Speaker
Seyed Meraj Rasouli
(Universidade da Beira Interior)
Description
By proposing an appropriate dynamical deformation between the momenta associated with the scalar field (of the Sáez–Ballester theory) and scale factor of the spatially flat FLRW metric, we establish a modified cosmological model. Subsequently, for some particular cases, by focusing on the early epoch of the universe, we show that our model provides a more successful description for evolution of the universe with respect to the corresponding standard models.
Author
Seyed Meraj Rasouli
(Universidade da Beira Interior)
