skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Probing neutrino mass hierarchy by comparing the charged-current and neutral-current interaction rates of supernova neutrinos

Journal Article · · Journal of Cosmology and Astroparticle Physics
 [1];  [2];  [3];  [4];  [4];  [3]
  1. Center for General Education, Chang Gung University,Kwei-Shan, Taoyuan, 333, Taiwan (China)
  2. Institute of Physics, National Chiao Tung University,Hsinchu, 300, Taiwan (China)
  3. Department of Electrophysics, National Chiao Tung University,Hsinchu, 300, Taiwan (China)
  4. Leung Center for Cosmology and Particle Astrophysics (LeCosPA), National Taiwan University, Taipei, 106, Taiwan (China)

The neutrino mass hierarchy is one of the neutrino fundamental properties yet to be determined. We introduce a method to determine neutrino mass hierarchy by comparing the interaction rate of neutral current (NC) interactions, ν(ν-bar)+p→ν(ν-bar)+p, and inverse beta decays (IBD), ν-bar{sub e}+p→n+e{sup +}, of supernova neutrinos in scintillation detectors. Neutrino flavor conversions inside the supernova are sensitive to neutrino mass hierarchy. Due to Mikheyev-Smirnov-Wolfenstein effects, the full swapping of ν-bar{sub e} flux with the ν-bar{sub x} (x=μ, τ) one occurs in the inverted hierarchy, while such a swapping does not occur in the normal hierarchy. As a result, more high energy IBD events occur in the detector for the inverted hierarchy than the high energy IBD events in the normal hierarchy. By comparing IBD interaction rate with the mass hierarchy independent NC interaction rate, one can determine the neutrino mass hierarchy.

Sponsoring Organization:
SCOAP3, CERN, Geneva (Switzerland)
OSTI ID:
22572121
Journal Information:
Journal of Cosmology and Astroparticle Physics, Vol. 2016, Issue 07; Other Information: PUBLISHER-ID: JCAP07(2016)039; OAI: oai:repo.scoap3.org:16558; cc-by Article funded by SCOAP3. Content from this work may be used under the terms of the Creative Commons Attribution 3.0 License. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.; Country of input: International Atomic Energy Agency (IAEA); ISSN 1475-7516
Country of Publication:
United States
Language:
English

Similar Records

Hybrid method to resolve the neutrino mass hierarchy by supernova (anti)neutrino induced reactions
Journal Article · Mon Feb 01 00:00:00 EST 2016 · Journal of Cosmology and Astroparticle Physics · OSTI ID:22572121

Neutrino oscillations in magnetically driven supernova explosions
Journal Article · Tue Sep 01 00:00:00 EDT 2009 · Journal of Cosmology and Astroparticle Physics · OSTI ID:22572121

Effects of neutrino temperatures and mass hierarchies on the detection of supernova neutrinos
Journal Article · Sat Apr 01 00:00:00 EST 2000 · Physical Review. D, Particles Fields · OSTI ID:22572121