Search results for "NEUTRINO"

showing 10 items of 1752 documents

Dynamical zero in ν¯e–e− scattering and the neutrino magnetic moment

2005

Abstract The Standard Model differential cross section for ν ¯ e – e − elastic scattering vanishes exactly, at lowest order, for forward electrons and incident ν ¯ e energy close to the rest energy of the electron. This dynamical zero is not induced by a fundamental symmetry of the Lagrangian but by a destructive interference between the left- and right-handed chiral couplings of the electron in the charged and neutral current amplitudes. We show that lowest-order analyses based on this favorable kinematic configuration are only mildly affected by the inclusion of the O ( α ) radiative corrections in the ν ¯ e – e − differential cross section, thus providing an excellent opportunity for the…

Elastic scatteringPhysicsNuclear and High Energy PhysicsRecoilNeutral currentMagnetic momentScatteringQuantum electrodynamicsElectronNeutrinoStandard ModelPhysics Letters B
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Dynamical zeros in neutrino-electron elastic scattering at leading order

1994

We show the existence of dynamical zeros in the helicity amplitudes for neutrino-electron elastic scattering at lowest order in the standard theory. In particular, the $\lambda=1/2$ non-flip electron helicity amplitude in the electron antineutrino process vanishes for an incident neutrino energy $E_{\nu}=m_{e}/(4sin^{2}\theta_{W})$ and forward electrons (maximum recoil energy). The rest of helicity amplitudes show kinematical zeros in this configuration and therefore the cross section vanishes. Prospects to search for neutrino magnetic moment are discussed.

Elastic scatteringPhysicsParticle physicsScatteringComputer Science::Information RetrievalFísicaFOS: Physical sciencesElectronLambdaHelicityStandard ModelHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)AmplitudeQuantum mechanicsNeutrinoPhysical Review D
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Search for Coherent Elastic Scattering of Solar B8 Neutrinos in the XENON1T Dark Matter Experiment

2021

We report on a search for nuclear recoil signals from solar $^8$B neutrinos elastically scattering off xenon nuclei in XENON1T data, lowering the energy threshold from 2.6 keV to 1.6 keV. We develop a variety of novel techniques to limit the resulting increase in backgrounds near the threshold. No significant $^8$B neutrino-like excess is found in an exposure of 0.6 t $\times$ y. For the first time, we use the non-detection of solar neutrinos to constrain the light yield from 1-2 keV nuclear recoils in liquid xenon, as well as non-standard neutrino-quark interactions. Finally, we improve upon world-leading constraints on dark matter-nucleus interactions for dark matter masses between 3 GeV/…

Elastic scatteringPhysicsPhysics::Instrumentation and DetectorsScatteringAstrophysics::High Energy Astrophysical PhenomenaSolar neutrinoDark matterGeneral Physics and Astronomychemistry.chemical_element01 natural sciences7. Clean energyNuclear physicsXenonRecoilchemistry0103 physical sciencesHigh Energy Physics::ExperimentNeutrinoNuclear Experiment010306 general physicsOrder of magnitudePhysical Review Letters
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Near-intrinsic energy resolution for 30-662 keV gamma rays in a high pressure xenon electroluminescent TPC

2013

We present the design, data and results from the NEXT prototype for Double Beta and Dark Matter (NEXT-DBDM) detector, a high-pressure gaseous natural xenon electroluminescent time projection chamber (TPC) that was built at the Lawrence Berkeley National Laboratory. It is a prototype of the planned NEXT-100 Xe-136 neutrino-less double beta decay (0 nu beta beta) experiment with the main objectives of demonstrating near-intrinsic energy resolution at energies up to 662 keV and of optimizing the NEXT-100 detector design and operating parameters. Energy resolutions of similar to 1% FWHM for 662 keV gamma rays were obtained at 10 and 15 atm and similar to 5% FWHM for 30 keV fluorescence xenon X-…

ElectroluminiscènciaNuclear and High Energy PhysicsXenonHigh-pressureDark matterchemistry.chemical_elementNuclear physicsTECNOLOGIA ELECTRONICAXenonDouble beta decayEnergy resolutionNeutrinoless double beta decayInstrumentationPhysicsTime projection chamberDetectorResolution (electron density)Gamma rayFísicaNuclear energyFull width at half maximumchemistryElectroluminescenceEnergia nuclearTPC
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A deep study of the high–energy transient sky

2021

This is an open access article. This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article's Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article's Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds t…

Electromagnetic spectrumESA voyage 2050; High-energy transient sky; Multi-messenger astrophysics; Space mission concept; X–/γ–ray polarimetry; X–/γ–ray telescopes01 natural sciences7. Clean energylaw.inventionSettore FIS/05 - Astronomia E AstrofisicalawNuclear astrophysicsoptical010303 astronomy & astrophysicsmedia_commonPhysicsdensityStrong gravityAstrophysics::Instrumentation and Methods for AstrophysicsnucleosynthesisimagingParticle accelerationHigh-energy transient skyNeutrinoburstparticlelensmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenainterferometerSpace mission conceptTelescope0103 physical sciencesTeVequation of statepolarization010308 nuclear & particles physicsGravitational wavenucleusgravitational radiationAmbientaleAstronomyAstronomy and AstrophysicsaccelerationsensitivityMulti-messenger astrophysicsUniversemonitoringelectromagneticX–/γ–ray telescopesangular resolution[SDU]Sciences of the Universe [physics]13. Climate actionSpace and Planetary Sciencegamma raygravitationX–/γ–ray polarimetry[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]ESA voyage 2050
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"Table 4" of "Search for a right-handed gauge boson decaying into a high-momentum heavy neutrino and a charged lepton in $pp$ collisions with the ATL…

2019

Observed 95% CL exclusion contours in the $(m_{N_R}, m_{W_R})$ plane in the muon channel.

Exclusion limits13000.0WR --> NR lRight-hanedeHeavy neutrinoGauge BosonLeft-Right SymmetricP P --> WR
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"Table 2" of "Search for a right-handed gauge boson decaying into a high-momentum heavy neutrino and a charged lepton in $pp$ collisions with the ATL…

2019

Observed 95% CL exclusion contours in the $(m_{N_R}, m_{W_R})$ plane in the electron channel.

Exclusion limits13000.0WR --> NR lRight-hanedeHeavy neutrinoGauge BosonLeft-Right SymmetricP P --> WR
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"Table 3" of "Search for a right-handed gauge boson decaying into a high-momentum heavy neutrino and a charged lepton in $pp$ collisions with the ATL…

2019

Expected 95% CL exclusion contours in the $(m_{N_R}, m_{W_R})$ plane in the muon channel.

Exclusion limits13000.0WR --> NR lRight-hanedeHeavy neutrinoGauge BosonLeft-Right SymmetricP P --> WR
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"Table 1" of "Search for a right-handed gauge boson decaying into a high-momentum heavy neutrino and a charged lepton in $pp$ collisions with the ATL…

2019

Expected 95% CL exclusion contours in the $(m_{N_R}, m_{W_R})$ plane in the electron channel.

Exclusion limits13000.0WR --> NR lRight-hanedeHeavy neutrinoGauge BosonLeft-Right SymmetricP P --> WR
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Observation of High-Energy Astrophysical Neutrinos in Three Years of IceCube Data

2014

A search for high-energy neutrinos interacting within the IceCube detector between 2010 and 2012 provided the first evidence for a high-energy neutrino flux of extraterrestrial origin. Results from an analysis using the same methods with a third year (2012-2013) of data from the complete IceCube detector are consistent with the previously reported astrophysical flux in the 100 TeV - PeV range at the level of $10^{-8}\, \mathrm{GeV}\, \mathrm{cm}^{-2}\, \mathrm{s}^{-1}\, \mathrm{sr}^{-1}$ per flavor and reject a purely atmospheric explanation for the combined 3-year data at $5.7 \sigma$. The data are consistent with expectations for equal fluxes of all three neutrino flavors and with isotrop…

FLUXACTIVE GALACTIC NUCLEICosmology and Nongalactic Astrophysics (astro-ph.CO)TELESCOPESolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaGeneral Physics and AstronomyFOS: Physical sciencesAstrophysics01 natural sciences7. Clean energyIceCubeIceCube Neutrino ObservatoryHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)SEARCH0103 physical sciencesddc:550010303 astronomy & astrophysicsGAMMA-RAY BURSTSPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsGlashow resonanceHigh Energy Physics::PhenomenologyASTRONOMYAstronomySolar neutrino problemBLAZARSPhysics and AstronomyNeutrino detector13. Climate actionLEPTONSJETSMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino astronomyEMISSIONAstrophysics - High Energy Astrophysical PhenomenaphysicsAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review Letters
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