activity
20122026
most citedObservational constraints on the interacting dark energy - dark matter (IDM) cosmological models

18 citations · 45 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.CO2026

Phase-Space Analysis of Quadratic Dark Energy: Stable Attractors and Their Observational Signatures

Sahar Mohammadi, Ebrahim Yusofi, Kosar Asadi

We present a comprehensive phase-space analysis of a quadratic dark energy model where the pressure includes a nonlinear term proportional to the square of the energy density. This…

astro-ph.CO2023

Stochastic Multiple Fields Inflation: Diffusion Dominated Regime

Kosar Asadi, Amin Nassiri-Rad, Hassan Firouzjahi

We study multiple fields inflation in diffusion dominated regime using stochastic formalism. The fields are under pure Brownian motion in a dS background with boundaries in hi…

hep-th2022★ 7 cited

Inflation with Stochastic Boundary

Amin Nassiri-Rad, Kosar Asadi, Hassan Firouzjahi

We study the Brownian motion of a field where there are boundaries in the inflationary field space. Both the field and the boundary undergo Brownian motions with the amplitudes of…

gr-qc2022★ 18 cited

Observational constraints on the interacting dark energy - dark matter (IDM) cosmological models

T. Harko, K. Asadi, H. Moshafi +1

Particle creation (or annihilation) mechanisms, described by either quantum field theoretical models, or by the thermodynamics of irreversible processes, play an important role in…

astro-ph.CO2016★ 2 cited

Consistency Relation and Non-Gaussianity in a Galileon Inflation

Kosar Asadi, Kourosh Nozari

We study a particular Galileon inflation in the light of Planck2015 observational data in order to constraint the model parameter space. We study the spectrum of the primordial mod…

astro-ph.CO2016★ 2 cited

The Size of Local Bispectrum and Trispectrum in a Non-Minimal Inflation

Kosar Asadi, Kourosh Nozari

Focusing on the local type primordial non-Gaussianities, we study the bispectrum and trispectrum during a non-minimal slow-roll inflation. We use the so-called formalism to in…