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DarkHistory: A code package for calculating modified cosmic ionization and thermal histories with dark matter and other exotic energy injections

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arxiv 1904.09296 v1 pith:3CWIHABQ submitted 2019-04-19 astro-ph.CO astro-ph.HEhep-ph

classification astro-ph.COastro-ph.HEhep-ph
keywords darkhistoryannihilationdarkdecaymattercodeeffectsionization
verification ladder T0 review T1 audit T2 compute T3 formal
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We present a new public Python package, DarkHistory, for computing the effects of dark matter annihilation and decay on the temperature and ionization history of the early universe. DarkHistory simultaneously solves for the evolution of the free electron fraction and gas temperature, and for the cooling of annihilation/decay products and the secondary particles produced in the process. Consequently, we can self-consistently include the effects of both astrophysical and exotic sources of heating and ionization, and automatically take into account backreaction, where modifications to the ionization/temperature history in turn modify the energy-loss processes for injected particles. We present a number of worked examples, demonstrating how to use the code in a range of different configurations, in particular for arbitrary dark matter masses and annihilation/decay final states. Possible applications of DarkHistory include mapping out the effects of dark matter annihilation/decay on the global 21cm signal and the epoch of reionization, as well as the effects of exotic energy injections other than dark matter annihilation/decay. The code is available at https://github.com/hongwanliu/DarkHistory with documentation at https://darkhistory.readthedocs.io . Data files required to run the code can be downloaded at https://doi.org/10.7910/DVN/DUOUWA .

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Cosmological constraints on TeV-scale dark matter subcomponents decaying between recombination and reionisation

    astro-ph.CO 2026-04 conditional novelty 6.0 of 10

    Future global 21-cm observations could beat CMB limits on TeV-scale decaying dark matter for lifetimes ≳10^15 s, especially for decays into neutrinos.

  2. Constraining the axiverse with reionization

    hep-ph 2025-07 conditional novelty 6.0 of 10

    Roughly 10 to 15 percent of explicit string theory axiverse models are disfavored by CMB reionization data unless reheating stayed below about 10^10 GeV.

  3. Not-quite-primordial black holes seeded by cosmic string loops

    astro-ph.CO 2025-07 conditional novelty 5.0 of 10

    Cosmic string loops moving through the early universe can seed halos that collapse into 10^5 solar mass black holes, potentially explaining JWST's little red dots.

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