output
20022026
most citedMoSi2N4 single-layer: a novel two-dimensional material with outstanding mechanical, thermal, electronic, optical, and photocatalytic properties

256 citations

Showing 2014Show all

23 papers · 1 filter

gr-qc2014★ 37 cited

Stability of cylindrical thin shell wormhole during evolution of universe from inflation to late time acceleration

M. R. Setare, A. Sepehri

In this paper, we consider the stability of cylindrical wormholes during evolution of universe from inflation to late time acceleration epochs. We show that there are two types of…

hep-th2014★ 51 cited

On the Generalized Minimal Massive Gravity

M. R. Setare

In this paper we study the Generalized Minimal Massive Gravity (GMMG) in asymptotically background. The generalized minimal massive gravity theory is realized by adding the…

gr-qc2014★ 19 cited

Late time acceleration in a non-commutative model of modified cosmology

B. Malekolkalami, K. Atazadeh, B. Vakili

We investigate the effects of noncommutativity between the position-position, position-momentum and momentum-momentum of a phase space corresponding to a modified cosmological mode…

quant-ph2014★ 104 cited

Non-Markovianity through flow of information between a system and an environment

S. Haseli, G. Karpat, S. Salimi +6

Exchange of information between a quantum system and its surrounding environment plays a fundamental role in the study of the dynamics of open quantum systems. Here we discuss the…

gr-qc2014★ 48 cited

Intermediate inflation from a non-canonical scalar field

K. Rezazadeh, K. Karami, P. Karimi

We study the intermediate inflation in a non-canonical scalar field framework with a power-like Lagrangian. We show that in contrast with the standard canonical intermediate inflat…

physics.gen-ph2014★ 6 cited

Inflation driven by q-de Sitter

M. R. Setare, D. Momeni, V. Kamali +1

We propose a generalised de Sitter scale factor for the cosmology of early and late time universe, including single scalar field is called as inflaton. This form of scale factor ha…