0000000000092886

AUTHOR

I. Neri

showing 5 related works from this author

Corrigendum to “Premature ovarian senescence and a high miscarriage rate impair fertility in women with HCV” [J Hepatol 68 (2018) 33–41](S01688278173…

2018

It has come to our attention that the PITER framework investigator, Alessandro Federico, was incorrectly listed as F. Alessandro in the original manuscript. Please note that the correct name of this author is Alessandro Federico (2nd University of Naples). The correct list of PITER investigators is in the footnote below.

HepatologyHepatitis B; EASL guidelines; Treatment; Interferon; Entecavir; Tenofovir; TAF; HBsAg; Hepatocellular carcinoma; HBV DNA; HBV reactivation; Mother to child transmissionHepatocellular carcinomaHBV reactivationEASL guidelinesHepatitis BEntecavirTreatmentHBsAgTAFHBV DNAMother to child transmissionInterferonTenofovirEASL guideline
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Search for heavy neutrinos at the NA48/2 and NA62 experiments at CERN

2018

© The Authors, published by EDP Sciences. The NA48/2 experiment at CERN has collected large samples of charged kaons decaying into a pion and two muons for the search of heavy nuetrinos. In addition, its successor NA62 has set new limits on the rate of charged kaon decay into a heavy neutral lepton (HNL) and a lepton, with = e, µ, using the data collected in 2007 and 2015. New limits on heavy neutrinos from kaon decays into pions, muons and positrons are presented in this report.

PhysicsParticle physicsLarge Hadron ColliderMuonPhysics::Instrumentation and Detectors010308 nuclear & particles physicsPhysicsQC1-999Nuclear TheoryHigh Energy Physics::PhenomenologyHeavy neutrino01 natural sciencesSettore FIS/04 - Fisica Nucleare e SubnuclearePhysics and Astronomy (all)Pion0103 physical sciencesHigh Energy Physics::ExperimentKaon decaysNeutrinoHeavy neutrinoNuclear Experiment010306 general physicsKaon decays Heavy neutrinoParticle Physics - ExperimentLepton
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Search for K+→ π+νν¯ at NA62

2018

Flavour physics is one of the most powerful fields for the search of new physics beyond the Standard Model. The kaon sector with the rare decay K+ → π+νν̅ provides one of the cleanest and most promising channels. NA62, a fixed target experiment at the CERN SPS, aims to measure BR (K+ → π+νν̅) with 10% precision to test the Standard Model validity up to an energy scale of hundreds of TeV. NA62 had dedicated data taking for the K+ → π+νν̅ measurement in 2016 and 2017 and will continue in 2018. Here preliminary results on a fraction of 2016 dataset are presented. The analysis of the complete 2016 data sample is expected to achieve the SM sensitivity.

PhysicsParticle physicsLarge Hadron Collider010308 nuclear & particles physicsPhysics beyond the Standard ModelPhysicsQC1-999Flavour Physicsrare Kaon decays01 natural sciencesMeasure (mathematics)Settore FIS/04 - Fisica Nucleare e SubnucleareStandard ModelPhysics and Astronomy (all)0103 physical sciences010306 general physicsFlavour Physics rare Kaon decays
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Multimessenger search for sources of gravitational waves and high-energy neutrinos: Initial results for LIGO-Virgo and IceCube

2014

Made available in DSpace on 2022-04-29T07:21:49Z (GMT). No. of bitstreams: 0 Previous issue date: 2014-11-17 We report the results of a multimessenger search for coincident signals from the LIGO and Virgo gravitational-wave observatories and the partially completed IceCube high-energy neutrino detector, including periods of joint operation between 2007-2010. These include parts of the 2005-2007 run and the 2009-2010 run for LIGO-Virgo, and IceCube's observation periods with 22, 59 and 79 strings. We find no significant coincident events, and use the search results to derive upper limits on the rate of joint sources for a range of source emission parameters. For the optimistic assumption of …

MECHANISMPhysics and Astronomy (miscellaneous)AstrophysicsFOLLOW-UP OBSERVATIONSASTROPHYSICAL SOURCESIceCubeneutrinoDetection of gravitational waveGravitational waves neutrinoObservatory[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]QCLIGO Scientific CollaborationQBPhysicsGAMMA-RAY BURSTS[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Settore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsASTRONOMYNuclear and High Energy Physics; Physics and Astronomy (miscellaneous)NEUTRINOSNeutrino detectorComputingMethodologies_DOCUMENTANDTEXTPROCESSINGNeutrinoSENSITIVITYGIANT FLARENuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]95.85.RyMUON NEUTRINOSAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Cosmology and Extragalactic AstrophysicsACCELERATIONGravitational wavesGeneral Relativity and Quantum CosmologyINSTABILITIESSettore FIS/05 - Astronomia e AstrofisicaCORE-COLLAPSE SUPERNOVAE[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]ddc:530SDG 7 - Affordable and Clean EnergyCORE-COLLAPSEDETECTOR/dk/atira/pure/sustainabledevelopmentgoals/affordable_and_clean_energyGravitational wave95.85.SzMAGNETIZED NEUTRON-STARS[ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]AstronomyTRANSIENTS95.85.Sz; 95.85.RyRELATIVISTIC STARSLIGOPhysics and Astronomy[ SDU.ASTR.HE ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Gamma-ray burstEMISSIONEnergy (signal processing)
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A first search for coincident gravitational waves and high energy neutrinos using LIGO, Virgo and ANTARES data from 2007

2013

A search for high-energy neutrinos coming from the direction of the Sun has been performed using the data recorded by the ANTARES neutrino telescope during 2007 and 2008. The neutrino selection criteria have been chosen to maximize the selection of possible signals produced by the self-annihilation of weakly interacting massive particles accumulated in the centre of the Sun with respect to the atmospheric background. After data unblinding, the number of neutrinos observed towards the Sun was found to be compatible with background expectations. The 90% CL upper limits in terms of spin-dependent and spin-independent WIMP-proton cross-sections are derived and compared to predictions of two sup…

AstrofísicaEXPLOSIONSHigh energyPhotonPOINT SOURCESSUPERCONDUCTING COSMIC STRINGSGravitational waves / experimentsGravitational waves/experimentsAstrophysics01 natural scienceshigh energy neutrinosgravitational wavesgravitational waves / experiment010303 astronomy & astrophysicsQCmedia_commonLine (formation)QBPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)GAMMA-RAY BURSTSdark matter detectorsGravitational waves / experiments; Neutrino astronomy; Astronomy and Astrophysicshigh energy neutrinos[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Settore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for Astrophysicsgravitational waves; gravitational waves / experiments; neutrino astronomy; high energy neutrinos; high energy neutrinosgravitational wavesgravitational wavesparticle physics - cosmology connectionNeutrino astronomyCOSMIC STRINGSRELATIVISTIC JETSNeutrinoAstrophysics - High Energy Astrophysical Phenomenasupersymmetry and cosmology[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]gravitational waves / experiments; neutrino astronomyTELESCOPEmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaSCIENCE RUNFOS: Physical sciencesddc:500.2GAMMA-RAY BURSTS; CORE-COLLAPSE SUPERNOVAE; SUPERCONDUCTING COSMIC STRINGS; MAGNETAR GIANT FLARES; SCIENCE RUN; RELATIVISTIC JETS; POINT SOURCES; BLACK-HOLES; LOCAL-RATE; TELESCOPEGravitational wavesGeneral Relativity and Quantum CosmologyCORE-COLLAPSE SUPERNOVAESettore FIS/05 - Astronomia e AstrofisicaCoincidentneutrino experiments0103 physical sciences010306 general physicsMAGNETAR GIANT FLARESBLACK-HOLESHigh Energy Astrophysical PhenomenaGravitational waveAstronomy[ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astronomy and AstrophysicsDRIVENUniverseLIGOGIANT FLARESLOCAL-RATEFISICA APLICADALUMINOSITYRADIATIONHigh Energy Physics::Experiment[ SDU.ASTR.HE ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Experiments[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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