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SUMMARY:Recent Results from Borexino
DTSTART;VALUE=DATE-TIME:20161013T101500Z
DTEND;VALUE=DATE-TIME:20161013T103000Z
DTSTAMP;VALUE=DATE-TIME:20260814T155751Z
UID:indico-contribution-74-744@cern.ch
DESCRIPTION:Speakers: Dominik Jeschke (Technical University of Munich)\nTh
 e Borexino experiment is taking data since 2007 at the „Laboratori Nazio
 nali del Gran Sasso“ in Italy accomplishing outstanding achievements in 
 the field of neutrino physics. Its success is strongly based on the unprec
 edented ultra-high radio-purity of the inner scintillator core.\nIn this t
 alk\, after introducing the main features of the detector\, the impressive
  results for solar and geo-neutrinos obtained by Borexino so far will be s
 ummarized. The main focus will be laid on the most recent and most promine
 nt results\, i.e. the first real-time measurement of the solar pp neutrino
  flux and the detection of the signal induced by geo-neutrinos with a sign
 ificance as high as 5.9 sigma. \nBesides the measurement of the pp neutrin
 o flux representing a direct probe of the major mechanism of energy produc
 tion in the Sun\, it makes Borexino the only experiment being able to prob
 e the entire solar neutrino spectrum and puts it in the unique position of
  being capable to test the MSW-LMA paradigm across the whole solar energy 
 range.  \nThe geo-neutrino data allow to infer information concerning impo
 rtant geophysical properties of the Earth that shall also be discussed. \n
 To conclude the talk\, the perspectives of the final stage of the Borexino
  solar neutrino program that are centered on the goal of measuring the onl
 y missing part of the solar neutrino spectrum\, the CNO neutrinos\, will b
 e outlined. In case of success\, this measurement would constitute the cli
 max of Borexino’s long search to reveal the properties of solar neutrino
 s and extend the understanding of our Sun.\n\nhttps://indico.particle.meph
 i.ru/event/4/contributions/744/
LOCATION:Milan Hotel Verdi
URL:https://indico.particle.mephi.ru/event/4/contributions/744/
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BEGIN:VEVENT
SUMMARY:Search for sterile neutrinos on the Gallium Germanium Neutrino Tel
 escope with artificial neutrino sources
DTSTART;VALUE=DATE-TIME:20161013T113000Z
DTEND;VALUE=DATE-TIME:20161013T114500Z
DTSTAMP;VALUE=DATE-TIME:20260814T155751Z
UID:indico-contribution-74-735@cern.ch
DESCRIPTION:Speakers: Vladimir Gavrin (INR RAS)\nThe current status of the
  short baseline experiment BEST with a 3MCi 51Cr artificial neutrino sourc
 e to search for transitions of electron neutrinos to sterile states on the
  Gallium Germanium Neutrino Telescope at the Baksan Neutrino Observatory I
 NR RAS is presented. The experiment has the great potential to search for 
 transitions of active neutrinos to sterile states with Δm2~ 1 eV2 and to 
 set the limits on short baseline electron neutrino disappearance oscillati
 on parameters. The possibilities of the further constraints of the oscilla
 tion parameters region with use of 65Zn source are discussed.\n\nhttps://i
 ndico.particle.mephi.ru/event/4/contributions/735/
LOCATION:Milan Hotel Verdi
URL:https://indico.particle.mephi.ru/event/4/contributions/735/
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SUMMARY:Sub-GeV atmospheric neutrinos background in organic liquid scintil
 lator mediums
DTSTART;VALUE=DATE-TIME:20161013T104500Z
DTEND;VALUE=DATE-TIME:20161013T110000Z
DTSTAMP;VALUE=DATE-TIME:20260814T155751Z
UID:indico-contribution-74-723@cern.ch
DESCRIPTION:Speakers: Viktor Atroshchenko (NRC Kurchatov Institute)\nAtmos
 pheric neutrinos are produced in interactions of cosmic rays with atomic n
 uclei in the Earth’s atmosphere. In low energy neutrino experiments they
  mainly considered as a background for studied processes. For atmospheric 
 neutrinos in energy range below 1 GeV we present semi-analytical expected 
 yield for four neutrino detection reactions: νp-ES\, νe-ES\, inverse β-
 decay and 12C(ν\, ν′)12C*(15.1 MeV)\, as well as results of Monte-Carl
 o simulation for other ν12C interaction channels. Calculations are made f
 or several neutrino experiments and include neutrino oscillation averaged 
 over neutrino arrival directions.\n\nhttps://indico.particle.mephi.ru/even
 t/4/contributions/723/
LOCATION:Milan Hotel Verdi
URL:https://indico.particle.mephi.ru/event/4/contributions/723/
END:VEVENT
BEGIN:VEVENT
SUMMARY:The search for sterile neutrinos in Troitsk $\\nu$-mass experiment
DTSTART;VALUE=DATE-TIME:20161013T110000Z
DTEND;VALUE=DATE-TIME:20161013T111500Z
DTSTAMP;VALUE=DATE-TIME:20260814T155751Z
UID:indico-contribution-74-705@cern.ch
DESCRIPTION:Speakers: Alexander Nozik (INR RAS)\nThe Troitsk $\\nu$-mass e
 xperiment was starter in the 1985 and was initially intended to search for
  the mass of electron neutrino. Currently it give the best direct upper li
 mit on that mass. In 2012\, after reanalyzing old data for traces of relat
 ively light sterile neutrinos (with masses up to 200 eV)\, the setup was m
 odified to search for sterile neutrinos in a wider range (up to 3 keV and 
 in future probably up to 5 keV).\nThe report contains a brief overview of 
 the experiment layout\, past results\, some unique techniques developed in
  this experiment and finally\, some preliminary results on keV sterile neu
 trinos.\n\nhttps://indico.particle.mephi.ru/event/4/contributions/705/
LOCATION:Milan Hotel Verdi
URL:https://indico.particle.mephi.ru/event/4/contributions/705/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Study in Support of Chromium-51 Accumulation in the SM-3 Reactor t
 o Fabricate a Neutrino Source
DTSTART;VALUE=DATE-TIME:20161013T111500Z
DTEND;VALUE=DATE-TIME:20161013T113000Z
DTSTAMP;VALUE=DATE-TIME:20260814T155751Z
UID:indico-contribution-74-701@cern.ch
DESCRIPTION:Speakers: Evgeny Romanov (JSC "SSC RIAR"\, ROSATOM)\nHigh-inte
 nsity artificial Cr-51 sources are used to calibrate solar neutrino detect
 ors. The necessary amount of Cr-51 can be obtained by irradiating chromium
  enriched in Cr-50 in a thermal neutron trap of the SM-3 high-flux reactor
  in JSC “SSC RIAR”. The paper presents the analysis of irradiation opt
 ions both using the existing trap and advanced trap designs to be used dur
 ing the reactor future refurbishment. The feasibility to produce 3.85Ci of
  Cr-51 by the end of irradiation is shown.\n\nhttps://indico.particle.meph
 i.ru/event/4/contributions/701/
LOCATION:Milan Hotel Verdi
URL:https://indico.particle.mephi.ru/event/4/contributions/701/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Status of the SOX project
DTSTART;VALUE=DATE-TIME:20161013T120000Z
DTEND;VALUE=DATE-TIME:20161013T121500Z
DTSTAMP;VALUE=DATE-TIME:20260814T155751Z
UID:indico-contribution-74-698@cern.ch
DESCRIPTION:Speakers: Alina Vishneva (DLNP JINR)\nRecent data of reactor n
 eutrino experiments give a hint for anomalously low antineutrino flux at s
 hort distances.\nA possible explanation of this anomaly is the presence of
  sterile neutrinos.\nSOX project is based on the idea of placing a neutrin
 o source close to a large volume detector in order to look for the flux su
 ppression and the oscillation pattern inside the detector volume. In this 
 project a ~100 kCi 144Ce-144Pr source is intended to be placed under the B
 orexino detector.\n\nhttps://indico.particle.mephi.ru/event/4/contribution
 s/698/
LOCATION:Milan Hotel Verdi
URL:https://indico.particle.mephi.ru/event/4/contributions/698/
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SUMMARY:Measurement of the spectrum of internal bremsstrahlung Cr51
DTSTART;VALUE=DATE-TIME:20161013T114500Z
DTEND;VALUE=DATE-TIME:20161013T120000Z
DTSTAMP;VALUE=DATE-TIME:20260814T155751Z
UID:indico-contribution-74-619@cern.ch
DESCRIPTION:Speakers: Valery Gorbachev (A)\nThe report presents the result
 s of measurements of the spectrum of internal bremsstrahlung (IB) Cr51. Th
 e isotope Cr51 was used for production of intense neutrino sources for cal
 ibrations of gallium solar neutrino detectors. By measuring the IB spectru
 m Cr51 it is planned to determine the source activity in the experiment BE
 ST to search for sterile neutrino in gallium target.\n\nhttps://indico.par
 ticle.mephi.ru/event/4/contributions/619/
LOCATION:Milan Hotel Verdi
URL:https://indico.particle.mephi.ru/event/4/contributions/619/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Methodology of experimental search for neutrinos from solar flares
  in Borexino detector
DTSTART;VALUE=DATE-TIME:20161013T103000Z
DTEND;VALUE=DATE-TIME:20161013T104500Z
DTSTAMP;VALUE=DATE-TIME:20260814T155751Z
UID:indico-contribution-74-486@cern.ch
DESCRIPTION:Speakers: Maria Toropova (NRC Kurchatov Institute)\nSolar flar
 es are sudden variations in brightness observed near the Sun's surface. So
 me theorethical models predict production of electron and muon neutrinos w
 ith energies up to few tens of MeV during solar flares. In 1980th the Home
 stake experiment reported excess of detected neutrino events possibly corr
 elated with large solar flares. Since then the interest to similar studies
  by other neutrino detectors has increased. In this talk we summarize the 
 status of experimental searches and describe the methodology for the study
  of neutrinos from solar flares in Borexino liquid scintillator detector.\
 n\nhttps://indico.particle.mephi.ru/event/4/contributions/486/
LOCATION:Milan Hotel Verdi
URL:https://indico.particle.mephi.ru/event/4/contributions/486/
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