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 $z 3$.
Description
Hints of dark photon dark matter from observations and hydrodynamical simulations of the low-redshift Lyman-$\alpha$ forest
%0 Generic
%1 bolton2022hints
%A Bolton, James S.
%A Caputo, Andrea
%A Liu, Hongwan
%A Viel, Matteo
%D 2022
%K library
%T Hints of dark photon dark matter from observations and hydrodynamical
simulations of the low-redshift Lyman-$\alpha$ forest
%U http://arxiv.org/abs/2206.13520
%X 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 $z 3$.
@misc{bolton2022hints,
abstract = {Recent work has suggested that an additional $\lesssim 6.9 \rm{\, eV}$ per
baryon of heating in the intergalactic medium is needed to reconcile
hydrodynamical simulations with Lyman-$\alpha$ forest absorption line widths at
redshift $z\simeq 0.1$. 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 $m_{A'}\sim 8\times 10^{-14}\rm\,eV\,c^{-2}$ and kinetic
mixing $\epsilon \sim 5\times 10^{-15}$ can alleviate the heating excess. A
prediction of this model is a non-standard thermal history for underdense gas
at $z \gtrsim 3$.},
added-at = {2022-06-29T11:31:14.000+0200},
author = {Bolton, James S. and Caputo, Andrea and Liu, Hongwan and Viel, Matteo},
biburl = {https://www.bibsonomy.org/bibtex/29673b12efffc3255233ec3d02eeadaf2/gpkulkarni},
description = {Hints of dark photon dark matter from observations and hydrodynamical simulations of the low-redshift Lyman-$\alpha$ forest},
interhash = {d98a9bc14c781ee28bae265cfeca2764},
intrahash = {9673b12efffc3255233ec3d02eeadaf2},
keywords = {library},
note = {cite arxiv:2206.13520Comment: 5+1 pages, 2+1 figures},
timestamp = {2022-06-29T11:31:14.000+0200},
title = {Hints of dark photon dark matter from observations and hydrodynamical
simulations of the low-redshift Lyman-$\alpha$ forest},
url = {http://arxiv.org/abs/2206.13520},
year = 2022
}