Cutoff in the Lyman-α forest power spectrum: Warm IGM or warm dark matter?

We re-analyse high redshift and high resolution Lyman-α forest spectra considered in [1], seeking to constrain the properties of warm dark matter particles. Compared to this previous work, we consider a wider range of thermal histories of the intergalactic medium. We find that both warm and cold dar...

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Main Authors: Antonella Garzilli, Alexey Boyarsky, Oleg Ruchayskiy
Format: Article
Language:English
Published: Elsevier 2017-10-01
Series:Physics Letters B
Online Access:http://www.sciencedirect.com/science/article/pii/S0370269317306445
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author Antonella Garzilli
Alexey Boyarsky
Oleg Ruchayskiy
author_facet Antonella Garzilli
Alexey Boyarsky
Oleg Ruchayskiy
author_sort Antonella Garzilli
collection DOAJ
description We re-analyse high redshift and high resolution Lyman-α forest spectra considered in [1], seeking to constrain the properties of warm dark matter particles. Compared to this previous work, we consider a wider range of thermal histories of the intergalactic medium. We find that both warm and cold dark matter models can explain the cut-off observed in the flux power spectra of high-resolution observations equally well. This implies, however, very different thermal histories and underlying reionization models. We discuss how to remove this degeneracy. Keywords: Cosmology, Methods, Quasars
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spelling doaj.art-aa48951412694eab8721a58ef5403f572022-12-21T16:54:08ZengElsevierPhysics Letters B0370-26932017-10-01773258264Cutoff in the Lyman-α forest power spectrum: Warm IGM or warm dark matter?Antonella Garzilli0Alexey Boyarsky1Oleg Ruchayskiy2Lorentz Institute, Leiden University, Niels Bohrweg 2, Leiden, NL-2333 CA, The Netherlands; Corresponding author.Lorentz Institute, Leiden University, Niels Bohrweg 2, Leiden, NL-2333 CA, The NetherlandsDiscovery Center, Niels Bohr Institute, Blegdamsvej 17, DK-2100 Copenhagen, DenmarkWe re-analyse high redshift and high resolution Lyman-α forest spectra considered in [1], seeking to constrain the properties of warm dark matter particles. Compared to this previous work, we consider a wider range of thermal histories of the intergalactic medium. We find that both warm and cold dark matter models can explain the cut-off observed in the flux power spectra of high-resolution observations equally well. This implies, however, very different thermal histories and underlying reionization models. We discuss how to remove this degeneracy. Keywords: Cosmology, Methods, Quasarshttp://www.sciencedirect.com/science/article/pii/S0370269317306445
spellingShingle Antonella Garzilli
Alexey Boyarsky
Oleg Ruchayskiy
Cutoff in the Lyman-α forest power spectrum: Warm IGM or warm dark matter?
Physics Letters B
title Cutoff in the Lyman-α forest power spectrum: Warm IGM or warm dark matter?
title_full Cutoff in the Lyman-α forest power spectrum: Warm IGM or warm dark matter?
title_fullStr Cutoff in the Lyman-α forest power spectrum: Warm IGM or warm dark matter?
title_full_unstemmed Cutoff in the Lyman-α forest power spectrum: Warm IGM or warm dark matter?
title_short Cutoff in the Lyman-α forest power spectrum: Warm IGM or warm dark matter?
title_sort cutoff in the lyman α forest power spectrum warm igm or warm dark matter
url http://www.sciencedirect.com/science/article/pii/S0370269317306445
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