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talk at this meeting; see also astro-ph/9811364, astro-ph/9811366, astro-ph/9811447, astro-ph/9811454
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Turner, M. S. talk at this meeting; see also astro-ph/9811364, astro-ph/9811366, astro-ph/9811447, astro-ph/9811454.
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Bahcall, J. N., talk at this meeting; see also astro-ph/9808162; Bahcall, J. N., Krastev, P. I. and Yu. Smirnov, A., Phys.Rev. D58, 096016 (1998).
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Bahcall, J. N., talk at this meeting; see also astro-ph/9808162; Bahcall, J. N., Krastev, P. I. and Yu. Smirnov, A., Phys.Rev. D58, 096016 (1998).
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E. Lisi, talk at this meeting; see also Fogli, G. L., Lisi, E., Marrone, A. and Scioscia, G., Phys. Rev. D59, 033001 (1999).
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Lisi, E.1
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E. Lisi, talk at this meeting; see also Fogli, G. L., Lisi, E., Marrone, A. and Scioscia, G., Phys. Rev. D59, 033001 (1999).
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Phys. Rev.
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For some recent work, see: King, S. F., Phys. Lett. B439, 350 (1998); Elwood. J. K., Irges, N. and Ramond, P., Phys. Rev. Lett. B81, 5064 (1998); Barger, V., et al., Phys. Rev. D58, 093016 (1998); Osland, P. and Vigdel, G. Phys. Lett. B438, 129 (1998); Joshipura, A. and Smirnov, A., Phys. Lett. B439, 103 (1998); Tanimoto, M., Phys. Rev. D59, 017304 (1999); Lazarides, G. and Vlachos, N., Phys. Lett. B441, 46 (1998); Barger, V., Weiler, T. and Whisnant, K., Phys. Lett. B440, 1 (1998); Pati, J., Nucl. Phys. Rev. Supp. 77, 299 (1999); Gonzalez-Carcia, M., et al., Nucl. Phys. B543, 3 (1999); Altarelli, G. and Feruglio, F., Phys. Lett. B439, 112 (1998).
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For some recent work, see: King, S. F., Phys. Lett. B439, 350 (1998); Elwood. J. K., Irges, N. and Ramond, P., Phys. Rev. Lett. B81, 5064 (1998); Barger, V., et al., Phys. Rev. D58, 093016 (1998); Osland, P. and Vigdel, G. Phys. Lett. B438, 129 (1998); Joshipura, A. and Smirnov, A., Phys. Lett. B439, 103 (1998); Tanimoto, M., Phys. Rev. D59, 017304 (1999); Lazarides, G. and Vlachos, N., Phys. Lett. B441, 46 (1998); Barger, V., Weiler, T. and Whisnant, K., Phys. Lett. B440, 1 (1998); Pati, J., Nucl. Phys. Rev. Supp. 77, 299 (1999); Gonzalez-Carcia, M., et al., Nucl. Phys. B543, 3 (1999); Altarelli, G. and Feruglio, F., Phys. Lett. B439, 112 (1998).
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For some recent work, see: King, S. F., Phys. Lett. B439, 350 (1998); Elwood. J. K., Irges, N. and Ramond, P., Phys. Rev. Lett. B81, 5064 (1998); Barger, V., et al., Phys. Rev. D58, 093016 (1998); Osland, P. and Vigdel, G. Phys. Lett. B438, 129 (1998); Joshipura, A. and Smirnov, A., Phys. Lett. B439, 103 (1998); Tanimoto, M., Phys. Rev. D59, 017304 (1999); Lazarides, G. and Vlachos, N., Phys. Lett. B441, 46 (1998); Barger, V., Weiler, T. and Whisnant, K., Phys. Lett. B440, 1 (1998); Pati, J., Nucl. Phys. Rev. Supp. 77, 299 (1999); Gonzalez-Carcia, M., et al., Nucl. Phys. B543, 3 (1999); Altarelli, G. and Feruglio, F., Phys. Lett. B439, 112 (1998).
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talk at this meeting
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However, combinations of structure-formation and cosmic microwave-background measurements may be sensitive to smaller neutrino masses: Tegmark, M., talk at this meeting; see also Hu, W., Eisenstein, D. J., Tegmark, M. and White, M., Phys. Rev. D59, 023512 (1999).
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