works on

From the 1 of 13 linked papers with an AI index.

activity
20242026
collaborators

13 papers

astro-ph.CO2026

Effective reheating in Gauss--Bonnet inflation with coupling

Ali Seidabadi, Sara Saghafi, Kourosh Nozari

We study effective reheating in a scalar--Gauss--Bonnet inflationary model with a phase-space-dependent coupling , in which a compact field-space feature is combined with a…

gr-qc2026

Probing Quantum Gravity through Chaotic Orbits and Strong-Field Effects in Kerr Black Holes Embedded in Perfect Fluid Dark Matter

Shubham Kala, Sara Saghafi, M. Yousaf +4

The paper investigates how quantum‑gravity corrections and perfect fluid dark matter affect photon trajectories around a rotating (Kerr) black hole, using chaos diagnostics such as…

gr-qc2026

Higher Dimensional Loop Quantum Black hole in de Sitter Spacetime: Quasinormal Modes and Shadow Signatures

Kourosh Nozari, Sara Saghafi, Ali Mohammadpour

We investigate the dynamical and optical properties of a higher-dimensional loop-quantum-corrected black hole in a de Sitter background. The quasinormal modes of massless scalar pe…

gr-qc2026

Thin Accretion Disks around Rotating Charged Black Holes in an Effective Higher-Curvature Spacetime

Mohammad Hassani, Kourosh Nozari, Sara Saghafi

We investigate the structure and emission properties of a thin accretion disk around a rotating charged black hole described by an effective higher-curvature-inspired spacetime, co…

gr-qc2026

Rotating Black Holes with Primary Scalar Hair: Shadow Signatures in Beyond Horndeski Gravity

Kourosh Nozari, Milad Hajebrahimi, Sara Saghafi +2

The Event Horizon Telescope (EHT) image of M87* provides a direct test of strong-field gravity, measuring an angular shadow diameter and a circularit…

astro-ph.CO2026

Beyond : Gauss--Bonnet inflation with

Ali Seidabadi, Sara Saghafi, Kourosh Nozari

Gauss--Bonnet inflation typically affects the dynamics over an extended portion of the trajectory, making it difficult to isolate a controlled imprint at CMB scales. We consider a…