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BEGIN:VEVENT
SUMMARY:The CUORE Experiment : Neutrinoless Double Beta Decay Results
DTSTART;VALUE=DATE-TIME:20181023T154000Z
DTEND;VALUE=DATE-TIME:20181023T155500Z
DTSTAMP;VALUE=DATE-TIME:20260714T014307Z
UID:indico-contribution-139-1373@cern.ch
DESCRIPTION:Speakers: Cristopher Alduino (University of South Carolina)\nT
 he Cryogenic Underground Observatory for Rare Events (CUORE) is the first 
 bolometric experiment searching for neutrinoless double beta decay (0νβ
 β) that has been able to reach the one-ton scale. The detector consists o
 f an array of 988 TeO2 crystals arranged in a compact cylindrical structur
 e of 19 towers. The construction of the experiment was completed in August
  2016 with the installation of all towers in the cryostat. Following a coo
 ldown\, diagnostic\, and optimization campaign\, routine data-taking began
  in spring 2017. In this talk\, we present the 0νββ results of CUORE fr
 om examining a total TeO2 exposure of 86.3 kg∙yr\, characterized by an a
 verage energy resolution of 7.7 keV FWHM and a background in the region of
  interest of 0.014 counts/(keV∙kg∙yr). In this physics run\, CUORE pla
 ced a lower limit on the 130Te 0νββ half-life of > 1.3 × 10^25 yr (90%
  C.L.). We then discuss the additional improvements in the detector perfor
 mance achieved in 2018 and the latest update on the study of other rare pr
 ocesses in Tellurium and the evaluation of the background budget.\n\nhttps
 ://indico.particle.mephi.ru/event/22/contributions/1373/
LOCATION:Hotel Intourist Kolomenskoye 4* Petrovskiy hall
URL:https://indico.particle.mephi.ru/event/22/contributions/1373/
END:VEVENT
BEGIN:VEVENT
SUMMARY:The first observation of effect of oscillation in Neutrino-4 exper
 iment on search for sterile neutrino
DTSTART;VALUE=DATE-TIME:20181023T134500Z
DTEND;VALUE=DATE-TIME:20181023T141000Z
DTSTAMP;VALUE=DATE-TIME:20260714T014307Z
UID:indico-contribution-139-1363@cern.ch
DESCRIPTION:Speakers: Anatolii Serebrov ()\nWe report Neutrino-4 experimen
 t results of measurements of reactor antineutrinos flux and spectrum depen
 dence on the distance in range 6-12 meters from the center of the reactor 
 core. The fit of experimental dependence with the law $1⁄L^2$\, where L 
 is the distance from the reactor center\, gave satisfactory result with go
 odness of fit 81%. However\, we discovered that the experimental neutrino 
 spectrum is different from the calculated one. Using experimental spectrum
  we performed the model independent analysis of restrictions on oscillatio
 n parameters $\\Delta m_{14}^2$ and $sin^2 2\\Theta_{14}$. The results of 
 this analysis exclude area of reactor and gallium anomaly at C.L more than
  99.7%\n($>3\\sigma$) for values $\\Delta m_{14}^2 \\le 4~eV^2$ and $sin^2
  2\\Theta_{14} > 0.1$. However\, we observed an oscillation effect at C.L.
  99.7% ($3\\sigma$) in vicinity of $\\Delta m_{14}^2 \\approx 7~eV^2$ and 
 $sin^2 2\\Theta_{14} \\approx 0.35$. The method of coherent addition of re
 sults of measurements\, which allows us to directly observe the effect of 
 oscillations\, is proposed. The analysis of that effect is presented. In g
 eneral\, it seems that the effect predicted in gallium and reactor experim
 ents is confirmed but at sufficiently large value of $\\Delta m_{14}^2$. F
 uture prospects of the experiment are discussed.\n\nhttps://indico.particl
 e.mephi.ru/event/22/contributions/1363/
LOCATION:Hotel Intourist Kolomenskoye 4* Petrovskiy hall
URL:https://indico.particle.mephi.ru/event/22/contributions/1363/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Neutrino recoil force in electron-capture decay of polarized nucle
 i: measurement prospects and potential applications
DTSTART;VALUE=DATE-TIME:20181024T074500Z
DTEND;VALUE=DATE-TIME:20181024T080000Z
DTSTAMP;VALUE=DATE-TIME:20260714T014307Z
UID:indico-contribution-139-1231@cern.ch
DESCRIPTION:Speakers: Oleg Titov ()\nDue to parity violation in the weak i
 nteraction\, a sample of radioactive atoms will experience a recoil force 
 from neutrino radiation accompanying electron capture by polarized nuclei.
  The recoil force resulting from anisotropy of neutrino angular distributi
 on can be measured by modern micromechanical devices. Both angular distrib
 ution and recoil force are calculated for the case of allowed nuclear tran
 sitions. We consider the most suitable radioactive isotopes for such a mea
 surement. Potential applications are discussed.\n\nhttps://indico.particle
 .mephi.ru/event/22/contributions/1231/
LOCATION:Hotel Intourist Kolomenskoye 4* Petrovskiy hall
URL:https://indico.particle.mephi.ru/event/22/contributions/1231/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Experimental program of the COHERENT collaboration
DTSTART;VALUE=DATE-TIME:20181024T073000Z
DTEND;VALUE=DATE-TIME:20181024T074500Z
DTSTAMP;VALUE=DATE-TIME:20260714T014307Z
UID:indico-contribution-139-1230@cern.ch
DESCRIPTION:Speakers: Alexey Konovalov (ITEP / MEPhI)\nThe goal of the COH
 ERENT collaboration is to observe coherent elastic neutrino-nucleus scatte
 ring (CEvNS) using different target nuclei and detector technologies. The 
 talk focuses on the ongoing experimental effort and plans following the fi
 rst observation.\n\nhttps://indico.particle.mephi.ru/event/22/contribution
 s/1230/
LOCATION:Hotel Intourist Kolomenskoye 4* Petrovskiy hall
URL:https://indico.particle.mephi.ru/event/22/contributions/1230/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Experimental study of CEvNS process
DTSTART;VALUE=DATE-TIME:20181024T071500Z
DTEND;VALUE=DATE-TIME:20181024T073000Z
DTSTAMP;VALUE=DATE-TIME:20260714T014307Z
UID:indico-contribution-139-1228@cern.ch
DESCRIPTION:Speakers: Dmitry Akimov ()\nA review of experiments aimed on d
 etection and study of the recently discovered process of coherent elastic 
 neutrino-nucleus scattering (CEvNS) is presented.\n\nhttps://indico.partic
 le.mephi.ru/event/22/contributions/1228/
LOCATION:Hotel Intourist Kolomenskoye 4* Petrovskiy hall
URL:https://indico.particle.mephi.ru/event/22/contributions/1228/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Project KATRIN: First results and future plans.
DTSTART;VALUE=DATE-TIME:20181024T070000Z
DTEND;VALUE=DATE-TIME:20181024T071500Z
DTSTAMP;VALUE=DATE-TIME:20260714T014307Z
UID:indico-contribution-139-1227@cern.ch
DESCRIPTION:Speakers: Nikita Titov (INR RAS)\nThe KArlsruhe TRItium Neutri
 no (KATRIN) experiment aims to make a model-independent determination of t
 he active electron antineutrino mass with an upper limit of 0.2 eV/c2 from
  the analysis of Tritium beta-spectrum shape near the endpoint. Experiment
 al set-up is fully assembled and undergoes multiple tests. Small amount of
  Tritium molecules were injected at June 2018 and first spectra were measu
 red. Experimental program for the nearest future includes determination of
  active electron antineutrino mass with an upper limit of 1.0 eV/c2 and pr
 eliminary search for sterile neutrinos with several keV mass.\n\nhttps://i
 ndico.particle.mephi.ru/event/22/contributions/1227/
LOCATION:Hotel Intourist Kolomenskoye 4* Petrovskiy hall
URL:https://indico.particle.mephi.ru/event/22/contributions/1227/
END:VEVENT
BEGIN:VEVENT
SUMMARY:The background simulation of experiment for searching of 2K-captur
 e in $^{124}$Xe
DTSTART;VALUE=DATE-TIME:20181024T064500Z
DTEND;VALUE=DATE-TIME:20181024T070000Z
DTSTAMP;VALUE=DATE-TIME:20260714T014307Z
UID:indico-contribution-139-1226@cern.ch
DESCRIPTION:Speakers: Vladimir Kazalov (INR RAS)\nDuring several years at 
 the Baksan Neutrino Observatory INR RAS is undergoing the experiment for s
 earching of 2K (2$\\nu$)-capture in $^{124}$Xe. This isotope has several a
 dvantages: 1) it has the largest kinetic energy of transition Q – 2.866 
 MeV\, among candidates of nuclei for which predicted the existence of ECEC
 \; 2) since xenon is the noble gas\, then it could be easily use as a syst
 em isotope-detecting medium in a gas detector. To search for 2K-capture in
  $^{124}$Xe the large volume copper proportional counter (LPC) is used.\n\
 nIn our work\, we present the results of the simulation\, with the Geant4 
 package\, of LPC background from the decays of $^{238}$U and $^{232}$Th nu
 clei in the construction materials of the LPC case\, as well as in element
 s of the low-background shield. The influence of neutrons produced in the 
 rock of the underground laboratory from the decay of $^{238}$U and $^{232}
 $Th\, where the experimental setup is located\, on the production of the $
 ^{125}$I isotope in the working gas of the detector\, upon capture of ther
 malized neutrons by the $^{124}$Xe isotope is considered. The $^{125}$I is
 otope can have a significant influence on the background of the experiment
  since the total energy release in its decay belongs to the same energy re
 gion as ROI of 2K-capture in $^{124}$Xe.\n\nhttps://indico.particle.mephi.
 ru/event/22/contributions/1226/
LOCATION:Hotel Intourist Kolomenskoye 4* Petrovskiy hall
URL:https://indico.particle.mephi.ru/event/22/contributions/1226/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Search for neutrinoless double beta decay with the KamLAND-Zen exp
 eriment
DTSTART;VALUE=DATE-TIME:20181024T063000Z
DTEND;VALUE=DATE-TIME:20181024T064500Z
DTSTAMP;VALUE=DATE-TIME:20260714T014307Z
UID:indico-contribution-139-1225@cern.ch
DESCRIPTION:Speakers: Dmitry Chernyak (Kavli Institute for the Physics and
  Mathematics of the Universe\, The University of Tokyo)\nNeutrinoless doub
 le beta decay is a hypothetical nuclear transition which if observed will 
 allow to establish Majorana nature of neutrino\, determine the absolute ne
 utrino mass and the neutrino-mass hierarchy\, to verify the lepton number 
 violation and possible contribution of right-handed admixture to weak inte
 raction\, help to test leptogenesis\, existence of Nambu-Goldstone bosons 
 (majorons) and other effects beyond the Standard Model.\n\nThe KamLAND-Zen
  experiment is searching for neutrinoless double beta decay of Xe-136 by u
 sing xenon-loaded liquid scintillator inside the KamLAND detector. The exp
 eriment is located in the Kamioka underground laboratory (Hida\, Japan) at
  the depth of approximately 1000 m.\n\nThe previous phase of the experimen
 t called KamLAND-Zen 400 used 13 tons of Xe-loaded liquid scintillator con
 tained in a 3.08-m-diameter spherical inner balloon placed at the center o
 f the KamLAND detector. The amount of the enriched xenon gas was almost 40
 0 kg. The KamLAND-Zen 400 experiment was finished at the end of 2015 with 
 the upper limits on the effective Majorana neutrino mass are in the range 
 of 61–165 meV.\n\nStatus of the current phase of the experiment called K
 amLAND-Zen 800 will be reported. The amount of enriched Xe during this pha
 se will be increased up to ~750 kg. The production and installation of a n
 ew 3.84-m-diameter mini-balloon will be shown. The expected sensitivity on
  the effective Majorana neutrino mass will be discussed.\n\nProgress on R&
 D for the next phase of the experiment – KamLAND2-Zen – will be also p
 resented.\n\nhttps://indico.particle.mephi.ru/event/22/contributions/1225/
LOCATION:Hotel Intourist Kolomenskoye 4* Petrovskiy hall
URL:https://indico.particle.mephi.ru/event/22/contributions/1225/
END:VEVENT
BEGIN:VEVENT
SUMMARY:EXO-200 results
DTSTART;VALUE=DATE-TIME:20181024T061500Z
DTEND;VALUE=DATE-TIME:20181024T063000Z
DTSTAMP;VALUE=DATE-TIME:20260714T014307Z
UID:indico-contribution-139-1224@cern.ch
DESCRIPTION:Speakers: Vladimir Belov ()\nEXO-200 is dedicated for study of
  the double beta decay of $^{136}$Xe using 200kg of enriched xenon. This l
 arge and homogeneous TPC filled with liquid xenon have proven to be excell
 ent tool in the search for neutrinoless double beta decay with ultra-low b
 ackground and state of the art sensitivity. The experiment made the first 
 observation of the $2\\beta2\\nu$ decay in $^{136}$Xe and the most precise
  measurement of half-life among any double beta decay isotopes to date. I 
 will report on current status and the latest results obtained.\n\nhttps://
 indico.particle.mephi.ru/event/22/contributions/1224/
LOCATION:Hotel Intourist Kolomenskoye 4* Petrovskiy hall
URL:https://indico.particle.mephi.ru/event/22/contributions/1224/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Double beta decay experiments: present and future
DTSTART;VALUE=DATE-TIME:20181024T060000Z
DTEND;VALUE=DATE-TIME:20181024T061500Z
DTSTAMP;VALUE=DATE-TIME:20260714T014307Z
UID:indico-contribution-139-1223@cern.ch
DESCRIPTION:Speakers: Alexander Barabash (ITEP)\nA.S. Barabash\n          
  NRC “Kurchatov Institute”\, Institute of Theoretical and   Experiment
 al\n           Physics\, B. Cheremushkinskaya 25\, 117218 Moscow\, Russia\
 n\n\n\n     This report  reviews of modern double beta decay experiments. 
 Results of the most sensitive current experiments are discussed. The main 
 attention is paid to KamLAND-Zen\, EXO\, GERDA-II\, MAJORANA-DEMONSTRATOR\
 , CUORE and CUPID-0 experiments. Best present limits on neutrinoless doubl
 e beta decay are presented.  In the second part of the review prospects of
  search for the neutrinoless double beta decay in new experiments with sen
 sitivity to effective Majorana neutrino mass $\\langle m_{\\nu} \\rangle$ 
 at the level of $\\sim$ (0.01-0.1) eV are discussed. The main attention is
  paid to LEGEND\, CUPID\, nEXO\, KamLAND-Zen-2\, SuperNEMO and SNO+ experi
 ments. Prospects to improve sensitivity of future experiments  to $\\langl
 e m_{\\nu} \\rangle$  up to a few meV are considered.\n\nhttps://indico.pa
 rticle.mephi.ru/event/22/contributions/1223/
LOCATION:Hotel Intourist Kolomenskoye 4* Petrovskiy hall
URL:https://indico.particle.mephi.ru/event/22/contributions/1223/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Experiment BEST-2 with a source of 65Zn on gallium target for the 
 search of neutrino oscillations on a short baseline
DTSTART;VALUE=DATE-TIME:20181023T152500Z
DTEND;VALUE=DATE-TIME:20181023T154000Z
DTSTAMP;VALUE=DATE-TIME:20260714T014307Z
UID:indico-contribution-139-1222@cern.ch
DESCRIPTION:Speakers: Valery Gorbachev (BNO\, INR RAS)\nA proposal for an 
 experiment on a 2-zone gallium target of a solar Gallium-germanium neutrin
 o telescope in the Baksan neutrino Observatory of the INR RAS with a sourc
 e of 65Zn for short baseline neutrino oscillations search is considered. T
 he possibilities of determining the parameters of oscillations\, the neces
 sary characteristics of the neutrino source\, the possibility of its produ
 ction and use are described. The expected results are compared with the BE
 ST experiment with the 51Cr source.\n\nhttps://indico.particle.mephi.ru/ev
 ent/22/contributions/1222/
LOCATION:Hotel Intourist Kolomenskoye 4* Petrovskiy hall
URL:https://indico.particle.mephi.ru/event/22/contributions/1222/
END:VEVENT
BEGIN:VEVENT
SUMMARY:New results from the OPERA experiment in the CNGS neutrino beam
DTSTART;VALUE=DATE-TIME:20181023T151000Z
DTEND;VALUE=DATE-TIME:20181023T152500Z
DTSTAMP;VALUE=DATE-TIME:20260714T014307Z
UID:indico-contribution-139-1221@cern.ch
DESCRIPTION:Speakers: Svetlana Vasina (JINR)\nA new data analysis was perf
 ormed\, based on looser selection criteria and multivariate approach. Osci
 llation parameters and tau neutrino cross-section have been determined wit
 h a reduced statistical uncertainty\, and the discovery of tau neutrino ap
 pearance is confirmed with an improved significance level. Moreover\, the 
 search for electron neutrino events has been extended to the full dataset\
 , exploiting an improved method for the electron neutrino energy estimatio
 n. New limits have been set in the 3+1 neutrino model.\n\nhttps://indico.p
 article.mephi.ru/event/22/contributions/1221/
LOCATION:Hotel Intourist Kolomenskoye 4* Petrovskiy hall
URL:https://indico.particle.mephi.ru/event/22/contributions/1221/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Latest results from T2K
DTSTART;VALUE=DATE-TIME:20181023T145500Z
DTEND;VALUE=DATE-TIME:20181023T151000Z
DTSTAMP;VALUE=DATE-TIME:20260714T014307Z
UID:indico-contribution-139-1220@cern.ch
DESCRIPTION:Speakers: Andy Chappell (University of Warwick)\nT2K is a long
 -baseline neutrino oscillation experiment based in Japan. A muon neutrino 
 (or antineutrino) beam is produced at JPARC and sent 295 km to the Super-K
 amiokande detector where neutrino oscillation is studied via muon neutrino
  disappearance and electron neutrino appearance channels. Such studies hav
 e demonstrated muon neutrino to electron neutrino oscillation and provide 
 precision measurements of the muon neutrino and antineutrino disappearance
  parameters\, acting as a probe of unknown physics\, including the potenti
 al to observe CP violation in neutrino mixing. In this talk\, we will pres
 ent our latest neutrino and antineutrino oscillation results and also pres
 ent the future prospects of the experiment.\n\nhttps://indico.particle.mep
 hi.ru/event/22/contributions/1220/
LOCATION:Hotel Intourist Kolomenskoye 4* Petrovskiy hall
URL:https://indico.particle.mephi.ru/event/22/contributions/1220/
END:VEVENT
BEGIN:VEVENT
SUMMARY:The latest results from the Daya Bay
DTSTART;VALUE=DATE-TIME:20181023T144000Z
DTEND;VALUE=DATE-TIME:20181023T145500Z
DTSTAMP;VALUE=DATE-TIME:20260714T014307Z
UID:indico-contribution-139-1219@cern.ch
DESCRIPTION:Speakers: Konstantin Treskov (Joint Institute for Nuclear Rese
 arch)\nDaya Bay was the first experiment to unambiguously measure a non-ze
 ro value of the $\\theta_{13}$  mixing angle and the first reactor experim
 ent to measure the $\\Delta m^2_{32}$ mass splitting. The experiment inclu
 des eight identically designed detectors and six nuclear reactors at basel
 ines ranging from 0.5 km to 1.6 km. A data set of nearly 4 million events 
 has been collected over 1958 days of data taking\, providing the most prec
 ise measurement of $\\theta_{13}$ and a measurement of $\\Delta m^2_{32}$ 
 with a precision rivaling that from accelerator experiments. These measure
 ments will be covered in this talk alongside with other significant result
 s such as high-statistics measurement of the absolute reactor antineutrino
  flux and spectrum\, as well as a search for light sterile neutrino mixing
 .\n\nhttps://indico.particle.mephi.ru/event/22/contributions/1219/
LOCATION:Hotel Intourist Kolomenskoye 4* Petrovskiy hall
URL:https://indico.particle.mephi.ru/event/22/contributions/1219/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Statistical data analysis in the DANSS experiment
DTSTART;VALUE=DATE-TIME:20181023T142500Z
DTEND;VALUE=DATE-TIME:20181023T144000Z
DTSTAMP;VALUE=DATE-TIME:20260714T014307Z
UID:indico-contribution-139-1330@cern.ch
DESCRIPTION:Speakers: Natalia Skrobova (ITEP\, LPI\, MIPT)\nDANSS is a one
  cubic meter highly segmented solid scintillator detector. It consists of 
 2500 scintillator strips\, covered with gadolinium loaded reflective coati
 ng and read out with SiPMs via wavelength shifting fibers. DANSS is placed
  under a 3 GW industrial reactor at the Kalinin NPP (Russia) on a movable 
 platform. The distance from the reactor core center is varied from 10.7 m 
 to 12.7 m on-line. The inverse beta decay (IBD) process is used to detect 
 antineutrinos. DANSS detects about 5000 IBD events per day with the backgr
 ound from cosmic muons at the level of few percent.\nSterile neutrinos are
  searched for assuming a 4 neutrino model (3 active and 1 sterile neutrino
 ). The exclusion area in the sterile neutrino parameter plane is obtained 
 using a ratio of positron energy spectra collected at different distances.
  Therefore results do not depend on the shape and normalization of the rea
 ctor νe spectrum\, as well as on the detector efficiency. The excluded ar
 ea covers a wide range of the sterile neutrino parameters up to $sin2\\the
 ta^{2}$ \n\nhttps://indico.particle.mephi.ru/event/22/contributions/1330/
LOCATION:Hotel Intourist Kolomenskoye 4* Petrovskiy hall
URL:https://indico.particle.mephi.ru/event/22/contributions/1330/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Reactor antineutrino measurements with DANSS experiment
DTSTART;VALUE=DATE-TIME:20181023T141000Z
DTEND;VALUE=DATE-TIME:20181023T142500Z
DTSTAMP;VALUE=DATE-TIME:20260714T014307Z
UID:indico-contribution-139-1218@cern.ch
DESCRIPTION:Speakers: Igor Alekseev (ITEP)\nExperiments with reactor antin
 eutrino provide a wide range of physics opportunities. Solid state scintil
 lator detector DANSS is placed just below the core of 3.1 GWatt industrial
  reactor of Kalinin Nuclear Power Plant. The detector features the world h
 ighest counting rate of 5000 neutrino events per day with the cosmic rays 
 induced background as low as 130 events per day. \n    The talk will cover
  detector performance of a year and a half operation\, effects of fuel bur
 ning over reactor campaign\, results of the search for oscillations into l
 ight sterile neutrinos.\n\nhttps://indico.particle.mephi.ru/event/22/contr
 ibutions/1218/
LOCATION:Hotel Intourist Kolomenskoye 4* Petrovskiy hall
URL:https://indico.particle.mephi.ru/event/22/contributions/1218/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Earth thermal flux in the light of geoneutrinos
DTSTART;VALUE=DATE-TIME:20181023T074500Z
DTEND;VALUE=DATE-TIME:20181023T080000Z
DTSTAMP;VALUE=DATE-TIME:20260714T014307Z
UID:indico-contribution-139-1210@cern.ch
DESCRIPTION:Speakers: Valery Sinev (INR RAS)\nThe Earth thermal flux value
  lays in wide region from 50 up to 250 TW according to number of estimatio
 ns. Upper limit could be achieved only if potassium abundance in the Earth
  exceeds 2%. In Borexino data the valley between beryllium neutrinos and 1
 1C spectrum is filled with betas from 210Bi. But it also contains CNO neut
 rinos. CNO cycle in the Sun could be depressed according to last researche
 s. This means that part of CNO spectrum could be from terrestrial 40K anti
 neutrinos because their spectra are very similar.\n\nhttps://indico.partic
 le.mephi.ru/event/22/contributions/1210/
LOCATION:Hotel Intourist Kolomenskoye 4* Moskvorechye 1 hall
URL:https://indico.particle.mephi.ru/event/22/contributions/1210/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Detecting neutrinos from the next galactic supernova in the NOvA d
 etectors
DTSTART;VALUE=DATE-TIME:20181023T073000Z
DTEND;VALUE=DATE-TIME:20181023T074500Z
DTSTAMP;VALUE=DATE-TIME:20260714T014307Z
UID:indico-contribution-139-1209@cern.ch
DESCRIPTION:Speakers: Andrey Sheshukov (Joint Institute for Nuclear Resear
 ch\, JINR)\nCore-collapse supernovae emit about 99% of their gravitational
  energy in a burst of neutrinos. This signal carries precious information 
 about the processes inside the collapsing core as well as neutrino propert
 ies.\nThe large liquid scintillator detectors used by the NOvA experiment 
 provide a possibility to detect such a signal. A dedicated trigger system 
 was developed to perform a search for inverse beta decay neutrino interact
 ion candidates in real time and detect potential supernova bursts\, saving
  the data from the detector for further offline analysis. \nThis system ha
 s been running in stable mode since November 2017. Recent improvements in 
 the detection algorithms allowed to extend the sensitivity range for the 9
 .6 $M_\\odot$ star collapse up to 7 kiloparsec.\n\nhttps://indico.particle
 .mephi.ru/event/22/contributions/1209/
LOCATION:Hotel Intourist Kolomenskoye 4* Moskvorechye 1 hall
URL:https://indico.particle.mephi.ru/event/22/contributions/1209/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Reconstruction of the spectrum of cascades generated by VHE muons 
 in IceCube
DTSTART;VALUE=DATE-TIME:20181023T071500Z
DTEND;VALUE=DATE-TIME:20181023T073000Z
DTSTAMP;VALUE=DATE-TIME:20260714T014307Z
UID:indico-contribution-139-1208@cern.ch
DESCRIPTION:Speakers: Semyon Khokhlov (National Research Nuclear Universit
 y MEPhI)\nOne of the best ways for investigations of VHE muons spectrum is
  measuring the spectrum of stochastic energy losses (cascades). IceCube is
  the world’s unique detector capable of measuring the cascade spectrum i
 n the energy region of tens TeV – one PeV where manifestation of prompt 
 muons is predicted. In events with muon bundles\, the longitudinal energy 
 deposit profile reconstructed by means of the maximum likelihood method is
  analyzed. Cascade energies and positions are estimated in the events in w
 hich the highest local energy deposit is much greater than median energy d
 eposit. The technique of cascade spectrum reconstruction has been tested w
 ith MC-simulated events. Criteria of events selection\, cascade parameters
  estimation accuracy and efficiency of spectrum reconstruction will be dis
 cussed.\n\nhttps://indico.particle.mephi.ru/event/22/contributions/1208/
LOCATION:Hotel Intourist Kolomenskoye 4* Moskvorechye 1 hall
URL:https://indico.particle.mephi.ru/event/22/contributions/1208/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Latest astrophysical and particle physics results and future prosp
 ects from IceCube
DTSTART;VALUE=DATE-TIME:20181023T070000Z
DTEND;VALUE=DATE-TIME:20181023T071500Z
DTSTAMP;VALUE=DATE-TIME:20260714T014307Z
UID:indico-contribution-139-1215@cern.ch
DESCRIPTION:Speakers: Thomas Stuttard (Niels Bohr Institute)\nThe IceCube 
 neutrino observatory uses a cubic km of deep South Pole ice instrumented w
 ith over 5000 optical sensors to detect Cherenkov light produced by astrop
 hysical and atmospheric neutrinos interacting in the ice. The detector pro
 bes neutrino energies from GeV to PeV\, propagation distances ranging from
  a few km to astrophysical scales\, and collects high statistics neutrino 
 samples due to its extremely large volume.\n\nIceCube has a broad physics 
 reach in both astrophysical and particle physics observations. Astrophysic
 al neutrinos are a crucial component of the nascent field of multimessenge
 r astronomy\, allowing observations of distant and extreme astrophysical p
 henomena. Additionally\, neutrinos of both astrophysical and atmospheric o
 rigin can be used to test our understanding of fundamental physics\, such 
 as neutrino oscillations and interactions with matter\, and to probe Beyon
 d Standard Model (BSM) theories.\n\nThis talk will present the latest resu
 lts from the IceCube collaboration and look ahead to future plans for next
  generation South Pole neutrino detection.\n\nhttps://indico.particle.meph
 i.ru/event/22/contributions/1215/
LOCATION:Hotel Intourist Kolomenskoye 4* Moskvorechye 1 hall
URL:https://indico.particle.mephi.ru/event/22/contributions/1215/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Calibration and rare physics searches with the SNO+ experiment
DTSTART;VALUE=DATE-TIME:20181023T064500Z
DTEND;VALUE=DATE-TIME:20181023T070000Z
DTSTAMP;VALUE=DATE-TIME:20260714T014307Z
UID:indico-contribution-139-1207@cern.ch
DESCRIPTION:Speakers: Martti Nirkko (University of Sussex)\nThe SNO+ colla
 boration has upgraded the SNO detector to pursue a wide range of physics g
 oals\, which will be achieved in three distinct phases. In the ongoing wat
 er phase\, a search for invisible nucleon decays with expected lifetime se
 nsitivities as high as $10^{28}-10^{30}$ years is being conducted. In the 
 upcoming scintillator phase\, the increased light yield will lower the ene
 rgy threshold\, allowing studies of solar neutrinos\, geoneutrinos\, react
 or antineutrinos\, and supernova neutrinos to begin. Finally\, in the doub
 le-beta phase\, the active volume will be doped with Tellurium\, allowing 
 the search for neutrinoless double-beta decay. In order to measure such ra
 re events\, both the backgrounds and the detector response must be well un
 derstood - precise calibration methods are therefore required. This presen
 tation will give an overview of the calibration methods and discuss the st
 atus of the nucleon decay search.\n\nhttps://indico.particle.mephi.ru/even
 t/22/contributions/1207/
LOCATION:Hotel Intourist Kolomenskoye 4* Moskvorechye 1 hall
URL:https://indico.particle.mephi.ru/event/22/contributions/1207/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Measurement of variations in the flux of atmospheric muons  using 
 underground LVD detector
DTSTART;VALUE=DATE-TIME:20181023T063000Z
DTEND;VALUE=DATE-TIME:20181023T064500Z
DTSTAMP;VALUE=DATE-TIME:20260714T014307Z
UID:indico-contribution-139-1216@cern.ch
DESCRIPTION:Speakers: Natalia Agafonova (INR RAS)\nData on the measurement
  of the flux of atmospheric muons by a scintillation detector LVD at 3300 
 m w.e. depth with an average energy of 280 GeV are presented. The results 
 of measuring the seasonal variation of the muon flux over 25 years of obse
 rvations are discussed.\n\nhttps://indico.particle.mephi.ru/event/22/contr
 ibutions/1216/
LOCATION:Hotel Intourist Kolomenskoye 4* Moskvorechye 1 hall
URL:https://indico.particle.mephi.ru/event/22/contributions/1216/
END:VEVENT
BEGIN:VEVENT
SUMMARY:New constraints on magnetic moments of solar neutrinos in Borexino
DTSTART;VALUE=DATE-TIME:20181023T061500Z
DTEND;VALUE=DATE-TIME:20181023T063000Z
DTSTAMP;VALUE=DATE-TIME:20260714T014307Z
UID:indico-contribution-139-1206@cern.ch
DESCRIPTION:Speakers: Alina Vishneva (DLNP JINR)\nEffective magnetic momen
 t of solar neutrinos is constrained using a 1291.5 days dataset of Borexin
 o Phase-II. The sought-for effect from electromagnetic neutrino interactio
 n is the contribution to the low-energy part of the $\\nu-e$ scattering cr
 oss section affecting the shapes of the electron recoil spectra. Spectral 
 fit of the solar neutrino data leads to the limit of $\\mu^{eff}_\\nu\n\nh
 ttps://indico.particle.mephi.ru/event/22/contributions/1206/
LOCATION:Hotel Intourist Kolomenskoye 4* Moskvorechye 1 hall
URL:https://indico.particle.mephi.ru/event/22/contributions/1206/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Neutrino astrophysics with Borexino: comprehensive study of proton
 -proton chain solar neutrinos
DTSTART;VALUE=DATE-TIME:20181023T060000Z
DTEND;VALUE=DATE-TIME:20181023T061500Z
DTSTAMP;VALUE=DATE-TIME:20260714T014307Z
UID:indico-contribution-139-1205@cern.ch
DESCRIPTION:Speakers: Evgeny Litvinovich (NRC Kurchatov Institute)\nFor th
 ousands years of human evolution we were curious about what the Sun is? An
 swers began to come during recent 50 years\, thanks to development of astr
 ophysics and helioseismology\, particle and neutrino physics. The latter r
 esearch field allows studying the Sun's deep interior and achieved enormou
 s progress during last ten years. This period of Sun's studies is marked b
 y the operation of the currently most sensitive solar neutrino detector Bo
 rexino\, which takes data in Gran Sasso national laboratories in Italy. Th
 anks to extreme radiopurity achieved in Borexino\, this is for the first t
 ime that a single detector is able to separately measure neutrinos produce
 d in various nuclear reactions of the solar proton-proton fusion chain. Bo
 rexino results indicate the preference of high over low metallicity solar 
 models - the step forward of extreme importance for solar physics. Neutrin
 o physics gains as well: for the first time Borexino examines the MSW-LMA 
 neutrino oscillation paradigm both in the vacuum and the matter dominated 
 regimes. In this talk I overview the wide set of Borexino accomplishments 
 done in the fields of solar and neutrino physics.\n\nhttps://indico.partic
 le.mephi.ru/event/22/contributions/1205/
LOCATION:Hotel Intourist Kolomenskoye 4* Moskvorechye 1 hall
URL:https://indico.particle.mephi.ru/event/22/contributions/1205/
END:VEVENT
END:VCALENDAR