Dark matter annihilation in the circumgalactic medium at high redshifts

AbstractAnnihilating dark matter (DM) models offer promising avenues for future DM detection, in particular via modification of astrophysical signals. However, when modelling such potential signals at high redshift, the emergence of both DM and baryonic structure, as well as the complexities of the...

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Bibliographic Details
Published inMonthly notices of the Royal Astronomical Society Vol. 474; no. 3; pp. 3067 - 3079
Main Authors Schön, S, Mack, K J, Wyithe, J S B
Format Journal Article
LanguageEnglish
Published London Oxford University Press 01.03.2018
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