Abstract
Weakly interacting, massive particles (WIMPs) have recently been proposed as a solution to the solar neutrino problem1–3. Whereas standard solar models consistently predict a detection rate of (high-energy) neutrinos 3 times higher than that observed in the Davis experiment4–6, the presence of hypothetical massive particles in the solar centre would resolve this discrepancy. Models which incorporate a relative number of 10−11 WIMPs with appropriate scattering cross-section would reduce the predicted neutrino detections by 37Cl to the observed value, without significant changes in the solar structure outside the central region1–3. We have subjected these models to an observational test of p–mode oscillation frequencies by computing frequency differences of low-degree, high-order oscillation frequencies. Although standard solar models also pass this test, WIMP models provide a better fit.
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References
- 1
Spergel, D. N. & Press, W. H. Astrophys. J. 294, 663–673 (1985).
- 2
Faulkner, J. & Gilliland, R. L. Astrophys. J. 299, 994–1000 (1985).
- 3
Gilliland, R. L., Faulkner, J., Press, W. H. & Spergel, D. N. Astrophys. J. (in the press).
- 4
Davis, R., Harmer, D. S. & Hoffman, K. C. Phys. Rev. Lett. 20, 1205–1209 (1968).
- 5
Bahcall, J. N., Huebner, W. F., Lubow, S. H., Parker, P. D. & Ulrich, R. K. Rev. Mod. Phys. 54, 767–799 (1982).
- 6
Bahcall, J. N., Cleveland, B. T., Davis, R. Jr & Rowley, J. K. Astrophys. J. 292, L79–82 (1985).
- 7
Schatzman, E., Maeder, A., Angrand, F. & Glowinski, R. Astr. Astrophys. 96, 1–16. (1981).
- 8
Provost, J. Observational Tests of Stellar Evolution Theory (eds Maeder, A. & Renzini, A.) 47–65 (Reidel, Dordrecht, 1984).
- 9
Tassoul, M. Astrophys. J. Suppl. Ser. 43, 469–490 (1980).
- 10
Christensen-Dalsgaard, J. Seismology of the Sun and the Distant Stars (ed. Gough, D. O.) 23–53 (Reidel, Dordrecht, 1986).
- 11
Gough, D. O. Phys. Bull. 34, 502–507 (1983).
- 12
Christensen-Dalsgaard, J. Space Research Prospects in Stellar Activity and Variability (eds Mangeney, A. & Praderie, F.) 11–46 (Observatoire de Paris, 1984).
- 13
Scherrer, P. H., Wilcox, J. M., Christensen-Dalsgaard, J. & Gough, D. O. Sol. Phys. 82, 75–87 (1983).
- 14
Gough, D. O. Adv. Space Res. 4, 85–102 (1984).
- 15
Christensen-Dalsgaard, J. Mon. Not. R. astr. Soc. 194, 229–250 (1981).
- 16
Christensen-Dalsgaard, J. Mon. Not. R. astr. Soc. 199, 735–761 (1982).
- 17
Claverie, A., Isaak, G. R., McLeod, C. P., van der Raay, H. B. & Roca Cortes, T. Nature 293, 443–445 (1981).
- 18
Grec, G., Fossat, E. & Pomerantz, M. Sol. Phys. 82, 55–66 (1983).
- 19
Duvall, T. L. & Harvey, J. W. Nature 302, 24–27 (1983).
- 20
Kuhn, J. R., Libbrecht, K. G. & Dicke, R. H. Nature 319, 128–131 (1986).
- 21
Delache, P. & Scherrer, P. H. Nature 306, 651–653 (1983).
- 22
van der Raay, H. B., Palle, P. L., Roca Cortes, T. Seismology of the Sun and the Distant Stars (ed. Gough, D. O.) 215–221 (Reidel, Dordrecht, 1986).
- 23
Faulkner, J., Gough, D. O. & Vahia, M. N. Nature (this issue).
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Affiliations
High Altitude Observatory, NCAR, PO Box 3000, Boulder, Colorado, 80307, USA
- W. Däppen
- & R. L. Gilliland
Astronomisk Institut, Aarhus Universitet, DK-8000, Aarhus C, Denmark
- J. Christensen-Dalsgaard
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Further reading
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What Have We Learned from Helioseismology, What Have We Really Learned, and What Do We Aspire to Learn?
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