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Contributions to cosmic reionization from dark matter annihilation and decay

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Author(s)
Zavala, Jesús
•
Liu, Hongwan
•
Slatyer, Tracy Robyn
Date Issued
September 2016
Journal
Physical Review D
Publisher
American Physical Society
Citation
Liu, Hongwan, Tracy R. Slatyer, and Jesús Zavala. “Contributions to Cosmic Reionization from Dark Matter Annihilation and Decay.” Physical Review D 94.6 (2016): n. pag. © 2016 American Physical Society
Version
Final published version
Abstract
Dark matter annihilation or decay could have a significant impact on the ionization and thermal history of the universe. In this paper, we study the potential contribution of dark matter annihilation (s-wave- or p-wave-dominated) or decay to cosmic reionization, via the production of electrons, positrons and photons. We map out the possible perturbations to the ionization and thermal histories of the universe due to dark matter processes, over a broad range of velocity-averaged annihilation cross sections/decay lifetimes and dark matter masses. We have employed recent numerical studies of the efficiency with which annihilation/decay products induce heating and ionization in the intergalactic medium, and in this work extended them down to a redshift of 1+z=4 for two different reionization scenarios. We also improve on earlier studies by using the results of detailed structure formation models of dark matter haloes and subhaloes that are consistent with up-to-date N-body simulations, with estimates on the uncertainties that originate from the smallest scales. We find that for dark matter models that are consistent with experimental constraints, a contribution of more than 10% to the ionization fraction at reionization is disallowed for all annihilation scenarios. Such a contribution is possible only for decays into electron/positron pairs, for light dark matter with mass m[subscript χ]≲100  MeV, and a decay lifetime τ[subscript χ]∼10[superscript 24]–10[superscript 25]  s.
MIT Department
Massachusetts Institute of Technology. Center for Theoretical Physics
Massachusetts Institute of Technology. Department of Physics
Terms of Use
Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.
Persistent DSpace Link
http://hdl.handle.net/1721.1/104895
DOI of Published Version
https://doi.org/10.1103/PhysRevD.94.063507
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