◽  
pp. 3
Author(s):  
Ivan Dimitrijevic ◽  
Branko Dragovich ◽  
Zoran Rakic ◽  
Jelena Stankovic

A nonlocal gravity model (2) was introduced and considered recently, and two exact cosmological solutions in flat space were presented. The first solution is related to some radiation effects generated by nonlocal dynamics on dark energy background, while the second one is a nonsingular time symmetric bounce. In the present paper, we investigate other possible exact cosmological solutions and find some the new ones in nonflat space. Used nonlocal gravity dynamics can change the background topology. To solve the corresponding equations of motion, we first look for a solution of the eigenvalue problem □(R−4Λ)=q(R−4Λ). We also discuss possible extension of this model with a nonlocal operator, symmetric under □⟷□−1, and its connection with another interesting nonlocal gravity model.


Nature ◽  
2010 ◽  
Author(s):  
Eugenie Samuel Reich
Keyword(s):  

Sign in / Sign up

Export Citation Format

Share Document