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Hints of dark photon dark matter from observations and hydrodynamical simulations of the low-redshift Lyman-$\alpha$ forest

, , , and . (2022)cite arxiv:2206.13520Comment: 5+1 pages, 2+1 figures.

Abstract

Recent work has suggested that an additional $6.9 \, eV$ per baryon of heating in the intergalactic medium is needed to reconcile hydrodynamical simulations with Lyman-$\alpha$ forest absorption line widths at redshift $z0.1$. Resonant conversion of dark photon dark matter into low frequency photons is a viable source of such heating. We perform the first hydrodynamical simulations including dark photon heating and show that dark photons with mass $m_A'810^-14\rm\,eV\,c^-2$ and kinetic mixing $510^-15$ can alleviate the heating excess. A prediction of this model is a non-standard thermal history for underdense gas at $z 3$.

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Hints of dark photon dark matter from observations and hydrodynamical simulations of the low-redshift Lyman-$\alpha$ forest

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