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How does the RSFP scenario effect the Solar neutrino data?

Yıl 2012, Cilt 33, Sayı 2, 25 - 31, 21.02.2013

Öz

Kaynakça

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  • S. P. Mikheev and A. Y. Smirnov, Sov. J. Nucl. Phys. 42, 913 (1985) [Yad. Fiz. 42,
  • (1985)]. S. P. Mikheev and A. Y. Smirnov, Nuovo Cim. C 9, 17 (1986).
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  • J. N. Abdurashitov et al. [SAGE Collaboration], J. Exp. Theor. Phys. 95, 181 (2002)
  • Zh. Eksp. Teor. Fiz. 122, 211 (2002)] [arXiv:astro-ph/0204245].
  • W. Hampel et al. [GALLEX Collaboration], Phys. Lett. B 447, 127 (1999).
  • M. Altmann et al. [GNO Collaboration], Phys. Lett. B 490, 16 (2000) [arXiv:hep- ex/0006034].
  • S. Fukuda et al. [Super-Kamiokande Collaboration], Phys. Rev. Lett. 86, 5651 (2001) arXiv:hep-ex/0103032]. S. Fukuda et al. [Super-Kamiokande Collaboration], Phys.
  • Rev. Lett. 86, 5656 (2001) [arXiv:hep-ex/0103033].
  • Q. R. Ahmad et al. [SNO Collaboration], Phys. Rev. Lett. 87, 071301 (2001) arXiv:nucl-ex/0106015].
  • Q. R. Ahmad et al. [SNO Collaboration], Phys. Rev. Lett. 89, 011301 (2002) arXiv:nucl-ex/0204008]. Q. R. Ahmad et al. [SNO Collaboration], Phys. Rev. Lett. , 011302 (2002) [arXiv:nucl-ex/0204009].
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  • (2004) [arXiv:hep-ph/0309299]. G. L. Fogli, E. Lisi, A. Marrone and A. Palazzo,
  • Phys. Lett. B 583, 149 (2004) [arXiv:hep-ph/0309100]. A. B. Balantekin, V. Barger,
  • D. Marfatia, S. Pakvasa and H. Yuksel, Phys. Lett. B 613, 61 (2005) [arXiv:hep- ph/0405019]. M. Maltoni, T. Schwetz, M. A. Tortola and J. W. F. Valle, New J. Phys. , 122 (2004) [arXiv:hep-ph/0405172].
  • W. J. Marciano and A. I. Sanda, Phys. Lett. B 67, 303 (1977). B. W. Lee and R. E. Shrock, Phys. Rev. D 16, 1444 (1977).
  • P. Vogel and J. Engel, Phys. Rev. D 39, 3378 (1989).
  • L. B. Okun, M. B. Voloshin and M. I. Vysotsky, Sov. J. Nucl. Phys. 44, 440 (1986) Yad. Fiz. 44, 677 (1986)].
  • E. K. Akhmedov, Phys. Lett. B 213, 64 (1988). E. K. Akhmedov and M. Y. Khlopov,
  • Mod. Phys. Lett. A 3, 451 (1988).
  • R. Barbieri and G. Fiorentini, Nucl. Phys. B 304, 909 (1988).
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  • A. B. Balantekin, P. J. Hatchell and F. Loreti, Phys. Rev. D 41, 3583 (1990).
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  • B. C. Chauhan and J. Pulido, JHEP 0406, 008 (2004) [arXiv:hep-ph/0402194].
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  • D. Yilmaz and A. U. Yilmazer, J. Phys. G 31, 57 (2005).
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  • J. M. Lattimer and J. Cooperstein, Phys. Rev. Lett. 61, 23 (1988).
  • R. Barbieri and R. N. Mohapatra, Phys. Rev. Lett. 61, 27 (1988).
  • G. G. Raffelt, Phys. Rev. Lett. 64, 2856 (1990).
  • D. W. Liu et al. [Super-Kamiokande Collaboration], Phys. Rev. Lett. 93, 021802 (2004) [arXiv:hep-ex/0402015].
  • A. B. Balantekin, AIP Conf. Proc. 847, 128 (2006) [arXiv:hep-ph/0601113].
  • S. Abe et al. [KamLAND Collaboration], Phys. Rev. Lett. 100, 221803 (2008) arXiv:0801.4589 [hep-ex]]. Feldman arXiv:physics/9711021]. R. D. Cousins, Phys. Rev. D , (1998)
  • G. L. Fogli, E. Lisi, A. Marrone, D. Montanino and A. Palazzo, Phys. Rev. D 66, (2002) [arXiv:hep-ph/0206162].
  • M. V. Garzelli and C. Giunti, Astropart. Phys. 17, 205 (2002) [arXiv:hep-ph/0007155].
  • M. V. Garzelli and C. Giunti, Phys. Rev. D 65, 093005 (2002) [arXiv:hep-ph/0111254].
  • M. V. Garzelli and C. Giunti, JHEP 0112, 017 (2001) [arXiv:hep-ph/0108191].
  • M. C. Gonzalez-Garcia and Y. Nir, Rev. Mod. Phys. 75, 345 (2003) [arXiv:hep- ph/0202058].
  • A. B. Balantekin and H. Yuksel, J. Phys. G 29, 665 (2003) [arXiv:hep-ph/0301072].
  • Y. Giomataris and J. D. Vergados, Nucl. Instrum. Meth. A 530, 330 (2004) [arXiv:hep- ex/0303045].
  • L. N. Bogdanova [MAMONT Collaboration], Nucl. Phys. A 721, 499 (2003).
  • G. C. McLaughlin and C. Volpe, Phys. Lett. B 591, 229 (2004) [arXiv:hep- ph/0312156].
  • C. Volpe, J. Phys. G 30, L1 (2004) [arXiv:hep-ph/0303222].
  • S. Couvidat, S. Turck-Chieze and A. G. Kosovichev, Astrophys. J. 599, 1434 (2003).
  • D. Yilmaz, Turk. J. Phys. 33, 63 (2009).

How does the RSFP scenario effect the Solar neutrino data?

Yıl 2012, Cilt 33, Sayı 2, 25 - 31, 21.02.2013

Öz

A joint analysis of solar neutrino data together with the latest KamLAND data is presented in the RSFP framework using the Wood-Saxon Shape of the Magnetic Field. It is investigated that how the latest KamLAND data effects the allowed regions at different µB values. A limit on µB value is found at the different confidence level intervals. It is shown that the RSFP scenerio does not have a crucial role on the solar neutrino data.

Kaynakça

  • J. N. Bahcall, W. F. Huebner, S. H. Lubow, P. D. Parker and R. K. Ulrich, Rev. Mod. Phys. 54, 767 (1982). J. N. Bahcall, M. H. Pinsonneault and S. Basu, Astrophys. J. , 990 (2001) [arXiv:astro-ph/0010346].
  • L. Wolfenstein, Phys. Rev. D 17, 2369 (1978).
  • S. P. Mikheev and A. Y. Smirnov, Sov. J. Nucl. Phys. 42, 913 (1985) [Yad. Fiz. 42,
  • (1985)]. S. P. Mikheev and A. Y. Smirnov, Nuovo Cim. C 9, 17 (1986).
  • B. T. Cleveland et al., Astrophys. J. 496, 505 (1998).
  • J. N. Abdurashitov et al. [SAGE Collaboration], J. Exp. Theor. Phys. 95, 181 (2002)
  • Zh. Eksp. Teor. Fiz. 122, 211 (2002)] [arXiv:astro-ph/0204245].
  • W. Hampel et al. [GALLEX Collaboration], Phys. Lett. B 447, 127 (1999).
  • M. Altmann et al. [GNO Collaboration], Phys. Lett. B 490, 16 (2000) [arXiv:hep- ex/0006034].
  • S. Fukuda et al. [Super-Kamiokande Collaboration], Phys. Rev. Lett. 86, 5651 (2001) arXiv:hep-ex/0103032]. S. Fukuda et al. [Super-Kamiokande Collaboration], Phys.
  • Rev. Lett. 86, 5656 (2001) [arXiv:hep-ex/0103033].
  • Q. R. Ahmad et al. [SNO Collaboration], Phys. Rev. Lett. 87, 071301 (2001) arXiv:nucl-ex/0106015].
  • Q. R. Ahmad et al. [SNO Collaboration], Phys. Rev. Lett. 89, 011301 (2002) arXiv:nucl-ex/0204008]. Q. R. Ahmad et al. [SNO Collaboration], Phys. Rev. Lett. , 011302 (2002) [arXiv:nucl-ex/0204009].
  • J. N. Bahcall, M. C. Gonzalez-Garcia and C. Pena-Garay, JHEP 0207, 054 (2002) arXiv:hep-ph/0204314]. P. C. de Holanda and A. Y. Smirnov, Astropart. Phys. 21,
  • (2004) [arXiv:hep-ph/0309299]. G. L. Fogli, E. Lisi, A. Marrone and A. Palazzo,
  • Phys. Lett. B 583, 149 (2004) [arXiv:hep-ph/0309100]. A. B. Balantekin, V. Barger,
  • D. Marfatia, S. Pakvasa and H. Yuksel, Phys. Lett. B 613, 61 (2005) [arXiv:hep- ph/0405019]. M. Maltoni, T. Schwetz, M. A. Tortola and J. W. F. Valle, New J. Phys. , 122 (2004) [arXiv:hep-ph/0405172].
  • W. J. Marciano and A. I. Sanda, Phys. Lett. B 67, 303 (1977). B. W. Lee and R. E. Shrock, Phys. Rev. D 16, 1444 (1977).
  • P. Vogel and J. Engel, Phys. Rev. D 39, 3378 (1989).
  • L. B. Okun, M. B. Voloshin and M. I. Vysotsky, Sov. J. Nucl. Phys. 44, 440 (1986) Yad. Fiz. 44, 677 (1986)].
  • E. K. Akhmedov, Phys. Lett. B 213, 64 (1988). E. K. Akhmedov and M. Y. Khlopov,
  • Mod. Phys. Lett. A 3, 451 (1988).
  • R. Barbieri and G. Fiorentini, Nucl. Phys. B 304, 909 (1988).
  • C. S. Lim and W. J. Marciano, Phys. Rev. D 37, 1368 (1988).
  • A. B. Balantekin, P. J. Hatchell and F. Loreti, Phys. Rev. D 41, 3583 (1990).
  • A. A. Bykov, V. Y. Popov, T. I. Rashba and V. B. Semikoz, arXiv:hep-ph/0002174.
  • B. C. Chauhan, arXiv:hep-ph/0204160.
  • E. K. Akhmedov and J. Pulido, Phys. Lett. B 553, 7 (2003) [arXiv:hep-ph/0209192].
  • B. C. Chauhan, J. Pulido and E. Torrente-Lujan, Phys. Rev. D 68, 033015 (2003) arXiv:hep-ph/0304297].
  • B. C. Chauhan and J. Pulido, JHEP 0406, 008 (2004) [arXiv:hep-ph/0402194].
  • A. B. Balantekin and C. Volpe, Phys. Rev. D 72, 033008 (2005) [arXiv:hep- ph/0411148].
  • D. Yilmaz and A. U. Yilmazer, J. Phys. G 31, 57 (2005).
  • T. Araki et al. [KamLAND Collaboration], Phys. Rev. Lett. 94, 081801 (2005) arXiv:hep-ex/0406035].
  • J. M. Lattimer and J. Cooperstein, Phys. Rev. Lett. 61, 23 (1988).
  • R. Barbieri and R. N. Mohapatra, Phys. Rev. Lett. 61, 27 (1988).
  • G. G. Raffelt, Phys. Rev. Lett. 64, 2856 (1990).
  • D. W. Liu et al. [Super-Kamiokande Collaboration], Phys. Rev. Lett. 93, 021802 (2004) [arXiv:hep-ex/0402015].
  • A. B. Balantekin, AIP Conf. Proc. 847, 128 (2006) [arXiv:hep-ph/0601113].
  • S. Abe et al. [KamLAND Collaboration], Phys. Rev. Lett. 100, 221803 (2008) arXiv:0801.4589 [hep-ex]]. Feldman arXiv:physics/9711021]. R. D. Cousins, Phys. Rev. D , (1998)
  • G. L. Fogli, E. Lisi, A. Marrone, D. Montanino and A. Palazzo, Phys. Rev. D 66, (2002) [arXiv:hep-ph/0206162].
  • M. V. Garzelli and C. Giunti, Astropart. Phys. 17, 205 (2002) [arXiv:hep-ph/0007155].
  • M. V. Garzelli and C. Giunti, Phys. Rev. D 65, 093005 (2002) [arXiv:hep-ph/0111254].
  • M. V. Garzelli and C. Giunti, JHEP 0112, 017 (2001) [arXiv:hep-ph/0108191].
  • M. C. Gonzalez-Garcia and Y. Nir, Rev. Mod. Phys. 75, 345 (2003) [arXiv:hep- ph/0202058].
  • A. B. Balantekin and H. Yuksel, J. Phys. G 29, 665 (2003) [arXiv:hep-ph/0301072].
  • Y. Giomataris and J. D. Vergados, Nucl. Instrum. Meth. A 530, 330 (2004) [arXiv:hep- ex/0303045].
  • L. N. Bogdanova [MAMONT Collaboration], Nucl. Phys. A 721, 499 (2003).
  • G. C. McLaughlin and C. Volpe, Phys. Lett. B 591, 229 (2004) [arXiv:hep- ph/0312156].
  • C. Volpe, J. Phys. G 30, L1 (2004) [arXiv:hep-ph/0303222].
  • S. Couvidat, S. Turck-Chieze and A. G. Kosovichev, Astrophys. J. 599, 1434 (2003).
  • D. Yilmaz, Turk. J. Phys. 33, 63 (2009).

Ayrıntılar

Birincil Dil İngilizce
Konular Mühendislik
Bölüm Editöriyal
Yazarlar

Deniz YILMAZ

Yayımlanma Tarihi 21 Şubat 2013
Yayınlandığı Sayı Yıl 2012, Cilt 33, Sayı 2

Kaynak Göster

Bibtex @araştırma makalesi { cumuscij57947, journal = {Cumhuriyet Üniversitesi Fen Edebiyat Fakültesi Fen Bilimleri Dergisi}, issn = {1300-1949}, eissn = {1300-1949}, address = {}, publisher = {Sivas Cumhuriyet Üniversitesi}, year = {2013}, volume = {33}, pages = {25 - 31}, doi = {}, title = {How does the RSFP scenario effect the Solar neutrino data?}, key = {cite}, author = {Yılmaz, Deniz} }
APA Yılmaz, D. (2013). How does the RSFP scenario effect the Solar neutrino data? . Cumhuriyet Üniversitesi Fen Edebiyat Fakültesi Fen Bilimleri Dergisi , 33 (2) , 25-31 . Retrieved from https://dergipark.org.tr/tr/pub/cumuscij/issue/4325/57947
MLA Yılmaz, D. "How does the RSFP scenario effect the Solar neutrino data?" . Cumhuriyet Üniversitesi Fen Edebiyat Fakültesi Fen Bilimleri Dergisi 33 (2013 ): 25-31 <https://dergipark.org.tr/tr/pub/cumuscij/issue/4325/57947>
Chicago Yılmaz, D. "How does the RSFP scenario effect the Solar neutrino data?". Cumhuriyet Üniversitesi Fen Edebiyat Fakültesi Fen Bilimleri Dergisi 33 (2013 ): 25-31
RIS TY - JOUR T1 - How does the RSFP scenario effect the Solar neutrino data? AU - Deniz Yılmaz Y1 - 2013 PY - 2013 N1 - DO - T2 - Cumhuriyet Üniversitesi Fen Edebiyat Fakültesi Fen Bilimleri Dergisi JF - Journal JO - JOR SP - 25 EP - 31 VL - 33 IS - 2 SN - 1300-1949-1300-1949 M3 - UR - Y2 - 2022 ER -
EndNote %0 Cumhuriyet Üniversitesi Fen-Edebiyat Fakültesi Fen Bilimleri Dergisi How does the RSFP scenario effect the Solar neutrino data? %A Deniz Yılmaz %T How does the RSFP scenario effect the Solar neutrino data? %D 2013 %J Cumhuriyet Üniversitesi Fen Edebiyat Fakültesi Fen Bilimleri Dergisi %P 1300-1949-1300-1949 %V 33 %N 2 %R %U
ISNAD Yılmaz, Deniz . "How does the RSFP scenario effect the Solar neutrino data?". Cumhuriyet Üniversitesi Fen Edebiyat Fakültesi Fen Bilimleri Dergisi 33 / 2 (Şubat 2013): 25-31 .
AMA Yılmaz D. How does the RSFP scenario effect the Solar neutrino data?. Cumhuriyet Üniversitesi Fen Edebiyat Fakültesi Fen Bilimleri Dergisi. 2013; 33(2): 25-31.
Vancouver Yılmaz D. How does the RSFP scenario effect the Solar neutrino data?. Cumhuriyet Üniversitesi Fen Edebiyat Fakültesi Fen Bilimleri Dergisi. 2013; 33(2): 25-31.
IEEE D. Yılmaz , "How does the RSFP scenario effect the Solar neutrino data?", Cumhuriyet Üniversitesi Fen Edebiyat Fakültesi Fen Bilimleri Dergisi, c. 33, sayı. 2, ss. 25-31, Şub. 2013