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