activity
20162021
most citedDark energy equation of state parameter and its variation at low redshifts

81 citations · 216 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.CO2021★ 33 cited

Observational constraints and predictions of the interacting dark sector with field-fluid mapping

Joseph P Johnson, Archana Sangwan, S. Shankaranarayanan

We consider an interacting field theory model that describes the dark energy - dark matter interaction. Only for a specific interaction term, this interacting field theory descript…

astro-ph.CO2020

Detectability of nGauss primordial magnetic fields in the B-mode polarization of CMB

Archana Sangwan, S. Shankaranarayanan

The origin of large-scale magnetic fields in the Universe is still unknown. Observations suggest the presence of nGauss primordial magnetic fields at the last scattering surface. T…

gr-qc2018★ 41 cited

Low redshift observational constraints on tachyon models of dark energy

Avinash Singh, Archana Sangwan, H. K. Jassal

The background evolution of an accelerated, dark energy dominated universe is aptly described by non-canonical tachyon scalar field models. The accelerated expansion of the univers…

astro-ph.CO2018★ 21 cited

Observational constraints on quintessence models of dark energy

Archana Sangwan, Ashutosh Tripathi, H. K. Jassal

Scalar fields aptly describe equation of state of dark energy. The scalar field models were initially proposed to circumvent the fine tuning problem of cosmological constant. Howev…

astro-ph.CO2017★ 40 cited

Reconstructing the dark energy potential

Archana Sangwan, Ankan Mukherjee, H. K. Jassal

Dark energy equation of state can be effectively described by that of a barotropic fluid. The barotropic fluid model describes the background evolution and the functional form of t…

astro-ph.CO2016★ 81 cited

Dark energy equation of state parameter and its variation at low redshifts

Ashutosh Tripathi, Archana Sangwan, H. K. Jassal

In this paper, we constrain dark energy models using a compendium of observations at low redshifts. We consider the dark energy as a barotropic fluid, with the equation of state a…