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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Published in | Monthly notices of the Royal Astronomical Society Vol. 474; no. 3; pp. 3067 - 3079 |
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Main Authors | , , |
Format | Journal Article |
Language | English |
Published |
London
Oxford University Press
01.03.2018
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Subjects | |
Online Access | Get full text |
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