activity
20182022
most citedPerturbations in a scalar field model with virtues of CDM

24 citations · 62 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.CO2022

Importance of high-frequency bands for thermal dust removal in ECHO

Aparajita Sen, Soumen Basak, Tuhin Ghosh +2

The Indian Consortium of Cosmologists has proposed a cosmic microwave background (CMB) space mission, Exploring Cosmic History and Origin (ECHO). A major scientific goal of the mis…

gr-qc2022★ 4 cited

Perturbation in an interacting dark universe

Srijita Sinha, Manisha Banerjee, Sudipta Das

In this paper we have considered an interacting model of dark energy and have looked into the evolution of the dark sectors. By solving the perturbation equations numerically, we h…

astro-ph.CO2021

Perturbations In Some Dark Energy Models

Srijita Sinha

Dark energy is the candidate that can produce effective negative pressure and make the galaxies and galaxy clusters move away from each other in an accelerated way. The structures…

astro-ph.CO2021★ 17 cited

Differentiating dark interactions with perturbation

Srijita Sinha

A cosmological model with an energy transfer between dark matter (DM) and dark energy (DE) can give rise to comparable energy densities at the present epoch. The present work deals…

astro-ph.CO2020★ 24 cited

Perturbations in a scalar field model with virtues of CDM

Srijita Sinha, Narayan Banerjee

In the era of precision cosmology, the cosmological constant gives quite an accurate description of the evolution of the Universe, but it is still plagued with the fine-tuning…

gr-qc2019★ 15 cited

Density perturbation in an interacting holographic dark energy model

Srijita Sinha, Narayan Banerjee

The present work deals with the evolution of the density contrasts for a cosmological model where along with the standard cold dark matter (CDM), the present Universe also contains…

gr-qc2018★ 2 cited

Density perturbation in the models reconstructed from jerk parameter

Srijita Sinha, Narayan Banerjee

The present work deals with the late time evolution of the linear density contrast in the dark energy models reconstructed from the jerk parameter. It is found that the non-interac…