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The Internal Structure of the Sun, its Pulsations and the Neutrino Problem

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The Comparative Study of the Planets

Part of the book series: NATO Advanced Study Institutes Series ((ASIC,volume 85))

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Abstract

The theory of the internal structure of the Sun is described. The standard models of the Sun predict a neutrino flux which is three time larger than that measured by Davis experiment. It is not clear whether this dramatic discrepancy depends on the ideas of stellar structure and evolution theory or on neutrino physics. A convincing attempt to reconcile theory and observations has been done constructing a solar model with a very low primordial abundance of heavy elements. This model predicts the correct neutrino flux, but has a convective zone much thinner than that of the standard model. The observed spectrum of 5 minute oscillations, which is extremely sensitive to the depth of the convection zone, can only be reproduced by the standard model indicating that neutrino flux is high. In recent times, a series of independent experiments have not excluded the possibility that neutrino is massive and oscillates in three different types. Should this be the case, assuming and equally probable mixure of the three neutrinos, the experiment of Davis should actually detect one third of the neutrino flux produced by the Sun at the Earth’s surface.

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References

  • Bahcall, J.N.: 1979, Space Science Reviews 24, pp. 227–251.

    Article  ADS  Google Scholar 

  • Belvedere, G., Gough, D.O., and Paternò, L.: 1981, preprint.

    Google Scholar 

  • Berthomieu, G., Cooper, A.J., Gough, D.O., Osaki, Y., Provost, J., and Rocca, A.: 1980, Nonradial and Nonlinear Stellar Pulsation, H.A. Hill and W. Dziembowski (eds.), Springer-Verlag, New York, pp. 307–312.

    Chapter  Google Scholar 

  • Christensen-Dalsgaard, J., Gough, D.O., and Morgan, J.G.: 1979, Astron. Astrophys. 73, pp. 121–128.

    ADS  Google Scholar 

  • Cox, J.P.: 1980, Theory of Stellar Pulsation, Princeton University Press, Princeton, New Jersey.

    Google Scholar 

  • Cox, J.P., and Giuli, R.T.: 1968, Principles of Stellar Structure, Vol. 1, Gordon and Breach, New York.

    Google Scholar 

  • Cox, A.N., and Steward, J.N.: 1970, Astrophys.J. Suppl. 19, pp. 243–259.

    Article  ADS  Google Scholar 

  • Davis, R., and Evans, J.C.: 1978, The New Solar Physics, J.A. Eddy (ed.), Westview Press, Boulder, Colorado, pp. 35–57.

    Google Scholar 

  • Deubner, F.L., Ulrich, R.K., and Rhodes, E.J.: 1979, Astron. Astrophys. 72, pp. 177–185.

    ADS  Google Scholar 

  • Fowler, W.A., Caughlam, G.R., and Zimmerman, B.A.: 1967, Annual Rev. Astron. Astrophys. 5, pp. 525–570.

    Article  ADS  Google Scholar 

  • Fowler, W.A., Caughlam, G.R., and Zimmerman, B.A.: 1975, Annual Rev. Astron. Astrophys. 13, pp. 69–112.

    Article  ADS  Google Scholar 

  • Hill, H.A.: 1978, The New Solar Physics, J.A. Eddy (ed.), Westview Press, Boulder, Colorado, pp. 135–214.

    Google Scholar 

  • Lubkin, G.B.: 1980, Physics Today, 33, 7, pp. 17–19.

    Article  ADS  Google Scholar 

  • Reeves, H.: 1966, Stellar Evolution, R.F. Stein and A.G. Cameron (eds.), Plenum Press, New York, pp. 83–122.

    Google Scholar 

  • Rosenwald, R.D., and Hill, H.A.: 1980, Nonradial and Nonlinear Stellar Pulsation, H.A. Hill and W. Dziembowski (eds.), Springer-Verlag, New York, pp. 404–412.

    Chapter  Google Scholar 

  • Stein, R.F.: 1966, Stellar Evolution, R.F. Stein and A.G. Cameron (eds.), Plenum Press, New York, pp. 3–79.

    Google Scholar 

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© 1982 D. Reidel Publishing Company

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Paternò, L. (1982). The Internal Structure of the Sun, its Pulsations and the Neutrino Problem. In: Coradini, A., Fulchignoni, M. (eds) The Comparative Study of the Planets. NATO Advanced Study Institutes Series, vol 85. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7810-2_13

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  • DOI: https://doi.org/10.1007/978-94-009-7810-2_13

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-009-7812-6

  • Online ISBN: 978-94-009-7810-2

  • eBook Packages: Springer Book Archive

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