PACS numbers

04.30.−w Gravitational waves 97.60.Gb Pulsars
  1. V.S. Beskin “Radio pulsars --- already fifty years!61 353–380 (2018)
    01.65.+g, 95.30.Qd, 97.60.Gb (all)
  2. D.H. Reitze “The first detections of gravitational waves emitted from binary black hole mergers60 823–829 (2017)
    04.25.dg, 04.30.−w, 04.80.Nn, 95.55.Ym (all)
  3. V.N. Rudenko “Gravitational-wave experiment in Russia60 830–842 (2017)
    04.30.−w, 04.80.Nn, 95.55.Ym (all)
  4. V.V. Zheleznyakov, E.Ya. Zlotnik et alDouble plasma resonance nd its manifestations in radio astronomy59 997–1020 (2016)
    96.60.P−, 96.60.Tf, 97.60.Gb, 52.35.−g, 52.35.Hr, 52.35.Qz (all)
  5. V.I. Pustovoit “On the direct detection of gravitational waves59 1034–1051 (2016)
    04.30.−w, 04.80.Nn, 95.55.Ym (all)
  6. V.B. Braginsky, I.A. Bilenko et alBackground to the discovery of gravitational waves59 879–885 (2016)
    04.30.−w, 04.80.Nn, 95.55.Ym (all)
  7. A.M. Cherepashchuk “Discovery of gravitational waves: a new chapter in black hole studies59 910–917 (2016)
    04.30.−w, 97.60.Lf, 97.80.−d (all)
  8. V.M. Lipunov “Astrophysical sense of the discovery of gravitational waves59 918–928 (2016)
    04.30.−w, 95.85.Sz, 97.80.−d (all)
  9. V.S. Beskin, A.A. Zheltoukhov “On the anomalous torque applied to a rotating magnetized sphere in a vacuum57 799–806 (2014)
    03.50.De, 41.20.−q, 97.60.Gb (all)
  10. V.S. Beskin, Ya.N. Istomin, A.A. Philippov “Radio pulsars: the search for truth56 164–179 (2013)
    52.35.−g, 95.30.Gv, 97.60.Gb (all)
  11. Commemoration of the 90th anniversary of the birth of Andrei Dmitrievich Sakharov (Scientific session of the Physical Sciences Division, Russian Academy of Sciences, 25 May 2011)55 169–216 (2012)
    01.10.Fv, 01.60.+q, 01.65.+g, 01.75.+m, 04.30.−w, 04.70.−s, 28.52.−s, 28.70.+y, 52.55.Fa, 95.36.+x, 98.70.Vc, 98.80.Cq, 98.80.−k (all)
  12. L.P. Grishchuk “Cosmological Sakharov oscillations and quantum mechanics of the early Universe55 210–216 (2012)
    04.30.−w, 98.70.Vc, 98.80.Cq (all)
  13. V.S. Beskin “Magnetohydrodynamic models of astrophysical jets53 1199–1233 (2010)
    95.30.Qd, 97.60.Gb, 97.60.Lf, 98.62.Nx (all)
  14. A.Yu. Potekhin “The physics of neutron stars53 1235–1256 (2010)
    26.60.−c, 97.60.Gb, 97.60.Jd (all)
  15. A.I. Nikishov, V.I. Ritus “Gravitational radiation of systems and the role of their force field53 1093–1122 (2010)
    04.20.−q, 04.30.−w, 41.60.−m (all)
  16. N.S. Kardashev “Radioastron: a radio telescope many times the size of Earth. Research program52 1127–1137 (2009)
    01.30.Bb, 95.55.Jz, 95.85.Bh, 95.85.Fm, 97.60.Gb (all)
  17. G.S. Bisnovatyi-Kogan “Binary and recycled pulsars: 30 years after observational discovery49 53–67 (2006)
    04.30.Db, 04.80.Cc, 97.60.Gb, 97.80.−d (all)
  18. V.N. Lukash “On the relation between tensor and scalar perturbation modes in Friedmann cosmology49 103–106 (2006)
    01.10.Fv, 04.30.−w, 04.62.+v, 98.80.−k (all)
  19. L.P. Grishchuk “Relic gravitational waves and cosmology48 1235–1247 (2005)
    04.30.−w, 04.62.+v, 98.80.−k (all)
  20. V.B. Braginskii “Adolescent years of experimental physics46 81–87 (2003)
    03.65.Ta, 04.30.−w, 04.80.Nn, 06.20.−f, 06.30.−k, 95.55.Ym (all)
  21. I.D. Novikov, I.D. Karachentsev et alScientific session of the Division of General Physics and Astronomy of the Russian Academy of Sciences (28 February, 2001)44 817–818 (2001)
    01.10.Fv, 95.85.Bh, 98.80.Cq, 98.80.Es, 95.35.+d, 98.65.−r, 04.70.-S, 97.80.Jp, 98.35.Jk, 47.37.+q, 97.60.Gb, 97.60.Jd (all)
  22. D.G. Yakovlev “Superfluidity in neutron stars44 823–826 (2001)
    47.37.+q, 97.60.Gb, 97.60.Jd (all)
  23. L.P. Grishchuk, V.M. Lipunov et alGravitational wave astronomy: in anticipation of first sources to be detected44 1–51 (2001)
    04.30.−w, 04.80.Nn, 95.55.Ym, 95.85.Sz (all)
  24. V.B. Braginskii “Gravitational-wave astronomy: new methods of measurements43 691–699 (2000)
    04.30.−w, 04.80.Nn, 95.55.Ym, 95.85.Sz (all)
  25. V.S. Beskin “Radio pulsars42 1071 (1999)
    04.40.Dg, 95.30.−k, 97.60.Gb, 98.70.Dk (all)
  26. D.A. Kirzhnits, S.N. Yudin “Paradoxes of superfluid rotation38 1283–1288 (1995)
    47.37.Tq, 97.60.Gb
  27. D.A. Kirzhnits “Pulsars and rotation of a superfluid liquid38 791–792 (1995)
    01.10.Fv, 97.60.Gb, 67.90.+z (all)
  28. C.M. Will “The binary pulsar, gravitational waves, and the Nobel prize37 697–703 (1994)
    97.60.Gb, 04.30.−w, 01.65.g (all)
  29. T.V. Shabanova “Discovery of a planetary system around PSR 0329+5437 618–621 (1994)
    97.82.+k, 97.60.Gb
  30. D.M. Sedrakyan, K.M. Shakhabasyan “Superfluidity and the magnetic field of pulsars34 (7) 555–571 (1991)
    97.60.Gb, 97.60.Jd, 26.60.+c, 97.10.Ld, 97.10.Cv (all)
  31. V.G. Ryasnyĭ “Supernova shells33 (5) 393–395 (1990)
    97.60.Bw, 96.10.+i, 97.60.Gb, 97.60.Jd, 96.60.qe (all)
  32. L.P. Grishchuk “Gravitational-wave astronomy31 940–954 (1988)
    04.30.Db, 97.60.Gb, 97.80.Gm, 97.30.Qt, 98.80.Es, 04.60.−m (all)
  33. A.D. Kuz’min “The pulsar time scale31 881–882 (1988)
    97.60.Gb, 04.30.−w (all)
  34. E.A. Mamidzhanyan, S.I. Nikol’skii “Possibility of experimental ultrahigh-energy gamma-ray astronomy30 542–543 (1987)
    98.70.Rz, 98.70.Sa, 97.60.Gb, 98.54.Aj, 98.58.Mj, 96.50.sd (all)
  35. V.B. Braginskii, L.P. Grishchuk “Gravitational wave astronomy30 81–82 (1987)
    04.30.−w, 97.60.Bw, 98.80.Bp, 98.80.Cq (all)
  36. V.S. Beskin, A.V. Gurevich, Ya.N. Istomin “Physics of pulsar magnetospheres29 946–970 (1986)
    97.60.Gb, 97.10.Ex, 97.10.Ld, 95.30.Qd, 98.70.Dk (all)
  37. 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)
  38. B.M. Vladimirskii, A.M. Gal’per et alCygnus X-3: a powerful galactic source of hard radiation28 153–169 (1985)
    98.70.Dk, 98.70.Qy, 98.70.Rz, 97.60.Gb, 97.60.Jd, 97.60.Lf (all)
  39. V.S. Strel’nitskii “Cosmic masers17 507–527 (1975)
    98.70.Vc, 98.58.Hf, 98.58.Mj, 98.54.Aj, 97.60.Gb, 97.10.Bt (all)
  40. Yu.N. Efremov, S.B. Novikov, P.V. Shcheglov “Prospects for development of ground-based optical astronomy18 151–160 (1975)
    98.80.Es, 98.54.Aj, 97.60.Gb, 95.30.Sf, 98.62.Js, 95.55.Cs (all)
  41. Ya.B. Zel’dovich “Neutron Stars and ’Black Holes’16 559–561 (1974)
    97.60.Jd, 97.60.Lf, 97.10.Kc, 97.10.Cv, 97.80.Jp, 97.60.Gb (all)
  42. A.M. Gal’per, V.G. Kirillov-Ugryumov, B.I. Luchkov “Observational gamma astronomy17 186–198 (1974)
    98.70.Rz, 98.70.Sa, 98.80.Es, 97.60.Gb (all)
  43. Yu.P. Shitov “Pulsar Observations at the Radioastronomical Station of the USSR Academy of Sciences Physics Institute16 288–289 (1973)
    97.60.Gb, 97.10.Ri, 95.55.Jz, 97.10.Sj, 97.10.Ex (all)
  44. V.V. Zheleznyakov “On the Origin of Pulsar Radiation16 289–290 (1973)
    97.60.Gb, 97.10.Cv, 97.10.Ex, 97.10.Ri (all)
  45. D.A. Kirzhnits “Extremal states of matter (ultrahigh pressures and temperatures)14 512–523 (1972)
    21.65.+f, 21.30.−x, 97.20.Rp, 26.60.+c, 97.60.Gb (all)
  46. B.M. Bolotovskii, V.L. Ginzburg “The Vavilov-Cerenkov Effect and the Doppler Effect in the Motion of Sources with Superluminal Velocity in Vacuum15 184–192 (1972)
    97.60.Gb, 97.10.Ri, 41.60.Bq (all)
  47. V.L. Ginzburg “PULSARS (Theoretical Concepts)14 83–103 (1971)
    97.60.Gb, 97.60.Jd, 97.10.Ld, 97.10.Ri (all)
  48. S.B. Pikel’ner “Magnetic Hydrodynamics of Solar Formations14 228–229 (1971)
    97.60.Gb, 97.60.Jd, 97.20.Rp, 98.35.Ac (all)
  49. V.L. Ginzburg “Pulsars — Present State of the Problem14 229–230 (1971)
    97.60.Gb, 97.60.Jd, 97.10.Ri (all)
  50. Ya.G. Dorfman “New Results from the Study of Plato’s Physics14 230–231 (1971)
    97.60.Gb, 97.60.Jd (all)
  51. V.L. Ginzburg “What problems of physics and astrophysics are of special importance and interest at present?14 21–39 (1971)
    74.72.−h, 71.35.−y, 04.30.−w, 98.80.Jk, 95.30.Sf, 97.60.Jd (all)
  52. V.L. Ginzburg “Pulsars (General Review)12 800–804 (1970)
    97.60.Gb, 97.60.Bw (all)
  53. N.M. Shakhovskoi, Yu.S. Efimov, V.I. Pronik “Polarization of the Crab Nebula Pulsar in the Optical Band12 804–805 (1970)
    97.60.Gb, 98.38.Mz, 95.55.Qf (all)
  54. V.I. Pronik, I.I. Pronik, K.K. Chuvaev “Distribution of the Energy in the Spectrum of the P Pulsar of the Crab Nebula12 805–805 (1970)
    97.60.Gb, 98.38.Mz, 98.38.Jw (all)
  55. Yu.I. Alekseev, V.V. Vitkevich, Yu.P. Shitov “Fine Structure of the Pulses of the Pulsar CP0808 and Variation of the Periods of the Second Class12 805–806 (1970)
    97.60.Gb, 98.70.Dk (all)
  56. Yu.I. Alekseev, V.V. Vitkevich et alThe New Pulsar PP094312 806–806 (1970)
    97.60.Gb
  57. V.V. Vitkevich, N.A. Lotova et alPulsar Flicker Due to the Inhomogeneities of the Interstellar Plasma12 806–806 (1970)
    98.38.Kx, 98.58.Kh, 97.60.Gb (all)
  58. A.A. Stepanyan, B.M. Vladimirskii et alPossible Existence of a Flux of 1013·eV γ Quanta from the Pulsar CP113312 806–806 (1970)
    95.45.+i, 97.60.Gb (all)
  59. L.M. Erukhimov “Oscillations of Pulsar Radio Emission12 806–807 (1970)
    98.70.Dk, 97.60.Gb (all)
  60. V.V. Zheleznyakov “Mechanisms of Pulsar Radiation12 807–808 (1970)
    97.60.Gb, 97.60.Jd, 41.60.Ap (all)
  61. N.S. Kardashev “Possibility of Observing Extragalactic Pulsars12 808–808 (1970)
    97.60.Gb, 97.60.Bw, 98.70.Dk, 98.54.Gr, 98.54.Aj (all)
  62. V.I. Slysh “Scattering of Pulsar X-rays in the Interstellar Medium12 808–808 (1970)
    97.60.Gb, 96.50.Dj, 98.38.Mz (all)
  63. I.S. Shklovskii “Concerning Pulsars12 808–809 (1970)
    97.60.Gb, 97.60.Jd (all)
  64. V.V. Vitkevich, Yu.P. Shitov, I.F. Malov “Concerning the Model of a Pulsar as a Rotating and Pulsating Neutron Star12 809–810 (1970)
    97.60.Gb, 97.60.Jd, 97.10.Sj, 97.10.Kc (all)
  65. V.B. Braginskii, V.N. Rudenko “Relativistic gravitational experiments13 165–181 (1970)
    04.80.Cc, 04.30.−w (all)
  66. V.L. Ginzburg, V.V. Zheleznyakov, V.V. Zaitsev “Coherent radio-emission mechanisms and magnetic pulsar models12 378–398 (1969)
    97.60.Gb, 97.10.Sj, 97.20.Rp, 97.60.Jd (all)
  67. I.S. Shklovskii “Discovery of pulsed sources of cosmic radio emission with strictly periodic variation of the flux11 435–436 (1968)
    98.70.Dk, 98.70.Sa, 98.70.Vc, 97.60.Gb (all)
  68. A. Trautman “The general theory of relativity9 319–339 (1966)
    04.20.−q, 04.30.−w (all)
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