DOE PAGES title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Presupernova neutrino signals as potential probes of neutrino mass hierarchy

Abstract

We assess the potential of using presupernova neutrino signals at the Jiangmen Underground Neutrino Observatory (JUNO) to probe the yet-unknown neutrino mass hierarchy. Using models for stars of 12, 15, 20, $$M_\bigodot$$, we find that if the $$\overline{v}_e$$ signals from such a star can be predicted precisely and the star is within ≈440–880 pc, the number of events detected within one day of its explosion allows to determine the hierarchy at the confidence level. For determination at this level using such signals from Betelgeuse, which is at a distance of $$≈$$222 pc, the uncertainty in the predicted number of signals needs to be $$≲$$14–30%. In view of more realistic uncertainties, we discuss and advocate a model-independent determination using both $$v_e$$ and $$\overline{v}_e$$ signals from Betelgeuse. This method is feasible if the cosmogenic background for $ν-$e scattering events can be reduced by a factor of ~ 2.5–10 from the current estimate. Such reduction might be achieved by using coincidence of the background events, the exploration of which for JUNO is highly desirable.

Authors:
ORCiD logo; ;
Publication Date:
Research Org.:
Univ. of Minnesota, Minneapolis, MN (United States)
Sponsoring Org.:
USDOE Office of Science (SC); German Research Foundation (DFG); Australian Research Council (ARC); National Natural Science Foundation of China (NSFC); Science and Technology Commission of Shanghai Municipality
OSTI Identifier:
1542680
Alternate Identifier(s):
OSTI ID: 1610085
Grant/Contract Number:  
FG02-87ER40328
Resource Type:
Published Article
Journal Name:
Physics Letters. B
Additional Journal Information:
Journal Name: Physics Letters. B Journal Volume: 796 Journal Issue: C; Journal ID: ISSN 0370-2693
Publisher:
Elsevier
Country of Publication:
Netherlands
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; Astronomy & Astrophysics; Physics

Citation Formats

Guo, Gang, Qian, Yong-Zhong, and Heger, Alexander. Presupernova neutrino signals as potential probes of neutrino mass hierarchy. Netherlands: N. p., 2019. Web. doi:10.1016/j.physletb.2019.07.030.
Guo, Gang, Qian, Yong-Zhong, & Heger, Alexander. Presupernova neutrino signals as potential probes of neutrino mass hierarchy. Netherlands. https://doi.org/10.1016/j.physletb.2019.07.030
Guo, Gang, Qian, Yong-Zhong, and Heger, Alexander. Tue . "Presupernova neutrino signals as potential probes of neutrino mass hierarchy". Netherlands. https://doi.org/10.1016/j.physletb.2019.07.030.
@article{osti_1542680,
title = {Presupernova neutrino signals as potential probes of neutrino mass hierarchy},
author = {Guo, Gang and Qian, Yong-Zhong and Heger, Alexander},
abstractNote = {We assess the potential of using presupernova neutrino signals at the Jiangmen Underground Neutrino Observatory (JUNO) to probe the yet-unknown neutrino mass hierarchy. Using models for stars of 12, 15, 20, $M_\bigodot$, we find that if the $\overline{v}_e$ signals from such a star can be predicted precisely and the star is within ≈440–880 pc, the number of events detected within one day of its explosion allows to determine the hierarchy at the confidence level. For determination at this level using such signals from Betelgeuse, which is at a distance of $≈$222 pc, the uncertainty in the predicted number of signals needs to be $≲$14–30%. In view of more realistic uncertainties, we discuss and advocate a model-independent determination using both $v_e$ and $\overline{v}_e$ signals from Betelgeuse. This method is feasible if the cosmogenic background for $ν-$e scattering events can be reduced by a factor of ~ 2.5–10 from the current estimate. Such reduction might be achieved by using coincidence of the background events, the exploration of which for JUNO is highly desirable.},
doi = {10.1016/j.physletb.2019.07.030},
journal = {Physics Letters. B},
number = C,
volume = 796,
place = {Netherlands},
year = {Tue Jul 16 00:00:00 EDT 2019},
month = {Tue Jul 16 00:00:00 EDT 2019}
}

Journal Article:
Free Publicly Available Full Text
Publisher's Version of Record
https://doi.org/10.1016/j.physletb.2019.07.030

Citation Metrics:
Cited by: 10 works
Citation information provided by
Web of Science

Save / Share:

Works referenced in this record:

Expected geoneutrino signal at JUNO
journal, March 2015

  • Strati, Virginia; Baldoncini, Marica; Callegari, Ivan
  • Progress in Earth and Planetary Science, Vol. 2, Issue 1
  • DOI: 10.1186/s40645-015-0037-6

Neutrino–electron scattering theory
journal, October 2003

  • Marciano, William J.; Parsa, Zohreh
  • Journal of Physics G: Nuclear and Particle Physics, Vol. 29, Issue 11
  • DOI: 10.1088/0954-3899/29/11/013

Collective Neutrino Oscillations
journal, November 2010


Cosmogenic C 11 production and sensitivity of organic scintillator detectors to pep and CNO neutrinos
journal, May 2005


Neutrino oscillations in matter
journal, May 1978


Review of Particle Physics
journal, August 2018


Evolutionary Tracks for Betelgeuse
journal, February 2016

  • Dolan, Michelle M.; Mathews, Grant J.; Lam, Doan Duc
  • The Astrophysical Journal, Vol. 819, Issue 1
  • DOI: 10.3847/0004-637X/819/1/7

Neutrinos from Beta Processes in a Presupernova: Probing the Isotopic Evolution of a Massive Star
journal, December 2017

  • Patton, Kelly M.; Lunardini, Cecilia; Farmer, Robert J.
  • The Astrophysical Journal, Vol. 851, Issue 1
  • DOI: 10.3847/1538-4357/aa95c4

Supernova Neutrino Detection
journal, November 2012


KamLAND SENSITIVITY TO NEUTRINOS FROM PRE-SUPERNOVA STARS
journal, February 2016


Neutrino Emissions in All Flavors up to the Pre-bounce of Massive Stars and the Possibility of Their Detections
journal, October 2017

  • Kato, Chinami; Nagakura, Hiroki; Furusawa, Shun
  • The Astrophysical Journal, Vol. 848, Issue 1
  • DOI: 10.3847/1538-4357/aa8b72

Presupernova Neutrinos: Realistic Emissivities from Stellar Evolution
journal, April 2017

  • Patton, Kelly M.; Lunardini, Cecilia; Farmer, Robert J.
  • The Astrophysical Journal, Vol. 840, Issue 1
  • DOI: 10.3847/1538-4357/aa6ba8

Neutrino Energy Loss in Stellar Interiors. VII. Pair, Photo-, Plasma, Bremsstrahlung, and Recombination Neutrino Processes
journal, January 1996

  • Itoh, Naoki; Hayashi, Hiroshi; Nishikawa, Akinori
  • The Astrophysical Journal Supplement Series, Vol. 102
  • DOI: 10.1086/192264

Detection possibility of the pair-annihilation neutrinos from the neutrino-cooled pre-supernova star
journal, June 2004


The evolution and explosion of massive stars
journal, November 2002


Neutrino physics with JUNO
journal, February 2016


Supernova signatures of neutrino mass ordering
journal, December 2017


PRE-SUPERNOVA NEUTRINO EMISSIONS FROM ONe CORES IN THE PROGENITORS OF CORE-COLLAPSE SUPERNOVAE: ARE THEY DISTINGUISHABLE FROM THOSE OF Fe CORES?
journal, July 2015


What can be learned from a future supernova neutrino detection?
journal, March 2018

  • Horiuchi, Shunsaku; Kneller, James P.
  • Journal of Physics G: Nuclear and Particle Physics, Vol. 45, Issue 4
  • DOI: 10.1088/1361-6471/aaa90a