activity
20092018
most citedNon-minimal quintessence and phantom with nearly flat potentials

65 citations · 148 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.CO2018★ 3 cited

Scalar spectral index in the presence of Primordial Black Holes

Gaveshna Gupta, Ramkishor Sharma, T. R. Seshadri

We study the possibility of reheating the universe in its early stages through the evaporation of Primordial Black Holes (PBHs) that are formed due to the collapse of the inhomogen…

hep-ph2016★ 10 cited

Plateau Inflation in SUGRA-MSSM

Girish Kumar Chakravarty, Gaveshna Gupta, Gaetano Lambiase +1

We explored a Higgs inflationary scenario in the SUGRA embedding of the MSSM in Einstein frame where the inflaton is contained in the Higgs doublet. We include all higher o…

astro-ph.CO2014★ 14 cited

Thawing quintessence from the inflationary epoch to today

Gaveshna Gupta, Raghavan Rangarajan, Anjan A. Sen

Using the latest observational data we obtain a lower bound on the initial value of the quintessence field in thawing quintessence models of dark energy. For potentials of the form…

astro-ph.CO2011★ 19 cited

GCG Parametrization for Growth Function and Current Constraints

Gaveshna Gupta, Somasri Sen, Anjan A. Sen

We study the linear growth function for large scale structures in a cosmological scenario where Generalised Chaplygin Gas (GCG) serves as dark energy candidate. We parametrize…

astro-ph.CO2011★ 17 cited

Constraining Thawing Quintessence

Gaveshna Gupta, Subhabrata Majumdar, Anjan A Sen

We look at observational constraints on the thawing class of scalar field models proposed to explain the late time acceleration of the universe. Using the recently introduced `Stat…

astro-ph.CO2011★ 11 cited

Observational Constraints on Axions as Quintessence in String Theory

Gaveshna Gupta, Sudhakar Panda, Anjan A Sen

We study the observational constraints for the axion models in string theory which can successfully act as quintessence. The evolution of the universe in this model is sensitive to…