Advertisement

Experiments for Solar Neutrinos and Supernova Neutrinos

  • Yoji Totsuka

Abstract

Solar energy is believed to be generated by nuclear fusion processes taking place in the core of the Sun. This belief must, of course, be tested experimentally.

Keywords

Solar Neutrino Neutrino Flux Neutrino Spectrum Standard Solar Model Solar Neutrino Problem 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

References

  1. [1]
    J.N. Bahcall and R.K. Ulrich, Rev. Mod. Phys. 60, 297 (1988).ADSCrossRefGoogle Scholar
  2. [1a]
    See also S. Turck-Chièze, S. Cahen, M. Cassè and C. Doom, Astrophys. J. 335, 415 (1988).ADSCrossRefGoogle Scholar
  3. [2]
    J.N. Bahcall, Rev. Mod. Phys. 50, 881 (1978). 8B ß-decays into the broad excited state (2+, 2.94 MeV). Thus eq.(1.2) must further be smeared with the width of this state.ADSCrossRefGoogle Scholar
  4. [2a]
    See J.N. Bahcall and B.R. Holstein, Phys. Rev. C33, 2121 (1986),MathSciNetADSCrossRefGoogle Scholar
  5. [2b]
    E.W. Warburton, Phys. Rev. C33, 303 (1986).ADSGoogle Scholar
  6. [3]
    J.N. Bahcall and M.H. Pinsonneault, Rev. Mod. Phys. 64, 885 (1992).ADSCrossRefGoogle Scholar
  7. [4]
    A. Colgate and R.H. White, Astrophys. J. 143, 626 (1966).ADSCrossRefGoogle Scholar
  8. [5]
    S.E. Woosley, J.R. Wilson and R. Mayle, Astrophys. J. 302, 19 (1986).ADSCrossRefGoogle Scholar
  9. [6]
    A. Burrows and J.M. Lattimer, Astrophys. J. 307, 178 (1986).ADSCrossRefGoogle Scholar
  10. [7]
    R. Mayle, Ph.D. Thesis, Univ. of California, Berkeley, 1985; UCRL-53713.Google Scholar
  11. [8]
    R. Mayle, J.R. Wilson and D.N. Schramm, Astrophys. J. 318, 288 (1987).ADSCrossRefGoogle Scholar
  12. [9]
    K. Sato and H. Suzuki, Phys. Rev. Lett. 58, 2722 (1987).ADSCrossRefGoogle Scholar
  13. [10]
    H. Suzuki, Doctor Thesis, Univ. of Tokyo, 1989.Google Scholar
  14. [11]
    L. Wolfenstein, Phys. Rev. D17, 2369 (1978);ADSGoogle Scholar
  15. [11a]
    S.P. Mikheyev and A.Yu. Smirnov, Nuovo Cimento C9, 17 (1986).CrossRefGoogle Scholar
  16. [12]
    J.N. Bahcall, Rev. Mod. Phys. 59, 505 (1987).ADSCrossRefGoogle Scholar
  17. [13]
    F.J. Kelly and H. Überall, Phys. Rev. lett. 16, 145 (1966).ADSCrossRefGoogle Scholar
  18. [14]
    S.D. Ellis and J.N. Bahcall, Nucl. Phys. A114, 636 (1968).CrossRefGoogle Scholar
  19. [15]
    S. Ying, W.C. Haxton and E.M. Henley, Phys. Rev. D40, 3211 (1989).ADSGoogle Scholar
  20. [16]
    N. Tatara, Y. Kohyama and K. Kubodera, Phys. Rev. C42, 1694 (1990).ADSGoogle Scholar
  21. [17]
    A.F.M. Ishaq and T.J. Kennett, Canadian J. Phys. 50, 3090 (1972).ADSCrossRefGoogle Scholar
  22. [18]
    J.N. Bahcall, “Neutrino Astrophysics”, Cambridge University Press, 1989.Google Scholar
  23. [19]
    Note the angular distribution of electrons from reaction v e z-1 Ae -Z A is given by 1 + v e α cos 0, where α is, (Math) (Math) (spin nan flip) (Math) (pin flip). where T is isospin of Z-1 A, and T 3 (i) and T 3 (f) are the third components of isospin of z-1 A and Z A, respectively. 40Ar has Jπ = 0+. Thus <σ>2 = 0 and α = 1. For v e 2H→e - pp, spin flips (J π; 1+ → 0+). Thus <l>2 = 0 and (Math)Google Scholar
  24. [20]
    J.N. Bahcall, M. Baldo-Ceolin, D.B. Cline and C. Rubbia, Phys. Lett. B178, 324 (1986).CrossRefGoogle Scholar
  25. [21]
    K.S. Hirata, et al., Phys. Rev. D44, 2241 (1991).ADSGoogle Scholar
  26. [22]
    Y. Suzuki, Frontiers of Neutrino Astrophysics, ed. Y. Suzuki and K. Nakamura, (Universal Academy Press Inc., 1992), p.61.Google Scholar
  27. [23]
    R. Davis Jr., Frontiers of Neutrino Astrophysics, ed. Y. Suzuki and K. Nakamura, (Universal Academy Press Inc., 1992), p.47.Google Scholar
  28. [24]
    P. Anselmann et al., GX27–1993/MPIH-Vll-1993/Chem(BNL) C-3991 (1993).Google Scholar
  29. [25]
    G.T. Zatsepin, Frontiers of Neutrino Astrophysics, ed. Y. Suzuki and K. Nakamura, (Universal Academy Press Inc., 1992), p.71.Google Scholar
  30. [26]
    J.N. Bahcall and R.K. Ulrich, Rev. Mod. Phys. 60, 297 (1988).ADSCrossRefGoogle Scholar
  31. [26a]
    See also S. Turck-Chièze, S. Cahen, M. Cassè and C. Doom, Astrophys. J. 335, 415 (1988).ADSCrossRefGoogle Scholar
  32. [27]
    “Scientific and Technical Description of the Mark II SNO Detector”, SNO-89–15, ed. by E.W. Beier and D. Sinclair.Google Scholar
  33. [28]
    L.M. Krauss, S.L. Glashow and D.N. Schramm, Nature 310, 191 (1984).ADSCrossRefGoogle Scholar
  34. [29]
    R. Davis, Phys. Rev. Lett. 12, 303 (1964);ADSCrossRefGoogle Scholar
  35. [29a]
    J.K. Rowley, B.T. Cleveland and R. Davis Jr., AIP Conference Proceedings No.126, p.1 (1985).CrossRefGoogle Scholar
  36. [30]
    A.I. Abazov et al., Phys. Rev. Lett. 67, 3332 (1991);ADSCrossRefGoogle Scholar
  37. [30]
    T.J. Bowles, Invited talk presented at NEUTRINO’92, Granada, 1992.Google Scholar
  38. [31]
    P. Anselmann et al., Phys. Lett. B285, 390 (1992).CrossRefGoogle Scholar
  39. [32]
    K. Lande, Invited talk presented at NEUTRINO’92, Granada, 1992.Google Scholar
  40. [33]
    G.S. Hurst et al., Phys. Rev. Lett. 53, 1116 (1984);ADSCrossRefGoogle Scholar
  41. [33a]
    G.S. Hurst et al., AIP Conference Proceedings No.126, p.152 (1985).CrossRefGoogle Scholar
  42. [34]
    J.N. Bahcall, Rev. Mod. Phys. 50, 881 (1978).ADSCrossRefGoogle Scholar
  43. [35]
    J.N. Bahcall and C.A. Barnes, Phys. Lett. 12, 48 (1964).ADSCrossRefGoogle Scholar
  44. [36]
    J. Rapaport et al. Phys. Rev. Lett. 47, 1518 (1981);ADSCrossRefGoogle Scholar
  45. [37]
    “Table of Isotopes”, ed. by CM. Lederer and V.S. Shirley, John Wiley & Sons, 1978.Google Scholar
  46. [38]
    R.G. Sextro, R.A. Gough and J. Cerny, Nucl. Phys. A234, 130 (1974).CrossRefGoogle Scholar
  47. [39]
    CD. Goodman et al., Phys. Rev. Lett. 44, 1755 (1980).ADSCrossRefGoogle Scholar
  48. [40]
    J. Rapaport et al., Phys. Rev. Lett. 47, 1518 (1981).ADSCrossRefGoogle Scholar
  49. [41]
    T.N. Taddeucci et al., Phys. Rev. C25, 1094 (1981).Google Scholar
  50. [42]
    J.N. Bahcall and R.K. Ulrich, Rev. Mod. Phys. 60, 297 (1988);ADSCrossRefGoogle Scholar
  51. [42a]
    J.N. Bahcall, “Neutrino Astrophysics”, Cambridge University Press, 1989.Google Scholar
  52. [43]
    W.C Haxton, Phys. Rev. Lett. 60, 768 (1988).ADSCrossRefGoogle Scholar
  53. [44]
    J. Engel, S. Pittel and P. Vogel, Phys. Rev. Lett. 67, 426 (1991).ADSCrossRefGoogle Scholar
  54. [45]
    S. Turck-Chièze, S. Cahen, M. Cassè and C. Doom, Astrophys. J. 335, 415 (1988).ADSCrossRefGoogle Scholar
  55. [46]
    J.A. Bearden and A.F. Burr, Rev. Mod. Phys. 39, 125 (1967).ADSCrossRefGoogle Scholar
  56. [47]
    A.H. Wapstra, G.J. Nijah and R. Van Lieshout, “Nuclear Spectroscopy Tables”, North-Holland Publ. 1959.Google Scholar
  57. [48]
    E. Henrich and K.H. Ebert, Angew. Chem. Int. Ed. Engl.Google Scholar
  58. [49]
    V.N. Gavrin et al., Proc. of Inside the Sun Conference, Versailles, ed. Berthomieu and Cribier (Kluwer Academic, 1989), p.201. 31, 1283 (1992).Google Scholar
  59. [50]
    R. Davis Jr., Frontiers of Neutrino Astrophysics, ed. Y. Suzuki and K. Nakamura, (Universal Academy Press Inc., 1992), p.47.Google Scholar
  60. [51]
    G.T. Zatsepin, Frontiers of Neutrino Astrophysics, ed. Y. Suzuki and K. Nakamura, (Universal Academy Press Inc., 1992), p.71.Google Scholar
  61. [52]
    F. von Feilitzsch, Invited talk presented at the International Conference on Neutral Currents Twenty Years Later, Paris, July 1993.Google Scholar
  62. [53]
    J. Rich and M. Spiro, DAPNIA/SPP 93–01, 1993; Texas/PASCOS 92; Relativistic Astrophysics and Particle Cosmology, ed. C.W. Akerlof and M.A. Srednicki, (Ann. N.Y. Acad. Sci., 1992), p.364.Google Scholar
  63. [54]
    K.S. Hirata, Doctor thesis, University of Tokyo, 1991; ICRR-Report-239–91–8 (Institute for Cosmic Ray Research, Univ. Tokyo); K.S. Hirata, et al., Ref. [21].Google Scholar
  64. [55]
    International Astronomical Union Circular (IAU Circular) no.4323 (1987).Google Scholar
  65. [56]
    J. Weneser, Phys. Rev. 105, 1335 (1957).ADSCrossRefGoogle Scholar
  66. [57]
    F.J. Kelly and H. Überall, Phys. Rev. Lett. 16, 145 (1966).ADSCrossRefGoogle Scholar
  67. [58]
    K. Hirata et al., Phys. Rev. Lett. 58, 1490 (1987).ADSCrossRefGoogle Scholar
  68. [59]
    K.S. Hirata et al., Phys. Rev. D38, 48 (1988).MathSciNetGoogle Scholar
  69. [60]
    R.M. Bionta et al., Phys. Rev. Lett. 58, 1494 (1987);ADSCrossRefGoogle Scholar
  70. [60a]
    C.B. Bratton et al., Phys. Rev. D37, 3361 (1988).ADSGoogle Scholar
  71. [61]
    M. Aglietta et al., Europhys. Lett. 3, 1315 (1987).ADSCrossRefGoogle Scholar
  72. [62]
    E.N. Alexeyev et al., Phys. Lett. B205, 209 (1988).CrossRefGoogle Scholar
  73. [63]
    Y. Totsuka, Proceedings of International Symposium on Underground Physics Experiments, ed. K. Nakamura, 1990, p.129; Y. Totsuka, ICRR-Report-227–90–20.Google Scholar

Copyright information

© Springer Japan 1994

Authors and Affiliations

  • Yoji Totsuka
    • 1
  1. 1.Institute for Cosmic Ray ResearchUniversity of TokyoJapan

Personalised recommendations