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19922023
most citedThe Angular Dependence of the Three-Point Correlation Function of the Cosmic Microwave Background Radiation as Predicted by Inflationary Cosmologies

198 citations · 963 across the 45 of their papers we have counts for

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16 papers · 1 filter

astro-ph.CO2021★ 22 cited

The paradigm of warm quintessential inflation and spontaneous baryogenesis

Soumen Basak, Sukannya Bhattacharya, Mayukh R. Gangopadhyay +3

In this paper, we consider a scenario of spontaneous baryogenesis in a framework of warm quintessential inflation where the residual inflaton field, left out after warm inflation,…

astro-ph.CO2018★ 19 cited

Study of warm inflationary models and their parameter estimation from CMB

Richa Arya, Raghavan Rangarajan

Observations of the temperature anisotropies in the Cosmic Microwave Background (CMB) radiation show that the models of inflation with the monomial potentials are inconsistent with…

astro-ph.CO2018★ 1 cited

A plausible solution to the problem of initial conditions for inflation

Suratna Das, Raghavan Rangarajan

We propose yet another solution to the initial condition problem of inflation associated with homogeneity beyond the horizon at the onset of inflation, in cases where inflation is…

astro-ph.CO2018

Current Status of Warm Inflation

Raghavan Rangarajan

Warm inflation is an inflationary scenario in which a thermal bath coexists with the inflaton during inflation. This is unlike standard cold inflation in which the Universe is effe…

astro-ph.CO2017★ 41 cited

Revisiting CMB constraints on Warm Inflation

Richa Arya, Arnab Dasgupta, Gaurav Goswami +2

We revisit the constraints that Planck 2015 temperature, polarization and lensing data impose on the parameters of warm inflation. To this end, we study warm inflation driven by a…

astro-ph.CO2016★ 4 cited

Gravitino production in a thermal Universe revisited

Richa Arya, Namit Mahajan, Raghavan Rangarajan

We study the production of spin 1/2 gravitinos in a thermal Universe. Taking into account supersymmetry breaking due to the finite thermal energy density of the Universe, there is…