Light Dark Matter in the NO$$\nu$$A Near Detector, a First Look at the New Data
Abstract
The neutrino oscillations experiment NOA is the agship of Fermi National Laboratory. The neutrino source NuMI is delivering record numbers of protons-on-target surpassing the most stringent dark matter production upper limits of current models in the under-10 GeV mass range. We take advantage of the sophisticated particle identication algorithms of the experiment to interrogate the data from the 300-ton, o-axis, low-Z, Near Detector of NOvA during the rst physics runs. We search for signatures of sub-GeV or Light Dark Matter (LDM), Axion-like-particles, and Heavy or Sterile Neutrinos that may scatter or decay in the volume of the detector.
- Authors:
-
- Tennessee U.
- Publication Date:
- Research Org.:
- Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), High Energy Physics (HEP)
- OSTI Identifier:
- 1250791
- Report Number(s):
- FERMILAB-CONF-15-371-ND; DESY-PROC-2015-02
1414317
- DOE Contract Number:
- AC02-07CH11359
- Resource Type:
- Conference
- Resource Relation:
- Conference: 11th Patras Workshop on Axions, WIMPs and WISPs, Zaragoza, Spain, 06/22-06/26/2015
- Country of Publication:
- United States
- Language:
- English
Citation Formats
Hatzikoutelis, Athanasios. Light Dark Matter in the NO$\nu$A Near Detector, a First Look at the New Data. United States: N. p., 2015.
Web.
Hatzikoutelis, Athanasios. Light Dark Matter in the NO$\nu$A Near Detector, a First Look at the New Data. United States.
Hatzikoutelis, Athanasios. 2015.
"Light Dark Matter in the NO$\nu$A Near Detector, a First Look at the New Data". United States. https://www.osti.gov/servlets/purl/1250791.
@article{osti_1250791,
title = {Light Dark Matter in the NO$\nu$A Near Detector, a First Look at the New Data},
author = {Hatzikoutelis, Athanasios},
abstractNote = {The neutrino oscillations experiment NOA is the agship of Fermi National Laboratory. The neutrino source NuMI is delivering record numbers of protons-on-target surpassing the most stringent dark matter production upper limits of current models in the under-10 GeV mass range. We take advantage of the sophisticated particle identication algorithms of the experiment to interrogate the data from the 300-ton, o-axis, low-Z, Near Detector of NOvA during the rst physics runs. We search for signatures of sub-GeV or Light Dark Matter (LDM), Axion-like-particles, and Heavy or Sterile Neutrinos that may scatter or decay in the volume of the detector.},
doi = {},
url = {https://www.osti.gov/biblio/1250791},
journal = {},
number = ,
volume = ,
place = {United States},
year = {Thu Jan 01 00:00:00 EST 2015},
month = {Thu Jan 01 00:00:00 EST 2015}
}
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