Simulated Neutrino Signals of Low and Intermediate Energy Neutrinos on Cd Detectors

Neutrino-nucleus reactions cross sections, obtained for neutrino energies in the range εν ≤ 100–120 MeV (low- and intermediate-energy range), which refer to promising neutrino detection targets of current terrestrial neutrino experiments, are presented and discussed. At first, we evaluated original...

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Main Authors: J. Sinatkas, Vaitsa Tsakstara, Odysseas Kosmas
Format: Article
Language:English
Published: Frontiers Media S.A. 2019-04-01
Series:Frontiers in Physics
Subjects:
Online Access:https://www.frontiersin.org/article/10.3389/fphy.2019.00042/full
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author J. Sinatkas
Vaitsa Tsakstara
Vaitsa Tsakstara
Odysseas Kosmas
author_facet J. Sinatkas
Vaitsa Tsakstara
Vaitsa Tsakstara
Odysseas Kosmas
author_sort J. Sinatkas
collection DOAJ
description Neutrino-nucleus reactions cross sections, obtained for neutrino energies in the range εν ≤ 100–120 MeV (low- and intermediate-energy range), which refer to promising neutrino detection targets of current terrestrial neutrino experiments, are presented and discussed. At first, we evaluated original cross sections for elastic scattering of neutrinos produced from various astrophysical and laboratory neutrino sources with the most abundant Cd isotopes 112Cd, 114Cd, and 116Cd. These isotopes constitute the main material of the COBRA detector aiming to search for neutrinoless double beta decay events and neutrino-nucleus scattering events at the Gran Sasso laboratory (LNGS). The coherent ν-nucleus reaction channel addressed with emphasis here, dominates the neutral current ν-nucleus scattering, events of which have only recently been observed for a first time in the COHERENT experiment at Oak Ridge. Subsequently, simulated ν-signals expected to be recorded at Cd detectors are derived through the application of modern simulation techniques and employment of reliable neutrino distributions of astrophysical ν-sources (as the solar, supernova, and Earth neutrinos), as well as laboratory neutrinos (like the reactor neutrinos, the neutrinos produced from pion-muon decay at rest and the β-beam neutrinos produced from the acceleration of radioactive isotopes at storage rings as e.g., at CERN).PACS numbers: 26.50.+x, 25.30.Pt, 97.60.Bw, 25.30.-c, 23.40.Bw, 21.60.Jz
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spelling doaj.art-48e60d86434b4563a820ab4864d0b83b2022-12-22T01:39:44ZengFrontiers Media S.A.Frontiers in Physics2296-424X2019-04-01710.3389/fphy.2019.00042426092Simulated Neutrino Signals of Low and Intermediate Energy Neutrinos on Cd DetectorsJ. Sinatkas0Vaitsa Tsakstara1Vaitsa Tsakstara2Odysseas Kosmas3Department of Informatics Engineering, Technological Institute of Western Macedonia, Kastoria, GreeceElectrical Engineering Department, Technological Institute of Western Macedonia, School of Applied Science, Kozani, GreeceDivision of Theoretical Physics, University of Ioannina, Ioannina, GreeceModelling and Simulation Centre, MACE, University of Manchester, Manchester, United KingdomNeutrino-nucleus reactions cross sections, obtained for neutrino energies in the range εν ≤ 100–120 MeV (low- and intermediate-energy range), which refer to promising neutrino detection targets of current terrestrial neutrino experiments, are presented and discussed. At first, we evaluated original cross sections for elastic scattering of neutrinos produced from various astrophysical and laboratory neutrino sources with the most abundant Cd isotopes 112Cd, 114Cd, and 116Cd. These isotopes constitute the main material of the COBRA detector aiming to search for neutrinoless double beta decay events and neutrino-nucleus scattering events at the Gran Sasso laboratory (LNGS). The coherent ν-nucleus reaction channel addressed with emphasis here, dominates the neutral current ν-nucleus scattering, events of which have only recently been observed for a first time in the COHERENT experiment at Oak Ridge. Subsequently, simulated ν-signals expected to be recorded at Cd detectors are derived through the application of modern simulation techniques and employment of reliable neutrino distributions of astrophysical ν-sources (as the solar, supernova, and Earth neutrinos), as well as laboratory neutrinos (like the reactor neutrinos, the neutrinos produced from pion-muon decay at rest and the β-beam neutrinos produced from the acceleration of radioactive isotopes at storage rings as e.g., at CERN).PACS numbers: 26.50.+x, 25.30.Pt, 97.60.Bw, 25.30.-c, 23.40.Bw, 21.60.Jzhttps://www.frontiersin.org/article/10.3389/fphy.2019.00042/fullnuclear detector responsesneutrino nucleus cross sectionssupernova neutrino detectionneutral-current neutrino-nucleus processesquasi-particle random phase approximation
spellingShingle J. Sinatkas
Vaitsa Tsakstara
Vaitsa Tsakstara
Odysseas Kosmas
Simulated Neutrino Signals of Low and Intermediate Energy Neutrinos on Cd Detectors
Frontiers in Physics
nuclear detector responses
neutrino nucleus cross sections
supernova neutrino detection
neutral-current neutrino-nucleus processes
quasi-particle random phase approximation
title Simulated Neutrino Signals of Low and Intermediate Energy Neutrinos on Cd Detectors
title_full Simulated Neutrino Signals of Low and Intermediate Energy Neutrinos on Cd Detectors
title_fullStr Simulated Neutrino Signals of Low and Intermediate Energy Neutrinos on Cd Detectors
title_full_unstemmed Simulated Neutrino Signals of Low and Intermediate Energy Neutrinos on Cd Detectors
title_short Simulated Neutrino Signals of Low and Intermediate Energy Neutrinos on Cd Detectors
title_sort simulated neutrino signals of low and intermediate energy neutrinos on cd detectors
topic nuclear detector responses
neutrino nucleus cross sections
supernova neutrino detection
neutral-current neutrino-nucleus processes
quasi-particle random phase approximation
url https://www.frontiersin.org/article/10.3389/fphy.2019.00042/full
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