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View article: <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msup><mml:mi>π</mml:mi><mml:mo>+</mml:mo></mml:msup><mml:msup><mml:mi>π</mml:mi><mml:mo>−</mml:mo></mml:msup></mml:math> Coulomb interaction study and its use in data processing
Coulomb interaction study and its use in data processing Open
In this work, the Coulomb effects (Coulomb correlations) in π+π− pairs produced in p+Ni collisions at 24 GeV/c, are studied using experimental π+π− pair distributions in Q, the relative momentum in the pair center-of-mass system (c.m.s.),…
View article: The π^+π^- Coulomb interaction study and its use in the data processing
The π^+π^- Coulomb interaction study and its use in the data processing Open
In this work the Coulomb effects (Coulomb correlations) in $π^+π^-$ pairs produced in p + Ni collisions at 24 GeV/$c$, are studied using experimental $π^+π^-$ pair distributions in $Q$, the relative momentum in the pair center of mass syst…
View article: Determination of the astrophysical factor of the <sup>3</sup>He(α,γ)<sup>7</sup>Be down to zero energy using the asymptotic normalization coefficient method
Determination of the astrophysical factor of the <sup>3</sup>He(α,γ)<sup>7</sup>Be down to zero energy using the asymptotic normalization coefficient method Open
The observation of neutrinos emitted in the p − p chain and in the CNO cycle can be employed to test the Standard Solar Model. The 3 He( α,γ ) 7 Be reaction is the first reaction of the 2nd and 3rd branch of the p − p chain, so the indeter…
View article: Determination of the <sup>3</sup>He(<i>α</i>, <i>γ</i>)<sup>7</sup>Be and <sup>6</sup>Li(<i>p</i>, <i>γ</i>)<sup>7</sup>Be astrophysical factors down to zero energy using the asymptotic normalization coefficients
Determination of the <sup>3</sup>He(<i>α</i>, <i>γ</i>)<sup>7</sup>Be and <sup>6</sup>Li(<i>p</i>, <i>γ</i>)<sup>7</sup>Be astrophysical factors down to zero energy using the asymptotic normalization coefficients Open
The p - p -chain reaction 3 He( α , γ ) 7 Be can sensitively influence the prediction of the 7 Be and 8 B neutrino fluxes. Despite its importance, the knowledge of its reaction cross section at energies of the core of the Sun (15 keV 30 ke…
View article: Astrophysical S-factor for the 3He(α,γ)7Be reaction via the asymptotic normalization coefficient (ANC) method
Astrophysical S-factor for the 3He(α,γ)7Be reaction via the asymptotic normalization coefficient (ANC) method Open
The detection of the neutrinos produced in the p-p chain and in the CNO cycle can be used to test the Standard Solar Model. The 3He(α,g)7Be reaction is the first reaction of the 2nd and 3rd branch of the p-p chain, therefore, the uncertain…
View article: Searches for sterile neutrinos at the DANSS experiment
Searches for sterile neutrinos at the DANSS experiment Open
DANSS is a one cubic meter highly segmented solid scintillator detector. It consists of 2500 scintillator strips (100$\times$4$\times$1 cm$^3$), covered with gadolinium loaded reflective coating and read out with SiPMs via wave length shif…
View article: Gigaton Volume Detector in Lake Baikal: status of the project
Gigaton Volume Detector in Lake Baikal: status of the project Open
Baikal-GVD is a kilometer-scale neutrino telescope under construction in Lake Baikal, which will be formed by multi-megaton subarrays – clusters of strings. A first demonstration cluster “Dubna” has been deployed in 2015 and comprises 192 …
View article: Measurements of the Reactor Antineutrino with Solid State Scintillation Detector
Measurements of the Reactor Antineutrino with Solid State Scintillation Detector Open
Measurements of reactor antineutrino play an important role in the efforts at the frontier of the modern physics. The DANSS collaboration presents preliminary results of a one year run with a cubic meter solid state detector placed below 3…
View article: Neutrino Physics at Kalinin Nuclear Power Plant: 2002 – 2017
Neutrino Physics at Kalinin Nuclear Power Plant: 2002 – 2017 Open
The results of the research in the field of neutrino physics obtained at Kalinin nuclear power plant during 15 years are presented. The investigations were performed in two directions. The first one includes GEMMA I and GEMMA II experiment…
View article: Data management and processing system for the Baikal-GVD telescope
Data management and processing system for the Baikal-GVD telescope Open
The Baikal-GVD neutrino telescope is being constructed in lake Baikal. The robust Baikal Analysis and Reconstruction Software (BARS) has been developed to convert raw data into physics results. To provide a stable and continuous analysis o…
View article: Search for cascade events with Baikal-GVD demonstration cluster "Dubna"
Search for cascade events with Baikal-GVD demonstration cluster "Dubna" Open
Deep underwater neutrino telescope „Dubna“ – the first, demonstration cluster of Baikal-GVD, has been deployed in April 2015 and was operating up to February 2016 in Lake Baikal. In 2016 this array was upgraded to baseline configuration of…
View article: Status of the Baikal-GVD experiment - 2017
Status of the Baikal-GVD experiment - 2017 Open
Baikal-GVD is a kilometer scale neutrino telescope under construction in Lake Baikal, which will be formed by multimegaton subarrays – clusters of strings. First demonstration cluster “Dubna” has been deployed in 2015 and comprises 192 opt…
View article: Baikal-GVD: Time Calibrations in 2016
Baikal-GVD: Time Calibrations in 2016 Open
In April 2015, the first part (cluster) of the newly constructed next-generation neutrino telescope, Gigaton Volume Detector (GVD), was put into operation in the lake Baikal and started with data taking followed by another cluster installe…
View article: New Improved Indirect Measurement of the <sup>19</sup>F(p, α)<sup>16</sup>O Reaction at Energies of Astrophysical Relevance
New Improved Indirect Measurement of the <sup>19</sup>F(p, α)<sup>16</sup>O Reaction at Energies of Astrophysical Relevance Open
Fluorine abundance determination is of great importance in stellar physics to understand s-elements production and mixing processes in asymptotic giant branch (AGB) stars. Up to now, theoretical models overproduce F abundances in AGB stars…
View article: The astrophysical S-factor of the direct <sup>18</sup>O(p, <i>γ</i>)<sup>19</sup>F capture by the ANC method
The astrophysical S-factor of the direct <sup>18</sup>O(p, <i>γ</i>)<sup>19</sup>F capture by the ANC method Open
Publication in the conference proceedings of EUSIPCO, Bucharest, Romania, 2012
View article: Detector of the reactor AntiNeutrino based on Solid-state plastic Scintillator (DANSS). Status and first results.
Detector of the reactor AntiNeutrino based on Solid-state plastic Scintillator (DANSS). Status and first results. Open
A detector of the reactor antineutrino based on a cubic meter of plastic scintillator is installed below 3.1 GW industrial reactor. The detector is placed on a movable platform which allows to change the distance to the reactor core center…
View article: DANSS: Detector of the reactor AntiNeutrino based on Solid Scintillator
DANSS: Detector of the reactor AntiNeutrino based on Solid Scintillator Open
The DANSS project is aimed at creating a relatively compact neutrino spectrometer which does not contain any flammable or other dangerous liquids and may therefore be located very close to the core of an industrial power reactor. As a resu…
View article: DANSS Experiment Data Acquisition System
DANSS Experiment Data Acquisition System Open
DANSS (Detector of the reactor AntiNeutrino based on Solid Scintillator) is a project aiming to measure a spectrum of reactor antineutrinos using inverse beta decay (IBD) in a plastic scintillator. The detector is located close to an indus…
View article: Study of<sup>16</sup>O(<sup>12</sup>C,α<sup>20</sup>Ne)α for the investigation of carbon-carbon fusion reaction via the Trojan Horse Method
Study of<sup>16</sup>O(<sup>12</sup>C,α<sup>20</sup>Ne)α for the investigation of carbon-carbon fusion reaction via the Trojan Horse Method Open
Carbon-carbon fusion reaction represents a nuclear process of great interest in astrophysics, since the carbon burning is connected with the third phase of massive stars (M > 8 M☉) evolution. In spite of several experimental works, carbon-…