Speaker
Shamaila Rani
(Institute for Theoretical Physics and Cosmology, Zhejiang University of Technology, Hangzhou 310023, China)
Description
For illustration of the cosmic accelerated expansion of the universe, we will consider the modified Friedmann equations of some torsion-based theory of gravity. In this way, the cosmological parameters such as equation of state, phase-plane, squared speed of sound etc are being developed and examined graphically. For more insights of parameters, power-law forms of scale factor and parameterized forms of Hubble parameter are utilized.
Primary author
Shamaila Rani
(Institute for Theoretical Physics and Cosmology, Zhejiang University of Technology, Hangzhou 310023, China)
