Spectrum of Supernova Neutrinos in Ultra-pure Scintillators
arXiv:1402.6953 · doi:10.1088/1475-7516/2014/07/051
Abstract
There is a great interest in measuring the non-electronic component of neutrinos from core collapse supernovae by observing, for the first time, also neutral-current reactions. In order to assess the physics potential of the ultra-pure scintillators in this respect, we study the entire expected energy spectrum in the Borexino, KamLAND and SNO+ detectors. We examine the various sources of uncertainties in the expectations, and in particular, those due to specific detector features and to the relevant cross sections. We discuss the possibility to identify the different neutrino flavors, and we quantify the effect of confusion, due to other components of the energy spectrum, overlapped with the neutral-current reactions of interest.
13 pages, 3 figures
References in corpus (10)
- Multiple Spectral Splits of Supernova Neutrinos
- Red supergiants as potential Type IIn supernova progenitors: Spatially resolved 4.6 micron CO emission around VY CMa and Betelgeuse
- Neutrino Mass Hierarchy and Stepwise Spectral Swapping of Supernova Neutrino Flavors
- Improved analysis of SN1987A antineutrino events
- Neutrino-Nucleus Reaction Cross Sections for Light Element Synthesis in Supernova Explosions
- A New Multi-Dimensional General Relativistic Neutrino Hydrodynamics Code for Core-Collapse Supernovae IV. The Neutrino Signal
- Overview of the Jiangmen Underground Neutrino Observatory (JUNO)
- Scintillation decay time and pulse shape discrimination in oxygenated and deoxygenated solutions of linear alkylbenzene for the SNO+ experiment
- Study of the effect of neutrino oscillations on the supernova neutrino signal in the LVD detector
- Measurement of the proton light response of various LAB based scintillators and its implication for supernova neutrino detection via neutrino-proton scattering
Cited by in corpus (21)
- Getting the Most from Detection of Galactic Supernova Neutrinos in Future Large Liquid-Scintillator Detectors
- Comparative analysis of SN1987A antineutrino fluence
- What can we learn on supernova neutrino spectra with water Cherenkov detectors?
- Supernova Neutrino Neutrino Astronomy
- Robust measurement of supernova spectra with future neutrino detectors
- Towards a complete reconstruction of supernova neutrino spectra in future large liquid-scintillator detectors
- A model-independent approach to the reconstruction of multi-flavor supernova neutrino energy spectra
- Measuring the neutron star compactness and binding energy with supernova neutrinos
- Nuclear structure uncertainties in coherent elastic neutrino-nucleus scattering
- Probing protoneutron stars with gamma-ray axionscopes
- Prospects for Pre-supernova Neutrino Observation in Future Large Liquid-scintillator Detectors
- Probing Neutrino Mass Hierarchy by Comparing the Charged-Current and Neutral-Current Interaction Rates of Supernova Neutrinos
- Prospects of the search for neutrino bursts from Supernovae with Baksan Large Volume Scintillation Detector
- Pinpointing astrophysical bursts of low-energy neutrinos embedded into the noise
- Borexino's search for low-energy neutrinos associated with gravitational wave events from GWTC-3 database
- A deuterated liquid scintillator for supernova neutrino detection
- Supernova neutrino scattering off Gadolinium odd isotopes in water Cherenkov detectors
- Supernova Neutrino Scattering off Gadolinium Even Isotopes in Water Cherenkov Detectors
- On Possibility of Determining Neutrino Mass Hierarchy by the Charged-Current and Neutral-Current Events of Supernova Neutrinos in Scintillation Detectors
- Search for Low-Energy Signals from Fast Radio Bursts with the Borexino Detector
- Supernova neutrino physics with a nuclear emulsion detector