0000000001104034

AUTHOR

B. K. Lubsandorzhiev

showing 4 related works from this author

The next-generation liquid-scintillator neutrino observatory LENA

2012

We propose the liquid-scintillator detector LENA (Low Energy Neutrino Astronomy) as a next-generation neutrino observatory on the scale of 50 kt. The outstanding successes of the Borexino and KamLAND experiments demonstrate the large potential of liquid-scintillator detectors in low-energy neutrino physics. LENA's physics objectives comprise the observation of astrophysical and terrestrial neutrino sources as well as the investigation of neutrino oscillations. In the GeV energy range, the search for proton decay and long-baseline neutrino oscillation experiments complement the low-energy program. Based on the considerable expertise present in European and international research groups, the …

Neutrino detectors; Liquid-scintillator detectors; Low-energy neutrinos; Proton decay; Longbaseline neutrino beamsParticle physicsPhysics - Instrumentation and Detectors[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Physics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaLongbaseline neutrino beamsFOS: Physical sciencesLow-energy neutrinos7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentNONuclear physicsLiquid-scintillator detectorsHigh Energy Physics - Experiment (hep-ex)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex][PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Neutrino detectorsNeutrino oscillationInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsBorexinoPhysics010308 nuclear & particles physicsFísicaAstronomy and AstrophysicsInstrumentation and Detectors (physics.ins-det)Proton decaySolar neutrino problem[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Neutrino detectorddc:540Measurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino astronomyAstrophysics - Instrumentation and Methods for Astrophysics
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Measuring the 14C content in liquid scintillators

2016

We are going to perform a series of measurements where the 14C/12C ratio will be measured from several liquid scintillator samples with a dedicated setup. The setup is designed with the aim of measuring ratios smaller than 10−18. Measurements take place in two underground laboratories: in the Baksan Neutrino Observatory, Russia and in the Pyh¨asalmi mine, Finland. In Baksan the measurements started in 2015 and in Pyh¨asalmi they start in the beginning of 2015. In order to fully understand the operation of the setup and its background contributions a development of simulation packages has also been started. Low-energy neutrino detection with a liquid scintillator requires that the intrinsic …

low-energy neutrino detectionhiililiquid scintillatorsisotope ratio
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Multi-pixel Geiger-mode avalanche photodiode and wavelength shifting fibre readout of plastic scintillator counters of the EMMA underground experiment

2009

The results of a development of a scintillator counter with wavelength shifting (WLS) fibre and a multi-pixel Geiger-mode avalanche photodiode readout are presented. The photodiode has a metal-resistor-semiconductor layered structure and operates in the limited Geiger mode. The scintillator counter has been developed for the EMMA underground cosmic ray experiment.

PhysicsNuclear and High Energy PhysicsOptical fiberPhysics - Instrumentation and DetectorsPixelbusiness.industryPhysics::Instrumentation and DetectorsAstrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesPhysics::Physics EducationCosmic rayInstrumentation and Detectors (physics.ins-det)ScintillatorAvalanche photodiodePhotodiodelaw.inventionWavelengthOpticslawGeiger counterOptoelectronicsbusinessInstrumentation
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Towards 14C-free liquid scintillator

2017

A series of measurements has been started where the 14C concentration is determined from several liquid scintillator samples. A dedicated setup has been designed and constructed with the aim of measuring concentrations smaller than 10−18. Measurements take place in two underground laboratories: in the Baksan Neutrino Observatory, Russia, and in the new Callio Lab in the Pyhäsalmi mine, Finland. Low-energy neutrino detection with a liquid scintillator requires that the intrinsic 14C concentration in the liquid is extremely low. In the Borexino CTF detector the concentration of 2 × 10−18 has been achieved being the lowest value ever measured. In principle, the older the oil or gas source that…

low-energy neutrino detectionPhysics::Instrumentation and Detectorsilmaisimethiilineutriinotliquid scintillatorsisotope ratio
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