User profiles for Mohammad Sami
M. SamiDirector, Centre for Cosmology and Science Popularisation(CCSP), SGT Univ.,Gurugram … Verified email at sgtuniversity.org Cited by 14980 |
Dynamics of dark energy
EJ Copeland, M Sami, S Tsujikawa - International Journal of Modern …, 2006 - World Scientific
We review in detail a number of approaches that have been adopted to try and explain the
remarkable observation of our accelerating universe. In particular we discuss the arguments …
remarkable observation of our accelerating universe. In particular we discuss the arguments …
Cosmological dynamics of a phantom field
We study the general features of a dynamics of a phantom field in the cosmological context.
In the case of an inverse coshyperbolic potential, we demonstrate that the phantom field can …
In the case of an inverse coshyperbolic potential, we demonstrate that the phantom field can …
PBHs and GWs from 𝕋2-inflation and NANOGrav 15-year data
…, F Felegray, A Talebian, M Sami - Journal of Cosmology …, 2023 - iopscience.iop.org
In this paper, we propose a novel mechanism in Bbb T 2-inflation to enhance the power
spectrum large enough to seed primordial black holes (PBHs) formation. To accomplish this, we …
spectrum large enough to seed primordial black holes (PBHs) formation. To accomplish this, we …
[HTML][HTML] The fate of (phantom) dark energy universe with string curvature corrections
M Sami, A Toporensky, PV Tretjakov, S Tsujikawa - Physics Letters B, 2005 - Elsevier
We study the evolution of (phantom) dark energy universe by taking into account the higher-order
string corrections to Einstein–Hilbert action with fixed dilaton and modulus fields. While …
string corrections to Einstein–Hilbert action with fixed dilaton and modulus fields. While …
Inflation with a quartic potential in the framework of Einstein-Gauss-Bonnet gravity
EO Pozdeeva, MR Gangopadhyay, M Sami… - Physical Review D, 2020 - APS
We investigate inflationary dynamics in the framework of the Einstein-Gauss-Bonnet gravity.
In the model under consideration, the inflaton field is nonminimally coupled to the Gauss-…
In the model under consideration, the inflaton field is nonminimally coupled to the Gauss-…
Paradigm of warm quintessential inflation and production of relic gravity waves
We consider the framework of quintessential inflation in the warm background which is
caused by the dissipation of the scalar field energy density into relativistic degrees of freedom. …
caused by the dissipation of the scalar field energy density into relativistic degrees of freedom. …
[HTML][HTML] What is needed of a scalar field if it is to unify inflation and late time acceleration?
N Jaman, M Sami - Galaxies, 2022 - mdpi.com
Quintessential inflation refers to scenarios in which a single scalar field is used to describe
inflation and late time acceleration. This review is dedicated to the framework of …
inflation and late time acceleration. This review is dedicated to the framework of …
Impact of climate change on the incidence and transfer of food-and water-borne diseases
M Anas, MA Sami, Z Siddiqui, K Khatoon… - Microbiomes and the …, 2021 - Springer
Presently, climate change is considered as a serious global environmental challenge
influencing growth and survival of pathogens of many food- and water-borne diseases as well as …
influencing growth and survival of pathogens of many food- and water-borne diseases as well as …
Stability analysis of de Sitter solutions in models with the Gauss-Bonnet term
We investigate the scalar field dynamics of models with nonminimally coupled scalar fields
in the presence of the Gauss-Bonnet term and derive the structure of the effective potential …
in the presence of the Gauss-Bonnet term and derive the structure of the effective potential …
T2-inflation: Sourced by energy–momentum squared gravity
In this paper, we examine chaotic inflation within the context of the energy–momentum
squared gravity (EMSG) focusing on the energy–momentum powered gravity (EMPG) that …
squared gravity (EMSG) focusing on the energy–momentum powered gravity (EMPG) that …