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The following HTML text is provided to enhance online readability. Many aspects of typography translate only awkwardly to HTML. Please use the page image as the authoritative form to ensure accuracy. [21] V. A. Kuz'min , Sov. Phys. JETP (Engl. Transl.) 22, 1059 ( 1966 ). [22] J. N. Bahcall , B. T. Cleveland , R. Davis, Jr. , et al. , Phys. Rev. Lett. 40, 1351 ( 1978 ). [23] H. Chen , Phys. Rev. Lett. 55, 1534 ( ); G. Aardsma et al. , Phys. Lett. B 194, 321 ( 1987 ); G. Ewan et al. , Sudbury Neutrino Observatory Proposal SNO-87-12 ( 1987 ). [24] Y. Totsuka , in Proceedings of the International Symposium on Underground Physics Experiments , edited by K. Nakamura ( ICRR, University of Tokyo , 1990 ), p. 129 ; A. Suzuki , in Proceedings of the Workshop on Elementary-Particle Picture of the Universe , Tsukuba, Japan , 1987 , edited by M. Yoshimura , Y. Totsuka , and K. Nakamura ( KEK Report No. 87-1 , Tsukuba , 1987 ), p. 136 ; M. Takita , in Frontiers of Neutrino Astrophysics , edited by Y. Suzuki and K. Nakamura ( Universal Academy Press, Inc. , Tokyo , 1993 ), p. 135 . [25] G. Ranucci for the Borexino Collaboration, Nucl. Phys. B (Proc. Suppl.) 32, 149 ( 1993 ); C. Arpasella et al. , in “Borexino at Gran Sasso: Proposal for a real-time detector for low energy solar neutrinos,” Vols. I and II , University of Milan , INFN report (unpublished) ; “Borexino-A Real Time Detector for Low Energy Solar Neutrinos,” proposal submitted to the NSF by Princeton University on behalf of the U.S. Borexino Collaboration, December, 1992 . [26] W. C. Haxton , Phys. Rev. Lett. 60, 768 ( 1988 ). [27] J. P. Revol , Frontiers of Neutrino Astrophysics , edited by Y. Suzuki and K. Nakamura ( Universal Academy Press, Inc. , Tokyo , 1993 ), p. 167 ; J. N. Bahcall , Mo Baldo-Ceolin , D. Cline , and C. Rubbia , Phys. Lett. B 178, 324 ( 1986 ); C. Rubbia , CERN-EP Internal Report 77-8 ( 1977 ); The ICARUS Collaboration , ICARUS II , A Second-Generation Proton Decay Experiment and Neutrino Observatory at the Gran Sasso Laboratory , Volume I ( September 1993 ), Volume II ( May 1994 ). [28] R. E. Lanou , H. J. Maris , and G. M. Seidel , Phys. Rev. Lett. 58, 2498 ( 1987 ); S. R. Bandler et al. , Phys. Rev. Lett. 68, 2429 ( 1992 ); F. S. Porter , Ph.D. Thesis , Brown University ( 1994 , unpublished); S. R. Bandler et al. , J. Low Temp. Phys. 93, 715 and 785 ( 1993 ). [29] J. Seguinot , T. Ypsilantis , and A. Zichichi , “A High Rate Solar Neutrino Detector with Energy Determination,” LPC92-31 , College de France , December 8, 1992. [30] P. D. Barnes et al. , J. Low Temp. Phys. 93, 791 ( 1993 ); W. Seidel et al. , ibid., 797 ; A. Alessandrello et al. , ibid., 815 . [31] A. Alessandrello et al. , Report No. INFN/SAE-92/28 ( 1992 , unpublished). [32] R. S. Raghavan , P. Raghavan , and T. Kovacs , Phys. Rev. Lett. 71, 4295 ( 1993 ). [33] I. R. Barabanov , G. V. Domagatsky , and G. T. Zatsepin , , edited by J. Schneps , T. Kafka , W. A. Mann , and P. Nath (World Scientific, Singapore , 1989 ), p. 331. [34] A. Kopylov , Frontiers of Neutrino Astrophysics , edited by Y. Suzuki and K. Nakamura ( Universal Academy Press, Inc. , Tokyo , 1993 ), p. 157. [35] J. N. Bahcall , Phys. Rev. Lett. 23, 251 ( 1969 ).
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