How does the RSFP scenario effect the Solar neutrino data?

Deniz Yılmaz

Research Article

How does the RSFP scenario effect the Solar neutrino data?

Year 2012, Volume: 33 Issue: 2, 25 - 31, 21.02.2013

Deniz Yılmaz

Abstract

References

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How does the RSFP scenario effect the Solar neutrino data?

Year 2012, Volume: 33 Issue: 2, 25 - 31, 21.02.2013

Deniz Yılmaz

Abstract

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.

Keywords

References

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).

There are 51 citations in total.

Details

Primary Language	English
Subjects	Engineering
Journal Section	Editorial
Authors	Deniz Yılmaz
Publication Date	February 21, 2013
Published in Issue	Year 2012 Volume: 33 Issue: 2

Cite

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.
AMA	Yılmaz D. How does the RSFP scenario effect the Solar neutrino data?. Cumhuriyet Üniversitesi Fen Edebiyat Fakültesi Fen Bilimleri Dergisi. February 2013;33(2):25-31.
Chicago	Yılmaz, Deniz. “How Does the RSFP Scenario Effect the Solar Neutrino Data?”. Cumhuriyet Üniversitesi Fen Edebiyat Fakültesi Fen Bilimleri Dergisi 33, no. 2 (February 2013): 25-31.
EndNote	Yılmaz D (February 1, 2013) How does the RSFP scenario effect the Solar neutrino data?. Cumhuriyet Üniversitesi Fen Edebiyat Fakültesi Fen Bilimleri Dergisi 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, vol. 33, no. 2, pp. 25–31, 2013.
ISNAD	Yılmaz, Deniz. “How Does the RSFP Scenario Effect the Solar Neutrino Data?”. Cumhuriyet Üniversitesi Fen Edebiyat Fakültesi Fen Bilimleri Dergisi 33/2 (February 2013), 25-31.
JAMA	Yılmaz D. How does the RSFP scenario effect the Solar neutrino data?. Cumhuriyet Üniversitesi Fen Edebiyat Fakültesi Fen Bilimleri Dergisi. 2013;33:25–31.
MLA	Yılmaz, Deniz. “How Does the RSFP Scenario Effect the Solar Neutrino Data?”. Cumhuriyet Üniversitesi Fen Edebiyat Fakültesi Fen Bilimleri Dergisi, vol. 33, no. 2, 2013, pp. 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.

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