Yu. G. Sobolev
Joint Institute for Nuclear Research
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Featured researches published by Yu. G. Sobolev.
Physics Letters B | 2010
G. Agakichiev; A. Balanda; D. Belver; A.V. Belyaev; A. Blanco; M. Böhmer; J. L. Boyard; P. Braun-Munzinger; P. Cabanelas; E. Castro; S. Chernenko; T. Christ; M. Destefanis; J. Diaz; F. Dohrmann; A. Dybczak; L. Fabbietti; O. Fateev; P. Finocchiaro; P. Fonte; J. Friese; I. Fröhlich; T. Galatyuk; J. A. Garzón; R. Gernhäuser; A. Gil; C. Gilardi; K. Göbel; M. Golubeva; D. González-Díaz
Abstract We report measurements of electron pair production in elementary p + p and d + p reactions at 1.25 GeV / u with the HADES spectrometer. For the first time, the electron pairs were reconstructed for n + p reactions by detecting the proton spectator from the deuteron breakup. We find that the yield of electron pairs with invariant mass M e + e − > 0.15 GeV / c 2 is about an order of magnitude larger in n + p reactions as compared to p + p . A comparison to model calculations demonstrates that the production mechanism is not sufficiently described yet. The electron pair spectra measured in C + C reactions are compatible with a superposition of elementary n + p and p + p collisions, leaving little room for additional electron pair sources in such light collision systems.
Physics Letters B | 2015
G. Agakishiev; O. W. Arnold; D. Belver; Alexander Belyaev; J.C. Berger-Chen; A. Blanco; M. Böhmer; J. L. Boyard; P. Cabanelas; S. Chernenko; A. Dybczak; E. Epple; L. Fabbietti; O. Fateev; P. Finocchiaro; P. Fonte; J. Friese; I. Fröhlich; T. Galatyuk; J. A. Garzón; R. Gernhäuser; K. Göbel; M. Golubeva; D. González-Díaz; F. Guber; M. Gumberidze; T. Heinz; T. Hennino; R. Holzmann; A. Ierusalimov
Employing the Bonn-Gatchina partial wave analysis framework (PWA), we have analyzed HADES data of the reaction p(3.5GeV ) + p !pK + �. This reaction might contain information about the kaonic cluster ”ppK − ” via its decay into p�. Due to interference effects in our coherent description of the data, a hypothetical KNN (or, specifically ”ppK − ”) cluster signal must not necessarily show up as a pronounced feature (e.g. a peak) in an invariant mass spectra like p�. Our PWA analysis includes a variety of resonant and non-resonant intermediate states and delivers a good description of our data (various angular distributions and two-hadron invariant mass spectra) without a contribution of a KNN cluster. At a confidence level of CLs=95% such a cluster can not contribute more than 2-12% to the total cross section with a pK + � final state, which translates into a production cross-section between 0.7 µb and 4.2 µb, respectively. The
Physics of Atomic Nuclei | 2007
Yu. A. Baurov; Yu. G. Sobolev; Yu. V. Ryabov; V. F. Kushniruk
Changes in the rate of the beta decay of radioactive elements whose periods are about 24 h and 27 d are detected on the basis of long-term investigations performed with the aid of scintillation and germanium-lithium gamma detectors. The use of the scintillation procedure yields results whose level of significance is much higher than 5%, while the procedure based on germanium—lithium detectors gives a more than 1% deviation from the average value of fluxes of gamma rays accompanying, for example, 60Co beta decay. With allowance for the rotation of the laboratory frame together with the Earth, deviations of the change in the rate of beta decay of radioactive elements single out three directions in the physical space.
Modern Physics Letters A | 2001
Yu. A. Baurov; A. A. Konradov; V. F. Kushniruk; E. A. Kuznetsov; Yu. G. Sobolev; Yu. V. Ryabov; A. P. Senkevich; S. V. Zadorozsny
Results of simultaneous measurements of beta-decay rate with the aid of Ge(Li)-detectors performed at two laboratories 140km apart (INR RAS, Troitsk, Co-60, and JINR, Dubna, Cs-137) during a period from 15.03.2000 till 10.04.2000, are presented. Regular deviations of the count rate of gamma-quanta following the beta-decay of
Nuclear Physics | 2013
L. Fabbietti; G. Agakishiev; C. Behnke; D. Belver; Alexander Belyaev; J.C. Berger-Chen; A. Blanco; C. Blume; M. Böhmer; P. Cabanelas; S. Chernenko; C. Dritsa; A. Dybczak; E. Epple; O. Fateev; P. Fonte; J. Friese; I. Fröhlich; T. Galatyuk; J. A. Garzón; K. Gill; M. Golubeva; D. González-Díaz; F. Guber; M. Gumberidze; S. Harabasz; T. Hennino; C. Höhne; R. Holzmann; P. Huck
\sim
Journal of Physics G | 2009
Yu. E. Penionzhkevich; S. M. Lukyanov; R. A. Astabatyan; N. A. Demekhina; M. P. Ivanov; R. Kalpakchieva; A. A. Kulko; E. R. Markaryan; V. A. Maslov; Yu. A. Muzychka; R. V. Revenko; N. K. Skobelev; V. Smirnov; Yu. G. Sobolev
0.7% (INR RAS, Co-60) and
European Physical Journal A | 2012
G. Agakishiev; H. Alvarez-Pol; A. Balanda; R. Bassini; M. Böhmer; H. Bokemeyer; J. L. Boyard; P. Cabanelas; S. Chernenko; T. Christ; M. Destefanis; F. Dohrmann; A. Dybczak; T. Eberl; L. Fabbietti; O. Fateev; P. Finocchiaro; J. Friese; I. Fröhlich; T. Galatyuk; J. A. Garzón; R. Gernhäuser; C. Gilardi; M. Golubeva; D. González-Dıaz; F. Guber; M. Gumberidze; T. Hennino; R. Holzmann; A. Ierusalimov
\sim
Physical Review C | 2001
A. S. Khrykin; V. F. Boreiko; Yu. G. Budyashov; S. B. Gerasimov; N. V. Khomutov; Yu. G. Sobolev; V. P. Zorin
0.2% (JINR, Cs-137) from the statistical average, are observed. The analysis of extremum deviations of gamma-quanta count rate shows that the set of directions of tangents to the Earths parallels of latitude at the extremum points of trajectories of motion in the space of each laboratory clearly forms three separate compact subsets of directions which agree, for two laboratories, to an accuracy of
Physical Review C | 2012
G. Agakishiev; L. Naumann; D. González-Díaz; O. Fateev; Y. Pachmayer; Yu. G. Sobolev; A. Reshetin; E. Moriniere; B. Spruck; S. Lang; M. Roy-Stephan; H. Tsertos; V. Pospíšil; A. Sadovsky; L. Fabbietti; V. Pechenov; Y. Zanevsky; J. Stroth; O. Pechenova; M. Traxler; A. Rustamov; B. Ramstein; C. Gilardi; P. Cabanelas; V. Metag; A. Toia; A. Tarantola; B. Michalska; J. Otwinowski; J.L. Boyard
\pm10^\circ
Journal of Physics G | 2002
Georgi Georgiev; G. Neyens; M. Hass; D. L. Balabanski; C. R. Bingham; C. Borcea; Nico Coulier; R. Coussement; J. M. Daugas; F. de Oliveira Santos; M. Gorska; H. Grawe; R. Grzywacz; M. Lewitowicz; H. Mach; I. Matea; R. D. Page; M. Pfützner; Yu. E. Penionzhkevich; Z. Podolyak; P. H. Regan; K. Rykaczewski; M. Sawicka; Na Smirnova; Yu. G. Sobolev; M. Stanoiu; Stéphanie Teughels; Katrien Vyvey
. This phenomenon is shown not to be explained on the basis of traditional notion. A possible explanation is suggested basing on the hypothesis that there exists a new anisotropic interaction caused by the cosmological vectorial potential \textbf{A}