Article: Study data from University of Canterbury update understanding of astrophysics.

"In the first part of this paper, we outline the construction of an inflationary cosmology in the framework where inflation is described by a universally evolving scalar field phi with potential V ( f). By considering a generic situation that inflaton attains a nearly constant velocity, during inflation, m(P)(-1) vertical bar d phi/dN vertical bar alpha + beta exp (beta N) (where N In a is the e-folding time), we reconstruct a scalar potential and find the conditions that have to be satisfied by the (reconstructed) potential to be consistent with the WMAP inflationary data," scientists in Christchurch, New Zealand report.

"The consistency of our model with the ...

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