activity
19932026
most citedReconstructing the Inflaton Potential---in Principle and in Practice

173 citations · 301 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2026

Constraints on magnetic monopoles from X-ray observations of neutron stars

Mainak Mukhopadhyay, Daniele Perri, Edward W. Kolb

Magnetic monopoles are captured efficiently by neutron stars, and if they catalyze nucleon decay, the decay products would thermalize and generate observable X-ray surface emission…

astro-ph.CO2010★ 20 cited

Harrison-Z'eldovich primordial spectrum is consistent with observations

S. Pandolfi, A. Cooray, E. Giusarma +4

Inflation predicts primordial scalar perturbations with a nearly scale-invariant spectrum and a spectral index approximately unity (the Harrison--Zel'dovich (HZ) spectrum). The fir…

astro-ph1996★ 7 cited

Cosmological Bounds to the Magnetic Moment of Heavy Tau Neutrinos

Dario Grasso, Edward W. Kolb

The magnetic moment of tau neutrinos in the MeV mass range may be large enough to modify the cosmological freeze-out calculation and determine the tau-neutrino relic density. In th…

astro-ph1995★ 23 cited

LIGHT PHOTINOS AS DARK MATTER

Glennys R. Farrar, Edward W. Kolb

There are good reasons to consider models of low-energy supersymmetry with very light photinos and gluinos. In a wide class of models the lightest -odd, color-singlet state cont…

astro-ph1993★ 78 cited

Reconstructing the Inflaton Potential---Perturbative Reconstruction to Second Order

Edmund Copeland, Edward W. Kolb, Andrew R. Liddle +1

One method to reconstruct the scalar field potential of inflation is a perturbative approach, where the values of the potential and its derivatives are calculated as an expansion i…

hep-ph1993★ 173 cited

Reconstructing the Inflaton Potential---in Principle and in Practice

Edmund Copeland, Edward W. Kolb, Andrew R. Liddle +1

Generalizing the original work by Hodges and Blumenthal, we outline a formalism which allows one, in principle, to reconstruct the potential of the inflaton field from knowledge of…