In 1972, Zeldovich proposed the methodology of
the electron positron pair production which can be used to approach the Early
Universe cosmology. In this paper, we first discuss this approach in relation
to an upper bound of a minimum time length, which compared to certain recent
graviton mass study, creates a productive cosmological scenario.
Namely, a
non-zero graviton mass gives a non-trivial a minimum scale factor and for a
temperature varying cosmological “constant” parameter leads to Quintessence.
Afterwards, we first consider more representations of density, and then compare
density in the case of certain strengths for the magnetic nonrotating universe.
In other words, we involve the weak energy condition versus a more generalized
point of view. Read more>>>>>>>>>>>>>>

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