Search Results - "Ryasny, V."
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1
Measurement of the velocity of neutrinos from the CNGS beam with the large volume detector
Published in Physical review letters (17-08-2012)“…We report the measurement of the time of flight of ∼17 GeV ν(μ) on the CNGS baseline (732 km) with the Large Volume Detector (LVD) at the Gran Sasso…”
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2
Measurement of neutron number generated by cosmic-ray muons in iron using the LVD
Published in Bulletin of the Russian Academy of Sciences. Physics (01-03-2015)“…The experiment to measure the neutrons numbers generated by muons in iron (Fe) and lead (Pb) carried out using LVD. A full Monte Carlo simulation of the actual…”
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3
Search for neutrino radiation from collapsing stars with the Artyomovsk scintillation detector
Published in Bulletin of the Russian Academy of Sciences. Physics (01-11-2013)“…The current status of an experiment designed to search for neutrino radiation from collapsing stars using the Artyomovsk Liquid Scintillation Detector is…”
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4
Generation of neutrons produced by muons from CERN neutrino beam
Published in Bulletin of the Russian Academy of Sciences. Physics (01-03-2015)“…Preliminary results of neutron generation by muons, produced in CERN neutrino beam with average energy 17 GeV in LVD experiment are presented for the period…”
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5
Single and multiple muons and the generation of neutrons in the LVD experiment
Published in Bulletin of the Russian Academy of Sciences. Physics (01-03-2011)“…The large geometric factor and good spatial resolution of the Large Volume Detector (LVD) ensures statistically significant and highly accurate measurements of…”
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6
Analysis of seasonal variations of the cosmic ray muon flux and neutrons produced by muons in the LVD detector
Published in Bulletin of the Russian Academy of Sciences. Physics (01-03-2011)“…The Russian-Italian Large Volume Detector (LVD) is located at the Gran Sasso underground laboratory at a depth of 3300 m w.e. To study the seasonal variations…”
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7
First CNGS events detected by LVD
Published in The European physical journal. C, Particles and fields (01-12-2007)“…The CERN Neutrino to Gran Sasso (CNGS) project aims to produce a high energy, wide band νμ beam at CERN and send it toward the INFN Gran Sasso National…”
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8
The search for different neutrino flavors from collapsing stars using the LVD detector
Published in Bulletin of the Russian Academy of Sciences. Physics (01-03-2011)“…The main goal of the Large Volume Detector (LVD) is to search for neutrino burst from gravitational stellar collapses in our Galaxy. The apparatus is shown to…”
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9
The energy spectrum of neutrons produced by cosmic ray muons in LVD
Published in Bulletin of the Russian Academy of Sciences. Physics (01-05-2009)“…The energy spectrum of neutrons produced by cosmic ray muons in the underground detector LVD (3650 m.w.e.) is obtained for the energy range of 30–450 MeV. The…”
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10
CNGS beam monitor with the LVD detector
Published in Nuclear instruments & methods in physics research. Section A, Accelerators, spectrometers, detectors and associated equipment (01-01-2004)“…The importance of an adequate CNGS beam monitor at the Gran Sasso Laboratory has been stressed in many papers. Since the number of internal ν μ CC and NC…”
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11
Search for neutrino emission from supernovae using the Large Volume Detector
Published in Bulletin of the Russian Academy of Sciences. Physics (01-05-2009)“…The basic task of the Large Volume Detector LVD situated at the underground Gran Sasso National Laboratory (Italy) is the search for neutrino bursts from…”
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12
IMPLICATION FOR THE CORE-COLLAPSE SUPERNOVA RATE FROM 21 YEARS OF DATA OF THE LARGE VOLUME DETECTOR
Published in The Astrophysical journal (20-03-2015)“…ABSTRACT The Large Volume Detector (LVD) has been continuously taking data since 1992 at the INFN Gran Sasso National Laboratory. The LVD is sensitive to…”
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13
Selection of neutrino burst candidates by pulse spatial distribution analysis
Published in Nuclear instruments & methods in physics research. Section A, Accelerators, spectrometers, detectors and associated equipment (01-06-1996)“…The method of analysis and possibilities of identification of neutrino bursts from collapsing stars using a spatial distribution of pulses in the multimodular…”
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14
Implication for the core collapse supernova rate from 21 years of data of the Large Volume Detector
Published 09-05-2015“…The Astrophysical Journal, 802:47, 2015 The Large Volume Detector (LVD) has been continuously taking data since 1992 at the INFN Gran Sasso National…”
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15
On-line recognition of supernova neutrino bursts in the LVD
Published in Astroparticle physics (2008)“…In this paper we show the capabilities of the Large Volume Detector (INFN Gran Sasso National Laboratory) to identify a neutrino burst associated with a…”
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16
Measurement of the velocity of neutrinos from the CNGS beam with the Large Volume Detector
Published 23-08-2012“…PRL 109, 070801 (2012) We report the measurement of the time-of-flight of ~17 GeV muon neutrinos on the CNGS baseline (732 km) with the Large Volume Detector…”
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Journal Article -
17
Study of the effect of neutrino oscillations on the supernova neutrino signal in the LVD detector
Published in Astroparticle physics (01-04-2007)“…The LVD detector, located in the INFN Gran Sasso National Laboratory (Italy), studies supernova neutrinos through the interactions with protons and carbon…”
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18
First CNGS events detected by LVD
Published 08-10-2007“…Eur.Phys.J.C52:849-855,2007 The CERN Neutrino to Gran Sasso (CNGS) project aims to produce a high energy, wide band $\nu_{\mu}$ beam at CERN and send it toward…”
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19
On-line recognition of supernova neutrino bursts in the LVD detector
Published 01-10-2007“…Astropart.Phys.28:516-522,2008 In this paper we show the capabilities of the Large Volume Detector (INFN Gran Sasso National Laboratory) to identify a neutrino…”
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20
Study of the effect of neutrino oscillation on the supernova neutrino signal with the LVD detector
Published in Nuclear physics. Section B, Proceedings supplement (01-01-2005)“…We present an update of our previous study [Nucl. Phys. B Proc. Suppl. 110 (2002) 410-413] on how ν oscillations affect the signal from a supernova core…”
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