The neutrino fog for dark matter-electron scattering experiments

Fuente: arXiv
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Main Authors: Carew, Ben, Caddell, Ashlee R., Maity, Tarak Nath, O'Hare, Ciaran A. J.
Format: Preprint
Published: 2023
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author Carew, Ben
Caddell, Ashlee R.
Maity, Tarak Nath
O'Hare, Ciaran A. J.
author_facet Carew, Ben
Caddell, Ashlee R.
Maity, Tarak Nath
O'Hare, Ciaran A. J.
contents The search for sub-GeV dark matter via scattering on electrons has ramped up in the last few years. Like in the case of dark matter scattering on nuclei, electron-recoil-based searches also face an ultimate background in the form of neutrinos. The so-called ``neutrino fog'' refers to the range of open dark-matter parameter space where the background of neutrinos can potentially prevent a conclusive discovery claim of a dark matter signal from being made. In this study, we map the neutrino fog for a range of electron recoil experiments based on silicon, germanium, xenon and argon targets. In analogy to the nuclear recoil case, we also calculate the ''edge'' to the neutrino fog, which can be used as a visual guide to where neutrinos become an important background -- this boundary excludes some parts of the key theory milestones used to motivate these experiments.
format Preprint
id arxiv_https___arxiv_org_abs_2312_04303
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle The neutrino fog for dark matter-electron scattering experiments
Carew, Ben
Caddell, Ashlee R.
Maity, Tarak Nath
O'Hare, Ciaran A. J.
High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
Solar and Stellar Astrophysics
High Energy Physics - Experiment
The search for sub-GeV dark matter via scattering on electrons has ramped up in the last few years. Like in the case of dark matter scattering on nuclei, electron-recoil-based searches also face an ultimate background in the form of neutrinos. The so-called ``neutrino fog'' refers to the range of open dark-matter parameter space where the background of neutrinos can potentially prevent a conclusive discovery claim of a dark matter signal from being made. In this study, we map the neutrino fog for a range of electron recoil experiments based on silicon, germanium, xenon and argon targets. In analogy to the nuclear recoil case, we also calculate the ''edge'' to the neutrino fog, which can be used as a visual guide to where neutrinos become an important background -- this boundary excludes some parts of the key theory milestones used to motivate these experiments.
title The neutrino fog for dark matter-electron scattering experiments
topic High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
Solar and Stellar Astrophysics
High Energy Physics - Experiment
url https://arxiv.org/abs/2312.04303