0000000000320416

AUTHOR

Edward W. Kolb

showing 3 related works from this author

Cosmological background solutions and cosmological backreactions

2009

The cosmological backreaction proposal, which attempts to account for observations without a primary dark energy source in the stress-energy tensor, has been developed and discussed by means of different approaches. Here, we focus on the concept of cosmological background solutions in order to develop a framework to study different backreaction proposals.

PhysicsTheoretical physicsGeneral Relativity and Quantum CosmologyCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics and Astronomy (miscellaneous)Dark energyFOS: Physical sciencesAstrophysicsTensorAstrophysics::Cosmology and Extragalactic AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyAstrophysics - Cosmology and Nongalactic Astrophysics
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Impact of general reionization scenarios on extraction of inflationary parameters

2010

Determination of whether the Harrison-Zel'dovich spectrum for primordial scalar perturbations is consistent with observations is sensitive to assumptions about the reionization scenario. In light of this result, we revisit constraints on inflationary models using more general reionization scenarios. While the bounds on the tensor-to-scalar ratio are largely unmodified, when different reionization schemes are addressed, hybrid models are back into the inflationary game. In the general reionization picture, we reconstruct both the shape and amplitude of the inflaton potential. We discuss how relaxing the simple reionization restriction affects the reconstruction of the potential through the c…

Inflation (cosmology)PhysicsNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Cosmic microwave backgroundCosmic background radiationAstrophysics::Instrumentation and Methods for AstrophysicsSpectral densityFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsInflatonCMB cold spotCosmologyGeneral Relativity and Quantum CosmologyFísica nuclearReionizationAstrophysics - Cosmology and Nongalactic Astrophysics
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Harrison-Zel'dovich primordial spectrum is consistent with observations

2010

Inflation predicts primordial scalar perturbations with a nearly scale-invariant spectrum and a spectral index approximately unity (the Harrison--Zel'dovich (HZ) spectrum). The first important step for inflationary cosmology is to check the consistency of the HZ primordial spectrum with current observations. Recent analyses have claimed that a HZ primordial spectrum is excluded at more than 99% c.l.. Here we show that the HZ spectrum is only marginally disfavored if one considers a more general reionization scenario. Data from the Planck mission will settle the issue.

Inflation (cosmology)PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Nuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Scalar (mathematics)Spectral densityFOS: Physical sciencesFísicaAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsCMB cold spotGeneral Relativity and Quantum CosmologyCosmologyHigh Energy Physics - Phenomenologysymbols.namesakeGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)Observational cosmologysymbolsPlanckAstrophysics - High Energy Astrophysical PhenomenaReionizationAstrophysics - Cosmology and Nongalactic Astrophysics
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