Published January 1, 2021
| Version v1
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Supernova neutrino burst detection with the deep underground neutrino experiment
Creators
- 1. Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA
- 2. Univ Atlantico, Atlantico, Colombia
- 3. Georgian Tech Univ, Tbilisi, Georgia
- 4. Brookhaven Natl Lab, Upton, NY 11973 USA
- 5. Univ Bristol, Bristol BS8 1TL, Avon, England
- 6. Variable Energy Cyclotron Ctr, Kolkata 700064, W Bengal, India
- 7. Univ Warwick, Coventry CV4 7AL, W Midlands, England
- 8. Univ Sussex, Brighton BN1 9RH, E Sussex, England
- 9. European Org Nucl Res, CERN, CH-1211 Meyrin, Switzerland
- 10. Swiss Fed Inst Technol, Zurich, Switzerland
- 11. Argonne Natl Lab, Argonne, IL 60439 USA
- 12. Univ Antananarivo, Antananarivo 101, Madagascar
- 13. SLAC Natl Accelerator Lab, Menlo Pk, CA 94025 USA
- 14. Inst Fis Corpuscular, Valencia 46980, Spain
- 15. Univ Basel, CH-4056 Basel, Switzerland
- 16. Univ Colima, Colima, Mexico
- 17. Univ Bern, CH-3012 Bern, Switzerland
Description
The deep underground neutrino experiment (DUNE), a 40-kton underground liquid argon time projection chamber experiment, will be sensitive to the electron-neutrino flavor component of the burst of neutrinos expected from the next Galactic core-collapse supernova. Such an observation will bring unique insight into the astrophysics of core collapse as well as into the properties of neutrinos. The general capabilities of DUNE for neutrino detection in the relevant few- to few-tens-of-MeV neutrino energy range will be described. As an example, DUNE's ability to constrain the nu(e) spectral parameters of the neutrino burst will be considered.
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