Hints of dark photon dark matter from observations and hydrodynamical simulations of the low-redshift Lyman- forest
arXiv:2206.13520 · doi:10.1103/PhysRevLett.129.211102
Abstract
Recent work has suggested that an additional per baryon of heating in the intergalactic medium is needed to reconcile hydrodynamical simulations with Lyman- forest absorption line widths at redshift . 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 and kinetic mixing can alleviate the heating excess. A prediction of this model is a non-standard thermal history for underdense gas at .
arXiv comment5+1 pages, 2+1 figures
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