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20242026
most citedCharged Wormhole Solutions in 4D Einstein-Gauss-Bonnet Gravity

7 citations · 10 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.CO2026

Models with Non-minimal Coupling in Primordial Universe and Cosmological Observations

Alireza Talebian, Hassan Firouzjahi, Fereshteh Felegary

A non-minimal coupling between gravity and the inflaton field is a generic contribution in inflationary cosmology. In this work, we consider models of inflation with a non-minimal…

gr-qc2025

k-inflation: Non-separable case meets ACT measurements

Tahere Fallahi Serish, Seyed Ali Hosseini Mansoori, Fereshteh Felegary +2

We investigate a non-separable subset of -essence in which the kinetic and potential sectors interact through an coupling, implemented via a potential-dependent prefac…

gr-qc2025

Probing single-field inflation: predictions, constraints, and theoretical viewpoints

Fereshteh Felegary, Thammarong Eadkhong, Farruh Atamurotov +1

This work investigates a single-field inflationary model, a specific class of the K-essence models where a coupling term exists between canonical Lagrangian and the potential. This…

gr-qc2024★ 1 cited

Tilt and Tensor-to-Scalar Ratio in Multi-Scalar Field Inflation: Non-Sum-Separable Case

Fereshteh Felegary, Seyed Ali Hosseini Mansoori, Tahere Fallahi Serish +1

The canonical multi-scalar field inflation where the kinetic and potential terms are sum-separable is ruled out by the current observations for the chaotic-type potential $V=\sum_{…

gr-qc2024★ 7 cited

Charged Wormhole Solutions in 4D Einstein-Gauss-Bonnet Gravity

Piyachat Panyasiripan, Fereshteh Felegary, Phongpichit Channuie

In the present work, we construct models of static wormholes within the framework of 4-dimensional Einstein-Gauss-Bonnet (4D EGB) gravity an (an)isotropic energy momentum tensor (E…

astro-ph.CO2024★ 2 cited

Observational constraints on thawing quintessence scalar field model

Fereshteh Felegary, Kazuharu Bamba

Thawing quintessence scalar field models with the various potential forms to explain the late-time cosmic acceleration are compared to the ΛCDM model in detail by analyzing cosmolo…