Galactic Positron Excess from Selectively Enhanced Dark Matter
Annihilation?
A. Das, B. Dasgupta, and A. Ray. (2019)cite arxiv:1911.03488Comment: 13 pages, 12 figures, 2 Tables, Comments welcome.
Abstract
Precision measurements of the positron flux in cosmic ray have revealed an
unexplained bump in the spectrum around $E300\,GeV$, not
clearly attributable to known astrophysical processes. We propose annihilation
of dark matter of mass $m_= 780\,GeV$ with a late-time cross
section $v = 4.6310^-24\,cm^3\,s^-1$ as a possible
source. The nonmonotonic dependence of the annihilation rate on dark matter
velocity, owing to a selective $p$-wave Sommerfeld enhancement, allows such a
large signal from the Milky Way without violating corresponding constraints
from dwarf galaxies. We briefly explore other signatures of this scenario, and
outline avenues to test it in future experiments.
Description
Galactic Positron Excess from Selectively Enhanced Dark Matter Annihilation?
%0 Generic
%1 das2019galactic
%A Das, Anirban
%A Dasgupta, Basudeb
%A Ray, Anupam
%D 2019
%K tifr
%T Galactic Positron Excess from Selectively Enhanced Dark Matter
Annihilation?
%U http://arxiv.org/abs/1911.03488
%X Precision measurements of the positron flux in cosmic ray have revealed an
unexplained bump in the spectrum around $E300\,GeV$, not
clearly attributable to known astrophysical processes. We propose annihilation
of dark matter of mass $m_= 780\,GeV$ with a late-time cross
section $v = 4.6310^-24\,cm^3\,s^-1$ as a possible
source. The nonmonotonic dependence of the annihilation rate on dark matter
velocity, owing to a selective $p$-wave Sommerfeld enhancement, allows such a
large signal from the Milky Way without violating corresponding constraints
from dwarf galaxies. We briefly explore other signatures of this scenario, and
outline avenues to test it in future experiments.
@misc{das2019galactic,
abstract = {Precision measurements of the positron flux in cosmic ray have revealed an
unexplained bump in the spectrum around $E\simeq 300\,\mathrm{GeV}$, not
clearly attributable to known astrophysical processes. We propose annihilation
of dark matter of mass $m_\chi = 780\,\mathrm{GeV}$ with a late-time cross
section $\sigma v = 4.63\times 10^{-24}\,\mathrm{cm^3\,s^{-1}}$ as a possible
source. The nonmonotonic dependence of the annihilation rate on dark matter
velocity, owing to a selective $p$-wave Sommerfeld enhancement, allows such a
large signal from the Milky Way without violating corresponding constraints
from dwarf galaxies. We briefly explore other signatures of this scenario, and
outline avenues to test it in future experiments.},
added-at = {2019-11-13T06:38:16.000+0100},
author = {Das, Anirban and Dasgupta, Basudeb and Ray, Anupam},
biburl = {https://www.bibsonomy.org/bibtex/2ca0ffce8d9696becde3bf4de553aec05/citekhatri},
description = {Galactic Positron Excess from Selectively Enhanced Dark Matter Annihilation?},
interhash = {79e3276aa31870c58b38d345316d642a},
intrahash = {ca0ffce8d9696becde3bf4de553aec05},
keywords = {tifr},
note = {cite arxiv:1911.03488Comment: 13 pages, 12 figures, 2 Tables, Comments welcome},
timestamp = {2019-11-13T06:38:16.000+0100},
title = {Galactic Positron Excess from Selectively Enhanced Dark Matter
Annihilation?},
url = {http://arxiv.org/abs/1911.03488},
year = 2019
}