from 27 February 2017 to 3 March 2017
Budker Institute of Nuclear Physics
Asia/Novosibirsk timezone
Home > Timetable > Session details
PDF | iCal

Instrumentation for Astroparticle and Neutrino physics

Place

Location: Budker Institute of Nuclear Physics
Address: 11, akademika Lavrentieva prospect, Novosibirsk, Russia
Date: 1 Mar 15:05 - 19:00

Conveners

    • Prof. Grigoriev, Dmitry (BINP)
    • Prof. Kudenko, Yury (Institute for Nuclear Research of RAS)

Timetable | Contribution List

Displaying 11 contributions out of 11
Type: Contributed Oral Session: Instrumentation for Astroparticle and Neutrino physics
Track: Instrumentation for Astroparticle and Neutrino physics
Antimatter experiments conducted at the Antiproton Decelerator (AD) at CERN address the fundamental questions why primordial antimatter is not observed in the present Universe. The weak equivalent principle (WEP) can be tested measuring the gravitational acceleration of antihydrogen atoms in the Earth's gravitational field that are horizontally emitted from a Penning trap. The antihydrogen atoms ... More
Presented by Dr. Sebastian GERBER on 1/3/2017 at 11:40
Type: Contributed Oral Session: Instrumentation for Astroparticle and Neutrino physics
Track: Instrumentation for Astroparticle and Neutrino physics
A new NEVOD-EAS array for detection of extensive air showers (EAS) in the energy range $10^{15}-10^{17} eV$ is being created in MEPhI (Moscow, Russia) on the basis of the Experimental Complex NEVOD. It will operate in conjunction with the Cherenkov Water Detector NEVOD and coordinate detector DECOR, as well as with detectors URAN and TREK which are now being constructed. The array will allow deter ... More
Presented by Mr. Ivan SHULZHENKO on 1/3/2017 at 11:20
Type: Contributed Oral Session: Instrumentation for Astroparticle and Neutrino physics
Track: Instrumentation for Astroparticle and Neutrino physics
The Large High Altitude Air Shower Observatory (LHAASO) project is scheduled to be built at Sichuan province in China. As a large scale complex of various detectors, its primary scientific goals are exploring the origin of the galactic cosmic ray, searching for very high energy gamma ray sources, and the precise measurement of the components at the knee region. To accomplish these tasks, the propo ... More
Presented by Mr. Xiaokun ZHAO
Type: Contributed Oral Session: Instrumentation for Astroparticle and Neutrino physics
Track: Instrumentation for Astroparticle and Neutrino physics
Direct search for dark matter particles (WIMP - Weakly Interacting Massive Particle) is produced in the detectors of recoil nuclei through observation of WIMP elastic scattering on atomic nuclei of detector matter. The current situation with the observation signals from dark matter particles is quite confusing. Some authors believe that one of the reasons for these differences among different ... More
Presented by Mr. Vladislav OLEINIKOV on 1/3/2017 at 17:20
Type: Contributed Oral Session: Instrumentation for Astroparticle and Neutrino physics
Track: Instrumentation for Astroparticle and Neutrino physics
Recent progress in the development of the detectors for neutrino oscillation experiments will be presented. The near and far detectors in current accelerator (T2K, NOVA) and reactor experiments will be described. An emphasis will be put on the neutrino detectors for the next generation oscillation experiments: a huge water Cherenkov detector HyperKamiokande, large volume liquid argon detectors fo ... More
Presented by Prof. Yury KUDENKO on 1/3/2017 at 8:05
Type: Contributed Oral Session: Instrumentation for Astroparticle and Neutrino physics
Track: Instrumentation for Astroparticle and Neutrino physics
The TAIGA observatory addresses ground-based gamma-ray astronomy at energies from a few TeV to several PeV, as well as cosmic ray physics from 100 TeV to several EeV. TAIGA will be located in the Tunka valley, ~50 km West from Lake Baikal. The different detectors of the TAIGA will be grouped in 6 arrays to measure Cherenkov and radio emission as well as electron and muon components of atmospheric ... More
Presented by Prof. Nikolay BUDNEV on 1/3/2017 at 17:40
Type: Contributed Oral Session: Instrumentation for Astroparticle and Neutrino physics
Track: Instrumentation for Astroparticle and Neutrino physics
Hyper-Kamiokande is a Large water Cherenkov detectors, such as the successful Super-Kamiokande, and the forthcoming Hyper-Kamiokande requires large aperture, high sensitivity photosensors able to detect the weak Cherenkov light generated by neutrino interactions or proton decay. As a consequence, the capability of a water Cherenkov detector largely relies on the performance of its photosensors. Cu ... More
Presented by Prof. Vincenzo BERARDI on 1/3/2017 at 9:40
Type: Contributed Oral Session: Instrumentation for Astroparticle and Neutrino physics
Track: Instrumentation for Astroparticle and Neutrino physics
Jiangmen Underground Neutrino Observatory (JUNO) is under construction in southern China which aims to measure the neutrino mass hierarchy and neutrino oscillation parameters using the reactor neutrinos from two nearby nuclear power plants 53km away. JUNO also has good capabilities of researches such as supernova neutrinos, geo-neutrinos, solar neutrinos and so on. Here the instrumentation of JUNO ... More
Presented by Prof. Yuekun HENG on 1/3/2017 at 8:50
Type: Contributed Oral Session: Instrumentation for Astroparticle and Neutrino physics
Track: Instrumentation for Astroparticle and Neutrino physics
The experiment on first observation of the elastic coherent scattering of neutrino off atomic nuclei is proposed with the use of the RED-100 emission two-phase xenon detector. This process was theoretically predicted more than 40 years ago by the Standard model of particle physics but has not been observed yet because of lack of the detection technique of the events with the low energy deposition ... More
Presented by Dr. Dmitry AKIMOV on 1/3/2017 at 17:00
Type: Contributed Oral Session: Instrumentation for Astroparticle and Neutrino physics
Track: Instrumentation for Astroparticle and Neutrino physics
Deep Underground Neutrino Experiment (DUNE) has chosen liquid argon (LAr) technology for the detection of neutrinos produced with proton beams at Fermilab and transmitted 1300 km through the Earth towards the Sanford Underground Research Facility (SURF) in South Dakota. Two basic configurations for LAr TPC are considered: a single phase and a dual phase. The former has already worked as a 300 ton ... More
Presented by Wladyslaw Henryk TRZASKA on 1/3/2017 at 15:30
Type: Contributed Oral Session: Instrumentation for Astroparticle and Neutrino physics
Track: Instrumentation for Astroparticle and Neutrino physics
To effectively detect elusive particles the use of a detector with high efficiency and enhanced sensitivity is required. Cryogenic scintillating bolometers are among the most promising detectors used for the investigation of rare nuclear processes due to their excellent background rejection capabilities thanks to the simultaneous and independent, double readout of heat and scintillation light indu ... More
Presented by Dr. Serge NAGORNY on 1/3/2017 at 18:00
Building timetable...