Inhomogeneous energy injection in the 21-cm power spectrum: Sensitivity to dark matter decay

The 21-cm signal provides a novel avenue to measure the thermal state of the Universe during cosmic dawn and reionization (redshifts <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"><a:mrow><a:mi>z</a:mi><a:mo>∼</a:mo><a:mn>5</a:mn><a:mi>–</a:mi><a:mn>30</a:mn></a:mrow></a:math>), and thus to probe energy injection from decaying or annihilating dark matter (DM). These DM processes are inherently inhomogeneous: both decay and annihilation are density-dependent, and furthermore, the fraction of injected energy that is deposited at each point depends on the gas ionization and density, leading to further anisotropies in absorption and propagation. In this work, we develop a new framework for modeling the impact of spatially inhomogeneous energy injection and deposition during cosmic dawn, accounting for ionization and baryon density dependence, as well as the attenuation of propagating photons. We showcase how this first completely inhomogeneous treatment affects the predicted 21-cm power spectrum in the presence of exotic sources of energy injection, and forecast the constraints that upcoming HERA measurements of the 21-cm power spectrum will set on DM decays to photons and to electron/positron pairs. These projected constraints considerably surpass those derived from CMB and Lyman-<c:math xmlns:c="http://www.w3.org/1998/Math/MathML" display="inline"><c:mi>α</c:mi></c:math> measurements, and for decays to electron/positron pairs they exceed all existing constraints in the sub-GeV mass range, reaching lifetimes of <e:math xmlns:e="http://www.w3.org/1998/Math/MathML" display="inline"><e:mrow><e:mo>∼</e:mo><e:msup><e:mrow><e:mn>10</e:mn></e:mrow><e:mrow><e:mn>28</e:mn></e:mrow></e:msup><e:mtext> </e:mtext><e:mtext> </e:mtext><e:mi mathvariant="normal">s</e:mi></e:mrow></e:math>. Our analysis demonstrates the unprecedented sensitivity of 21-cm cosmology to exotic sources of energy injection during the cosmic dark ages. Our code, 21cm, includes all these effects and is publicly available in an accompanying release.

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Publication Details

Journal
Physical review. D/Physical review. D.
Published
2025-02-06
DOI
https://doi.org/10.1103/physrevd.111.043015
Citations
20
Primary Topic
Radio Astronomy Observations and Technology
Type
article
Field-Weighted Citation Impact
23.10

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article

Inhomogeneous energy injection in the 21-cm power spectrum: Sensitivity to dark matter decay

Joshua W. Foster, Yitian Sun, Julián B. Muñoz, Tracy R. Slatyer et al.
20 citations
Physical review. D/Physical review. D.
Radio Astronomy Observations and Technology
23.10
article

Inhomogeneous energy injection in the 21-cm power spectrum: Sensitivity to dark matter decay

Joshua W. Foster, Yitian Sun, Julián B. Muñoz, Tracy R. Slatyer, Hongwan Liu
article en
20 citations

Abstract

The 21-cm signal provides a novel avenue to measure the thermal state of the Universe during cosmic dawn and reionization (redshifts <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"><a:mrow><a:mi>z</a:mi><a:mo>∼</a:mo><a:mn>5</a:mn><a:mi>–</a:mi><a:mn>30</a:mn></a:mrow></a:math>), and thus to probe energy injection from decaying or annihilating dark matter (DM). These DM processes are inherently inhomogeneous: both decay and annihilation are density-dependent, and furthermore, the fraction of injected energy that is deposited at each point depends on the gas ionization and density, leading to further anisotropies in absorption and propagation. In this work, we develop a new framework for modeling the impact of spatially inhomogeneous energy injection and deposition during cosmic dawn, accounting for ionization and baryon density dependence, as well as the attenuation of propagating photons. We showcase how this first completely inhomogeneous treatment affects the predicted 21-cm power spectrum in the presence of exotic sources of energy injection, and forecast the constraints that upcoming HERA measurements of the 21-cm power spectrum will set on DM decays to photons and to electron/positron pairs. These projected constraints considerably surpass those derived from CMB and Lyman-<c:math xmlns:c="http://www.w3.org/1998/Math/MathML" display="inline"><c:mi>α</c:mi></c:math> measurements, and for decays to electron/positron pairs they exceed all existing constraints in the sub-GeV mass range, reaching lifetimes of <e:math xmlns:e="http://www.w3.org/1998/Math/MathML" display="inline"><e:mrow><e:mo>∼</e:mo><e:msup><e:mrow><e:mn>10</e:mn></e:mrow><e:mrow><e:mn>28</e:mn></e:mrow></e:msup><e:mtext> </e:mtext><e:mtext> </e:mtext><e:mi mathvariant="normal">s</e:mi></e:mrow></e:math>. Our analysis demonstrates the unprecedented sensitivity of 21-cm cosmology to exotic sources of energy injection during the cosmic dark ages. Our code, 21cm, includes all these effects and is publicly available in an accompanying release.

Physical review. D/Physical review. D.Vol. 111(4)
Fermi National Accelerator Laboratory (US), University of Chicago (US), Massachusetts Institute of Technology (US), The University of Texas at Austin (US)
National Science Foundation, U.S. Department of Energy, Simons Foundation, University of Chicago, Office of Science, Kavli Institute for Cosmological Physics, University of Chicago, High Energy Physics, Fermilab
Openalex Percentile: Top 0%
Radio Astronomy Observations and Technology
23.10
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