activity
20072023
most citedLogarithmic corrections of charged hairy black hole in (2+1) dimension

95 citations · 901 across the 31 of their papers we have counts for

collaborators

31 papers

hep-th2023★ 25 cited

de Sitter Swampland Conjecture in String Field Inflation

J. Sadeghi, B. Pourhassan, S. Noori Gashti +2

In this paper, we study a particular type of inflation by using non-local Friedman equations that are somehow derived from the zero levels of string field theory and express a tach…

gr-qc2022★ 10 cited

Smeared Mass Source Wormholes in Modified Gravity with the Lorentzian Density Distribution Function

J. Sadeghi, B. Pourhassan, S. Noori Gashti +1

Wormholes are speculative structures linking disparate space-time points. Their geometry can be obtained by solving Einstein equations with tolerating the violation of null energy…

astro-ph.CO2022★ 36 cited

Pleasant behavior of swampland conjectures in the face of specific inflationary models

S. Noori Gashti, J. Sadeghi, B. Pourhassan

Recently researchers have been studying various conditions as swampland criteria in cosmological implications. They have studied many inflation models with different swampland cond…

gr-qc2022★ 43 cited

Weak Gravity Conjecture, Black Branes and Violations of Universal Thermodynamic Relation

J. Sadeghi, B. Pourhassan, S. Noori Gashti +1

The universal thermodynamic relations between corrections to entropy and extremality for various black holes solutions have been studied. In this regard, we hereby consider a numbe…

gr-qc2021★ 28 cited

Swampland Conjecture and Inflation Model from Brane Perspective

J. Sadeghi, B. Pourhassan, S. Noori Gashti +1

Over the past few decades, inflation models have been studied by researchers from different perspectives and conditions in order to introduce a model for the expanding universe. In…

gr-qc2021★ 23 cited

Cosmic evolution of the logarithmic f(R) model and the dS swampland conjecture

J. Sadeghi, B. Pourhassan, S. Noori Gashti +2

In this paper, we study the inflationary scenario in logarithmic f(R) gravity, where the rate of inflation roll is constant. On the other hand, our gravitational f(R) model is a po…