# Hybrid method to resolve the neutrino mass hierarchy by supernova (anti)neutrino induced reactions

```@article{Vale2015HybridMT,
title={Hybrid method to resolve the neutrino mass hierarchy by supernova (anti)neutrino induced reactions},
author={Deni Vale and Thomas Rauscher and Nils Paar},
journal={Journal of Cosmology and Astroparticle Physics},
year={2015},
volume={2016},
pages={007 - 007}
}```
• Published 24 September 2015
• Physics
• Journal of Cosmology and Astroparticle Physics
We introduce a hybrid method to determine the neutrino mass hierarchy by simultaneous measurements of responses of at least two detectors to antineutrino and neutrino fluxes from accretion and cooling phases of core-collapse supernovae. The (anti)neutrino-nucleus cross sections for 56Fe and 208Pb are calculated in the framework of the relativistic nuclear energy density functional and weak interaction Hamiltonian, while the cross sections for inelastic scattering on free protons p(ν̄e,e+)n are…
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## References

SHOWING 1-10 OF 281 REFERENCES
Large-scale calculations of supernova neutrino-induced reactions in Z=8-82 target nuclei
• Physics
• 2013
Background: In the environment of high neutrino fluxes provided in core-collapse supernovae or neutron star mergers, neutrino-induced reactions with nuclei contribute to the nucleosynthesis
The neutrino signal at HALO: learning about the primary supernova neutrino fluxes and neutrino properties
• Physics
• 2011
Core-collapse supernova neutrinos undergo a variety of phenomena when they travel from the high neutrino density region and large matter densities to the Earth. We perform analytical calculations of
Neutrino mass hierarchy and three-flavor spectral splits of supernova neutrinos
• Physics
• 2010
It was recently realized that three-flavor effects could peculiarly modify the development of spectral splits induced by collective oscillations, for supernova neutrinos emitted during the cooling
Simulation of coherent nonlinear neutrino flavor transformation in the supernova environment: Correlated neutrino trajectories
• Physics
• 2006
We present results of large-scale numerical simulations of the evolution of neutrino and antineutrino flavors in the region above the late-time post-supernova-explosion proto-neutron star. Our
Inclusive charged-current neutrino-nucleus reactions calculated with the relativistic quasiparticle random-phase approximation
• Physics
• 2008
Inclusive neutrino-nucleus cross sections are calculated using a consistent relativistic mean-field theoretical framework. The weak lepton-hadron interaction is expressed in the standard
Neutrino mass hierarchy and stepwise spectral swapping of supernova neutrino flavors.
• Physics
Physical review letters
• 2007
Large-scale numerical calculations show that in the normal neutrino mass hierarchy case, E(C) decreases as the assumed effective 2x2 vacuum nu(e)<==>nu(mu,tau) mixing angle (approximately theta13) is decreased.
Signatures of collective and matter effects on supernova neutrinos at large detectors
• Physics
• 2010
We calculate the expected galactic supernova neutrino signal at large next-generation underground detectors. At different epochs after the explosion, the primary fluxes can be quite different. For
Effects of neutrino oscillations on nucleosynthesis and neutrino signals for an 18 M ⊙ supernova model
• Physics
• 2015
In this paper, we explore the effects of neutrino flavor oscillations on supernova nucleosynthesis and on the neutrino signals. Our study is based on detailed information about the neutrino spectra
Multiangle effects in self-induced oscillations for different supernova neutrino fluxes
• Physics
• 2011
The non-isotropic nature of the neutrino emission from a supernova (SN) core might potentially affect the flavor evolution of the neutrino ensemble, via neutrino-neutrino interactions in the deepest