Hints of dark matter-neutrino interactions in Lyman-$\alpha$ data
D. Hooper, and M. Lucca. (2021)cite arxiv:2110.04024Comment: 4+2 pages with 2 figures. Comments are very welcome.
Abstract
In this letter we investigate the possibility that dark matter and (massive)
neutrinos can interact via a simple, constant cross section. Building on
previous numerical efforts, we constrain this model with CMB, BAO and, in
particular, Lyman-$\alpha$ data. We find that the latter hint to a significant
departure from $Łambda$CDM, with a preference for an interaction strength
about 3$\sigma$ away from zero. We trace the origin of this preference back to
the additional tilt that the interacting scenario can imprint on the
Lyman-$\alpha$ flux, solving a well-known tension between early-time and
Lyman-$\alpha$ probes. Future work including complementary Lyman-$\alpha$ data
will be crucial in order to test these results.
Description
Hints of dark matter-neutrino interactions in Lyman-$\alpha$ data
%0 Generic
%1 hooper2021hints
%A Hooper, Deanna C.
%A Lucca, Matteo
%D 2021
%K library
%T Hints of dark matter-neutrino interactions in Lyman-$\alpha$ data
%U http://arxiv.org/abs/2110.04024
%X In this letter we investigate the possibility that dark matter and (massive)
neutrinos can interact via a simple, constant cross section. Building on
previous numerical efforts, we constrain this model with CMB, BAO and, in
particular, Lyman-$\alpha$ data. We find that the latter hint to a significant
departure from $Łambda$CDM, with a preference for an interaction strength
about 3$\sigma$ away from zero. We trace the origin of this preference back to
the additional tilt that the interacting scenario can imprint on the
Lyman-$\alpha$ flux, solving a well-known tension between early-time and
Lyman-$\alpha$ probes. Future work including complementary Lyman-$\alpha$ data
will be crucial in order to test these results.
@misc{hooper2021hints,
abstract = {In this letter we investigate the possibility that dark matter and (massive)
neutrinos can interact via a simple, constant cross section. Building on
previous numerical efforts, we constrain this model with CMB, BAO and, in
particular, Lyman-$\alpha$ data. We find that the latter hint to a significant
departure from $\Lambda$CDM, with a preference for an interaction strength
about 3$\sigma$ away from zero. We trace the origin of this preference back to
the additional tilt that the interacting scenario can imprint on the
Lyman-$\alpha$ flux, solving a well-known tension between early-time and
Lyman-$\alpha$ probes. Future work including complementary Lyman-$\alpha$ data
will be crucial in order to test these results.},
added-at = {2021-10-11T07:02:10.000+0200},
author = {Hooper, Deanna C. and Lucca, Matteo},
biburl = {https://www.bibsonomy.org/bibtex/24f8a6dc07c0eab341d1162ec4ba0687a/gpkulkarni},
description = {Hints of dark matter-neutrino interactions in Lyman-$\alpha$ data},
interhash = {5a4dfa91c3393c6fda60abe1e099dbdf},
intrahash = {4f8a6dc07c0eab341d1162ec4ba0687a},
keywords = {library},
note = {cite arxiv:2110.04024Comment: 4+2 pages with 2 figures. Comments are very welcome},
timestamp = {2021-10-11T07:02:10.000+0200},
title = {Hints of dark matter-neutrino interactions in Lyman-$\alpha$ data},
url = {http://arxiv.org/abs/2110.04024},
year = 2021
}