How does the RSFP scenario effect the Solar neutrino data?

Deniz Yılmaz

Araştırma Makalesi

How does the RSFP scenario effect the Solar neutrino data?

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

Deniz Yılmaz

Öz

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).

How does the RSFP scenario effect the Solar neutrino data?

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

Deniz Yılmaz

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.

Anahtar Kelimeler

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).

Toplam 51 adet kaynakça vardır.

Ayrıntılar

Birincil Dil	İngilizce
Konular	Mühendislik
Bölüm	Editöriyal
Yazarlar	Deniz Yılmaz
Yayımlanma Tarihi	21 Şubat 2013
Yayımlandığı Sayı	Yıl 2012 Cilt: 33 Sayı: 2

Kaynak Göster

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. Şubat 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, sy. 2 (Şubat 2013): 25-31.
EndNote	Yılmaz D (01 Şubat 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, c. 33, sy. 2, ss. 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 (Şubat 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, c. 33, sy. 2, 2013, ss. 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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