Search

Your search keyword '"V.M. Serezhin"' showing total 4 results
Start Over Author "V.M. Serezhin"
4 results on '"V.M. Serezhin"'

1. Observation of muon pairs in neutrino interactions at Serpukhov 70 GeV accelarator

Author

V.G. Platonov, V.D. Khovansky, V.F. Perelygin, S.A. Zeldovich, V.I. Kurbakov, V.M. Serezhin, V.P. Zhigunov, A.V. Kulikov, V.N. Rychenkov, Yu M. Sviridov, V.G. Shevchenko, Yu.G. Stroganov, V.A. Smotryaev, V.Ya. Uglekov, V.N. Goryachev, V.Sh. Epstein, N.V. Kalganov, V.I. Kochetkov, V.A. Zhemanov, L.A. Klimenko, Ya.A. Zudin, Yu.G. Kornelyuk, I.S. Trostin, A.E. Asratyan, Alexandre Rozanov, V.G. Rybakov, V. V. Krendelev, I.P. Maksimov, A.S. Vovenko, A.I. Mukhin, M.S. Ryabinin, V.V. Shamanov, A.A. Volkov, M. A. Kubantsev, A.P. Bugorsky, A. A. Zaytsev, V.S. Kaftanov, E.A. Grigoriev, K.E. Shestermanov, and V.A. Yarba

Subjects
Physics, Nuclear physics, Nuclear and High Energy Physics, Range (particle radiation), Particle physics, Muon, Energy interval, Spark chamber, Neutrino
Abstract

A search for dimuons produced in a spark chamber experiment in neutrino and antineutrino beams of the Serpukhov accelerator is reported. The clear dimuon signal has been observed in vN interactions. R v = N (2 ω )/ N (1 ω )⩾ (6.2 ± 1.7) × 10 −3 in the energy interval 7.5 ÷ 30 GeV. From antineutrino data we conclude that in the same energy range R v ⩽ 1.1. × 10 −2 (90% C.L.) .

Published
1977

2. Charged current neutrino interactions below 30 GeV

Author

A.I. Mukhin, A.A. Zaitsev, V.A. Smotryaev, Yu.G. Stroganov, I.P. Maksimov, Alexandre Rozanov, V.V. Shamanov, Yu.G. Kornelyuk, L.A. Klimenko, R.M. Fakhrutdinov, A.A. Volkov, A.S. Vovenko, V. G. Kartashova, A.V. Kulikov, V.I. Kurbakov, V.I. Kochetkov, V.M. Serezhin, S.A. Zeldovich, V.S. Kaftanov, E.A. Grigoriev, M.S. Ryabinin, V.F. Perelygin, V.D. Khovansky, V.G. Shevchenko, Yu M. Sviridov, V.N. Goryachev, K.E. Shestermanov, I.S. Trostin, V.A. Gemanov, V.P. Zhigunov, M.M. Savitsky, V.A. Yarba, N.V. Kalganov, A.E. Asratyan, V.Sh. Epstein, V.G. Platonov, M. A. Kubantsev, A.P. Bugorsky, Yu.A. Zudin, and B.F. Polyakov

Subjects
Nuclear physics, Physics, Nuclear and High Energy Physics, Particle physics, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Physics::Accelerator Physics, High Energy Physics::Experiment, Spark chamber, Neutrino, Nuclear Experiment, Charged current, Beam (structure)
Abstract

Charged current data of a spark chamber neutrino experiment at the 70 GeV Serpukhov accelerator (10 200 events in the v beam and 3600 events in the v beam with energies up to 30 GeV) have been analyzed. Total neutrino and antineutrino cross sections and v-distributions are obtained.

Published
1978

3. Quasielastic neutrino and antineutrino scattering total cross-sections, axial-vector form-factor

Author

A.I. Mukhin, V.I. Kurbakov, L.A. Klimenko, V.M. Serezhin, M.S. Ryabinin, K.E. Shestermanov, V.A. Smotryaev, V.I. Kochetkov, N.V. Kalganov, S. V. Belikov, A. P. Bygorsky, V.F. Perelygin, V.G. Shevchenko, V.V. Shamanov, S.A. Zeldovich, V.A. Zhemanov, A.A. Volkov, Yu M. Sviridov, I.S. Trostin, V.Sh. Epstein, Yu.G. Kornelyuk, and A. A. Zaytsev

Subjects
Physics, Nuclear and High Energy Physics, Particle physics, Physics::Instrumentation and Detectors, Scattering, Form factor (quantum field theory), Elementary particle, Nuclear physics, Dipole, High Energy Physics::Experiment, Neutrino, Spark chamber, Nuclear Experiment, Pseudovector, Charged current
Abstract

Experimental results on the study of quasielastic reactionsv μ n→μ − p and $$\bar v_u p \to \mu ^ + n$$ in the energy range 3–30 GeV are presented in this paper. Spark chamber detector with Al filters has been exposed to the wide-band neutrino and antineutrino beams at Serpukhov. Neutrino and antineutrino data have been used to reconstruct the behaviour of axial-vector form-factorF A (Q 2). We measured the total cross-sections as a function of energy. The parameterM A =(1.00±0.04) GeV/c2 has been determined under the assumption of the dipole parametrization and CVC hypothesis. Upper limit for the second class currents was estimated.

Published
1985

4. Further Search for Muonic Pairs in the Neutrino and Antineutrino Beams at the IHEP 70 GeV Accelerator

Author

Yu.A. Zudin, M. A. Kubantsev, A.P. Bugorsky, V.V. Shamanov, Yu. G. Komelyuk, A.I. Mukhin, V.I. Kurbakov, V.F. Perelygin, L.A. Klimenko, V. V. Krendelev, Alexandre Rozanov, A.A. Zaitsev, V.S. Kaftanov, E.A. Grigoriev, A.S. Vovenko, A.A. Volkov, V.G. Rybakov, K.E. Shestermanov, V. A. Kochetkov, Yu.M. Sviridov, V.Ya. Uglekov, V.P. Zhigunov, N.V. Kalganov, M.S. Ryabinin, I.P. Maksimov, V.G. Platonov, V.A. Smotryaev, V.M. Serezhin, Yu.G. Stroganov, V.N. Rychenkov, V.D. Khovansky, I.S. Trostin, V.A. Yarba, S.A. Zeldovich, V.A. Zhemanov, A.V. Kulikov, V.G. Shevchenko, V.N. Goryachev, A.E. Asratyan, and V.Sh. Epstein

Subjects
Nuclear physics, Physics, High energy, Low energy, High Energy Physics::Experiment, Fermilab, Neutrino, Spectral line
Abstract

The search for dimuon production in vN and vN interactions at the Serpukhov accelerator was started in December, 1974. Preliminary data after analysis of part of the statistics of the neutrino exposure showed no effect [1, 2]. In further measurements we changed the neutrino spectrum. Namely, we suppressed the low energy part and enriched the high energy part. It was done because similar experiments at Fermilab [3, 4] indicated predominant dimuon production at energies E v ≳ 30 GeV. Fig. 1 shows qualitatively the variation of the neutrino spectra from the first to the second run.

Published
1977

Catalog

Books, media, physical & digital resources
See catalog results