Search results for "energy [photon]"

showing 10 items of 18329 documents

Neutrino Flavor Sensitivity of Large Liquid Scintillator Detectors

2015

Scintillator detectors are known for their good light yield, energy resolution, timing characteristics and pulse shape discrimination capabilities. These features make the next-generation liquid scintillation detector LENA[1] (Low Energy Neutrino Astronomy) the optimal choice for a wide range of astro-particle topics including supernova-, solar-, and geo neutrinos. In addition to the excellent calorimetric and timing properties, scintillartor detectors (LSDs) are also capable of topology reconstruction sufficient to discriminate with adequate efficiency between electron and muon neutrino induced charge current events and neutral current events in the GeV energy range. This feature makes LEN…

neutrino mass hierarchyPhysics::Instrumentation and Detectorsneutrino physicsliquid scintillation detectorsHigh Energy Physics::Experiment
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Coherence in neutrino oscillations

2011

The theory of neutrino oscillations has turned out to be the most reasonable explanation to the observed violations in lepton number conservation of solar and atmospheric neutrino fluxes. A derivation of the most important results of this theory is first given using a plane wave treatment and subsequently using a three-dimensional shape-independent wave packet approach. Both methods give the same oscillation patterns, but only the latter one serves as a decent starting point for analyzing coherence in neutrino oscillations. A numerical analysis of the oscillation patterns on various distance scales is also given to graphically illustrate the phenomenon of neutrino oscillation and loss of co…

neutrino oscillationsneutrino physicsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::Phenomenologyquantum mechanicscoherence
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Phenomenology of non-standard neutrino interactions

2016

Today neutrino physics is in a privileged position within the fascinating field of particle physics. From the discovery of neutrino oscillations by Super-Kamiokande in 1998, the door to physics beyond the Standard Model (SM in what follows) has been opened. This fact implies that neutrinos have to be massive in opposition to the Standard Model assumption. However, this is not a surprise completely, but it was already hinted from theoretical and experimental observations in the two decades prior to the discovery of the oscillatory phenomenon, as neutrino masses included in unification models or the observed deficit of the atmospheric and solar neutrino fluxes. As a consequence of this new pa…

neutrino oscillationsnsi boundsnon-standard neutrino interactionsnon-unitarityHigh Energy Physics::PhenomenologyUNESCO::FÍSICA::Física de altas energías::Física teórica altas energíasneutrinoneutrino experimentsnsi constraints:FÍSICA::Física de altas energías::Física teórica altas energías [UNESCO]phenomenologyHigh Energy Physics::Experimentparticle physicsnon-unitary lepton mixing matrixseesaw modelsnsi
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Numerical studies on neutrino oscillation physics in long baseline experiments

2018

This thesis examines the prospects of future long baseline neutrino oscillation experiments. Using computer simulation techniques, we calculate the experimental sensitivities for two experimental configurations in a set of important questions which are all relevant for modern day neutrino physics. First, we set focus on the determination of the θ23 octant, where the aim is to find whether the atmospheric neutrino mixing angle θ23 lies in the high octant, θ23 > 45◦, or in the low octant, θ23 < 45◦. On the other hand, we study how well the long baseline experiments could test the limits of the Standard Model by seeking deviations from the oscillation patterns that follow from the standard three…

neutrino physicsHigh Energy Physics::Phenomenologyneutrino telescopesneutriinotsimulointinumeerinen analyysihiukkasfysiikkamassa (fysiikka)
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Search for sterile neutrinos in the CC verbatim_mark>mathend000# mode at the new CERN-SBLNF

2013

The possible existence of non-active neutrinos for the ElectroWeak interactions was first proposed in 1967 by B. Pontecorvo who named them "sterile" neutrinos. Recent tensions among world-wide experimental data renewed the possibility of one or more sterile neutrino states. Several "anomalies" emerged in radioactive sources and reactor neutrino experiments, as well as the long-standing LSND and the recent MiniBooNE hints for neutrino and antineutrino oscillations with a δm2 at the eV2 scale, not compatible with the standard 3 × 3 neutrino mixing scenario. While a huge effort is being devoted to establish the standard three-neutrino mixing paradigm no conclusive experiment was carried out to…

neutrino sterile oscillation ccPhysics::Instrumentation and DetectorsHigh Energy Physics::Phenomenologyneutrino sterileHigh Energy Physics::Experimentoscillationcc
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Search for a diffuse flux of high-energy ¿µ with the ANTARES neutrino telescope

2011

A search for a diffuse flux of astrophysical muon neutrinos, using data collected by the ANTARES neutrino telescope is presented. A $(0.83\times 2\pi)$ sr sky was monitored for a total of 334 days of equivalent live time. The searched signal corresponds to an excess of events, produced by astrophysical sources, over the expected atmospheric neutrino background. The observed number of events is found compatible with the background expectation. Assuming an $E^{-2}$ flux spectrum, a 90% c.l. upper limit on the diffuse $\nu_\mu$ flux of $E^2\Phi_{90%} = 5.3 \times 10^{-8} \ \mathrm{GeV\ cm^{-2}\ s^{-1}\ sr^{-1}} $ in the energy range 20 TeV - 2.5 PeV is obtained. Other signal models with differ…

neutrino telescope; antares; diffuse muon neutrino fluxNuclear and High Energy PhysicsParticle physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]media_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaNeutrino telescopeFluxAstrophysicsNeutrino telescope01 natural sciences7. Clean energySpectral lineMUONSLIMITS0103 physical sciencesNeutrins010306 general physicsDETECTORmedia_commonPhysicsRange (particle radiation)MuonsMuonANTARES:Física [Àrees temàtiques de la UPC]010308 nuclear & particles physicsMuon Collaboration[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::Instrumentation and Methods for AstrophysicsNeutrino astrophysics[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]MODELDiffuse muon neutrino fluxSky:Física::Astronomia i astrofísica [Àrees temàtiques de la UPC]High Energy Physics::ExperimentFísica nuclearNeutrinoAstrophysics - High Energy Astrophysical PhenomenaEnergy (signal processing)
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Neutrino masses and their implications for low energy experiments and the LHC

2020

Neutrino oscillations constitute the first experimental evidence of new physics. Con- trary to the prediction of the Standard Model, neutrinos are now well-established as particles with mass. In this thesis we study four topics related to neutrino masses. We examine a class of patterns of Majorana neutrino mass matrices, called two-zero textures, that could lead to the building of the underlying flavour theory. Using a purely numerical technique, we compare the constraints given by the textures with the most updated data of oscillation parameters. We find that the most promising textures are those of class A with normal ordering. Further, we revisit the case of excluded textures and study t…

neutrino:FÍSICA [UNESCO]High Energy Physics::PhenomenologyUNESCO::FÍSICAHigh Energy Physics::ExperimentLHC
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Muon neutrino charged current quasi-elastic interactions in the T2K off-axis near detector

2015

246 páginas. Tesis Doctoral del Departamento de Física Atómica, Molecular y Nuclear de la Universidad de Valencia y del Instituto de Física Corpuscular (IFIC).

neutrinoexperiment:FÍSICA [UNESCO]Physics::Instrumentation and DetectorsUNESCO::FÍSICAinteractionHigh Energy Physics::ExperimentFísica de Partículasquasi-elasticcharged current
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Deep Underground Neutrino Experiment (DUNE) Near Detector Conceptual Design Report

2021

The Deep Underground Neutrino Experiment (DUNE) is an international, world-class experiment aimed at exploring fundamental questions about the universe that are at the forefront of astrophysics and particle physics research. DUNE will study questions pertaining to the preponderance of matter over antimatter in the early universe, the dynamics of supernovae, the subtleties of neutrino interaction physics, and a number of beyond the Standard Model topics accessible in a powerful neutrino beam. A critical component of the DUNE physics program involves the study of changes in a powerful beam of neutrinos, i.e., neutrino oscillations, as the neutrinos propagate a long distance. The experiment co…

neutrinoneutriino-oskillaationeutrino oscillationsnear detectorDUNEPhysics::Instrumentation and DetectorsilmaisimettutkimuslaitteetneutriinotHigh Energy Physics::ExperimenthiukkasfysiikkaDeep Underground Neutrino Experiment
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Neutrino-nucleus scattering off 136Xe

2015

Background: Theoretical estimates of the cross sections for the neutrino-nucleus scattering off relevant nuclei for supernova neutrinos are essential for many applications in neutrino physics and astrophysics. The double- β-decaying nucleus 136Xe nucleus is used by the EXO Collaboration in the search for neutrinoless double-β decay. A ton-scale experiment based on 136Xe could also be used for studies of supernova neutrinos and/or solar neutrinos. Purpose: The purpose of the present work is, thus, to perform a study of the charged-current and neutral-current nuclear responses to supernova neutrinos for 136Xe. Method: The cross sections are computed by using the well-established framework for…

neutrino-nucleus scatteringAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyNuclear TheorynucleiHigh Energy Physics::ExperimentNuclear Experimentsupernova neutrinos
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