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

Abstract
HTML
Reference
Related

PDF

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)

[1]	Yessica Lenis , R. Martinez-Ramirez , Eduardo Peinado , William A. Ponce . Two-zero textures for Dirac Neutrinos. Chinese Physics C, 2025, 49(3): 1-9.
[2]	M.V. Smirnov , Zhoujun Hu , Shuaijie Li , Jiajie Ling . Potential of octant degeneracy resolution in JUNO. Chinese Physics C, 2019, 43(3): 033001. doi: 10.1088/1674-1137/43/3/033001
[3]	Kuan Liu , Chun-Sheng An , Xin Li , Hai-Nan Lin . Matter effects and coherent effect of neutrinos produced from ${{\gamma}}$-ray bursts. Chinese Physics C, 2019, 43(10): 105102. doi: 10.1088/1674-1137/43/10/105102
[4]	Yueling Yang , Yupei Guo , Junfeng Sun , Na Wang , Qin Chang , Gongru Lu . B_u → ψM decays and S-D wave mixing effects. Chinese Physics C, 2018, 42(11): 113102. doi: 10.1088/1674-1137/42/11/113102
[5]	John F. Beacom , Shaomin Chen , Jianping Cheng , Sayed N. Doustimotlagh , Yuanning Gao , Guanghua Gong , Hui Gong , Lei Guo , Ran Han , Hong-Jian He , Xingtao Huang , Jianmin Li , Jin Li , Mohan Li , Xueqian Li , Wei Liao , Guey-Lin Lin , Zuowei Liu , William McDonough , Ondrej Šrámek , Jian Tang , Linyan Wan , Yuanqing Wang , Zhe Wang , Zongyi Wang , Hanyu Wei , Yufei Xi , Ye Xu , Xun-Jie Xu , Zhenwei Yang , Chunfa Yao , Minfang Yeh , Qian Yue , Liming Zhang , Yang Zhang , Zhihong Zhao , Yangheng Zheng , Xiang Zhou , Xianglei Zhu , Kai Zuber . Physics prospects of the Jinping neutrino experiment. Chinese Physics C, 2017, 41(2): 023002. doi: 10.1088/1674-1137/41/2/023002
[6]	Ming-Yang Huang , Xin-Heng Guo , Bing-Lin Young . Detection of supernova neutrinos at spallation neutron sources. Chinese Physics C, 2016, 40(7): 073102. doi: 10.1088/1674-1137/40/7/073102
[7]	Yu-feng Li , Yi-fang Wang , Zhi-zhong Xing . Terrestrial matter effects on reactor antineutrino oscillations at JUNO or RENO-50: how small is small?. Chinese Physics C, 2016, 40(9): 091001. doi: 10.1088/1674-1137/40/9/091001
[8]	Long Zhu , Jun Su , Ching-Yuan Huang , Feng-Shou Zhang . Effects of entrance channel on fusion probability in hot fusion reactions. Chinese Physics C, 2016, 40(12): 124105. doi: 10.1088/1674-1137/40/12/124105
[9]	HAN Jie , BAO Jing-Dong . Modified fusion probability by reflection boundary. Chinese Physics C, 2015, 39(5): 054104. doi: 10.1088/1674-1137/39/5/054104
[10]	ZHANG Yi-Chun , CHEN Xiao-Su , HE Miao , HUANG Xing-Tao , WANG Meng , LI Wei-Dong , ZHANG Zi-Ping . Mixing MC events in reactor neutrino experiment. Chinese Physics C, 2013, 37(1): 016201. doi: 10.1088/1674-1137/37/1/016201
[11]	MO Xiao-Hu , ZHANG Jian-Yong , ZHANG Qing-Jiang , Achasov Mikhail , CAI Xiao , FU Cheng-Dong , Harris Fred , LIU Qian , Muchnoi Nikolay , QIN Qing , QU Hua-Min , WANG Yi-Fang , XU Jin-Qiang , ZHANG Tian-Bao . Study of radiation background at the north crossing point of the BEPCⅡ in collision mode. Chinese Physics C, 2011, 35(7): 642-655. doi: 10.1088/1674-1137/35/7/009
[12]	WANG Bin , CHEN Ya-Zheng , LI Xue-Qian . Earthquake forecast via neutrino tomography. Chinese Physics C, 2011, 35(4): 325-332. doi: 10.1088/1674-1137/35/4/002
[13]	Young Bing-Lin . Current status of neutrino physics. Chinese Physics C, 2010, 34(2): 287-298. doi: 10.1088/1674-1137/34/2/026
[14]	GUO Xin-Heng , HUANG Ming-Yang , Young Bing-Lin . Supernova neutrino detection on earth. Chinese Physics C, 2010, 34(2): 257-261. doi: 10.1088/1674-1137/34/2/020
[15]	LI Hong-Nian , YING Li-Jian , NI Jing-Fu , LI Gang , WANG Peng , KURASH Ibrahim , QIAN Hai-Jie , . Fine structure of K₃C₆₀ photoionization cross-section oscillations. Chinese Physics C, 2009, 33(11): 991-995. doi: 10.1088/1674-1137/33/11/012
[16]	QI Bin , MENG Jie , ZHANG Shuang-Quan , WANG Shou-Yu , PENG Jing . Chiral doublet bands and energy-level crossing. Chinese Physics C, 2009, 33(S1): 43-45. doi: 10.1088/1674-1137/33/S1/014
[17]	WANG Hai-Jun . Lorentz violation constrained by triplicity of lepton families and neutrino oscillations. Chinese Physics C, 2009, 33(6): 487-493. doi: 10.1088/1674-1137/33/6/016
[18]	GU Pei-Hong , BI Xiao-Jun , FENG Bo , YOUNG Bing-Lin , ZHANG Xin-Min . Detecting dark energy in long baseline neutrino oscillations. Chinese Physics C, 2008, 32(7): 530-535. doi: 10.1088/1674-1137/32/7/004
[19]	Hou Boyu , Shi Kangjie , Yue Ruihong . The Crossing Matrices and Correlation Function of SU_K(2) Wess-Zumino-Witten Model with Fractional Level. Chinese Physics C, 1992, 16(S2): 163-172.
[20]	Xing Zheng , Wu Xingju . Rotational Effect on Electromagnetic Transitions After Band-Crossing. Chinese Physics C, 1991, 15(S1): 93-100.

Access

Get Citation

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

RIS(for EndNote,Reference Manager,ProCite)

BibTex

Txt

Milestone

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

Fund

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

Article Metric

Article Views(1700)
PDF Downloads(28)
Cited by(0)

Policy on re-use

To reuse of subscription content published by CPC, the users need to request permission from CPC, unless the content was published under an Open Access license which automatically permits that type of reuse.

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

Abstract：

References

Access

Article Metrics

Metrics

通讯作者: 陈斌, bchen63@163.com

Email This Article

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

Corresponding author: Jing Xu,

HTML

目录