activity
20162021
most citedLogamediate Inflation in f(T) Teleparallel Gravity

34 citations · 88 across the 3 of their papers we have counts for

collaborators

9 papers

gr-qc202126 cited

Primordial black holes formation and secondary gravitational waves in nonminimal derivative coupling inflation

Zeinab Teimoori, Kazem Rezazadeh, Kayoomars Karami

We study the possibility of the Primordial Black Holes (PBHs) formation with the aim of finding a considerable fraction of Dark Matter (DM), using the gravitationally enhanced fric…

astro-ph.CO202128 cited

Mechanism of primordial black holes production and secondary gravitational waves in -attractor Galileon inflationary scenario

Zeinab Teimoori, Kazem Rezazadeh, Mariwan Ahmed Rasheed +1

We study the process of the Primordial Black Holes (PBHs) production in the novel framework, namely -attractor Galileon inflation (G-inflation) model. In our framework, we take…

gr-qc2020

The growth of DM and DE perturbations in DBI non-canonical scalar field scenario

K. Rezazadeh, S. Asadzadeh, K. Fahimi +2

We study the effect of varying sound speed on clustering dark energy in the Dirac-Born-Infeld (DBI) scenario. The DBI action is included in the class of -essence models, and it…

hep-th2019

Non-Minimal M-flation

Amjad Ashoorioon, Kazem Rezazadeh

We show how in a matrix inflationary model in which there is a non-minimal coupling between the matrix inflatons and gravity --hence dubbed Non-$\MM$-flation-- some of the disadvan…

gr-qc2018

Warm DBI inflation with constant sound speed

S. Rasouli, K. Rezazadeh, A. Abdolmaleki +1

We study inflation with the Dirac-Born-Infeld (DBI) noncanonical scalar field in both the cold and warm scenarios. We consider the Anti-de Sitter warp factor for…

gr-qc2018

Structure formation in clustering DBI dark energy model with constant sound speed

K. Fahimi, K. Karami, S. Asadzadeh +1

Within the framework of DBI non-canonical scalar field model of dark energy, we study the growth of dark matter perturbations in the both linear and non-linear regimes. In our DBI…