PACS numbers

95.30.Cq Elementary particle processes
  1. S.V. Troitsky “Constraints on models of the origin of high-energy astrophysical neutrinosPhys. Usp. 64 1261–1285 (2021)
    95.30.Cq, 95.55.Vj, 98.70.Vc (all)
  2. D.S. Gorbunov “Sterile neutrinos and their roles in particles physics and cosmologyPhys. Usp. 57 503–511 (2014)
    12.60.−i, 14.60.Pq, 95.30.Cq (all)
  3. V.A. Rubakov “Elementary particle physics and cosmology: current status and prospectsPhys. Usp. 42 1193–1203 (1999)
    11.15.Kc, 11.30.Fs, 12.15.−y, 95.30.Cq (all)
  4. V.A. Rubakov, M.E. Shaposhnikov “Electroweak baryon number non-conservation in the early Universe and in high-energy collisionsPhys. Usp. 39 461–502 (1996)
    11.15.Kc, 11.30.Fs, 12.15.−y, 95.30.Cq (all)
  5. A.D. Sakharov “Violation of CP in variance, C asymmetry, and baryon asymmetry of the universeSov. Phys. Usp. 34 (5) 392–393 (1991)
    98.80.Cq, 98.80.Es, 11.30.Er, 14.65.−q, 95.30.Cq (all)
  6. V.L. Ginzburg, M.A. Markov et alGeorgii Timofeevich Zatsepin (On his seventieth birthday)Sov. Phys. Usp. 30 441–442 (1987)
    01.60.+q, 96.50.sd, 96.50.sb, 95.30.Cq, 96.60.Jw, 26.65.+t (all)
  7. A.E. Chudakov “Search for heavy magnetic monopoles in an experiment at the Baksan underground scintillation telescopeSov. Phys. Usp. 28 1054–1055 (1985)
    14.80.Hv, 29.40.Mc, 12.10.Dm, 96.50.S−, 95.30.Cq (all)
  8. T.M. Aliev, M.I. Vysotskii “Prospects for detecting photons produced by the decay of primordial neutrinos in the universeSov. Phys. Usp. 24 1008–1012 (1981)
    98.80.Bp, 95.30.Cq, 14.60.Gh, 13.10.+q (all)
  9. Ya.B. Zel’dovich, M.Yu. Khlopov “The neutrino mass in elementary-particle physics and in big bang cosmologySov. Phys. Usp. 24 755–774 (1981)
    98.80.Bp, 95.30.Cq, 14.60.Gh, 12.20.Hx (all)
  10. V.P. Chechev, Ya.M. Kramarovskii “The theory of nucleosynthesis in stars: the slow neutron capture processSov. Phys. Usp. 24 566–584 (1981)
    97.10.Cv, 95.30.Cq (all)
  11. L.B. Okun’ “Contemporary status and prospects of high-energy physicsSov. Phys. Usp. 24 341–365 (1981)
    11.10.−z, 11.90.+t, 12.20.Hx, 95.30.Cq (all)
  12. I.L. Rozental’ “Physical laws and the numerical values of fundamental constantsSov. Phys. Usp. 23 296–305 (1980)
    95.30.Cq, 06.20.Jr (all)
  13. Ya.B. Zel’dovich “Gravitation, charges, cosmology, and coherenceSov. Phys. Usp. 20 945–955 (1977)
    98.80.Dr, 97.60.Lf, 95.30.Cq, 95.30.Sf (all)
  14. I.L. Rozental’ “Cosmic objects and elementary particlesSov. Phys. Usp. 20 167–173 (1977)
    95.30.Cq, 97.20.−w, 97.60.Lf, 98.80.−k (all)
  15. Ya.B. Zel’dovich “The cosmological constant and the theory of elementary particlesSov. Phys. Usp. 11 381–393 (1968)
    98.80.Es, 98.80.Cq, 95.30.Cq, 98.54.Aj (all)
  16. I.L. Rozental’ “Interaction of cosmic muons of high energySov. Phys. Usp. 11 49–65 (1968)
    96.50.sb, 95.30.Cq, 96.60.Vg, 14.40.Aq (all)
  17. E.L. Feinberg “The problem of quarks in cosmic raysSov. Phys. Usp. 10 256–261 (1967)
    96.50.sb, 14.65.−q, 11.30.Ly, 95.30.Cq (all)
  18. Ya.B. Zel’dovich, L.B. Okun, S.B. Pikel’ner “Quarks: astrophysical and physicochemical aspectsSov. Phys. Usp. 8 702–709 (1966)
    95.30.Cq, 14.65.−q, 98.80.Cq, 11.30.Ly, 96.50.S−, 14.20.Dh (all)
  19. B.M. Pontekorvo “Elementary particle physics is expensive: is it necessary?Sov. Phys. Usp. 8 617–618 (1966)
    14.20.Jn, 96.50.sb, 25.30.Mr, 12.39.−x, 95.30.Cq (all)
  20. E.L. Feinberg “Cosmic rays and elementary particle physicsSov. Phys. Usp. 8 619–627 (1966)
    96.50.sd, 95.30.Cq, 13.75.Gx, 13.15.+g, 12.20.−m, 14.40.Aq (all)
  21. Ya.B. Zel’dovich “The theory of the expanding Universe as originated by A. A. FridmanSov. Phys. Usp. 6 475–494 (1964)
    95.30.Cq, 95.30.Sf, 98.62.Py (all)
  22. B.M. Pontekorvo “The neutrino and its role in astrophysicsSov. Phys. Usp. 6 1–12 (1963)
    14.60.Lm, 13.60.−r, 12.15.Mm, 13.66.−a, 98.80.Cq, 95.30.Cq (all)
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