0000000000235166

AUTHOR

F. Froborg

showing 4 related works from this author

Recent Borexino results and perspectives of the SOX measurement

2017

International audience; Borexino is a liquid scintillator detector sited underground in the Laboratori Nazionali del Gran Sasso (Italy). Its physics program, until the end of this year, is focussed on the study of solar neutrinos, in particular from the Beryllium, pp, pep and CNO fusion reactions. Knowing the reaction chains in the sun provides insights towards physics disciplines such as astrophysics (star physics, star formation, etc.), astroparticle and particle physics. Phase II started in 2011 and its aim is to improve the phase I results, in particular the measurements of the neutrino fluxes from the pep and CNO processes. By the end of this year, data taking from the sun will be over…

Sterile neutrinoneutrino: solarPhysics::Instrumentation and DetectorsSolar neutrinoQC1-999scintillation counter: liquidanomaly[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]7. Clean energy01 natural sciencesStandard ModelNuclear physics0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear fusion010306 general physicsNeutrino oscillationBorexinoPhysicsgallium010308 nuclear & particles physicsStar formationPhysicsstar: formationstabilityneutrino: sterilesensitivityberylliumGran SassoLSNDelectron: lifetimeHigh Energy Physics::ExperimentBorexinoneutrino: oscillationnuclear reactorNeutrinoneutrino: geophysicstalk: Kolymbari 2017/08/17experimental results
researchProduct

Seasonal Modulation of the $^7$Be Solar Neutrino Rate in Borexino

2017

We detected the seasonal modulation of the $^7$Be neutrino interaction rate with the Borexino detector at the Laboratori Nazionali del Gran Sasso in Italy. The period, amplitude, and phase of the observed time evolution of the signal are consistent with its solar origin, and the absence of an annual modulation is rejected at 99.99\% C.L. The data are analyzed using three methods: the sinusoidal fit, the Lomb-Scargle and the Empirical Mode Decomposition techniques, which all yield results in excellent agreement.

liquid scintillators detectorsPhysics - Instrumentation and Detectorsexperimental methodsneutrino: solarPhysics::Instrumentation and DetectorsSolar neutrinolow background detectorsSolar neutrinos01 natural sciencesflux: time dependenceneutrino: fluxHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Liquid scintillators detectors; Low background detectors; Neutrino oscillations; Solar neutrinos; Astronomy and Astrophysics[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Borexinoneutrino: interactionMSW effectPhysicsNeutrino oscillationsDetectorAstrophysics::Instrumentation and Methods for AstrophysicsInstrumentation and Detectors (physics.ins-det)neutrino electron: elastic scatteringmodulationAmplitudeModulationsolar neutrinosBorexinoNeutrinoLiquid scintillators detectorFLUXLow background detectordata analysis methodNeutrino oscillationFOS: Physical sciencesSolar neutrinoNuclear physicsTIME-SERIES ANALYSIS[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]Low background detectorsLiquid scintillators detectorsSEARCH0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]SPACED DATA010306 general physicsNeutrino oscillationbackground: radioactivityneutrino oscillations010308 nuclear & particles physicsAstronomy and AstrophysicsEMPIRICAL MODE DECOMPOSITIONberylliumGran SassoHigh Energy Physics::Experimentneutrino: oscillationEvent (particle physics)experimental results
researchProduct

Limiting neutrino magnetic moments with Borexino Phase-II solar neutrino data

2017

A search for the solar neutrino effective magnetic moment has been performed using data from 1291.5 days exposure during the second phase of the Borexino experiment. No significant deviations from the expected shape of the electron recoil spectrum from solar neutrinos have been found, and a new upper limit on the effective neutrino magnetic moment of $\mu_{\nu}^{eff}$ $<$ 2.8$\cdot$10$^{-11}$ $\mu_{B}$ at 90\% c.l. has been set using constraints on the sum of the solar neutrino fluxes implied by the radiochemical gallium experiments.Using the limit for the effective neutrino moment, new limits for the magnetic moments of the neutrino flavor states, and for the elements of the neutrino magne…

Physics and Astronomy (miscellaneous)neutrino: solarPhysics::Instrumentation and DetectorsSolar neutrino01 natural sciencesHigh Energy Physics - ExperimentNeutrino detectorHigh Energy Physics - Experiment (hep-ex)SPIN ROTATIONHigh Energy Physics - Phenomenology (hep-ph)electron: recoil[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Astrophysics::Solar and Stellar AstrophysicsBorexinoS066MGMgalliumPhysicsMagnetic momentneutrino: magnetic momentHigh Energy Physics - Phenomenologyneutrino: momentNeutrino detectorneutrino: flavorneutrino: MajoranaMeasurements of neutrino speedBorexinoNeutrinoupper limitParticle physicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesSolar neutrinoDECAYSMagnetic momentNuclear physicsstatistical analysis[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]0103 physical sciencesddc:530010306 general physicsNeutrino oscillationDETECTORELECTROMAGNETIC PROPERTIES010308 nuclear & particles physicsHigh Energy Physics::PhenomenologySolar neutrino problemMAJORANA NEUTRINOS[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]electron: energy spectrum[ PHYS.HPHE ] Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics::Experimentexperimental resultsPhysical Review D
researchProduct

The Monte Carlo simulation of the Borexino detector

2017

We describe the Monte Carlo (MC) simulation package of the Borexino detector and discuss the agreement of its output with data. The Borexino MC 'ab initio' simulates the energy loss of particles in all detector components and generates the resulting scintillation photons and their propagation within the liquid scintillator volume. The simulation accounts for absorption, reemission, and scattering of the optical photons and tracks them until they either are absorbed or reach the photocathode of one of the photomultiplier tubes. Photon detection is followed by a comprehensive simulation of the readout electronics response. The algorithm proceeds with a detailed simulation of the electronics c…

Physics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsSolar neutrinoMonte Carlo methodscintillation counter: liquidSolar neutrinosenergy resolution01 natural sciences7. Clean energyLarge volume liquid scintillator detectorHigh Energy Physics - Experiment[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Large volume liquid scintillator detectorsBorexinoPhysicsphotomultipliertrack data analysisDetectorefficiency: quantumddc:540GEANTBorexinoNeutrinophoton: yieldnumerical calculations: Monte CarloPhotomultiplierdata analysis methodenergy lossScintillatorSolar neutrinoprogrammingphoton: reflectionMonte Carlo simulationsNuclear physics0103 physical sciencesphoton: scattering[INFO]Computer Science [cs][PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsbackground: radioactivityMonte Carlo simulationdetector: designScintillation010308 nuclear & particles physicsbibliographyAstronomy and AstrophysicscalibrationLarge volume liquid scintillator detectors; Monte Carlo simulations; Solar neutrinos; Astronomy and Astrophysicsattenuation: lengthpile-upelectronics: readout
researchProduct