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researcher

E. Kolb

83 papers hereh-index 5820.1k citations253 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • sole author4
  • first author29
  • middle author35
  • last author14

Across the 82 of 83 papers where every author was matched, so the position is known.

fields
  • astro-ph41
  • hep-ph27
  • astro-ph.CO7
  • hep-th4
  • astro-ph.IM1
  • cond-mat1
same name
  • E. Kolb — 8 papers, h 14
  • E. Kolb — 1 paper, h 1

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
19932023
most citedReconstructing the Inflaton Potential --- an Overview

837 citations · 8.3k across the 83 of their papers we have counts for

collaborators
Showing 2004Show all

4 papers · 1 filter

astro-ph2004★ 91 cited

Isocurvature constraints on gravitationally produced superheavy dark matter

Daniel J. H. Chung, Edward W. Kolb, Antonio Riotto +1

We show that the isocurvature perturbations imply that the gravitationally produced superheavy dark matter must have masses larger than few times the Hubble expansion rate at the e…

astro-ph2004★ 68 cited

Curvature Perturbations from Broken Symmetries

Edward W. Kolb, Antonio Riotto, Alberto Vallinotto

We present a new general mechanism to generate curvature perturbations after the end of the slow-roll phase of inflation. Our model is based on the simple assumption that the poten…

astro-ph2004★ 29 cited

Cosmological influence of super-Hubble perturbations

Edward W. Kolb, Sabino Matarrese, Alessio Notari +1

The existence of cosmological perturbations of wavelength larger than the Hubble radius is a generic prediction of the inflationary paradigm. We provide the derivation beyond pertu…

hep-ph2004★ 175 cited

Effect of inhomogeneities on the expansion rate of the Universe

Edward W. Kolb, Sabino Matarrese, Alessio Notari +1

While the expansion rate of a homogeneous isotropic Universe is simply proportional to the square-root of the energy density, the expansion rate of an inhomogeneous Universe also d…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.