output
20042026
most citedThe holographic dark energy in non-flat Brans-Dicke cosmology

297 citations

Showing 2019Show all

9 papers · 1 filter

hep-th201924 cited

Critical behavior of AdS Gauss-Bonnet massive black holes in the presence of external string cloud

Hadi Ranjbari, Mehdi Sadeghi, M. Ghanaatian +1

Following previous study about AdS-Schwarzschild black holes minimally coupled to a cloud of strings in the context of massive gravity {Ghanaatian:2019} and inspired by strong conn…

hep-th20192 cited

Thermodynamics of static solutions in (n+1)-dimensional Quintic Quasitopological gravity

A. Bazrafshan, F. Naeimipour, A. R. Olamaei +1

Based on the fact that some important theories like string and M-theories predict spacetime with higher dimensions, so, in this paper, we aim to construct a theory of quintic quasi…

math.FA2019

Further Inequalities for the Numerical Radius of Hilbert Space Operators

S. Tafazoli, H. R. Moradi, S. Furuichi +1

In this article, we present some new inequalities for numerical radius of Hilbert space operators via convex functions. Our results generalize and improve earlier results by El-Had…

math.AC2019

Tilting Modules Over Gorensetein -Injective Gorensetein -flat Modules

M. Amini

Let T be a tilting module.In this paper, some relative Gorenstein projective and Gortenstein injective modules are studied.

math-ph20192 cited

Solvable Systems Featuring 2 Dependent Variables Evolving in Discrete-Time via 2 Nonlinearly-Coupled First-Order Recursion Relations with Polynomial Right-Hand Sides

Francesco Calogero, Farrin Payandeh

The evolution equations mentioned in the title of this paper read as follows: x~n = P(n)(x1; x2) , n = 1, 2 , where l is the "discrete-time" independent variable taking integer val…

math-ph20191 cited

Two Peculiar Classes of Solvable Systems Featuring 2 Dependent Variables Evolving in Discrete-Time via 2 Nonlinearly-Coupled First-Order Recursion Relations

Francesco Calogero, Farrin Payandeh

In this paper we identify certain peculiar systems of 2 discrete-time evolution equations,x~n = F^(n)(x1; x2) , n = 1, 2 , which are algebraically solvable. Here l is the "discrete…