Results for the case of the quadratic potential with a step
As an illustration, in this page, we list the various results from BINGO for the case of the quadratic potential with a step. The model parameters correspond to those that lead to the best fit to the WMAP seven-year data. (for details, see, D. K. Hazra, L. Sriramkumar and J. Martin, BINGO: A code for the efficient computation of the scalar bi-spectrum , JCAP 1305, 026 (2013)).
Evolution of the scalar field ϕ : phi.eps
The behaviour of the slow roll parameter ϵ : epsilon.eps
The evolution of the Hubble parameter H : hubble.eps
The resulting primordial power spectrum : powerspectra.eps
The non-Gaussianity parameter fNL : fnl-qp-stp.eps
The 2D and 3D plots of fNL:
Quadratic potential with a step
Quadratic potential with a step : 3D contour
plots of bispectrum