A closed universe with hybrid nonlocality
Abstract
In this paper, we explore some cosmological solutions of the Friedmann–Lemaître–Robertson–Walker (FLRW) closed universe with nonlocal de Sitter gravity √dS and nonlocal scalar field which has its origin in p-adic string theory. In this case, we have that both geometrical and matter sectors of equations of motion (EoM) are nonlocal. The cosmological constant Λ plays a role of dark energy (DE) and is related to the mass of scalar field as m=ℏc√Λ6=1.5×10−69kg. We found that the cosmological constant Λ depends on prime number p as a discrete parameter and we conjectured that Λ is not constant during the universe evolution.