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Title: Implementation of an Upward-Going Muon Trigger for Indirect Dark Matter Searches at the NO$$\nu$$A Far Detector

Conference ·
OSTI ID:1226350
 [1];  [1];  [1];  [2];  [3];  [1]
  1. Univ. of Virginia, Charlottesville, VA (United States)
  2. Univ. of Virginia, Charlottesville, VA (United States); Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
  3. Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)

The NO$$\nu$$A collaboration has constructed a 14,000 ton, fine-grained, low-Z, total absorption tracking calorimeter at an off-axis angle to an upgraded NuMI neutrino beam. This detector, with its excellent granularity and energy resolution and relatively low-energy neutrino thresholds, was designed to observe electron neutrino appearance in a muon neutrino beam, but it also has unique capabilities suitable for more exotic efforts. In fact, if an efficient upward-going muon trigger with sufficient cosmic ray background rejection can be demonstrated, NO$$\nu$$A will be capable of a competitive indirect dark matter search for low-mass WIMPs. The cosmic ray muon rate at the NO$$\nu$$A far detector is about 100 kHz and provides the primary challenge for triggering and optimizing such a search analysis. The status of the NO$$\nu$$A upward-going muon trigger is presented.

Research Organization:
Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
Sponsoring Organization:
USDOE Office of Science (SC), High Energy Physics (HEP)
DOE Contract Number:
AC02-07CH11359
OSTI ID:
1226350
Report Number(s):
FERMILAB-CONF-15-197-ND; arXiv eprint number arXiv:1510.07571; TRN: US1700241
Resource Relation:
Conference: 21. International Conference on Computing in High Energy and Nuclear Physics, Okinawa, JP (United States), 13-17 Apr 2015
Country of Publication:
United States
Language:
English