Recent progress in neutrino factory and muon collider research within the Muon Collaboration

Physical Review Special Topics - Accelerators and Beams

Volumn 6, Issue 8, 2003, Pages 22-73

  Alsharo'a, Mohammad M ^a   Ankenbrandt, Charles M ^b   Atac, Muzaffer ^b   Autin, Bruno R ^c   Balbekov, Valeri I ^b   Barger, Vernon D ^d   Benary, Odette ^e   Bennett, J Roger J ^f   Berger, Michael S ^g   Berg, J Scott ^h   Berz, Martin ⁱ   Black, Edgar L ^a   Blondel, Alain ^j   Bogacz, S Alex ^k   Bonesini, M ^l   Bracker, Stephen B ^m   Bross, Alan D ^b   Bruno, Luca ^c   Buckley Geer, Elizabeth J ^b   Caldwell, Allen C ⁿ   Campanelli, Mario ^j   Cassel, Kevin W ^a   Catanesi, M Gabriela ^l   Chattopadhyay, Swapan ^k   Chou, Weiren ^b   Cline, David B ^o   Coney, Linda R ⁿ   Conrad, Janet M ⁿ   Corlett, John N ^p   Cremaldi, Lucien ^m   Cummings, Mary Anne ^q   Darve, Christine ^b   DeJongh, Fritz ^b   Drozhdin, Alexandr ^b   Drumm, Paul ^f   Elvira, V Daniel ^b   Errede, Deborah ^r   Fabich, Adrian ^c   Fawley, William M ^p   Fernow, Richard C ^h   Ferrario, Massimo ^l   Finley, David A ^b   Fisch, Nathaniel J ^s   Fukui, Yasuo ^o   Furman, Miguel A ^p   Gabriel, Tony A ^t   Galea, Raphael ⁿ   Gallardo, Juan C ^h   Garoby, Roland ^c   Garren, Alper A ^o   Geer, Stephen H ^b   Gilardoni, Simone ^c   Van Ginneken, Andreas J ^b   Ginzburg, Ilya F ^u   Godang, Romulus ^m   Goodman, Maury ^v   Gosz, Michael R ^a   Green, Michael A ^p   Gruber, Peter ^c   Gunion, John F ^w   Gupta, Ramesh ^h   Haines, John R ^t   Hanke, Klaus ^c   Hanson, Gail G ^x   Han, Tao ^d   Haney, Michael ^r   Hartill, Don ^y   Hartline, Robert E ^z   Haseroth, Helmut D ^c   Hassanein, Ahmed ^v   Hoffman, Kara ^aa   Holtkamp, Norbert ^t   Holzer, E Barbara ^c   Johnson, Colin ^c   Johnson, Rolland P ^z   Johnstone, Carol ^b   Jungmann, Klaus ^ab   Kahn, Stephen A ^h   Kaplan, Daniel M ^a   Keil, Eberhard K ^b   Kim, Eun San ^ac   Kim, Kwang Je ^aa   King, Bruce J ^ad   Kirk, Harold G ^h   Kuno, Yoshitaka ^ae   Ladran, Tony S ^p   Lau, Wing W ^af   Learned, John G ^ag   Lebedev, Valeri ^b   Lebrun, Paul ^b   Lee, Kevin ^o   Lettry, Jacques A ^c   Laveder, Marco ^l   Li, Derun ^p   Lombardi, Alessandra ^c   Lu, Changguo ^s   Makino, Kyoko ^r   Malkin, Vladimir ^s   Marfatia, D ^ah   McDonald, Kirk T ^s   Mezzetto, Mauro ^l   Miller, John R ^ai   Mills, Frederick E ^b   Mocioiu, I ^aj   Mokhov, Nikolai V ^b   Monroe, Jocelyn ⁿ   Moretti, Alfred ^b   Mori, Yoshiharu ^ak   Neuffer, David V ^b   Ng, King Yuen ^b   Norem, James H ^v   Onel, Yasar ^al   Oreglia, Mark ^aa   Ozaki, Satoshi ^h   Padamsee, Hasan ^y   Pakvasa, Sandip ^ag   Palmer, Robert B ^h   Parker, Brett ^h   Parsa, Zohreh ^h   Penn, Gregory ^am   Pischalnikov, Yuriy ^o   Popovic, Milorad B ^b   Qian, Zubao ^b   Radicioni, Emilio ^l   Raja, Rajendran ^b   Ravn, Helge L ^c   Reed, Claude B ^v   Reginato, Louis L ^p   Rehak, Pavel ^h   Rimmer, Robert A ^k   Roberts, Thomas J ^a   Roser, Thomas ^h   Rossmanith, Robert ^an   Samulyak, Roman V ^h   Scanlan, Ronald M ^p   Schlenstedt, Stefan ^ao   Schwandt, Peter ^g   Sessler, Andrew M ^p   Shaevitz, Michael H ⁿ   Shrock, Robert ^aj   Sievers, Peter ^c   Silvestrov, Gregory I ^ap   Simos, Nick ^h   Skrinsky, Alexander N ^ap   Solomey, Nickolas ^a   Spampinato, Philip T ^t   Spentzouris, Panagiotis ^b   Stefanski, R ^b   Stoltz, Peter ^aq   Stumer, Iuliu ^h   Summers, Donald J ^m   Teng, Lee C ^v   Thieberger, Peter A ^h   Tigner, Maury ^y   Todosow, Michael ^h   Tollestrup, Alvin V ^b   Torun, Yaǧmur ^a   Trbojevic, Dejan ^h   Usubov, Zafar U ^b   Vsevolozhskaya, Tatiana A ^ap   Wah, Yau ^aa   Wang, Chun Xi ^v   Wang, Haipeng ^k   Weggel, Robert J ^h   Whisnant, K ^ar   Willen, Erich H ^h   Wilson, Edmund J N ^c   Winn, David R ^as   Wurtele, Jonathan S ^p,am   Wu, Vincent ^at   Yokoi, Takeichiro ^ak   Yoon, Moohyun ^ac   York, Richard ⁱ   Yu, Simon ^p   Zeller, Al ⁱ   Zhao, Yongxiang ^h   Zisman, Michael S ^p   more..

^a ILLINOIS INSTITUTE OF TECHNOLOGY   (United States)

^b FERMI NATIONAL ACCELERATOR LABORATORY   (United States)

^c CERN   (Switzerland)

^d University of Wisconsin Madison   (United States)

^e TEL AVIV UNIVERSITY   (Israel)

^f RUTHERFORD APPLETON LABORATORY   (United Kingdom)

^g INDIANA UNIVERSITY   (United States)

^h BROOKHAVEN NATIONAL LABORATORY   (United States)

ⁱ MICHIGAN STATE UNIVERSITY   (United States)

^j UNIVERSITY OF GENEVA   (Switzerland)

^k THOMAS JEFFERSON NATIONAL ACCELERATOR FACILITY   (United States)

^l INFN SEZIONE DI ROMA   (Italy)

^m UNIVERSITY OF MISSISSIPPI   (United States)

ⁿ Och Spine at New York Presbyterian Hospitals   (United States)

^o UNIVERSITY OF CALIFORNIA   (United States)

^p LAWRENCE BERKELEY NATIONAL LABORATORY   (United States)

^q NORTHERN ILLINOIS UNIVERSITY   (United States)

^r UNIVERSITY OF ILLINOIS AT URBANA CHAMPAIGN   (United States)

^s PRINCETON UNIVERSITY   (United States)

^t OAK RIDGE NATIONAL LABORATORY   (United States)

^u SOBOLEV INSTITUTE OF MATHEMATICS   (Russian Federation)

^v ARGONNE NATIONAL LABORATORY   (United States)

^w UNIVERSITY OF CALIFORNIA   (United States)

^x UNIVERSITY OF CALIFORNIA   (United States)

^y Department of Obstetrics Gynecology   (United States)

^z MUONS INC   (United States)

^aa UNIVERSITY OF CHICAGO   (United States)

^ab UNIVERSITY OF GRONINGEN   (Netherlands)

^ac Pohang University of Science and Technology (POSTECH)   (South Korea)

^ad NORTHWESTERN UNIVERSITY   (United States)

^ae OSAKA UNIVERSITY   (Japan)

^af UNIVERSITY OF OXFORD   (United Kingdom)

^ag UNIVERSITY OF HAWAII   (United States)

^ah BOSTON UNIVERSITY   (United States)

^ai FLORIDA STATE UNIVERSITY   (United States)

^aj STONY BROOK UNIVERSITY   (United States)

^ak HIGH ENERGY ACCELERATOR RESEARCH ORGANIZATION KEK   (Japan)

^al UNIVERSITY OF IOWA   (United States)

^am UNIVERSITY OF CALIFORNIA   (United States)

^an KARLSRUHE INSTITUTE OF TECHNOLOGY   (Germany)

^ao DESY   (Germany)

^ap BUDKER INSTITUTE OF NUCLEAR PHYSICS   (Russian Federation)

^aq TECH X CORPORATION   (United States)

^ar IOWA STATE UNIVERSITY   (United States)

^as FAIRFIELD UNIVERSITY   (United States)

^at UNIVERSITY OF CINCINNATI   (United States)

more..

Author keywords

[No Author keywords available]

Indexed keywords

EID: 4143118523     PISSN: 10984402     EISSN: 10984402     Source Type: Journal    
DOI: 10.1103/PhysRevSTAB.6.081001     Document Type: Article

References (274)

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53. Some of the text quoted here appears in the study-II document [29]. We would like to thank Robert Shrock for helpful comments.
54. Fits and references to the Homestake, Kamiokande, GALLEX, SAGE, Super Kamiokande, and SNO data include N. Hata and P. Langacker, Phys. Rev. D 56, 6107 (1997); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 58, 096016 (1998); J. Bahcall and P. Krastev, Phys. Lett. B 436, 243 (1998); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 60, 093001 (1999); hep-ph/0103179; M. Gonzalez-Garcia, C. Peña-Garay, and J. W. F. Valle, Phys. Rev. D 63, 013007 (2001); M. Gonzalez-Garcia et al., Phys. Rev. D 63, 033005 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, Phys. Rev. D 64, 073009 (2001); P. Krastev and A. Smirnov, Phys. Rev. D 65, 073022 (2002); J. N. Bahcall, M. C. Gonzalez-Garcia, and C. Peña-Garay, hep-ph/0111150; M. Maltoni, T. Schwetz, and J. W. F. Valle, Phys. Rev. D 65, 093004 (2002). Recent discussions of flux calculations are found in J. Bahcall, Phys. Rep. 333, 47 (2000), hep-ph/0009044, Proceedings of Neutrino-2000, and http://www.sns.ias. edu/-jnb/; V. Barger, D. Marfatia, and K. Whisnant, Phys. Rev. Lett. 88, 011302 (2002); Phys. Lett. B 509, 19 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, hep-ph/0204253. Super Kamiokande data are reported and analyzed in SuperKamiokande Collaboration, Y. Fukuda et al., Phys. Rev. Lett. 82, 1810 (1999); S. Fukuda et al., Phys. Rev. Lett. 86, 5651 (2001). For recent reviews, see, e.g., Y. Suzuki, Nucl. Phys. B, Proc. Suppl. 91, 29 (2001); Y. Takeuchi, in Proceedings of the International Conference on High Energy Physics, Osaka, http://ichep2000.hep.sci.osaka-u.ac.jp; Proceedings of the Fifth Topical Workshop at the Gran Sasso National Laboratory: Solar Neutrinos, Assergi, Italy, 2001 (to be published). [35] L. Wolfenstein, Phys. Rev. D 17, 2369 (1978). [36] V. Barger, K. Whisnant, S. Pakvasa, and R. J. N. Phillips, Phys. Rev. D 22, 2718 (1980). [37] V. Barger et al., Phys. Rev. D 22, 1636 (1980). [38] S. P. Mikheyev and A. Smirnov, Yad. Fiz. 42, 1441 (1985) [Sov. J. Nucl. Phys. 42, 913 (1986)]; Nuovo Cimento Soc. Ital. Fis., C 9, 17 (1986); S. P. Rosen and J. Gelb, Phys. Rev. D 34, 969 (1986); S. Parke, Phys. Rev. Lett. 57, 1275 (1986); W. Haxton, Phys. Rev. Lett. 57, 1271 (1986); T. K. Kuo and J. Pantaleone, Rev. Mod. Phys. 61, 937 (1989).
55. Fits and references to the Homestake, Kamiokande, GALLEX, SAGE, Super Kamiokande, and SNO data include N. Hata and P. Langacker, Phys. Rev. D 56, 6107 (1997); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 58, 096016 (1998); J. Bahcall and P. Krastev, Phys. Lett. B 436, 243 (1998); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 60, 093001 (1999); hep-ph/0103179; M. Gonzalez-Garcia, C. Peña-Garay, and J. W. F. Valle, Phys. Rev. D 63, 013007 (2001); M. Gonzalez-Garcia et al., Phys. Rev. D 63, 033005 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, Phys. Rev. D 64, 073009 (2001); P. Krastev and A. Smirnov, Phys. Rev. D 65, 073022 (2002); J. N. Bahcall, M. C. Gonzalez-Garcia, and C. Peña-Garay, hep-ph/0111150; M. Maltoni, T. Schwetz, and J. W. F. Valle, Phys. Rev. D 65, 093004 (2002). Recent discussions of flux calculations are found in J. Bahcall, Phys. Rep. 333, 47 (2000), hep-ph/0009044, Proceedings of Neutrino-2000, and http://www.sns.ias. edu/-jnb/; V. Barger, D. Marfatia, and K. Whisnant, Phys. Rev. Lett. 88, 011302 (2002); Phys. Lett. B 509, 19 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, hep-ph/0204253. Super Kamiokande data are reported and analyzed in SuperKamiokande Collaboration, Y. Fukuda et al., Phys. Rev. Lett. 82, 1810 (1999); S. Fukuda et al., Phys. Rev. Lett. 86, 5651 (2001). For recent reviews, see, e.g., Y. Suzuki, Nucl. Phys. B, Proc. Suppl. 91, 29 (2001); Y. Takeuchi, in Proceedings of the International Conference on High Energy Physics, Osaka, http://ichep2000.hep.sci.osaka-u.ac.jp; Proceedings of the Fifth Topical Workshop at the Gran Sasso National Laboratory: Solar Neutrinos, Assergi, Italy, 2001 (to be published). [35] L. Wolfenstein, Phys. Rev. D 17, 2369 (1978). [36] V. Barger, K. Whisnant, S. Pakvasa, and R. J. N. Phillips, Phys. Rev. D 22, 2718 (1980). [37] V. Barger et al., Phys. Rev. D 22, 1636 (1980). [38] S. P. Mikheyev and A. Smirnov, Yad. Fiz. 42, 1441 (1985) [Sov. J. Nucl. Phys. 42, 913 (1986)]; Nuovo Cimento Soc. Ital. Fis., C 9, 17 (1986); S. P. Rosen and J. Gelb, Phys. Rev. D 34, 969 (1986); S. Parke, Phys. Rev. Lett. 57, 1275 (1986); W. Haxton, Phys. Rev. Lett. 57, 1271 (1986); T. K. Kuo and J. Pantaleone, Rev. Mod. Phys. 61, 937 (1989).
56. Fits and references to the Homestake, Kamiokande, GALLEX, SAGE, Super Kamiokande, and SNO data include N. Hata and P. Langacker, Phys. Rev. D 56, 6107 (1997); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 58, 096016 (1998); J. Bahcall and P. Krastev, Phys. Lett. B 436, 243 (1998); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 60, 093001 (1999); hep-ph/0103179; M. Gonzalez-Garcia, C. Peña-Garay, and J. W. F. Valle, Phys. Rev. D 63, 013007 (2001); M. Gonzalez-Garcia et al., Phys. Rev. D 63, 033005 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, Phys. Rev. D 64, 073009 (2001); P. Krastev and A. Smirnov, Phys. Rev. D 65, 073022 (2002); J. N. Bahcall, M. C. Gonzalez-Garcia, and C. Peña-Garay, hep-ph/0111150; M. Maltoni, T. Schwetz, and J. W. F. Valle, Phys. Rev. D 65, 093004 (2002). Recent discussions of flux calculations are found in J. Bahcall, Phys. Rep. 333, 47 (2000), hep-ph/0009044, Proceedings of Neutrino-2000, and http://www.sns.ias. edu/-jnb/; V. Barger, D. Marfatia, and K. Whisnant, Phys. Rev. Lett. 88, 011302 (2002); Phys. Lett. B 509, 19 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, hep-ph/0204253. Super Kamiokande data are reported and analyzed in SuperKamiokande Collaboration, Y. Fukuda et al., Phys. Rev. Lett. 82, 1810 (1999); S. Fukuda et al., Phys. Rev. Lett. 86, 5651 (2001). For recent reviews, see, e.g., Y. Suzuki, Nucl. Phys. B, Proc. Suppl. 91, 29 (2001); Y. Takeuchi, in Proceedings of the International Conference on High Energy Physics, Osaka, http://ichep2000.hep.sci.osaka-u.ac.jp; Proceedings of the Fifth Topical Workshop at the Gran Sasso National Laboratory: Solar Neutrinos, Assergi, Italy, 2001 (to be published). [35] L. Wolfenstein, Phys. Rev. D 17, 2369 (1978). [36] V. Barger, K. Whisnant, S. Pakvasa, and R. J. N. Phillips, Phys. Rev. D 22, 2718 (1980). [37] V. Barger et al., Phys. Rev. D 22, 1636 (1980). [38] S. P. Mikheyev and A. Smirnov, Yad. Fiz. 42, 1441 (1985) [Sov. J. Nucl. Phys. 42, 913 (1986)]; Nuovo Cimento Soc. Ital. Fis., C 9, 17 (1986); S. P. Rosen and J. Gelb, Phys. Rev. D 34, 969 (1986); S. Parke, Phys. Rev. Lett. 57, 1275 (1986); W. Haxton, Phys. Rev. Lett. 57, 1271 (1986); T. K. Kuo and J. Pantaleone, Rev. Mod. Phys. 61, 937 (1989).
57. Fits and references to the Homestake, Kamiokande, GALLEX, SAGE, Super Kamiokande, and SNO data include N. Hata and P. Langacker, Phys. Rev. D 56, 6107 (1997); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 58, 096016 (1998); J. Bahcall and P. Krastev, Phys. Lett. B 436, 243 (1998); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 60, 093001 (1999); hep-ph/0103179; M. Gonzalez-Garcia, C. Peña-Garay, and J. W. F. Valle, Phys. Rev. D 63, 013007 (2001); M. Gonzalez-Garcia et al., Phys. Rev. D 63, 033005 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, Phys. Rev. D 64, 073009 (2001); P. Krastev and A. Smirnov, Phys. Rev. D 65, 073022 (2002); J. N. Bahcall, M. C. Gonzalez-Garcia, and C. Peña-Garay, hep-ph/0111150; M. Maltoni, T. Schwetz, and J. W. F. Valle, Phys. Rev. D 65, 093004 (2002). Recent discussions of flux calculations are found in J. Bahcall, Phys. Rep. 333, 47 (2000), hep-ph/0009044, Proceedings of Neutrino-2000, and http://www.sns.ias. edu/-jnb/; V. Barger, D. Marfatia, and K. Whisnant, Phys. Rev. Lett. 88, 011302 (2002); Phys. Lett. B 509, 19 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, hep-ph/0204253. Super Kamiokande data are reported and analyzed in SuperKamiokande Collaboration, Y. Fukuda et al., Phys. Rev. Lett. 82, 1810 (1999); S. Fukuda et al., Phys. Rev. Lett. 86, 5651 (2001). For recent reviews, see, e.g., Y. Suzuki, Nucl. Phys. B, Proc. Suppl. 91, 29 (2001); Y. Takeuchi, in Proceedings of the International Conference on High Energy Physics, Osaka, http://ichep2000.hep.sci.osaka-u.ac.jp; Proceedings of the Fifth Topical Workshop at the Gran Sasso National Laboratory: Solar Neutrinos, Assergi, Italy, 2001 (to be published). [35] L. Wolfenstein, Phys. Rev. D 17, 2369 (1978). [36] V. Barger, K. Whisnant, S. Pakvasa, and R. J. N. Phillips, Phys. Rev. D 22, 2718 (1980). [37] V. Barger et al., Phys. Rev. D 22, 1636 (1980). [38] S. P. Mikheyev and A. Smirnov, Yad. Fiz. 42, 1441 (1985) [Sov. J. Nucl. Phys. 42, 913 (1986)]; Nuovo Cimento Soc. Ital. Fis., C 9, 17 (1986); S. P. Rosen and J. Gelb, Phys. Rev. D 34, 969 (1986); S. Parke, Phys. Rev. Lett. 57, 1275 (1986); W. Haxton, Phys. Rev. Lett. 57, 1271 (1986); T. K. Kuo and J. Pantaleone, Rev. Mod. Phys. 61, 937 (1989).
58. Fits and references to the Homestake, Kamiokande, GALLEX, SAGE, Super Kamiokande, and SNO data include N. Hata and P. Langacker, Phys. Rev. D 56, 6107 (1997); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 58, 096016 (1998); J. Bahcall and P. Krastev, Phys. Lett. B 436, 243 (1998); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 60, 093001 (1999); hep-ph/0103179; M. Gonzalez-Garcia, C. Peña-Garay, and J. W. F. Valle, Phys. Rev. D 63, 013007 (2001); M. Gonzalez-Garcia et al., Phys. Rev. D 63, 033005 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, Phys. Rev. D 64, 073009 (2001); P. Krastev and A. Smirnov, Phys. Rev. D 65, 073022 (2002); J. N. Bahcall, M. C. Gonzalez-Garcia, and C. Peña-Garay, hep-ph/0111150; M. Maltoni, T. Schwetz, and J. W. F. Valle, Phys. Rev. D 65, 093004 (2002). Recent discussions of flux calculations are found in J. Bahcall, Phys. Rep. 333, 47 (2000), hep-ph/0009044, Proceedings of Neutrino-2000, and http://www.sns.ias. edu/-jnb/; V. Barger, D. Marfatia, and K. Whisnant, Phys. Rev. Lett. 88, 011302 (2002); Phys. Lett. B 509, 19 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, hep-ph/0204253. Super Kamiokande data are reported and analyzed in SuperKamiokande Collaboration, Y. Fukuda et al., Phys. Rev. Lett. 82, 1810 (1999); S. Fukuda et al., Phys. Rev. Lett. 86, 5651 (2001). For recent reviews, see, e.g., Y. Suzuki, Nucl. Phys. B, Proc. Suppl. 91, 29 (2001); Y. Takeuchi, in Proceedings of the International Conference on High Energy Physics, Osaka, http://ichep2000.hep.sci.osaka-u.ac.jp; Proceedings of the Fifth Topical Workshop at the Gran Sasso National Laboratory: Solar Neutrinos, Assergi, Italy, 2001 (to be published). [35] L. Wolfenstein, Phys. Rev. D 17, 2369 (1978). [36] V. Barger, K. Whisnant, S. Pakvasa, and R. J. N. Phillips, Phys. Rev. D 22, 2718 (1980). [37] V. Barger et al., Phys. Rev. D 22, 1636 (1980). [38] S. P. Mikheyev and A. Smirnov, Yad. Fiz. 42, 1441 (1985) [Sov. J. Nucl. Phys. 42, 913 (1986)]; Nuovo Cimento Soc. Ital. Fis., C 9, 17 (1986); S. P. Rosen and J. Gelb, Phys. Rev. D 34, 969 (1986); S. Parke, Phys. Rev. Lett. 57, 1275 (1986); W. Haxton, Phys. Rev. Lett. 57, 1271 (1986); T. K. Kuo and J. Pantaleone, Rev. Mod. Phys. 61, 937 (1989).
59. Fits and references to the Homestake, Kamiokande, GALLEX, SAGE, Super Kamiokande, and SNO data include N. Hata and P. Langacker, Phys. Rev. D 56, 6107 (1997); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 58, 096016 (1998); J. Bahcall and P. Krastev, Phys. Lett. B 436, 243 (1998); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 60, 093001 (1999); hep-ph/0103179; M. Gonzalez-Garcia, C. Peña-Garay, and J. W. F. Valle, Phys. Rev. D 63, 013007 (2001); M. Gonzalez-Garcia et al., Phys. Rev. D 63, 033005 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, Phys. Rev. D 64, 073009 (2001); P. Krastev and A. Smirnov, Phys. Rev. D 65, 073022 (2002); J. N. Bahcall, M. C. Gonzalez-Garcia, and C. Peña-Garay, hep-ph/0111150; M. Maltoni, T. Schwetz, and J. W. F. Valle, Phys. Rev. D 65, 093004 (2002). Recent discussions of flux calculations are found in J. Bahcall, Phys. Rep. 333, 47 (2000), hep-ph/0009044, Proceedings of Neutrino-2000, and http://www.sns.ias. edu/-jnb/; V. Barger, D. Marfatia, and K. Whisnant, Phys. Rev. Lett. 88, 011302 (2002); Phys. Lett. B 509, 19 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, hep-ph/0204253. Super Kamiokande data are reported and analyzed in SuperKamiokande Collaboration, Y. Fukuda et al., Phys. Rev. Lett. 82, 1810 (1999); S. Fukuda et al., Phys. Rev. Lett. 86, 5651 (2001). For recent reviews, see, e.g., Y. Suzuki, Nucl. Phys. B, Proc. Suppl. 91, 29 (2001); Y. Takeuchi, in Proceedings of the International Conference on High Energy Physics, Osaka, http://ichep2000.hep.sci.osaka-u.ac.jp; Proceedings of the Fifth Topical Workshop at the Gran Sasso National Laboratory: Solar Neutrinos, Assergi, Italy, 2001 (to be published). [35] L. Wolfenstein, Phys. Rev. D 17, 2369 (1978). [36] V. Barger, K. Whisnant, S. Pakvasa, and R. J. N. Phillips, Phys. Rev. D 22, 2718 (1980). [37] V. Barger et al., Phys. Rev. D 22, 1636 (1980). [38] S. P. Mikheyev and A. Smirnov, Yad. Fiz. 42, 1441 (1985) [Sov. J. Nucl. Phys. 42, 913 (1986)]; Nuovo Cimento Soc. Ital. Fis., C 9, 17 (1986); S. P. Rosen and J. Gelb, Phys. Rev. D 34, 969 (1986); S. Parke, Phys. Rev. Lett. 57, 1275 (1986); W. Haxton, Phys. Rev. Lett. 57, 1271 (1986); T. K. Kuo and J. Pantaleone, Rev. Mod. Phys. 61, 937 (1989).
60. Fits and references to the Homestake, Kamiokande, GALLEX, SAGE, Super Kamiokande, and SNO data include N. Hata and P. Langacker, Phys. Rev. D 56, 6107 (1997); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 58, 096016 (1998); J. Bahcall and P. Krastev, Phys. Lett. B 436, 243 (1998); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 60, 093001 (1999); hep-ph/0103179; M. Gonzalez-Garcia, C. Peña-Garay, and J. W. F. Valle, Phys. Rev. D 63, 013007 (2001); M. Gonzalez-Garcia et al., Phys. Rev. D 63, 033005 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, Phys. Rev. D 64, 073009 (2001); P. Krastev and A. Smirnov, Phys. Rev. D 65, 073022 (2002); J. N. Bahcall, M. C. Gonzalez-Garcia, and C. Peña-Garay, hep-ph/0111150; M. Maltoni, T. Schwetz, and J. W. F. Valle, Phys. Rev. D 65, 093004 (2002). Recent discussions of flux calculations are found in J. Bahcall, Phys. Rep. 333, 47 (2000), hep-ph/0009044, Proceedings of Neutrino-2000, and http://www.sns.ias. edu/-jnb/; V. Barger, D. Marfatia, and K. Whisnant, Phys. Rev. Lett. 88, 011302 (2002); Phys. Lett. B 509, 19 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, hep-ph/0204253. Super Kamiokande data are reported and analyzed in SuperKamiokande Collaboration, Y. Fukuda et al., Phys. Rev. Lett. 82, 1810 (1999); S. Fukuda et al., Phys. Rev. Lett. 86, 5651 (2001). For recent reviews, see, e.g., Y. Suzuki, Nucl. Phys. B, Proc. Suppl. 91, 29 (2001); Y. Takeuchi, in Proceedings of the International Conference on High Energy Physics, Osaka, http://ichep2000.hep.sci.osaka-u.ac.jp; Proceedings of the Fifth Topical Workshop at the Gran Sasso National Laboratory: Solar Neutrinos, Assergi, Italy, 2001 (to be published). [35] L. Wolfenstein, Phys. Rev. D 17, 2369 (1978). [36] V. Barger, K. Whisnant, S. Pakvasa, and R. J. N. Phillips, Phys. Rev. D 22, 2718 (1980). [37] V. Barger et al., Phys. Rev. D 22, 1636 (1980). [38] S. P. Mikheyev and A. Smirnov, Yad. Fiz. 42, 1441 (1985) [Sov. J. Nucl. Phys. 42, 913 (1986)]; Nuovo Cimento Soc. Ital. Fis., C 9, 17 (1986); S. P. Rosen and J. Gelb, Phys. Rev. D 34, 969 (1986); S. Parke, Phys. Rev. Lett. 57, 1275 (1986); W. Haxton, Phys. Rev. Lett. 57, 1271 (1986); T. K. Kuo and J. Pantaleone, Rev. Mod. Phys. 61, 937 (1989).
61. Fits and references to the Homestake, Kamiokande, GALLEX, SAGE, Super Kamiokande, and SNO data include N. Hata and P. Langacker, Phys. Rev. D 56, 6107 (1997); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 58, 096016 (1998); J. Bahcall and P. Krastev, Phys. Lett. B 436, 243 (1998); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 60, 093001 (1999); hep-ph/0103179; M. Gonzalez-Garcia, C. Peña-Garay, and J. W. F. Valle, Phys. Rev. D 63, 013007 (2001); M. Gonzalez-Garcia et al., Phys. Rev. D 63, 033005 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, Phys. Rev. D 64, 073009 (2001); P. Krastev and A. Smirnov, Phys. Rev. D 65, 073022 (2002); J. N. Bahcall, M. C. Gonzalez-Garcia, and C. Peña-Garay, hep-ph/0111150; M. Maltoni, T. Schwetz, and J. W. F. Valle, Phys. Rev. D 65, 093004 (2002). Recent discussions of flux calculations are found in J. Bahcall, Phys. Rep. 333, 47 (2000), hep-ph/0009044, Proceedings of Neutrino-2000, and http://www.sns.ias. edu/-jnb/; V. Barger, D. Marfatia, and K. Whisnant, Phys. Rev. Lett. 88, 011302 (2002); Phys. Lett. B 509, 19 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, hep-ph/0204253. Super Kamiokande data are reported and analyzed in SuperKamiokande Collaboration, Y. Fukuda et al., Phys. Rev. Lett. 82, 1810 (1999); S. Fukuda et al., Phys. Rev. Lett. 86, 5651 (2001). For recent reviews, see, e.g., Y. Suzuki, Nucl. Phys. B, Proc. Suppl. 91, 29 (2001); Y. Takeuchi, in Proceedings of the International Conference on High Energy Physics, Osaka, http://ichep2000.hep.sci.osaka-u.ac.jp; Proceedings of the Fifth Topical Workshop at the Gran Sasso National Laboratory: Solar Neutrinos, Assergi, Italy, 2001 (to be published). [35] L. Wolfenstein, Phys. Rev. D 17, 2369 (1978). [36] V. Barger, K. Whisnant, S. Pakvasa, and R. J. N. Phillips, Phys. Rev. D 22, 2718 (1980). [37] V. Barger et al., Phys. Rev. D 22, 1636 (1980). [38] S. P. Mikheyev and A. Smirnov, Yad. Fiz. 42, 1441 (1985) [Sov. J. Nucl. Phys. 42, 913 (1986)]; Nuovo Cimento Soc. Ital. Fis., C 9, 17 (1986); S. P. Rosen and J. Gelb, Phys. Rev. D 34, 969 (1986); S. Parke, Phys. Rev. Lett. 57, 1275 (1986); W. Haxton, Phys. Rev. Lett. 57, 1271 (1986); T. K. Kuo and J. Pantaleone, Rev. Mod. Phys. 61, 937 (1989).
62. Fits and references to the Homestake, Kamiokande, GALLEX, SAGE, Super Kamiokande, and SNO data include N. Hata and P. Langacker, Phys. Rev. D 56, 6107 (1997); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 58, 096016 (1998); J. Bahcall and P. Krastev, Phys. Lett. B 436, 243 (1998); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 60, 093001 (1999); hep-ph/0103179; M. Gonzalez-Garcia, C. Peña-Garay, and J. W. F. Valle, Phys. Rev. D 63, 013007 (2001); M. Gonzalez-Garcia et al., Phys. Rev. D 63, 033005 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, Phys. Rev. D 64, 073009 (2001); P. Krastev and A. Smirnov, Phys. Rev. D 65, 073022 (2002); J. N. Bahcall, M. C. Gonzalez-Garcia, and C. Peña-Garay, hep-ph/0111150; M. Maltoni, T. Schwetz, and J. W. F. Valle, Phys. Rev. D 65, 093004 (2002). Recent discussions of flux calculations are found in J. Bahcall, Phys. Rep. 333, 47 (2000), hep-ph/0009044, Proceedings of Neutrino-2000, and http://www.sns.ias. edu/-jnb/; V. Barger, D. Marfatia, and K. Whisnant, Phys. Rev. Lett. 88, 011302 (2002); Phys. Lett. B 509, 19 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, hep-ph/0204253. Super Kamiokande data are reported and analyzed in SuperKamiokande Collaboration, Y. Fukuda et al., Phys. Rev. Lett. 82, 1810 (1999); S. Fukuda et al., Phys. Rev. Lett. 86, 5651 (2001). For recent reviews, see, e.g., Y. Suzuki, Nucl. Phys. B, Proc. Suppl. 91, 29 (2001); Y. Takeuchi, in Proceedings of the International Conference on High Energy Physics, Osaka, http://ichep2000.hep.sci.osaka-u.ac.jp; Proceedings of the Fifth Topical Workshop at the Gran Sasso National Laboratory: Solar Neutrinos, Assergi, Italy, 2001 (to be published). [35] L. Wolfenstein, Phys. Rev. D 17, 2369 (1978). [36] V. Barger, K. Whisnant, S. Pakvasa, and R. J. N. Phillips, Phys. Rev. D 22, 2718 (1980). [37] V. Barger et al., Phys. Rev. D 22, 1636 (1980). [38] S. P. Mikheyev and A. Smirnov, Yad. Fiz. 42, 1441 (1985) [Sov. J. Nucl. Phys. 42, 913 (1986)]; Nuovo Cimento Soc. Ital. Fis., C 9, 17 (1986); S. P. Rosen and J. Gelb, Phys. Rev. D 34, 969 (1986); S. Parke, Phys. Rev. Lett. 57, 1275 (1986); W. Haxton, Phys. Rev. Lett. 57, 1271 (1986); T. K. Kuo and J. Pantaleone, Rev. Mod. Phys. 61, 937 (1989).
63. Fits and references to the Homestake, Kamiokande, GALLEX, SAGE, Super Kamiokande, and SNO data include N. Hata and P. Langacker, Phys. Rev. D 56, 6107 (1997); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 58, 096016 (1998); J. Bahcall and P. Krastev, Phys. Lett. B 436, 243 (1998); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 60, 093001 (1999); hep-ph/0103179; M. Gonzalez-Garcia, C. Peña-Garay, and J. W. F. Valle, Phys. Rev. D 63, 013007 (2001); M. Gonzalez-Garcia et al., Phys. Rev. D 63, 033005 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, Phys. Rev. D 64, 073009 (2001); P. Krastev and A. Smirnov, Phys. Rev. D 65, 073022 (2002); J. N. Bahcall, M. C. Gonzalez-Garcia, and C. Peña-Garay, hep-ph/0111150; M. Maltoni, T. Schwetz, and J. W. F. Valle, Phys. Rev. D 65, 093004 (2002). Recent discussions of flux calculations are found in J. Bahcall, Phys. Rep. 333, 47 (2000), hep-ph/0009044, Proceedings of Neutrino-2000, and http://www.sns.ias. edu/-jnb/; V. Barger, D. Marfatia, and K. Whisnant, Phys. Rev. Lett. 88, 011302 (2002); Phys. Lett. B 509, 19 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, hep-ph/0204253. Super Kamiokande data are reported and analyzed in SuperKamiokande Collaboration, Y. Fukuda et al., Phys. Rev. Lett. 82, 1810 (1999); S. Fukuda et al., Phys. Rev. Lett. 86, 5651 (2001). For recent reviews, see, e.g., Y. Suzuki, Nucl. Phys. B, Proc. Suppl. 91, 29 (2001); Y. Takeuchi, in Proceedings of the International Conference on High Energy Physics, Osaka, http://ichep2000.hep.sci.osaka-u.ac.jp; Proceedings of the Fifth Topical Workshop at the Gran Sasso National Laboratory: Solar Neutrinos, Assergi, Italy, 2001 (to be published). [35] L. Wolfenstein, Phys. Rev. D 17, 2369 (1978). [36] V. Barger, K. Whisnant, S. Pakvasa, and R. J. N. Phillips, Phys. Rev. D 22, 2718 (1980). [37] V. Barger et al., Phys. Rev. D 22, 1636 (1980). [38] S. P. Mikheyev and A. Smirnov, Yad. Fiz. 42, 1441 (1985) [Sov. J. Nucl. Phys. 42, 913 (1986)]; Nuovo Cimento Soc. Ital. Fis., C 9, 17 (1986); S. P. Rosen and J. Gelb, Phys. Rev. D 34, 969 (1986); S. Parke, Phys. Rev. Lett. 57, 1275 (1986); W. Haxton, Phys. Rev. Lett. 57, 1271 (1986); T. K. Kuo and J. Pantaleone, Rev. Mod. Phys. 61, 937 (1989).
64. Fits and references to the Homestake, Kamiokande, GALLEX, SAGE, Super Kamiokande, and SNO data include N. Hata and P. Langacker, Phys. Rev. D 56, 6107 (1997); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 58, 096016 (1998); J. Bahcall and P. Krastev, Phys. Lett. B 436, 243 (1998); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 60, 093001 (1999); hep-ph/0103179; M. Gonzalez-Garcia, C. Peña-Garay, and J. W. F. Valle, Phys. Rev. D 63, 013007 (2001); M. Gonzalez-Garcia et al., Phys. Rev. D 63, 033005 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, Phys. Rev. D 64, 073009 (2001); P. Krastev and A. Smirnov, Phys. Rev. D 65, 073022 (2002); J. N. Bahcall, M. C. Gonzalez-Garcia, and C. Peña-Garay, hep-ph/0111150; M. Maltoni, T. Schwetz, and J. W. F. Valle, Phys. Rev. D 65, 093004 (2002). Recent discussions of flux calculations are found in J. Bahcall, Phys. Rep. 333, 47 (2000), hep-ph/0009044, Proceedings of Neutrino-2000, and http://www.sns.ias. edu/-jnb/; V. Barger, D. Marfatia, and K. Whisnant, Phys. Rev. Lett. 88, 011302 (2002); Phys. Lett. B 509, 19 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, hep-ph/0204253. Super Kamiokande data are reported and analyzed in SuperKamiokande Collaboration, Y. Fukuda et al., Phys. Rev. Lett. 82, 1810 (1999); S. Fukuda et al., Phys. Rev. Lett. 86, 5651 (2001). For recent reviews, see, e.g., Y. Suzuki, Nucl. Phys. B, Proc. Suppl. 91, 29 (2001); Y. Takeuchi, in Proceedings of the International Conference on High Energy Physics, Osaka, http://ichep2000.hep.sci.osaka-u.ac.jp; Proceedings of the Fifth Topical Workshop at the Gran Sasso National Laboratory: Solar Neutrinos, Assergi, Italy, 2001 (to be published). [35] L. Wolfenstein, Phys. Rev. D 17, 2369 (1978). [36] V. Barger, K. Whisnant, S. Pakvasa, and R. J. N. Phillips, Phys. Rev. D 22, 2718 (1980). [37] V. Barger et al., Phys. Rev. D 22, 1636 (1980). [38] S. P. Mikheyev and A. Smirnov, Yad. Fiz. 42, 1441 (1985) [Sov. J. Nucl. Phys. 42, 913 (1986)]; Nuovo Cimento Soc. Ital. Fis., C 9, 17 (1986); S. P. Rosen and J. Gelb, Phys. Rev. D 34, 969 (1986); S. Parke, Phys. Rev. Lett. 57, 1275 (1986); W. Haxton, Phys. Rev. Lett. 57, 1271 (1986); T. K. Kuo and J. Pantaleone, Rev. Mod. Phys. 61, 937 (1989).
65. Fits and references to the Homestake, Kamiokande, GALLEX, SAGE, Super Kamiokande, and SNO data include N. Hata and P. Langacker, Phys. Rev. D 56, 6107 (1997); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 58, 096016 (1998); J. Bahcall and P. Krastev, Phys. Lett. B 436, 243 (1998); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 60, 093001 (1999); hep-ph/0103179; M. Gonzalez-Garcia, C. Peña-Garay, and J. W. F. Valle, Phys. Rev. D 63, 013007 (2001); M. Gonzalez-Garcia et al., Phys. Rev. D 63, 033005 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, Phys. Rev. D 64, 073009 (2001); P. Krastev and A. Smirnov, Phys. Rev. D 65, 073022 (2002); J. N. Bahcall, M. C. Gonzalez-Garcia, and C. Peña-Garay, hep-ph/0111150; M. Maltoni, T. Schwetz, and J. W. F. Valle, Phys. Rev. D 65, 093004 (2002). Recent discussions of flux calculations are found in J. Bahcall, Phys. Rep. 333, 47 (2000), hep-ph/0009044, Proceedings of Neutrino-2000, and http://www.sns.ias. edu/-jnb/; V. Barger, D. Marfatia, and K. Whisnant, Phys. Rev. Lett. 88, 011302 (2002); Phys. Lett. B 509, 19 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, hep-ph/0204253. Super Kamiokande data are reported and analyzed in SuperKamiokande Collaboration, Y. Fukuda et al., Phys. Rev. Lett. 82, 1810 (1999); S. Fukuda et al., Phys. Rev. Lett. 86, 5651 (2001). For recent reviews, see, e.g., Y. Suzuki, Nucl. Phys. B, Proc. Suppl. 91, 29 (2001); Y. Takeuchi, in Proceedings of the International Conference on High Energy Physics, Osaka, http://ichep2000.hep.sci.osaka-u.ac.jp; Proceedings of the Fifth Topical Workshop at the Gran Sasso National Laboratory: Solar Neutrinos, Assergi, Italy, 2001 (to be published). [35] L. Wolfenstein, Phys. Rev. D 17, 2369 (1978). [36] V. Barger, K. Whisnant, S. Pakvasa, and R. J. N. Phillips, Phys. Rev. D 22, 2718 (1980). [37] V. Barger et al., Phys. Rev. D 22, 1636 (1980). [38] S. P. Mikheyev and A. Smirnov, Yad. Fiz. 42, 1441 (1985) [Sov. J. Nucl. Phys. 42, 913 (1986)]; Nuovo Cimento Soc. Ital. Fis., C 9, 17 (1986); S. P. Rosen and J. Gelb, Phys. Rev. D 34, 969 (1986); S. Parke, Phys. Rev. Lett. 57, 1275 (1986); W. Haxton, Phys. Rev. Lett. 57, 1271 (1986); T. K. Kuo and J. Pantaleone, Rev. Mod. Phys. 61, 937 (1989).
66. Fits and references to the Homestake, Kamiokande, GALLEX, SAGE, Super Kamiokande, and SNO data include N. Hata and P. Langacker, Phys. Rev. D 56, 6107 (1997); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 58, 096016 (1998); J. Bahcall and P. Krastev, Phys. Lett. B 436, 243 (1998); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 60, 093001 (1999); hep-ph/0103179; M. Gonzalez-Garcia, C. Peña-Garay, and J. W. F. Valle, Phys. Rev. D 63, 013007 (2001); M. Gonzalez-Garcia et al., Phys. Rev. D 63, 033005 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, Phys. Rev. D 64, 073009 (2001); P. Krastev and A. Smirnov, Phys. Rev. D 65, 073022 (2002); J. N. Bahcall, M. C. Gonzalez-Garcia, and C. Peña-Garay, hep-ph/0111150; M. Maltoni, T. Schwetz, and J. W. F. Valle, Phys. Rev. D 65, 093004 (2002). Recent discussions of flux calculations are found in J. Bahcall, Phys. Rep. 333, 47 (2000), hep-ph/0009044, Proceedings of Neutrino-2000, and http://www.sns.ias. edu/-jnb/; V. Barger, D. Marfatia, and K. Whisnant, Phys. Rev. Lett. 88, 011302 (2002); Phys. Lett. B 509, 19 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, hep-ph/0204253. Super Kamiokande data are reported and analyzed in SuperKamiokande Collaboration, Y. Fukuda et al., Phys. Rev. Lett. 82, 1810 (1999); S. Fukuda et al., Phys. Rev. Lett. 86, 5651 (2001). For recent reviews, see, e.g., Y. Suzuki, Nucl. Phys. B, Proc. Suppl. 91, 29 (2001); Y. Takeuchi, in Proceedings of the International Conference on High Energy Physics, Osaka, http://ichep2000.hep.sci.osaka-u.ac.jp; Proceedings of the Fifth Topical Workshop at the Gran Sasso National Laboratory: Solar Neutrinos, Assergi, Italy, 2001 (to be published). [35] L. Wolfenstein, Phys. Rev. D 17, 2369 (1978). [36] V. Barger, K. Whisnant, S. Pakvasa, and R. J. N. Phillips, Phys. Rev. D 22, 2718 (1980). [37] V. Barger et al., Phys. Rev. D 22, 1636 (1980). [38] S. P. Mikheyev and A. Smirnov, Yad. Fiz. 42, 1441 (1985) [Sov. J. Nucl. Phys. 42, 913 (1986)]; Nuovo Cimento Soc. Ital. Fis., C 9, 17 (1986); S. P. Rosen and J. Gelb, Phys. Rev. D 34, 969 (1986); S. Parke, Phys. Rev. Lett. 57, 1275 (1986); W. Haxton, Phys. Rev. Lett. 57, 1271 (1986); T. K. Kuo and J. Pantaleone, Rev. Mod. Phys. 61, 937 (1989).
67. Fits and references to the Homestake, Kamiokande, GALLEX, SAGE, Super Kamiokande, and SNO data include N. Hata and P. Langacker, Phys. Rev. D 56, 6107 (1997); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 58, 096016 (1998); J. Bahcall and P. Krastev, Phys. Lett. B 436, 243 (1998); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 60, 093001 (1999); hep-ph/0103179; M. Gonzalez-Garcia, C. Peña-Garay, and J. W. F. Valle, Phys. Rev. D 63, 013007 (2001); M. Gonzalez-Garcia et al., Phys. Rev. D 63, 033005 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, Phys. Rev. D 64, 073009 (2001); P. Krastev and A. Smirnov, Phys. Rev. D 65, 073022 (2002); J. N. Bahcall, M. C. Gonzalez-Garcia, and C. Peña-Garay, hep-ph/0111150; M. Maltoni, T. Schwetz, and J. W. F. Valle, Phys. Rev. D 65, 093004 (2002). Recent discussions of flux calculations are found in J. Bahcall, Phys. Rep. 333, 47 (2000), hep-ph/0009044, Proceedings of Neutrino-2000, and http://www.sns.ias. edu/-jnb/; V. Barger, D. Marfatia, and K. Whisnant, Phys. Rev. Lett. 88, 011302 (2002); Phys. Lett. B 509, 19 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, hep-ph/0204253. Super Kamiokande data are reported and analyzed in SuperKamiokande Collaboration, Y. Fukuda et al., Phys. Rev. Lett. 82, 1810 (1999); S. Fukuda et al., Phys. Rev. Lett. 86, 5651 (2001). For recent reviews, see, e.g., Y. Suzuki, Nucl. Phys. B, Proc. Suppl. 91, 29 (2001); Y. Takeuchi, in Proceedings of the International Conference on High Energy Physics, Osaka, http://ichep2000.hep.sci.osaka-u.ac.jp; Proceedings of the Fifth Topical Workshop at the Gran Sasso National Laboratory: Solar Neutrinos, Assergi, Italy, 2001 (to be published). [35] L. Wolfenstein, Phys. Rev. D 17, 2369 (1978). [36] V. Barger, K. Whisnant, S. Pakvasa, and R. J. N. Phillips, Phys. Rev. D 22, 2718 (1980). [37] V. Barger et al., Phys. Rev. D 22, 1636 (1980). [38] S. P. Mikheyev and A. Smirnov, Yad. Fiz. 42, 1441 (1985) [Sov. J. Nucl. Phys. 42, 913 (1986)]; Nuovo Cimento Soc. Ital. Fis., C 9, 17 (1986); S. P. Rosen and J. Gelb, Phys. Rev. D 34, 969 (1986); S. Parke, Phys. Rev. Lett. 57, 1275 (1986); W. Haxton, Phys. Rev. Lett. 57, 1271 (1986); T. K. Kuo and J. Pantaleone, Rev. Mod. Phys. 61, 937 (1989).
68. Fits and references to the Homestake, Kamiokande, GALLEX, SAGE, Super Kamiokande, and SNO data include N. Hata and P. Langacker, Phys. Rev. D 56, 6107 (1997); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 58, 096016 (1998); J. Bahcall and P. Krastev, Phys. Lett. B 436, 243 (1998); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 60, 093001 (1999); hep-ph/0103179; M. Gonzalez-Garcia, C. Peña-Garay, and J. W. F. Valle, Phys. Rev. D 63, 013007 (2001); M. Gonzalez-Garcia et al., Phys. Rev. D 63, 033005 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, Phys. Rev. D 64, 073009 (2001); P. Krastev and A. Smirnov, Phys. Rev. D 65, 073022 (2002); J. N. Bahcall, M. C. Gonzalez-Garcia, and C. Peña-Garay, hep-ph/0111150; M. Maltoni, T. Schwetz, and J. W. F. Valle, Phys. Rev. D 65, 093004 (2002). Recent discussions of flux calculations are found in J. Bahcall, Phys. Rep. 333, 47 (2000), hep-ph/0009044, Proceedings of Neutrino-2000, and http://www.sns.ias. edu/-jnb/; V. Barger, D. Marfatia, and K. Whisnant, Phys. Rev. Lett. 88, 011302 (2002); Phys. Lett. B 509, 19 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, hep-ph/0204253. Super Kamiokande data are reported and analyzed in SuperKamiokande Collaboration, Y. Fukuda et al., Phys. Rev. Lett. 82, 1810 (1999); S. Fukuda et al., Phys. Rev. Lett. 86, 5651 (2001). For recent reviews, see, e.g., Y. Suzuki, Nucl. Phys. B, Proc. Suppl. 91, 29 (2001); Y. Takeuchi, in Proceedings of the International Conference on High Energy Physics, Osaka, http://ichep2000.hep.sci.osaka-u.ac.jp; Proceedings of the Fifth Topical Workshop at the Gran Sasso National Laboratory: Solar Neutrinos, Assergi, Italy, 2001 (to be published). [35] L. Wolfenstein, Phys. Rev. D 17, 2369 (1978). [36] V. Barger, K. Whisnant, S. Pakvasa, and R. J. N. Phillips, Phys. Rev. D 22, 2718 (1980). [37] V. Barger et al., Phys. Rev. D 22, 1636 (1980). [38] S. P. Mikheyev and A. Smirnov, Yad. Fiz. 42, 1441 (1985) [Sov. J. Nucl. Phys. 42, 913 (1986)]; Nuovo Cimento Soc. Ital. Fis., C 9, 17 (1986); S. P. Rosen and J. Gelb, Phys. Rev. D 34, 969 (1986); S. Parke, Phys. Rev. Lett. 57, 1275 (1986); W. Haxton, Phys. Rev. Lett. 57, 1271 (1986); T. K. Kuo and J. Pantaleone, Rev. Mod. Phys. 61, 937 (1989).
69. Fits and references to the Homestake, Kamiokande, GALLEX, SAGE, Super Kamiokande, and SNO data include N. Hata and P. Langacker, Phys. Rev. D 56, 6107 (1997); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 58, 096016 (1998); J. Bahcall and P. Krastev, Phys. Lett. B 436, 243 (1998); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 60, 093001 (1999); hep-ph/0103179; M. Gonzalez-Garcia, C. Peña-Garay, and J. W. F. Valle, Phys. Rev. D 63, 013007 (2001); M. Gonzalez-Garcia et al., Phys. Rev. D 63, 033005 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, Phys. Rev. D 64, 073009 (2001); P. Krastev and A. Smirnov, Phys. Rev. D 65, 073022 (2002); J. N. Bahcall, M. C. Gonzalez-Garcia, and C. Peña-Garay, hep-ph/0111150; M. Maltoni, T. Schwetz, and J. W. F. Valle, Phys. Rev. D 65, 093004 (2002). Recent discussions of flux calculations are found in J. Bahcall, Phys. Rep. 333, 47 (2000), hep-ph/0009044, Proceedings of Neutrino-2000, and http://www.sns.ias. edu/-jnb/; V. Barger, D. Marfatia, and K. Whisnant, Phys. Rev. Lett. 88, 011302 (2002); Phys. Lett. B 509, 19 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, hep-ph/0204253. Super Kamiokande data are reported and analyzed in SuperKamiokande Collaboration, Y. Fukuda et al., Phys. Rev. Lett. 82, 1810 (1999); S. Fukuda et al., Phys. Rev. Lett. 86, 5651 (2001). For recent reviews, see, e.g., Y. Suzuki, Nucl. Phys. B, Proc. Suppl. 91, 29 (2001); Y. Takeuchi, in Proceedings of the International Conference on High Energy Physics, Osaka, http://ichep2000.hep.sci.osaka-u.ac.jp; Proceedings of the Fifth Topical Workshop at the Gran Sasso National Laboratory: Solar Neutrinos, Assergi, Italy, 2001 (to be published). [35] L. Wolfenstein, Phys. Rev. D 17, 2369 (1978). [36] V. Barger, K. Whisnant, S. Pakvasa, and R. J. N. Phillips, Phys. Rev. D 22, 2718 (1980). [37] V. Barger et al., Phys. Rev. D 22, 1636 (1980). [38] S. P. Mikheyev and A. Smirnov, Yad. Fiz. 42, 1441 (1985) [Sov. J. Nucl. Phys. 42, 913 (1986)]; Nuovo Cimento Soc. Ital. Fis., C 9, 17 (1986); S. P. Rosen and J. Gelb, Phys. Rev. D 34, 969 (1986); S. Parke, Phys. Rev. Lett. 57, 1275 (1986); W. Haxton, Phys. Rev. Lett. 57, 1271 (1986); T. K. Kuo and J. Pantaleone, Rev. Mod. Phys. 61, 937 (1989).
70. Fits and references to the Homestake, Kamiokande, GALLEX, SAGE, Super Kamiokande, and SNO data include N. Hata and P. Langacker, Phys. Rev. D 56, 6107 (1997); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 58, 096016 (1998); J. Bahcall and P. Krastev, Phys. Lett. B 436, 243 (1998); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 60, 093001 (1999); hep-ph/0103179; M. Gonzalez-Garcia, C. Peña-Garay, and J. W. F. Valle, Phys. Rev. D 63, 013007 (2001); M. Gonzalez-Garcia et al., Phys. Rev. D 63, 033005 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, Phys. Rev. D 64, 073009 (2001); P. Krastev and A. Smirnov, Phys. Rev. D 65, 073022 (2002); J. N. Bahcall, M. C. Gonzalez-Garcia, and C. Peña-Garay, hep-ph/0111150; M. Maltoni, T. Schwetz, and J. W. F. Valle, Phys. Rev. D 65, 093004 (2002). Recent discussions of flux calculations are found in J. Bahcall, Phys. Rep. 333, 47 (2000), hep-ph/0009044, Proceedings of Neutrino-2000, and http://www.sns.ias. edu/-jnb/; V. Barger, D. Marfatia, and K. Whisnant, Phys. Rev. Lett. 88, 011302 (2002); Phys. Lett. B 509, 19 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, hep-ph/0204253. Super Kamiokande data are reported and analyzed in SuperKamiokande Collaboration, Y. Fukuda et al., Phys. Rev. Lett. 82, 1810 (1999); S. Fukuda et al., Phys. Rev. Lett. 86, 5651 (2001). For recent reviews, see, e.g., Y. Suzuki, Nucl. Phys. B, Proc. Suppl. 91, 29 (2001); Y. Takeuchi, in Proceedings of the International Conference on High Energy Physics, Osaka, http://ichep2000.hep.sci.osaka-u.ac.jp; Proceedings of the Fifth Topical Workshop at the Gran Sasso National Laboratory: Solar Neutrinos, Assergi, Italy, 2001 (to be published). [35] L. Wolfenstein, Phys. Rev. D 17, 2369 (1978). [36] V. Barger, K. Whisnant, S. Pakvasa, and R. J. N. Phillips, Phys. Rev. D 22, 2718 (1980). [37] V. Barger et al., Phys. Rev. D 22, 1636 (1980). [38] S. P. Mikheyev and A. Smirnov, Yad. Fiz. 42, 1441 (1985) [Sov. J. Nucl. Phys. 42, 913 (1986)]; Nuovo Cimento Soc. Ital. Fis., C 9, 17 (1986); S. P. Rosen and J. Gelb, Phys. Rev. D 34, 969 (1986); S. Parke, Phys. Rev. Lett. 57, 1275 (1986); W. Haxton, Phys. Rev. Lett. 57, 1271 (1986); T. K. Kuo and J. Pantaleone, Rev. Mod. Phys. 61, 937 (1989).
71. Fits and references to the Homestake, Kamiokande, GALLEX, SAGE, Super Kamiokande, and SNO data include N. Hata and P. Langacker, Phys. Rev. D 56, 6107 (1997); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 58, 096016 (1998); J. Bahcall and P. Krastev, Phys. Lett. B 436, 243 (1998); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 60, 093001 (1999); hep-ph/0103179; M. Gonzalez-Garcia, C. Peña-Garay, and J. W. F. Valle, Phys. Rev. D 63, 013007 (2001); M. Gonzalez-Garcia et al., Phys. Rev. D 63, 033005 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, Phys. Rev. D 64, 073009 (2001); P. Krastev and A. Smirnov, Phys. Rev. D 65, 073022 (2002); J. N. Bahcall, M. C. Gonzalez-Garcia, and C. Peña-Garay, hep-ph/0111150; M. Maltoni, T. Schwetz, and J. W. F. Valle, Phys. Rev. D 65, 093004 (2002). Recent discussions of flux calculations are found in J. Bahcall, Phys. Rep. 333, 47 (2000), hep-ph/0009044, Proceedings of Neutrino-2000, and http://www.sns.ias. edu/-jnb/; V. Barger, D. Marfatia, and K. Whisnant, Phys. Rev. Lett. 88, 011302 (2002); Phys. Lett. B 509, 19 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, hep-ph/0204253. Super Kamiokande data are reported and analyzed in SuperKamiokande Collaboration, Y. Fukuda et al., Phys. Rev. Lett. 82, 1810 (1999); S. Fukuda et al., Phys. Rev. Lett. 86, 5651 (2001). For recent reviews, see, e.g., Y. Suzuki, Nucl. Phys. B, Proc. Suppl. 91, 29 (2001); Y. Takeuchi, in Proceedings of the International Conference on High Energy Physics, Osaka, http://ichep2000.hep.sci.osaka-u.ac.jp; Proceedings of the Fifth Topical Workshop at the Gran Sasso National Laboratory: Solar Neutrinos, Assergi, Italy, 2001 (to be published). [35] L. Wolfenstein, Phys. Rev. D 17, 2369 (1978). [36] V. Barger, K. Whisnant, S. Pakvasa, and R. J. N. Phillips, Phys. Rev. D 22, 2718 (1980). [37] V. Barger et al., Phys. Rev. D 22, 1636 (1980). [38] S. P. Mikheyev and A. Smirnov, Yad. Fiz. 42, 1441 (1985) [Sov. J. Nucl. Phys. 42, 913 (1986)]; Nuovo Cimento Soc. Ital. Fis., C 9, 17 (1986); S. P. Rosen and J. Gelb, Phys. Rev. D 34, 969 (1986); S. Parke, Phys. Rev. Lett. 57, 1275 (1986); W. Haxton, Phys. Rev. Lett. 57, 1271 (1986); T. K. Kuo and J. Pantaleone, Rev. Mod. Phys. 61, 937 (1989).
72. Fits and references to the Homestake, Kamiokande, GALLEX, SAGE, Super Kamiokande, and SNO data include N. Hata and P. Langacker, Phys. Rev. D 56, 6107 (1997); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 58, 096016 (1998); J. Bahcall and P. Krastev, Phys. Lett. B 436, 243 (1998); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 60, 093001 (1999); hep-ph/0103179; M. Gonzalez-Garcia, C. Peña-Garay, and J. W. F. Valle, Phys. Rev. D 63, 013007 (2001); M. Gonzalez-Garcia et al., Phys. Rev. D 63, 033005 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, Phys. Rev. D 64, 073009 (2001); P. Krastev and A. Smirnov, Phys. Rev. D 65, 073022 (2002); J. N. Bahcall, M. C. Gonzalez-Garcia, and C. Peña-Garay, hep-ph/0111150; M. Maltoni, T. Schwetz, and J. W. F. Valle, Phys. Rev. D 65, 093004 (2002). Recent discussions of flux calculations are found in J. Bahcall, Phys. Rep. 333, 47 (2000), hep-ph/0009044, Proceedings of Neutrino-2000, and http://www.sns.ias. edu/-jnb/; V. Barger, D. Marfatia, and K. Whisnant, Phys. Rev. Lett. 88, 011302 (2002); Phys. Lett. B 509, 19 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, hep-ph/0204253. Super Kamiokande data are reported and analyzed in SuperKamiokande Collaboration, Y. Fukuda et al., Phys. Rev. Lett. 82, 1810 (1999); S. Fukuda et al., Phys. Rev. Lett. 86, 5651 (2001). For recent reviews, see, e.g., Y. Suzuki, Nucl. Phys. B, Proc. Suppl. 91, 29 (2001); Y. Takeuchi, in Proceedings of the International Conference on High Energy Physics, Osaka, http://ichep2000.hep.sci.osaka-u.ac.jp; Proceedings of the Fifth Topical Workshop at the Gran Sasso National Laboratory: Solar Neutrinos, Assergi, Italy, 2001 (to be published). [35] L. Wolfenstein, Phys. Rev. D 17, 2369 (1978). [36]
73. Fits and references to the Homestake, Kamiokande, GALLEX, SAGE, Super Kamiokande, and SNO data include N. Hata and P. Langacker, Phys. Rev. D 56, 6107 (1997); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 58, 096016 (1998); J. Bahcall and P. Krastev, Phys. Lett. B 436, 243 (1998); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 60, 093001 (1999); hep-ph/0103179; M. Gonzalez-Garcia, C. Peña-Garay, and J. W. F. Valle, Phys. Rev. D 63, 013007 (2001); M. Gonzalez-Garcia et al., Phys. Rev. D 63, 033005 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, Phys. Rev. D 64, 073009 (2001); P. Krastev and A. Smirnov, Phys. Rev. D 65, 073022 (2002); J. N. Bahcall, M. C. Gonzalez-Garcia, and C. Peña-Garay, hep-ph/0111150; M. Maltoni, T. Schwetz, and J. W. F. Valle, Phys. Rev. D 65, 093004 (2002). Recent discussions of flux calculations are found in J. Bahcall, Phys. Rep. 333, 47 (2000), hep-ph/0009044, Proceedings of Neutrino-2000, and http://www.sns.ias. edu/-jnb/; V. Barger, D. Marfatia, and K. Whisnant, Phys. Rev. Lett. 88, 011302 (2002); Phys. Lett. B 509, 19 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, hep-ph/0204253. Super Kamiokande data are reported and analyzed in SuperKamiokande Collaboration, Y. Fukuda et al., Phys. Rev. Lett. 82, 1810 (1999); S. Fukuda et al., Phys. Rev. Lett. 86, 5651 (2001). For recent reviews, see, e.g., Y. Suzuki, Nucl. Phys. B, Proc. Suppl. 91, 29 (2001); Y. Takeuchi, in Proceedings of the International Conference on High Energy Physics, Osaka, http://ichep2000.hep.sci.osaka-u.ac.jp; Proceedings of the Fifth Topical Workshop at the Gran Sasso National Laboratory: Solar Neutrinos, Assergi, Italy, 2001 (to be published). [35] L. Wolfenstein, Phys. Rev. D 17, 2369 (1978). [36] V. Barger, K. Whisnant, S. Pakvasa, and R. J. N. Phillips, Phys. Rev. D 22, 2718 (1980). [37] V. Barger et al., Phys. Rev. D 22, 1636 (1980). [38] S. P. Mikheyev and A. Smirnov, Yad. Fiz. 42, 1441 (1985) [Sov. J. Nucl. Phys. 42, 913 (1986)]; Nuovo Cimento Soc. Ital. Fis., C 9, 17 (1986); S. P. Rosen and J. Gelb, Phys. Rev. D 34, 969 (1986); S. Parke, Phys. Rev. Lett. 57, 1275 (1986); W. Haxton, Phys. Rev. Lett. 57, 1271 (1986); T. K. Kuo and J. Pantaleone, Rev. Mod. Phys. 61, 937 (1989).
74. Fits and references to the Homestake, Kamiokande, GALLEX, SAGE, Super Kamiokande, and SNO data include N. Hata and P. Langacker, Phys. Rev. D 56, 6107 (1997); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 58, 096016 (1998); J. Bahcall and P. Krastev, Phys. Lett. B 436, 243 (1998); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 60, 093001 (1999); hep-ph/0103179; M. Gonzalez-Garcia, C. Peña-Garay, and J. W. F. Valle, Phys. Rev. D 63, 013007 (2001); M. Gonzalez-Garcia et al., Phys. Rev. D 63, 033005 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, Phys. Rev. D 64, 073009 (2001); P. Krastev and A. Smirnov, Phys. Rev. D 65, 073022 (2002); J. N. Bahcall, M. C. Gonzalez-Garcia, and C. Peña-Garay, hep-ph/0111150; M. Maltoni, T. Schwetz, and J. W. F. Valle, Phys. Rev. D 65, 093004 (2002). Recent discussions of flux calculations are found in J. Bahcall, Phys. Rep. 333, 47 (2000), hep-ph/0009044, Proceedings of Neutrino-2000, and http://www.sns.ias. edu/-jnb/; V. Barger, D. Marfatia, and K. Whisnant, Phys. Rev. Lett. 88, 011302 (2002); Phys. Lett. B 509, 19 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, hep-ph/0204253. Super Kamiokande data are reported and analyzed in SuperKamiokande Collaboration, Y. Fukuda et al., Phys. Rev. Lett. 82, 1810 (1999); S. Fukuda et al., Phys. Rev. Lett. 86, 5651 (2001). For recent reviews, see, e.g., Y. Suzuki, Nucl. Phys. B, Proc. Suppl. 91, 29 (2001); Y. Takeuchi, in Proceedings of the International Conference on High Energy Physics, Osaka, http://ichep2000.hep.sci.osaka-u.ac.jp; Proceedings of the Fifth Topical Workshop at the Gran Sasso National Laboratory: Solar Neutrinos, Assergi, Italy, 2001 (to be published). [35] L. Wolfenstein, Phys. Rev. D 17, 2369 (1978). [36] V. Barger, K. Whisnant, S. Pakvasa, and R. J. N. Phillips, Phys. Rev. D 22, 2718 (1980). [37] V. Barger et al., Phys. Rev. D 22, 1636 (1980). [38] S. P. Mikheyev and A. Smirnov, Yad. Fiz. 42, 1441 (1985) [Sov. J. Nucl. Phys. 42, 913 (1986)]; Nuovo Cimento Soc. Ital. Fis., C 9, 17 (1986); S. P. Rosen and J. Gelb, Phys. Rev. D 34, 969 (1986); S. Parke, Phys. Rev. Lett. 57, 1275 (1986); W. Haxton, Phys. Rev. Lett. 57, 1271 (1986); T. K. Kuo and J. Pantaleone, Rev. Mod. Phys. 61, 937 (1989).
75. Fits and references to the Homestake, Kamiokande, GALLEX, SAGE, Super Kamiokande, and SNO data include N. Hata and P. Langacker, Phys. Rev. D 56, 6107 (1997); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 58, 096016 (1998); J. Bahcall and P. Krastev, Phys. Lett. B 436, 243 (1998); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 60, 093001 (1999); hep-ph/0103179; M. Gonzalez-Garcia, C. Peña-Garay, and J. W. F. Valle, Phys. Rev. D 63, 013007 (2001); M. Gonzalez-Garcia et al., Phys. Rev. D 63, 033005 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, Phys. Rev. D 64, 073009 (2001); P. Krastev and A. Smirnov, Phys. Rev. D 65, 073022 (2002); J. N. Bahcall, M. C. Gonzalez-Garcia, and C. Peña-Garay, hep-ph/0111150; M. Maltoni, T. Schwetz, and J. W. F. Valle, Phys. Rev. D 65, 093004 (2002). Recent discussions of flux calculations are found in J. Bahcall, Phys. Rep. 333, 47 (2000), hep-ph/0009044, Proceedings of Neutrino-2000, and http://www.sns.ias. edu/-jnb/; V. Barger, D. Marfatia, and K. Whisnant, Phys. Rev. Lett. 88, 011302 (2002); Phys. Lett. B 509, 19 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, hep-ph/0204253. Super Kamiokande data are reported and analyzed in SuperKamiokande Collaboration, Y. Fukuda et al., Phys. Rev. Lett. 82, 1810 (1999); S. Fukuda et al., Phys. Rev. Lett. 86, 5651 (2001). For recent reviews, see, e.g., Y. Suzuki, Nucl. Phys. B, Proc. Suppl. 91, 29 (2001); Y. Takeuchi, in Proceedings of the International Conference on High Energy Physics, Osaka, http://ichep2000.hep.sci.osaka-u.ac.jp; Proceedings of the Fifth Topical Workshop at the Gran Sasso National Laboratory: Solar Neutrinos, Assergi, Italy, 2001 (to be published). [35] L. Wolfenstein, Phys. Rev. D 17, 2369 (1978). [36] V. Barger, K. Whisnant, S. Pakvasa, and R. J. N. Phillips, Phys. Rev. D 22, 2718 (1980). [37] V. Barger et al., Phys. Rev. D 22, 1636 (1980). [38] S. P. Mikheyev and A. Smirnov, Yad. Fiz. 42, 1441 (1985) [Sov. J. Nucl. Phys. 42, 913 (1986)]; Nuovo Cimento Soc. Ital. Fis., C 9, 17 (1986); S. P. Rosen and J. Gelb, Phys. Rev. D 34, 969 (1986); S. Parke, Phys. Rev. Lett. 57, 1275 (1986); W. Haxton, Phys. Rev. Lett. 57, 1271 (1986); T. K. Kuo and J. Pantaleone, Rev. Mod. Phys. 61, 937 (1989).
76. Fits and references to the Homestake, Kamiokande, GALLEX, SAGE, Super Kamiokande, and SNO data include N. Hata and P. Langacker, Phys. Rev. D 56, 6107 (1997); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 58, 096016 (1998); J. Bahcall and P. Krastev, Phys. Lett. B 436, 243 (1998); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 60, 093001 (1999); hep-ph/0103179; M. Gonzalez-Garcia, C. Peña-Garay, and J. W. F. Valle, Phys. Rev. D 63, 013007 (2001); M. Gonzalez-Garcia et al., Phys. Rev. D 63, 033005 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, Phys. Rev. D 64, 073009 (2001); P. Krastev and A. Smirnov, Phys. Rev. D 65, 073022 (2002); J. N. Bahcall, M. C. Gonzalez-Garcia, and C. Peña-Garay, hep-ph/0111150; M. Maltoni, T. Schwetz, and J. W. F. Valle, Phys. Rev. D 65, 093004 (2002). Recent discussions of flux calculations are found in J. Bahcall, Phys. Rep. 333, 47 (2000), hep-ph/0009044, Proceedings of Neutrino-2000, and http://www.sns.ias. edu/-jnb/; V. Barger, D. Marfatia, and K. Whisnant, Phys. Rev. Lett. 88, 011302 (2002); Phys. Lett. B 509, 19 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, hep-ph/0204253. Super Kamiokande data are reported and analyzed in SuperKamiokande Collaboration, Y. Fukuda et al., Phys. Rev. Lett. 82, 1810 (1999); S. Fukuda et al., Phys. Rev. Lett. 86, 5651 (2001). For recent reviews, see, e.g., Y. Suzuki, Nucl. Phys. B, Proc. Suppl. 91, 29 (2001); Y. Takeuchi, in Proceedings of the International Conference on High Energy Physics, Osaka, http://ichep2000.hep.sci.osaka-u.ac.jp; Proceedings of the Fifth Topical Workshop at the Gran Sasso National Laboratory: Solar Neutrinos, Assergi, Italy, 2001 (to be published). [35] L. Wolfenstein, Phys. Rev. D 17, 2369 (1978). [36] V. Barger, K. Whisnant, S. Pakvasa, and R. J. N. Phillips, Phys. Rev. D 22, 2718 (1980). [37] V. Barger et al., Phys. Rev. D 22, 1636 (1980). [38] S. P. Mikheyev and A. Smirnov, Yad. Fiz. 42, 1441 (1985) [Sov. J. Nucl. Phys. 42, 913 (1986)]; Nuovo Cimento Soc. Ital. Fis., C 9, 17 (1986); S. P. Rosen and J. Gelb, Phys. Rev. D 34, 969 (1986); S. Parke, Phys. Rev. Lett. 57, 1275 (1986); W. Haxton, Phys. Rev. Lett. 57, 1271 (1986); T. K. Kuo and J. Pantaleone, Rev. Mod. Phys. 61, 937 (1989).
77. Fits and references to the Homestake, Kamiokande, GALLEX, SAGE, Super Kamiokande, and SNO data include N. Hata and P. Langacker, Phys. Rev. D 56, 6107 (1997); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 58, 096016 (1998); J. Bahcall and P. Krastev, Phys. Lett. B 436, 243 (1998); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 60, 093001 (1999); hep-ph/0103179; M. Gonzalez-Garcia, C. Peña-Garay, and J. W. F. Valle, Phys. Rev. D 63, 013007 (2001); M. Gonzalez-Garcia et al., Phys. Rev. D 63, 033005 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, Phys. Rev. D 64, 073009 (2001); P. Krastev and A. Smirnov, Phys. Rev. D 65, 073022 (2002); J. N. Bahcall, M. C. Gonzalez-Garcia, and C. Peña-Garay, hep-ph/0111150; M. Maltoni, T. Schwetz, and J. W. F. Valle, Phys. Rev. D 65, 093004 (2002). Recent discussions of flux calculations are found in J. Bahcall, Phys. Rep. 333, 47 (2000), hep-ph/0009044, Proceedings of Neutrino-2000, and http://www.sns.ias. edu/-jnb/; V. Barger, D. Marfatia, and K. Whisnant, Phys. Rev. Lett. 88, 011302 (2002); Phys. Lett. B 509, 19 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, hep-ph/0204253. Super Kamiokande data are reported and analyzed in SuperKamiokande Collaboration, Y. Fukuda et al., Phys. Rev. Lett. 82, 1810 (1999); S. Fukuda et al., Phys. Rev. Lett. 86, 5651 (2001). For recent reviews, see, e.g., Y. Suzuki, Nucl. Phys. B, Proc. Suppl. 91, 29 (2001); Y. Takeuchi, in Proceedings of the International Conference on High Energy Physics, Osaka, http://ichep2000.hep.sci.osaka-u.ac.jp; Proceedings of the Fifth Topical Workshop at the Gran Sasso National Laboratory: Solar Neutrinos, Assergi, Italy, 2001 (to be published). [35] L. Wolfenstein, Phys. Rev. D 17, 2369 (1978). [36] V. Barger, K. Whisnant, S. Pakvasa, and R. J. N. Phillips, Phys. Rev. D 22, 2718 (1980). [37] V. Barger et al., Phys. Rev. D 22, 1636 (1980). [38] S. P. Mikheyev and A. Smirnov, Yad. Fiz. 42, 1441 (1985) [Sov. J. Nucl. Phys. 42, 913 (1986)]; Nuovo Cimento Soc. Ital. Fis., C 9, 17 (1986); S. P. Rosen and J. Gelb, Phys. Rev. D 34, 969 (1986); S. Parke, Phys. Rev. Lett. 57, 1275 (1986); W. Haxton, Phys. Rev. Lett. 57, 1271 (1986); T. K. Kuo and J. Pantaleone, Rev. Mod. Phys. 61, 937 (1989).
78. Fits and references to the Homestake, Kamiokande, GALLEX, SAGE, Super Kamiokande, and SNO data include N. Hata and P. Langacker, Phys. Rev. D 56, 6107 (1997); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 58, 096016 (1998); J. Bahcall and P. Krastev, Phys. Lett. B 436, 243 (1998); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 60, 093001 (1999); hep-ph/0103179; M. Gonzalez-Garcia, C. Peña-Garay, and J. W. F. Valle, Phys. Rev. D 63, 013007 (2001); M. Gonzalez-Garcia et al., Phys. Rev. D 63, 033005 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, Phys. Rev. D 64, 073009 (2001); P. Krastev and A. Smirnov, Phys. Rev. D 65, 073022 (2002); J. N. Bahcall, M. C. Gonzalez-Garcia, and C. Peña-Garay, hep-ph/0111150; M. Maltoni, T. Schwetz, and J. W. F. Valle, Phys. Rev. D 65, 093004 (2002). Recent discussions of flux calculations are found in J. Bahcall, Phys. Rep. 333, 47 (2000), hep-ph/0009044, Proceedings of Neutrino-2000, and http://www.sns.ias. edu/-jnb/; V. Barger, D. Marfatia, and K. Whisnant, Phys. Rev. Lett. 88, 011302 (2002); Phys. Lett. B 509, 19 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, hep-ph/0204253. Super Kamiokande data are reported and analyzed in SuperKamiokande Collaboration, Y. Fukuda et al., Phys. Rev. Lett. 82, 1810 (1999); S. Fukuda et al., Phys. Rev. Lett. 86, 5651 (2001). For recent reviews, see, e.g., Y. Suzuki, Nucl. Phys. B, Proc. Suppl. 91, 29 (2001); Y. Takeuchi, in Proceedings of the International Conference on High Energy Physics, Osaka, http://ichep2000.hep.sci.osaka-u.ac.jp; Proceedings of the Fifth Topical Workshop at the Gran Sasso National Laboratory: Solar Neutrinos, Assergi, Italy, 2001 (to be published). [35] L. Wolfenstein, Phys. Rev. D 17, 2369 (1978). [36] V. Barger, K. Whisnant, S. Pakvasa, and R. J. N. Phillips, Phys. Rev. D 22, 2718 (1980). [37] V. Barger et al., Phys. Rev. D 22, 1636 (1980). [38] S. P. Mikheyev and A. Smirnov, Yad. Fiz. 42, 1441 (1985) [Sov. J. Nucl. Phys. 42, 913 (1986)]; Nuovo Cimento Soc. Ital. Fis., C 9, 17 (1986); S. P. Rosen and J. Gelb, Phys. Rev. D 34, 969 (1986); S. Parke, Phys. Rev. Lett. 57, 1275 (1986); W. Haxton, Phys. Rev. Lett. 57, 1271 (1986); T. K. Kuo and J. Pantaleone, Rev. Mod. Phys. 61, 937 (1989).
79. Fits and references to the Homestake, Kamiokande, GALLEX, SAGE, Super Kamiokande, and SNO data include N. Hata and P. Langacker, Phys. Rev. D 56, 6107 (1997); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 58, 096016 (1998); J. Bahcall and P. Krastev, Phys. Lett. B 436, 243 (1998); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 60, 093001 (1999); hep-ph/0103179; M. Gonzalez-Garcia, C. Peña-Garay, and J. W. F. Valle, Phys. Rev. D 63, 013007 (2001); M. Gonzalez-Garcia et al., Phys. Rev. D 63, 033005 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, Phys. Rev. D 64, 073009 (2001); P. Krastev and A. Smirnov, Phys. Rev. D 65, 073022 (2002); J. N. Bahcall, M. C. Gonzalez-Garcia, and C. Peña-Garay, hep-ph/0111150; M. Maltoni, T. Schwetz, and J. W. F. Valle, Phys. Rev. D 65, 093004 (2002). Recent discussions of flux calculations are found in J. Bahcall, Phys. Rep. 333, 47 (2000), hep-ph/0009044, Proceedings of Neutrino-2000, and http://www.sns.ias. edu/-jnb/; V. Barger, D. Marfatia, and K. Whisnant, Phys. Rev. Lett. 88, 011302 (2002); Phys. Lett. B 509, 19 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, hep-ph/0204253. Super Kamiokande data are reported and analyzed in SuperKamiokande Collaboration, Y. Fukuda et al., Phys. Rev. Lett. 82, 1810 (1999); S. Fukuda et al., Phys. Rev. Lett. 86, 5651 (2001). For recent reviews, see, e.g., Y. Suzuki, Nucl. Phys. B, Proc. Suppl. 91, 29 (2001); Y. Takeuchi, in Proceedings of the International Conference on High Energy Physics, Osaka, http://ichep2000.hep.sci.osaka-u.ac.jp; Proceedings of the Fifth Topical Workshop at the Gran Sasso National Laboratory: Solar Neutrinos, Assergi, Italy, 2001 (to be published). [35] L. Wolfenstein, Phys. Rev. D 17, 2369 (1978). [36] V. Barger, K. Whisnant, S. Pakvasa, and R. J. N. Phillips, Phys. Rev. D 22, 2718 (1980). [37] V. Barger et al., Phys. Rev. D 22, 1636 (1980). [38] S. P. Mikheyev and A. Smirnov, Yad. Fiz. 42, 1441 (1985) [Sov. J. Nucl. Phys. 42, 913 (1986)]; Nuovo Cimento Soc. Ital. Fis., C 9, 17 (1986); S. P. Rosen and J. Gelb, Phys. Rev. D 34, 969 (1986); S. Parke, Phys. Rev. Lett. 57, 1275 (1986); W. Haxton, Phys. Rev. Lett. 57, 1271 (1986); T. K. Kuo and J. Pantaleone, Rev. Mod. Phys. 61, 937 (1989).
80. Fits and references to the Homestake, Kamiokande, GALLEX, SAGE, Super Kamiokande, and SNO data include N. Hata and P. Langacker, Phys. Rev. D 56, 6107 (1997); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 58, 096016 (1998); J. Bahcall and P. Krastev, Phys. Lett. B 436, 243 (1998); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 60, 093001 (1999); hep-ph/0103179; M. Gonzalez-Garcia, C. Peña-Garay, and J. W. F. Valle, Phys. Rev. D 63, 013007 (2001); M. Gonzalez-Garcia et al., Phys. Rev. D 63, 033005 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, Phys. Rev. D 64, 073009 (2001); P. Krastev and A. Smirnov, Phys. Rev. D 65, 073022 (2002); J. N. Bahcall, M. C. Gonzalez-Garcia, and C. Peña-Garay, hep-ph/0111150; M. Maltoni, T. Schwetz, and J. W. F. Valle, Phys. Rev. D 65, 093004 (2002). Recent discussions of flux calculations are found in J. Bahcall, Phys. Rep. 333, 47 (2000), hep-ph/0009044, Proceedings of Neutrino-2000, and http://www.sns.ias. edu/-jnb/; V. Barger, D. Marfatia, and K. Whisnant, Phys. Rev. Lett. 88, 011302 (2002); Phys. Lett. B 509, 19 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, hep-ph/0204253. Super Kamiokande data are reported and analyzed in SuperKamiokande Collaboration, Y. Fukuda et al., Phys. Rev. Lett. 82, 1810 (1999); S. Fukuda et al., Phys. Rev. Lett. 86, 5651 (2001). For recent reviews, see, e.g., Y. Suzuki, Nucl. Phys. B, Proc. Suppl. 91, 29 (2001); Y. Takeuchi, in Proceedings of the International Conference on High Energy Physics, Osaka, http://ichep2000.hep.sci.osaka-u.ac.jp; Proceedings of the Fifth Topical Workshop at the Gran Sasso National Laboratory: Solar Neutrinos, Assergi, Italy, 2001 (to be published). [35] L. Wolfenstein, Phys. Rev. D 17, 2369 (1978). [36] V. Barger, K. Whisnant, S. Pakvasa, and R. J. N. Phillips, Phys. Rev. D 22, 2718 (1980). [37] V. Barger et al., Phys. Rev. D 22, 1636 (1980). [38] S. P. Mikheyev and A. Smirnov, Yad. Fiz. 42, 1441 (1985) [Sov. J. Nucl. Phys. 42, 913 (1986)]; Nuovo Cimento Soc. Ital. Fis., C 9, 17 (1986); S. P. Rosen and J. Gelb, Phys. Rev. D 34, 969 (1986); S. Parke, Phys. Rev. Lett. 57, 1275 (1986); W. Haxton, Phys. Rev. Lett. 57, 1271 (1986); T. K. Kuo and J. Pantaleone, Rev. Mod. Phys. 61, 937 (1989).
81. Fits and references to the Homestake, Kamiokande, GALLEX, SAGE, Super Kamiokande, and SNO data include N. Hata and P. Langacker, Phys. Rev. D 56, 6107 (1997); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 58, 096016 (1998); J. Bahcall and P. Krastev, Phys. Lett. B 436, 243 (1998); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 60, 093001 (1999); hep-ph/0103179; M. Gonzalez-Garcia, C. Peña-Garay, and J. W. F. Valle, Phys. Rev. D 63, 013007 (2001); M. Gonzalez-Garcia et al., Phys. Rev. D 63, 033005 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, Phys. Rev. D 64, 073009 (2001); P. Krastev and A. Smirnov, Phys. Rev. D 65, 073022 (2002); J. N. Bahcall, M. C. Gonzalez-Garcia, and C. Peña-Garay, hep-ph/0111150; M. Maltoni, T. Schwetz, and J. W. F. Valle, Phys. Rev. D 65, 093004 (2002). Recent discussions of flux calculations are found in J. Bahcall, Phys. Rep. 333, 47 (2000), hep-ph/0009044, Proceedings of Neutrino-2000, and http://www.sns.ias. edu/-jnb/; V. Barger, D. Marfatia, and K. Whisnant, Phys. Rev. Lett. 88, 011302 (2002); Phys. Lett. B 509, 19 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, hep-ph/0204253. Super Kamiokande data are reported and analyzed in SuperKamiokande Collaboration, Y. Fukuda et al., Phys. Rev. Lett. 82, 1810 (1999); S. Fukuda et al., Phys. Rev. Lett. 86, 5651 (2001). For recent reviews, see, e.g., Y. Suzuki, Nucl. Phys. B, Proc. Suppl. 91, 29 (2001); Y. Takeuchi, in Proceedings of the International Conference on High Energy Physics, Osaka, http://ichep2000.hep.sci.osaka-u.ac.jp; Proceedings of the Fifth Topical Workshop at the Gran Sasso National Laboratory: Solar Neutrinos, Assergi, Italy, 2001 (to be published). [35] L. Wolfenstein, Phys. Rev. D 17, 2369 (1978). [36] V. Barger, K. Whisnant, S. Pakvasa, and R. J. N. Phillips, Phys. Rev. D 22, 2718 (1980). [37] V. Barger et al., Phys. Rev. D 22, 1636 (1980). [38] S. P. Mikheyev and A. Smirnov, Yad. Fiz. 42, 1441 (1985) [Sov. J. Nucl. Phys. 42, 913 (1986)]; Nuovo Cimento Soc. Ital. Fis., C 9, 17 (1986); S. P. Rosen and J. Gelb, Phys. Rev. D 34, 969 (1986); S. Parke, Phys. Rev. Lett. 57, 1275 (1986); W. Haxton, Phys. Rev. Lett. 57, 1271 (1986); T. K. Kuo and J. Pantaleone, Rev. Mod. Phys. 61, 937 (1989).
82. Fits and references to the Homestake, Kamiokande, GALLEX, SAGE, Super Kamiokande, and SNO data include N. Hata and P. Langacker, Phys. Rev. D 56, 6107 (1997); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 58, 096016 (1998); J. Bahcall and P. Krastev, Phys. Lett. B 436, 243 (1998); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 60, 093001 (1999); hep-ph/0103179; M. Gonzalez-Garcia, C. Peña-Garay, and J. W. F. Valle, Phys. Rev. D 63, 013007 (2001); M. Gonzalez-Garcia et al., Phys. Rev. D 63, 033005 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, Phys. Rev. D 64, 073009 (2001); P. Krastev and A. Smirnov, Phys. Rev. D 65, 073022 (2002); J. N. Bahcall, M. C. Gonzalez-Garcia, and C. Peña-Garay, hep-ph/0111150; M. Maltoni, T. Schwetz, and J. W. F. Valle, Phys. Rev. D 65, 093004 (2002). Recent discussions of flux calculations are found in J. Bahcall, Phys. Rep. 333, 47 (2000), hep-ph/0009044, Proceedings of Neutrino-2000, and http://www.sns.ias. edu/-jnb/; V. Barger, D. Marfatia, and K. Whisnant, Phys. Rev. Lett. 88, 011302 (2002); Phys. Lett. B 509, 19 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, hep-ph/0204253. Super Kamiokande data are reported and analyzed in SuperKamiokande Collaboration, Y. Fukuda et al., Phys. Rev. Lett. 82, 1810 (1999); S. Fukuda et al., Phys. Rev. Lett. 86, 5651 (2001). For recent reviews, see, e.g., Y. Suzuki, Nucl. Phys. B, Proc. Suppl. 91, 29 (2001); Y. Takeuchi, in Proceedings of the International Conference on High Energy Physics, Osaka, http://ichep2000.hep.sci.osaka-u.ac.jp; Proceedings of the Fifth Topical Workshop at the Gran Sasso National Laboratory: Solar Neutrinos, Assergi, Italy, 2001 (to be published). [35] L. Wolfenstein, Phys. Rev. D 17, 2369 (1978). [36] V. Barger, K. Whisnant, S. Pakvasa, and R. J. N. Phillips, Phys. Rev. D 22, 2718 (1980). [37] V. Barger et al., Phys. Rev. D 22, 1636 (1980). [38] S. P. Mikheyev and A. Smirnov, Yad. Fiz. 42, 1441 (1985) [Sov. J. Nucl. Phys. 42, 913 (1986)]; Nuovo Cimento Soc. Ital. Fis., C 9, 17 (1986); S. P. Rosen and J. Gelb, Phys. Rev. D 34, 969 (1986); S. Parke, Phys. Rev. Lett. 57, 1275 (1986); W. Haxton, Phys. Rev. Lett. 57, 1271 (1986); T. K. Kuo and J. Pantaleone, Rev. Mod. Phys. 61, 937 (1989).
83. Fits and references to the Homestake, Kamiokande, GALLEX, SAGE, Super Kamiokande, and SNO data include N. Hata and P. Langacker, Phys. Rev. D 56, 6107 (1997); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 58, 096016 (1998); J. Bahcall and P. Krastev, Phys. Lett. B 436, 243 (1998); J. Bahcall, P. Krastev, and A. Smirnov, Phys. Rev. D 60, 093001 (1999); hep-ph/0103179; M. Gonzalez-Garcia, C. Peña-Garay, and J. W. F. Valle, Phys. Rev. D 63, 013007 (2001); M. Gonzalez-Garcia et al., Phys. Rev. D 63, 033005 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, Phys. Rev. D 64, 073009 (2001); P. Krastev and A. Smirnov, Phys. Rev. D 65, 073022 (2002); J. N. Bahcall, M. C. Gonzalez-Garcia, and C. Peña-Garay, hep-ph/0111150; M. Maltoni, T. Schwetz, and J. W. F. Valle, Phys. Rev. D 65, 093004 (2002). Recent discussions of flux calculations are found in J. Bahcall, Phys. Rep. 333, 47 (2000), hep-ph/0009044, Proceedings of Neutrino-2000, and http://www.sns.ias. edu/-jnb/; V. Barger, D. Marfatia, and K. Whisnant, Phys. Rev. Lett. 88, 011302 (2002); Phys. Lett. B 509, 19 (2001); V. Barger, D. Marfatia, K. Whisnant, and B. P. Wood, hep-ph/0204253. Super Kamiokande data are reported and analyzed in SuperKamiokande Collaboration, Y. Fukuda et al., Phys. Rev. Lett. 82, 1810 (1999); S. Fukuda et al., Phys. Rev. Lett. 86, 5651 (2001). For recent reviews, see, e.g., Y. Suzuki, Nucl. Phys. B, Proc. Suppl. 91, 29 (2001); Y. Takeuchi, in Proceedings of the International Conference on High Energy Physics, Osaka, http://ichep2000.hep.sci.osaka-u.ac.jp; Proceedings of the Fifth Topical Workshop at the Gran Sasso National Laboratory: Solar Neutrinos, Assergi, Italy, 2001 (to be published). [35] L. Wolfenstein, Phys. Rev. D 17, 2369 (1978). [36] V. Barger, K. Whisnant, S. Pakvasa, and R. J. N. Phillips, Phys. Rev. D 22, 2718 (1980). [37] V. Barger et al., Phys. Rev. D 22, 1636 (1980). [38] S. P. Mikheyev and A. Smirnov, Yad. Fiz. 42, 1441 (1985) [Sov. J. Nucl. Phys. 42, 913 (1986)]; Nuovo Cimento Soc. Ital. Fis., C 9, 17 (1986); S. P. Rosen and J. Gelb, Phys. Rev. D 34, 969 (1986); S. Parke, Phys. Rev. Lett. 57, 1275 (1986); W. Haxton, Phys. Rev. Lett. 57, 1271 (1986); T. K. Kuo and J. Pantaleone, Rev. Mod. Phys. 61, 937 (1989).
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