PACS numbers

14.60.Lm Ordinary neutrinos 14.60.Pq Neutrino mass and mixing 96.50.Vg Energetic particles 96.50.sb Composition, energy spectra and interactions
  1. Yu.G. Kudenko “Neutrino oscillations: recent advances and future prospects61 739–747 (2018)
    14.60.Pq, 25.30.Pt (all)
  2. V.A. Bednyakov, D.V. Naumov, O.Yu. Smirnov “Neutrino physics and JINR59 225–253 (2016)
    13.15.+g, 14.60.Lm, 14.60.Pq, 14.60.St, 26.65.+t (all)
  3. Yu.G. Kudenko “Long baseline neutrino accelerator experiments: results and prospects57 462–469 (2014)
    14.60.Pq, 25.30.Pt (all)
  4. A.S. Barabash “Double beta decay experiments: current status and prospects57 482–488 (2014)
    14.60.Pq, 23.40.−s (all)
  5. S.M. Bilenky “Bruno Pontecorvo and the neutrino57 489–496 (2014)
    01.60+q, 01.65.+g, 14.60.Pq (all)
  6. A.G. Olshevskiy “Reactor neutrino experiments: results and prospects57 497–502 (2014)
    13.15.+g, 14.60.Pq, 29.40.Mc (all)
  7. D.S. Gorbunov “Sterile neutrinos and their roles in particles physics and cosmology57 503–511 (2014)
    12.60.−i, 14.60.Pq, 95.30.Cq (all)
  8. A.V. Derbin “Solar neutrino experiments57 512–524 (2014)
    26.65.+t, 14.60.Pq, 95.55.Vj (all)
  9. Yu.G. Kudenko “T2K observation of muon-to-electron neutrino oscillations56 1120–1125 (2013)
    14.60.Pq, 25.30.Pt (all)
  10. Modern problems in the physical sciences (Scientific session of the Physical Sciences Division of the Russian Academy of Sciences, 16 November 2011)55 607–632 (2012)
    01.10.Fv, 06.60.Jn, 07.07.Hj, 14.60.Pq, 29.40.Gx, 29.50.+v, 74.25.Ha, 74.25.Op, 74.50.+r, 74.72.−h, 74.72.Hs, 85.60.−q (all)
  11. N.G. Polukhina “Nuclear track detection: advances and potential in astrophysics, particle physics and applied research55 614–625 (2012)
    14.60.Pq, 29.40.Gx, 29.50.+v (all)
  12. Forty years of the Institute for Nuclear Research (Scientific session of the Physical Sciences Division of the Russian Academy of Sciences, 22 December 2010)54 939–974 (2011)
    01.10.Fv, 01.52.+r, 01.65.+g, 14.60.Pq, 14.60.−z, 25.30.Pt, 26.65.+t, 28.60.+s, 29.20.−c, 29.40.Ka, 32.80.Qk, 32.80.Wr, 42.55.−f, 87.56.B−, 95.55.Vj, 96.50.sb, 96.50.sh, 96.60.Vg (all)
  13. I.I. Tkachev “Telescope Array Observatory observations of the Greisen—Zatsepin—Kuzmin effect54 954–961 (2011)
    95.55.Vj, 96.50.sb, 96.50.sh (all)
  14. Yu.G. Kudenko “T2K neutrino experiment: first results54 961–968 (2011)
    14.60.Pq, 25.30.Pt (all)
  15. Yu.G. Kudenko “Study of neutrino oscillations in long-baseline accelerator experiments54 549–572 (2011)
    12.60.−i, 14.60.Pq, 25.30.Pt (all)
  16. Yu.I. Stozhkov, G.A. Bazilevskaya “S N Vernov and cosmic ray research in the Earth atmosphere54 210–215 (2011)
    94.20.wq, 96.50.Vg, 96.50.Wx (all)
  17. A.B. Aleksandrov, A.V. Bagulya et alCharge spectrum of galactic cosmic ray nuclei as measured in meteorite olivines53 805–808 (2010)
    21.10.Ft, 26.40.+r, 95.55.Vj, 96.30.Za, 96.50.sb (all)
  18. I.S. Tsukerman “Neutrino oscillations and the CPT48 825–840 (2005)
    11.30.−j, 11.30.Er, 14.60.Pq, 14.60.St (all)
  19. E.Kh. Akhmedov “Neutrino oscillations in three- and four-flavor schemes47 117–124 (2004)
    11.30.Fs, 14.60.Pq, 26.65.+t (all)
  20. S.M. Bilen’kii “Neutrino masses, mixing and oscillations46 1137–1152 (2003)
    13.15.+g, 14.60.Pq, 14.60.St (all)
  21. A. Bettini “Physics beyond the Standard Model: experiments at the Gran Sasso Laboratory44 931–954 (2001)
    12.60.−i, 14.60.Pq, 26.65.+t, 95.35.+d (all)
  22. S.S. Gershtein, E.P. Kuznetsov, V.A. Ryabov “The nature of neutrino mass and the phenomenon of neutrino oscillations40 773–806 (1997)
    14.60.Pq, 12.15.Ff (all)
  23. Yu.V. Kozlov, V.P. Martem’yanov, K.N. Mukhin “Neutrino mass problem: the state of the art40 807–842 (1997)
    14.60.Pq, 12.15.Ff (all)
  24. Yu.N. Eroshenko “Physics news on the Internet (based on electronic preprints)38 683–684 (1995)
    01.10.Cr, 04.80.Cc, 14.60.Pq, 74.25.Ha (all)
  25. V.L. Ginzburg “The origin of cosmic rays (Forty years later)36 (7) 587–591 (1993)
    98.70.Sa, 96.50.sb, 96.50.sd, 98.70.Dk (all)
  26. L.A. Khalfin “Fate of the universe and the heavy 17-keV neutrino35 (8) 717–719 (1992)
    23.40.Bw, 26.50.+x, 26.35.+c, 14.60.Pq, 14.60.Lm (all)
  27. S.T. Belyaev, S.S. Gershtein et alIsai Izrailevich Gurevich (on his eightieth birthday)35 (8) 723–724 (1992)
    01.60.+q, 96.50.sb, 21.65.+f, 14.60.Lm, 13.40.Em, 28.41.Te (all)
  28. I.V. Andreev, V.L. Ginzburg et alEvgenii L’vovich Feinberg (on his eightieth birthday)35 (6) 533–534 (1992)
    01.60.+q, 23.40.−s, 29.30.Hs, 96.50.sb (all)
  29. G.V. Domogatskii, G.T. Zatsepin et alAleksandr Evgen’evich Chudakov (on his seventieth birthday)34 (7) 637–638 (1991)
    01.60.+q, 96.50.sb, 13.85.−t, 41.60.Bq (all)
  30. A.P. Aleksandrov, A.F. Apalin et alPetr Efimovich Spivak (on his eightieth birthday)34 (7) 639–640 (1991)
    01.60.+q, 14.60.Pq, 23.40.−s, 13.30.Eg, 14.20.Dh, 29.40.−n (all)
  31. A.D. Erlykin, E.A. Mamidzhanyan “Autumn school ’Interactions of hadrons at super-accelerator energies’34 (4) 334–339 (1991)
    01.40.E−, 29.40.Mc, 96.50.sd, 13.60.Hb, 96.50.sb (all)
  32. B.A. Trubnikov “On the possible generation of cosmic rays in plasma pinches33 (12) 1061–1071 (1990)
    98.70.Sa, 96.50.sb, 96.50.Tf, 52.40.Kh, 94.05.Jq (all)
  33. M.B. Voloshin, V.N. Gribov et alLev Borisovich Okun’ (on his sixtieth birthday)32 643–644 (1989)
    01.60.+q, 13.25.Es, 11.30.Er, 14.60.Lm, 13.40.Em (all)
  34. V.L. Dadykin, G.T. Zatsepin, O.G. Ryazhskaya “Events detected by underground detectors on February 23, 198732 459–468 (1989)
    97.10.Bt, 95.30.Sf, 97.60.Bw, 14.60.Lm, 29.40.Mc (all)
  35. A.D. Erlykin, E.A. Mamidzhanyan, V.A. Tsarev “Autumn school ’Interaction of hadrons at above-accelerator energies’32 380–383 (1989)
    96.50.sb, 96.50.sd, 97.60.Bw, 98.62.Ra, 01.40.E− (all)
  36. V.L. Ginzburg “Astrophysical aspects of cosmic-ray research (first 75 years and outlook for the future)31 491–510 (1988)
    96.50.sb, 98.70.Sa, 98.80.−k, 01.30.Cc (all)
  37. G.B. Khristiansen “Prospects for studying cosmic rays at ultrahigh energies (1015-1021 eV)30 1110–1112 (1987)
    96.50.sb, 98.70.Vc, 96.50.sd, 98.70.Sa (all)
  38. G.T. Zatsepin, Yu.A. Nechin, G.B. Khristiansen “Use of the magnetic induction of iron in cosmic-ray and high-energy physics30 1007–1008 (1987)
    41.20.Gz, 75.60.Ej, 96.50.sb, 96.50.sd (all)
  39. S.P. Mikheev, A.Yu. Smirnov “Resonance oscillations of neutrinos in matter30 759–790 (1987)
    14.60.Pq, 14.60.Lm, 96.60.Jw, 96.50.Vg (all)
  40. V.L. Ginzburg, M.A. Markov et alGeorgii Timofeevich Zatsepin (On his seventieth birthday)30 441–442 (1987)
    01.60.+q, 96.50.sd, 96.50.sb, 95.30.Cq, 96.60.Jw, 26.65.+t (all)
  41. A.P. Aleksandrov, V.A. Ambartsumyan et alAnatolii Alekseevich Logunov (On his sixtieth birthday)30 290–292 (1987)
    01.60.+q, 11.10.Hi, 11.10.Gh, 96.50.sb, 13.75.Cs (all)
  42. S.P. Mikheev, A.Yu. Smirnov “Neutrino oscillations in a medium with variable density29 1155–1157 (1986)
    14.60.Lm, 14.60.Pq, 96.50.Vg, 96.50.sb (all)
  43. M.G. Shchepkin “Majorana neutrino and double beta decay29 1062–1063 (1986)
    14.60.Lm, 14.60.Pq, 11.30.Qc, 23.40.Bw, 11.30.Er (all)
  44. L.A. Mikaelyan “Neutrino experiments on the reactor at the Roven nuclear power plant29 1063–1064 (1986)
    29.40.Mc, 13.15.+g, 14.60.Lm, 14.60.Pq (all)
  45. M.B. Voloshin, M.I. Vysotskii, L.B. Okun’ “Possible electromagnetic properties of the neutrino and variations of the solar neutrino flux29 1070–1070 (1986)
    14.60.Lm, 96.50.sb, 96.50.Vg, 13.40.Em, 11.30.Ly, 97.20.−w (all)
  46. I.M. Dremin “Toponium29 903–923 (1986)
    12.38.Bx, 14.65.Dw, 14.65.Ha, 12.39.Pn, 14.80.Ly, 14.60.Lm (all)
  47. Abdus Salam (On his sixtieth birthday)29 722–722 (1986)
    99.10.Np, 14.60.Lm, 11.30.−j, 11.15.−q, 12.15.−y (all)
  48. V.S. Berezinskii “High energy neutrino astrophysics28 728–730 (1985)
    96.50.sb, 97.60.Gb, 13.75.Cs, 97.60.Bw, 97.10.Cv, 97.20.Li (all)
  49. Yu.G. Abov, V.V. Vladimirskii et alAleksandr Ovseevich Vaisenberg (Obituary)28 733–734 (1985)
    01.60.+q, 96.50.sb, 13.20.Cz, 14.40.Aq, 13.35.Bv, 14.60.Ef (all)
  50. Z.G. Berezhiani, D.L. Chkareuli “Horizontal symmetry: masses and mixing angles of quarks and leptons of different generations; neutrino mass and neutrino oscillation28 104–105 (1985)
    14.60.Pq, 14.60.Lm, 11.30.Ly, 11.30.Er, 14.65.−q (all)
  51. G.A. Askar’yan “Investigation of the Earth by means of neutrinos. Neutrino geology27 896–900 (1984)
    96.50.sb, 91.60.Pn (all)
  52. M.G. Shchepkin “Double beta decay and the neutrino mass27 555–578 (1984)
    23.40.Bw, 12.10.−g, 14.60.Lm, 14.60.Pq, 27.60.+j (all)
  53. A.K. Likhoded “Tenth All-Union School on Inelastic Interactions at High Energies27 647–648 (1984)
    01.40.E−, 96.50.sb, 11.30.Rd, 96.50.sd, 25.40.−h, 24.85.+p (all)
  54. G.A. Gusev, I.M. Zheleznykh “On the possibility of detection of neutrinos and muons on the basis of radio radiation of cascades in natural dielectric media (antarctic ice sheet and so forth)27 550–552 (1984)
    96.50.sd, 96.50.sb, 95.55.Vj, 14.80.Hv, 14.80.Ly (all)
  55. A.I. Akhiezer, M.P. Rekalo “Electric charge of elementary particles18 864–874 (1975)
    13.40.Em, 14.60.Cd, 14.60.Ef, 14.20.Dh, 14.20.Jn, 14.60.Lm (all)
  56. V.L. Ginzburg “The origin of Cosmic Rays (Present State of the Problem)18 795–796 (1975)
    01.10.Fv, 96.50.sb, 98.70.Sa, 97.60.Bw (all)
  57. G.B. Zhdanov “Errata to the article by G. B. Zhdanov, ’Search for Transuranium Elements,’ Vol. 16, No. 516 944–944 (1974)
    25.85.Ca, 21.60.Cs, 27.90.+b, 96.50.sb, 21.10.Ky, 23.60.+e (all)
  58. M.A. Markov “Global properties of matter in collapsed state (’black holes’)16 587–599 (1974)
    04.70.−s, 97.60.Lf, 95.30.Sf, 14.60.Lm, 13.40.Em (all)
  59. G.B. Zhdanov “Search for transuranium elements (methods, results, and prospects)16 642–657 (1974)
    25.85.Ca, 21.60.Cs, 27.90.+b, 96.50.sb, 21.10.Ky, 23.60.+e (all)
  60. M.A. Gintzburg “Visual observation of cosmic rays16 163–164 (1973)
    96.50.sf, 95.85.Ry, 96.50.Vg, 96.60.Vg (all)
  61. Yu.V. Gaponov “The complete experiment in β decay13 647–662 (1971)
    23.40.Bw, 14.60.Lm, 11.30.Er, 27.30.+t, 21.10.Tg (all)
  62. B. Pontekorvo “Some new proposals for experiments in the field of neutrino physics14 235–241 (1971)
    13.15.+g, 14.60.Pq, 13.66.−a, 11.30.Er (all)
  63. E.P. Shabalin “Probabilities of weak processes with neutral lepton currents11 524–524 (1969)
    12.15.Mm, 13.20.Eb, 14.40.Aq, 13.15.+g, 14.60.Lm, 14.20.Dh (all)
  64. B.M. Pontekorvo “Conservation of leptons and baryons and the neutrino mass11 528–529 (1969)
    14.20.−c, 14.60.Pq, 23.40.−s, 29.40.Gx, 29.40.Wk (all)
  65. F.L. Shapiro “Electric dipole moments of elementary particles11 345–352 (1968)
    13.40.Em, 11.30.Er, 14.60.Lm, 14.20.Dh (all)
  66. A.M. Baldin, A.A. Komar, E.L. Feinberg “Moiseĭ Aleksandrovich Markov (on his sixtieth birthday)11 453–454 (1968)
    01.60.+q, 13.40.Gp, 14.40.−n, 14.20.−c, 14.60.Lm (all)
  67. I.L. Rozental’ “Interaction of cosmic muons of high energy11 49–65 (1968)
    96.50.sb, 95.30.Cq, 96.60.Vg, 14.40.Aq (all)
  68. V.R. Lazarenko “Double beta decay and the properties of the neutrino9 860–873 (1967)
    23.40.Hc, 21.10.Ma, 14.60.Lm (all)
  69. E.L. Feinberg “The problem of quarks in cosmic rays10 256–261 (1967)
    96.50.sb, 14.65.−q, 11.30.Ly, 95.30.Cq (all)
  70. D.I. Blokhintsev “High-energy physics and the fundamental principles of modern theory8 612–613 (1966)
    96.50.sb, 96.50.Vg, 13.85.Dz, 13.60.Fz, 11.10.−z, 11.30.Er (all)
  71. B.M. Pontekorvo “Elementary particle physics is expensive: is it necessary?8 617–618 (1966)
    14.20.Jn, 96.50.sb, 25.30.Mr, 12.39.−x, 95.30.Cq (all)
  72. V.L. Ginzburg, S.I. Syrovatskii “Origin of cosmic rays9 223–235 (1966)
    96.50.sb, 95.30.Qd, 98.54.Gr, 97.60.Bw (all)
  73. D. Ivanenko, Yu. Lomsadze “Conference on the theory of elementary particles7 462–467 (1964)
    01.10.Fv, 14.60.Pq, 11.55.Jy, 11.15.−q, 11.10.−z, 13.75.Gx (all)
  74. V.L. Ginzburg, L.V. Kurnosova et alSoviet satellite and rocket investigations of the nuclear component of cosmic rays7 230–269 (1964)
    96.50.sb, 98.70.Sa, 98.70.Vc, 98.38.Am, 95.55.−n (all)
  75. S.I. Nikol’skii “Extensive air showers of cosmic radiation5 849–877 (1963)
    96.50.sd, 96.50.sb, 98.70.Vc (all)
  76. B.M. Pontekorvo “The neutrino and its role in astrophysics6 1–12 (1963)
    14.60.Lm, 13.60.−r, 12.15.Mm, 13.66.−a, 98.80.Cq, 95.30.Cq (all)
  77. V.L. Ginzburg “Cosmic rays on Earth and in the Universe4 553–575 (1962)
    96.50.sb, 96.50.Vg, 94.20.wq, 94.30.Xy, 98.70.Sa (all)
  78. N.A. Dobrotin, N.L. Grigorov et alSERGEĬ NIKOLAEVICH VERNOV (on his fiftieth birthday)3 810–812 (1961)
    01.60.+q, 96.50.sd, 96.50.sb (all)
  79. V.L. Ginzburg, S.I. Syrovatskii “Present status of the question of the origin of cosmic rays3 504–541 (1961)
    96.50.sb, 96.50.Dj, 97.60.Bw, 96.60.Q−, 98.70.Sa (all)
  80. N.A. Dobrotin “International cosmic ray conference2 974–986 (1960)
    98.70.Sa, 96.50.sd, 96.50.sb (all)
  81. Ya.A. Smorodinskii “The present state of the theory of beta decay2 1–37 (1959)
    23.40.Bw, 11.30.Er, 13.40.Em, 13.30.Ce, 14.60.Lm, 13.35.Bv (all)
  82. G.G. Getmantsev, V.L. Ginzburg, I.S. Shklovskii “Radio astronomical investigations with the aid of artificial satellites1 65–67 (1958)
    95.40.+s, 98.70.Vc, 96.50.sb (all)
© 1918–2019 Uspekhi Fizicheskikh Nauk
Email: ufn@ufn.ru Editorial office contacts About the journal Terms and conditions