activity
20002005
most citedNon-Gaussian Signatures in the Cosmic Background Radiation from Warm Inflation

102 citations · 302 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph2005★ 78 cited

Non-Gaussian perturbations from multi-field inflation

Laura E. Allen, Sujata Gupta, David Wands

We show how the primordial bispectrum of density perturbations from inflation may be characterised in terms of manifestly gauge-invariant cosmological perturbations at second order…

astro-ph2005★ 34 cited

Dynamics and Non-Gaussianity in the Weak-Dissipative Warm Inflation Scenario

Sujata Gupta

We calculate the general solutions for a warm inflationary scenario with weak dissipation, reviewing the dissipative dynamics of the two-fluid system, and calculate the bispectrum…

astro-ph2003★ 49 cited

Curvature and isocurvature perturbations in a three-fluid model of curvaton decay

Sujata Gupta, Karim A. Malik, David Wands

We study the evolution of the cosmological perturbations after inflation in curvaton models where the non-relativistic curvaton decays into both radiation and a cold dark matter co…

astro-ph2002★ 102 cited

Non-Gaussian Signatures in the Cosmic Background Radiation from Warm Inflation

S. Gupta, A. Berera, A. F. Heavens +1

We calculate the bispectrum of the gravitational field fluctuations generated during warm inflation, where dissipation of the vacuum potential during inflation is the mechanism for…

astro-ph2001★ 14 cited

Fast Parameter Estimation from the CMB Power Spectrum

Sujata Gupta, Alan F. Heavens

The statistical properties of a map of the primary fluctuations in the cosmic microwave background (CMB) may be specified to high accuracy by a few thousand power spectra measureme…

astro-ph2000★ 25 cited

Full-sky correlations of peaks in the microwave background

Alan F. Heavens, Sujata Gupta

We compute precise predictions for the two-point correlation function of local maxima (or minima) in the temperature of the microwave background, under the assumption that it is a…