Effects of a reverse shock wave on neutrino oscillations in a new supernova model

Jing Xu; Ming Lu; Xin-Heng Guo; Li-Jun Hu

doi:10.1088/1674-1137/42/11/113103

Chinese Physics C> 2018, Vol. 42> Issue(11) : 113103 DOI: 10.1088/1674-1137/42/11/113103

Effects of a reverse shock wave on neutrino oscillations in a new supernova model

Jing Xu ^1,, ,
Ming Lu ¹ ,
Xin-Heng Guo ² ,
Li-Jun Hu ³

1.
Physics Department, Yantai University, Yantai 264005, China
2.
College of Nuclear Science and Techonology, Beijing Normal University, Beijing 100875, China
3.
College of Mechanical and Electrical Engineering, Cangzhou Normal University, Cangzhou 061000, China

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Abstract：
It is known that in supernova explosions, there might be a reverse shock wave in addition to the forward shock wave during the explosion phase, when the mass of supernova is in a certain range. In this paper, we propose to add the reverse shock wave to the previous supernova model, in which only the forward shock wave was included, and thus obtain a new model. By analyzing the resonance condition as well as the density jump in the new model and using the Landau-Zener method, an expression for the crossing probability in high density matter (P_H) is given. We proceed to study how P_H varies with time and with neutrino energy when both the reverse shock wave and the forward shock wave are considered. From comparison with the previous results, where only the effects of the forward shock wave were considered, it is clear that the reverse shock wave brings significant changes to P_H.
- neutrino oscillations ,
- shock wave effects ,
- crossing probability ,
- supernova models

References

[1]	G. L. Fogli, E. Lisi, D. Montanino, and A. Mirizzi, Phys. Rev. D, 68:033005(2003),[hep-ph/0304056]
[2]	G. L. Fogli, E. Lisi, A. Mirizzi, and D. Montanino, JCAP, 04:002(2005),[hep-ph/0412046]
[3]	G. L. Fogli, E. Lisi, A. Mirizzi, and D. Montanino, JCAP, 06:012(2006),[hep-ph/0603033]
[4]	R. C. Schirato and G. M. Fuller,[hep-ph/0205390]
[5]	M. Y. Huang, X. H. Guo, and B. L. Young, Phys. Rev. D, 82:033011(2010), arXiv:1003.1197[astro-ph.HE]
[6]	J. Xu, M. Y. Huang, L. J. Hu, X. H. Guo, and B. L. Young, Commun. Theor. Phys., 61(2):2, 226(2014)
[7]	T. K. Kuo and J. T. Pantaleone, Rev. Mod. Phys., 61:937(1989)
[8]	T. K. Kuo and J. T. Pantaleone, Phys. Rev. D, 39:1930(1989)
[9]	K. Kotake, K. Sato, and K. Takahashi, Rept. Prog. Phys., 69:971(2006)
[10]	S. P. Mikheev and A. Y. Smirnov, Sov. J. Nucl. Phys., 42:913(1985),[Yad. Fiz., 42:1441(1985)]
[11]	S. P. Mikheev and A. Y. Smirnov, Sov. Phys. JETP, 64:4(1986), arXiv:0706.0454[hep-ph]
[12]	L. Wolfenstein, Phys. Rev. D, 17:2369(1978)
[13]	Landau. L., Phys. Z. Sowjetunion, 2:46(1932).
[14]	C. Zener, Proc. R. Soc. A, 137:696(1932)
[15]	L. D. Landau and E. M. Lifshitz, Quantum Mechanics:Non-Relativistic Theory (Pergamon, New York) 1977.
[16]	X. H. Guo, M. Y. Huang, and B. L. Young, Phys. Rev. D, 79:113007(2009), arXiv:0806.2720[hep-ph]
[17]	F. P. An et al (DAYA-BAY Collaboration), Phys. Rev. Lett., 108:171803(2012), arXiv:1203.1669[hep-ex]
[18]	J. Kneller, C. Volpe, Phys. Rev. D, 82:123004(2010), arXiv:1006.0913[astro-ph.HE]
[19]	T. Lund and J. P. Kneller, Phys. Rev. D, 88:02308(2013), arXiv:1304.6372[hep-ph]
[20]	S. Galais, J. Kneller, C. Volpe, and J. Gava, Phys. Rev. D, 81:053002(2010), arXiv:0906.5294[hep-ph]
[21]	K. M. Patton, J. P. Kneller, and G. C. McLaughlin, Phys. Rev. D, 89:073022(2014), arXiv:1310.5643[hep-ph]
[22]	A. Wongwathanarat, E. Mueller, and H. T. Janka, Astron. Astrophys., 577:A48(2015), arXiv:1409.5431[astro-ph.HE]
[23]	S. M. Couch and C. D. Ott, arXiv:1408.1399[astro-ph.HE]
[24]	J. Xu, L. J. Hu, R. C. Li, X. H. Guo, and B. L. Young, Commun. Theor. Phys., 65(4):506(2016)
[25]	H. A. Bethe, Rev. Mod. Phys., 62:801(1990); G. E. Brown, H. A. Bethe, and G. Baym, Nucl. Phys. A, 375:481(1982)
[26]	M. C. Gonzalez-Garcia and M. Maltoni, Phys. Rep., 460:1(2008); T. Schwetz, M. Tortola, and J. W. F. Valle, New. J. Phys., 10:113011(2008)

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[17]	Zhong Yunxiao , Hu Jimin . Fission Probability Calculation by Solving Fokker-PIank Equation with Variation Method. Chinese Physics C, 1994, 18(Z1): 79-86.
[18]	Yan Jun , Hu Shike . Compact Baby Universe Model in 10 Dimensions and Probability Function of Quantum Gravity. Chinese Physics C, 1991, 15(S4): 353-360.
[19]	Xing Zheng , Wu Xingju . Rotational Effect on Electromagnetic Transitions After Band-Crossing. Chinese Physics C, 1991, 15(S1): 93-100.
[20]	SUN Chang-Pu . SOLAR-NEUTRINO OSCILLATIONS IN MATTER WITH VARYING DENSITY. Chinese Physics C, 1989, 13(5): 403-410.

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Jing Xu, Ming Lu, Xin-Heng Guo and Li-Jun Hu. Effects of a reverse shock wave on neutrino oscillations in a new supernova model[J]. Chinese Physics C, 2018, 42(11): 113103. doi: 10.1088/1674-1137/42/11/113103

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Received: 2018-05-14
Revised: 2018-07-31

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Supported by National Natural Science Foundation of China (11605150) and Natural Science Foundation of Shandong Province (ZR2016AQ02)

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通讯作者: 陈斌, bchen63@163.com

1.
沈阳化工大学材料科学与工程学院沈阳 110142

Effects of a reverse shock wave on neutrino oscillations in a new supernova model

Corresponding author: Jing Xu,

1. Physics Department, Yantai University, Yantai 264005, China

2. College of Nuclear Science and Techonology, Beijing Normal University, Beijing 100875, China

3. College of Mechanical and Electrical Engineering, Cangzhou Normal University, Cangzhou 061000, China

Received Date: 2018-05-14

Accepted Date: 2018-07-31

Available Online: 2018-11-05

Fund Project: Supported by National Natural Science Foundation of China (11605150) and Natural Science Foundation of Shandong Province (ZR2016AQ02)

Abstract: It is known that in supernova explosions, there might be a reverse shock wave in addition to the forward shock wave during the explosion phase, when the mass of supernova is in a certain range. In this paper, we propose to add the reverse shock wave to the previous supernova model, in which only the forward shock wave was included, and thus obtain a new model. By analyzing the resonance condition as well as the density jump in the new model and using the Landau-Zener method, an expression for the crossing probability in high density matter (P_H) is given. We proceed to study how P_H varies with time and with neutrino energy when both the reverse shock wave and the forward shock wave are considered. From comparison with the previous results, where only the effects of the forward shock wave were considered, it is clear that the reverse shock wave brings significant changes to P_H.

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Effects of a reverse shock wave on neutrino oscillations in a new supernova model

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