S. V. Laptev
Russian Academy of Sciences
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Featured researches published by S. V. Laptev.
Physics of Atomic Nuclei | 2003
I. V. Ajinenko; S. A. Akimenko; G. I. Britvich; I. G. Britvich; K. V. Datsko; A. P. Filin; A. V. Inyakin; A. S. Konstantinov; V. F. Konstantinov; I. Ya. Korolkov; V. M. Leontiev; V. P. Novikov; V. F. Obraztsov; V.A. Polyakov; V. I. Romanovsky; V. I. Shelikhov; N. E. Smirnov; M. M. Soldatov; O. G. Tchikilev; E. Usenko; M. V. Vasiliev; E. V. Vlasov; V. I. Yakimchuk; O. P. Yushchenko; V. N. Bolotov; S. V. Laptev; V. A. Lebedev; A. R. Pastsjak; A. Yu. Polyarush; R. Kh. Sirodeev
The decay K− → μ−νπ0 has been studied using in-flight decays detected with the ISTRA+ setup operating in the 25-GeV negative secondary beam of the U-70 PS. About 112K events were used for the analysis. The λ+ and λ0 slope parameters of the decay form factors f+(t) and f0(t) have been measured: λ+=0.0321±0.004(stat.)±0.002(syst.), λ0=0.0209±0.004(stat.)±0.002(syst.); the correlation dλ0/dλ+=−0.46. The limits on the possible tensor and scalar couplings have been derived: fT/f+(0)=−0.021±0.028(stat.)±0.014(theor.), fS/f+(0)=0.004±0.005(stat.)±0.005(theor.).
Physics of Atomic Nuclei | 2002
I. V. Ajinenko; S. A. Akimenko; G. A. Akopdzhanov; K. S. Belous; G. I. Britvich; I. G. Britvich; A. P. Filin; V. N. Govorun; A. V. Inyakin; V. A. Khmelnikov; A. S. Konstantinov; V. F. Konstantinov; I. Ya. Korolkov; V. M. Leontiev; V. P. Novikov; V. F. Obraztsov; V.A. Polyakov; V. I. Romanovsky; V. M. Ronjin; V. A. Senko; N. A. Shalanda; M. M. Shapkin; V. I. Shelikhov; N. E. Smirnov; A. A. Sokolov; O. G. Tchikilev; E. V. Vlasov; O. P. Yushchenko; V. N. Bolotov; S. V. Laptev
The decay K− → e−νπ0 has been studied using in-flight decays detected with the ISTRA+ setup working at the 25-GeV negative secondary beam of the U-70 PS. About 130K events were used for the analysis. The λ+ parameter of the vector form factor has been measured: λ+=0.0293±0.0015(stat.)±0.002(syst.). The limits on the possible tensor and scalar couplings have been derived: fT/f+(0)=−0.045±0.060(stat.) and fS/f+(0)=−0.019−0.016+0.025(stat.).
Physics of Atomic Nuclei | 2007
O. G. Tchikilev; S. A. Akimenko; G. I. Britvich; K. V. Datsko; A. P. Filin; A. V. Inyakin; V. A. Khmelnikov; A. S. Konstantinov; I. Ya. Korolkov; V. M. Leontiev; V. P. Novikov; V. F. Obraztsov; V.A. Polyakov; V. I. Romanovsky; V. I. Shelikhov; V. A. Uvarov; O. P. Yushchenko; V. N. Bolotov; S. V. Laptev; V. A. Duk; A. Yu. Polyarush
Using data collected with the ISTRA+ spectrometer during the 2001 run of the U-70 proton synchrotron in Protvino, the first observation of the radiative kaon decay K− → µ−π0γν is reported. The ratio Br(Kµ3γ, 5 < E*γ < 30 MeV)/Br(Kµ3) is found to be [0.270 ± 0.029(stat.) ± 0.026(syst.)]% and the ratio Br(Kµ3γ, 30 < E*γ < 60 MeV)/Br(Kµ3) = [0.0448 ± 0.0068(stat.) ± 0.0099(syst.)]%. These ratios are consistent with the theoretical predictions 0.21 and 0.047%, respectively. The measured angular distribution asymmetry for the region 5 < E*γ < 30 MeV, A(cos ϑ*µγ) = 0.093 ± 0.141, is two standard deviations away from the theoretical prediction of 0.354. The measured asymmetry in the T-odd variable ξ = pγ · (pµ × pπ)/mK3 is −0.03 ± 0.13.Using data collected with the ISTRA+ spectrometer during the 2001 run of the U-70 proton synchrotron in Protvino, we report the first observation of the radiative kaon decay K- -->mu-pi0gammanu. We find Br(Kmu3g)/Br(Kmu3) for two regions 5<Eg<30 and 30<Eg<60 MeV consistent with theoretical predictions. The measured angular distribution asymmetry for the first region, 0.093+/-0.141, is two standard deviations away from the theoretical prediction of 0.354. The measured asymmetry in the T-odd variable is -0.03+/-0.13.
Physics of Atomic Nuclei | 2007
S. A. Akimenko; V. N. Bolotov; G. I. Britvich; K. V. Datsko; V. A. Duk; A. P. Filin; E. N. Gushchin; A. V. Inyakin; V. A. Khmelnikov; A. S. Konstantinov; V. F. Konstantinov; I. Yu. Korol'Kov; S. V. Laptev; V. A. Lebedev; V. M. Leontiev; A. E. Mazurov; V. P. Novikov; V. F. Obraztsov; V.A. Polyakov; A. Yu. Polyarush; V. E. Postoev; V. I. Romanovsky; V. I. Shelikhov; O. G. Tchikilev; V. A. Uvarov; O. P. Yushchenko
AbstractResults of study of the
Physics Letters B | 2004
O. G. Tchikilev; S. A. Akimenko; G. I. Britvich; K. V. Datsko; A. P. Filin; A. V. Inyakin; V. A. Khmelnikov; A. S. Konstantinov; V. F. Konstantinov; I. Y. Korolkov; V. M. Leontiev; V. P. Novikov; V. F. Obraztsov; V.A. Polyakov; V. I. Romanovsky; V. I. Shelikhov; N. E. Smirnov; V. A. Uvarov; O. P. Yushchenko; V. N. Bolotov; S. V. Laptev; A. R. Pastsjak; A. Yu. Polyarush
arXiv: High Energy Physics - Experiment | 2004
V. A. Uvarov; S. A. Akimenko; G. I. Britvich; K. V. Datsko; A. P. Filin; A. V. Inyakin; V. A. Khmelnikov; A. S. Konstantinov; V. F. Konstantinov; I. Y. Korolkov; V. M. Leontiev; V. P. Novikov; V. F. Obraztsov; V.A. Polyakov; V. I. Romanovsky; V. M. Ronjin; V. I. Shelikhov; N. E. Smirnov; O. G. Tchikilev; O. P. Yushchenko; V. N. Bolotov; V. A. Duk; S. V. Laptev; A. Yu. Polyarush
K^ - \to \pi ^0 e^ - \overline \nu \gamma
Physics of Atomic Nuclei | 2006
V. A. Uvarov; S. A. Akimenko; V. N. Bolotov; G. I. Britvich; K. V. Datsko; V. A. Duk; A. P. Filin; A. V. Inyakin; V. A. Khmelnikov; A. S. Konstantinov; V. F. Konstantinov; I. Ya. Korolkov; S. V. Laptev; V. M. Leontiev; V. P. Novikov; V. F. Obraztsov; V.A. Polyakov; A. Yu. Polyarush; V. I. Romanovsky; V. M. Ronjin; V. I. Shelikhov; N. E. Smirnov; O. G. Tchikilev; O. P. Yushchenko
Instruments and Experimental Techniques | 2012
Yu. K. Gavrilov; E. N. Gushchin; S. V. Laptev; V. E. Postoev; S. N. Filippov
decay at the ISTRA+ setup are presented. We observed 4476 events of this decay. The branching ratio is found to be
Physics of Atomic Nuclei | 2006
V. A. Uvarov; S. A. Akimenko; V. N. Bolotov; G. I. Britvich; K. V. Datsko; V. A. Duk; A. P. Filin; A. V. Inyakin; V. A. Khmelnikov; A. S. Konstantinov; V. F. Konstantinov; I. Ya. Korolkov; S. V. Laptev; V. M. Leontiev; V. P. Novikov; V. F. Obraztsov; V.A. Polyakov; A. Yu. Polyarush; V. I. Romanovsky; V. M. Ronjin
Instruments and Experimental Techniques | 2001
V. N. Bolotov; G. I. Britvich; B. Zh. Zalikhanov; Yu. Ivanshin; P. A. Kurbatov; V. F. Konstantinov; S. V. Laptev; V. A. Lebedev; M. G. Frolov
R = \frac{{Br(K^ - \to \pi ^0 e^ - \overline \nu _e \gamma )}}{{Br(K^ - \to \pi ^0 e^ - \overline \nu _e )}}