SOLAR-NEUTRINO OSCILLATIONS IN MATTER WITH VARYING DENSITY

SUN Chang-Pu

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2024年10月30日

Chinese Physics C> 1989, Vol. 13> Issue(5) : 403-410

SOLAR-NEUTRINO OSCILLATIONS IN MATTER WITH VARYING DENSITY

SUN Chang-Pu ^,

Northeast Normal niversity,Changchun

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Abstract：
By making use of the High-order Adiabatio Approximation Method proposed by the author,the problems of Solarneutrino oscillations are studied and high-order approximate solutions for the oscillation equations are obtained.For the cases with two and three generations,we find out non-adiabatic corrections to the probability of neutrino transition and also discuss the relations of CP-violation,Berry's phases and neutrino oscillations.

References

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L. Wolfenstein, Phys. Rev., D17(1978), 2369.[2] S. P. Mikheyev and A. Yu. Smirnov, Sou. J. Nucl. Phys., 42(1985), 913.[3] V. Rethe, Phys. Rev. Lett., 56(1986), 1305.[4] A. Messiah, in "86' Massive Neutrinos" p373.[5] V. Barger et al, Phys. Rev., D34(1986), 980.[6] C. W. Kim and W. Sze, Phys. Rev., D35(1987), 1040.[7] S. T. Petcov and S. Toshev, Phys. Lett., B187(1987). 120.[8] T. K. Kuo and J. Pantaleone, Phys. Rev. Lett., 57(1986), 1805.[9] W. C. Haxton, Phys. Rev., D35(1987), 2352.[10] S. T. Petcov, Phys. Lett., B200(1988), 273.[11] S. Toshev, Phys. Letr., B196(1987), 170.[12] T. Kaneko, Prog. Theor. Phys., 78(1987), 532.[13] 孙昌璞，高能物理与核物理，12(1988)，351.[14] C-P Sun (Hrgg) , J. Phys. A, 21(1988), 1595.[13] 孙昌璞，高能物理与核物理，13(1988)109.[16] S. M. Bilenky and S. T. Petcov, Rev. M. Phys.. 59(1987), 671.[17] E. D. Commins and P. H. Bucksbaum, Weak Interactions of Leptons and Quarks. (Cambridge Univ. Press,1963) 369-379.

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SUN Chang-Pu. SOLAR-NEUTRINO OSCILLATIONS IN MATTER WITH VARYING DENSITY[J]. Chinese Physics C, 1989, 13(5): 403-410.

SUN Chang-Pu. SOLAR-NEUTRINO OSCILLATIONS IN MATTER WITH VARYING DENSITY[J]. Chinese Physics C, 1989, 13(5): 403-410. shu

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Received: 1900-01-01
Revised: 1900-01-01

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沈阳化工大学材料科学与工程学院沈阳 110142

SOLAR-NEUTRINO OSCILLATIONS IN MATTER WITH VARYING DENSITY

SUN Chang-Pu ^,

Corresponding author: SUN Chang-Pu,

Northeast Normal niversity,Changchun

Received Date: 1900-01-01
Accepted Date: 1900-01-01
Available Online: 1989-05-05

Abstract: By making use of the High-order Adiabatio Approximation Method proposed by the author,the problems of Solarneutrino oscillations are studied and high-order approximate solutions for the oscillation equations are obtained.For the cases with two and three generations,we find out non-adiabatic corrections to the probability of neutrino transition and also discuss the relations of CP-violation,Berry's phases and neutrino oscillations.