Physics prospects of the Jinping neutrino experiment

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 &Scaron;r&aacute;mek; 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

doi:10.1088/1674-1137/41/2/023002

Chinese Physics C> 2017, Vol. 41> Issue(2) : 023002 DOI: 10.1088/1674-1137/41/2/023002

Physics prospects of the Jinping neutrino experiment

John F. Beacom ¹ ,
Shaomin Chen ^2,, ,
Jianping Cheng ² ,
Sayed N. Doustimotlagh ² ,
Yuanning Gao ² ,
Guanghua Gong ² ,
Hui Gong ² ,
Lei Guo ² ,
Ran Han ³ ,
Hong-Jian He ² ,
Xingtao Huang ⁴ ,
Jianmin Li ² ,
Jin Li ² ,
Mohan Li ² ,
Xueqian Li ⁵ ,
Wei Liao ⁶ ,
Guey-Lin Lin ⁷ ,
Zuowei Liu ² ,
William McDonough ⁸ ,
Ondrej Šrámek ⁹ ,
Jian Tang ¹⁰ ,
Linyan Wan ² ,
Yuanqing Wang ¹¹ ,
Zhe Wang ^2,, ,
Zongyi Wang ¹¹ ,
Hanyu Wei ² ,
Yufei Xi ¹² ,
Ye Xu ¹³ ,
Xun-Jie Xu ² ,
Zhenwei Yang ² ,
Chunfa Yao ¹⁴ ,
Minfang Yeh ¹⁵ ,
Qian Yue ² ,
Liming Zhang ² ,
Yang Zhang ² ,
Zhihong Zhao ¹¹ ,
Yangheng Zheng ¹⁶ ,
Xiang Zhou ¹⁷ ,
Xianglei Zhu ² ,
Kai Zuber ¹⁸

Abstract
HTML
Reference
Related

PDF

Abstract：
The China Jinping Underground Laboratory (CJPL), which has the lowest cosmic-ray muon flux and the lowest reactor neutrino flux of any laboratory, is ideal to carry out low-energy neutrino experiments. With two detectors and a total fiducial mass of 2000 tons for solar neutrino physics (equivalently, 3000 tons for geo-neutrino and supernova neutrino physics), the Jinping neutrino experiment will have the potential to identify the neutrinos from the CNO fusion cycles of the Sun, to cover the transition phase for the solar neutrino oscillation from vacuum to matter mixing, and to measure the geo-neutrino flux, including the Th/U ratio. These goals can be fulfilled with mature existing techniques. Efforts on increasing the target mass with multi-modular neutrino detectors and on developing the slow liquid scintillator will increase the Jinping discovery potential in the study of solar neutrinos, geo-neutrinos, supernova neutrinos, and dark matter.
- CJPL ,
- Jinping neutrino experiment ,
- solar neutrino ,
- geo-neutrino ,
- supernova neutrino

References

[1]	K. J. Kang et al, Journal of Physics:Conference Series 203:012028(2010)
[2]	Q. Yue et al, Phys. Rev. D (R), 90:091701(2014)
[3]	M. J. Xiao et al, Sci China-Phys Mech Astron, 57:2024(2014)
[4]	Jianmin Li, Xiangdong Ji, Wick Haxton, and Joseph S.Y. Wang, Physics Procedia, 61:576(2015)
[5]	Ke-Jun Kang et al, Front. Phys., 8(4):412(2013)
[6]	F. Duncan, A. J. Noble, and D. Sinclair, Annu. Rev. Nucl. Part. Sci., 60:163(2010)
[7]	C. Arpesella, Appl. Radiat. Isot. 47:991, (1996)
[8]	Precision Measurement of Neutrino Oscillation Parameters and Investigation of Nuclear Georeactor Hypothesis with KamLAND, Chao Zhang, PhD. Thesis, California Institute of Technology (2011)
[9]	Y. C. WU, Chinese Phys. C, 37:086001(2013)
[10]	Corey Adams et al (LBNE Collaboration), arXiv:1307.7335(2013)
[11]	M. Yeh et al, Nucl. Instrum. Methods. A, 51:660(2011)
[12]	J. R. Alonso et al, arXiv:1409.5864v3(2014)
[13]	M. H. Li et al, Nucl. Instrum. Methods. A, 830:303(2016)
[14]	S. Agostinelli et al, Nuclear Instruments and Methods in Physics Research A, 506:250(2003)
[15]	J. Allison et al, IEEE Trans. Nucl. Sci., 53:270(2006)
[16]	J. Bahcall, SLAC Beam Line 31N1, 2-12(2001)[arXiv:astro-ph/0009259(2000)]
[17]	W.C. Haxton, Nature, 512:378(2014)
[18]	A.B. McDonald, New Journal of Physics, 6:121(2004)
[19]	Solar neutrinos the first thirty years, edited by J. Bahcall, et al, Westview Press (1994)
[20]	A. Serenelli, Eur. Phys. J. A, 52:78(2016)
[21]	Neutrino Astrophysics, J. Bahcall, Cambridge University Press (1989)
[22]	W.C. Haxton, R.G. and A. Serenelli, Astrophys. J. 687:678(2008)
[23]	A. Serenelli, C. Pea-Garay, and W.C. Haxton, Phys. Rev. D, 87:043001(2013)
[24]	E.G. Adelberger et al, Rev. Mod. Phys., 70:1265(1998)
[25]	E.G. Adelberger et al, Rev. Mod. Phys., 83:195(2011)
[26]	W. Liu et al, Nuclear Physics A, 616:131(1997)
[27]	B. Pontecorvo, Sov. Phys. JETP, 6:429(1957) and 26:984(1968)
[28]	Z. Maki, M. Nakagawa, and S. Sakata, Prog. Theor. Phys., 28:870(1962)
[29]	L. Wolfenstein, Phys. Rev. D, 17:2369(1978)
[30]	S.P. Mikheev and A.Y. Smirnov, Sov. J. Nucl. Phys., 42:913(1985); Nuovo Cimento, 9C:17(1986)
[31]	B.T. Cleveland et al, Astrophys. J. 496:505(1998)
[32]	J.N. Abdurashitov et al (SAGE Collaboration), Phys. Rev. C, 80:015807(2009)
[33]	P. Anselmann et al (GALLEX Collaboration), Phys. Lett. B, 285:376(1992)
[34]	M. Altmann et al (GNO Collaboration), Phys. Lett. B, 616:174(2005)
[35]	Y. Fukuda et al (Kamiokande Collaboration), Phys. Rev. Lett., 77:1683(1996)
[36]	S. Fukuda et al (Super-Kamiokande Collaboration), Phys. Lett. B, 539:179(2002)
[37]	Q.R. Ahmad et al (SNO Collaboration), Phys. Rev. Lett., 89:011301(2001)
[38]	G. Bellini et al (Borexino Collaboration), Phys. Rev. D, 89:112007(2014)
[39]	R.B. Leighton, R.W. Noyes, and G.W. Simon, Astrophys. J. 135:474(1962)
[40]	W.C. Haxton, R.G. Hamish Robertson, and A. Serenelli, Annu. Rev. Astron. Astrophys., 51:21(2013)
[41]	J. Bahcall and C. Pea-Garay, New J. of Phys., 6:63(2004)
[42]	J. Bahcall and R. K. Ulrich, Rev. Mod. Phys., 60:297(1988)
[43]	J. Bahcall and C. Pea-Garay, JHEP, 11:004(2003)
[44]	A. Serenelli et al, Astrophys. J. 705:L123(2009)
[45]	A. Serenelli, W. C. Haxton, and C. Pea-Garay, Astrophys. J. 743:24(2011)
[46]	P. C. de Holanda and A. Yu. Smirnov, Phys. Rev. D 69:113002(2004)
[47]	R. Bonventre et al, Phys. Rev. D, 88:053010(2013)
[48]	A. Friedland, C. Lunardini, and C. Pea-Garay, Phys. Lett. B, 594:347(2004)
[49]	M. Maltoni and A. Yu. Smirnov, Eur. Phys. J. A, 52:87(2016)
[50]	K. Abe, et al (Super-Kamiokande Collaboration), Phys. Rev. D, 94:052010(2016)
[51]	S. Abe, et al (KamLAND Collaboration), Phys. Rev. L, 100:221803(2008)
[52]	J. N. Bahcall and P. I. Krastev, Phys. Rev. C. 56:2839(1997)
[53]	J. N. Bahcall, P. I. Krastev, and A. Yu. Smirnov, Phys. Rev. D. 60:093001(1999)
[54]	A. Renshaw et al, Phys. Rev. Lett.. 112:091805(2014)
[55]	A. Serenelli, S. Basu, J.W. Ferguson, and M. Asplund, Astrophys. J. 705:L123(2009)
[56]	J. Bahcall, A. Serenelli, and S. Basu, Astrophys. J. Suppl. Ser., 165:400(2006)
[57]	S. J. Park, Phys. Rev. Lett., 57:1275(1986)
[58]	W. C. Haxton, Phys. Rev. Lett., 57:1271(1986)
[59]	P. C. de Holanda, Wei Liao, and A. Yu. Smirnov, Nucl. Phys. B, 702:307(2004)
[60]	J. Bahcall, M. H. Pinsonneault, and S. Basu, Astrophys. J. 555:990(2001)
[61]	G. L. Fogli, E. Lisi, D. Montanino, and A. Palazzo1, Phys. Rev. D, 62:113004(2000)
[62]	E. Lisi, A. Marrone, D. Montanino, A. Palazzo, and S. T. Petcov, Phys. Rev. D, 63:093002(2000)
[63]	S. Goswami and A. Y. Smirnov, Phys. Rev. D, 72:053011(2005)
[64]	C. Giunti and C. W. Kim, Fundamentals of Neutrino Physics and Astrophysics, Oxford University Press (2007)
[65]	B. Aharmim, et al (SNO Collaboration) Phys. Rev. C, 72:055502(2005)
[66]	L. Oberauera, C. Grieba, F. Feilitzscha, and I. Mannoc, Nucl. Instr. and Meth. A, 530:453(2004)
[67]	K. Abe, et. al. (Super-Kamiokande Collaboration), Phys. Rev. D 83:052010(2011)
[68]	C. Arpesella et al (Borexino Collaboration), Phys. Rev. Lett., 101:091302(2008)
[69]	G. Bellini et al (Borexino Collaboration), Phys. Rev. Lett., 107:141302(2011)
[70]	G. Bellini et al (Borexino Collaboration), Phys. Rev. Lett., 108:051302(2012)
[71]	G. Bellini et al (Borexino Collaboration), Phys. Rev. D, 82:033006(2010)
[72]	G. Bellini et al (Borexino Collaboration), Nature, 512:383(2014)
[73]	B. Aharmim et al (SNO Collaboration), Phys. Rev. C, 88:025501(2013)
[74]	F. P. An et al (Daya Bay Collaboration), Phys. Rev. Lett., 112:061801(2014)
[75]	Jia-Hua Cheng et al, Nucl. Instr. and Meth. A, 827:165(2016)
[76]	O.G. Miranda, M.A. Trtola, and J.W.F. Valle, JHEP, 10:008(2006)
[77]	M.C. Gonzalez-Garcia, P.C. de Holanda, E. Masso and R. Zukanovich Funchalc, JCAP, 0806:019(2008)
[78]	V. Barger, P. Huber, and D. Marfatia, Phys. Rev. Lett., 95:211802(2005)
[79]	M. Maltoni and A.Y. Smirnov, Eur. Phys. J. A, 52:87(2016)
[80]	William F. McDonough and Ondmřej rmek, Environ. Earth Sci. 71:3787(2014)
[81]	C Jaupart, S Labrosse, and J-C Mareschal, Treatise on geophysics, 7:253(2007)
[82]	Ondmřej mrmmek et al, Earth Planet. Sci. Lett., 361:356(2013)
[83]	G. Bellini et al, Prog. Part. Nucl. Phys., 73:1(2013)
[84]	Ondmřej mrmmek et al, Sci. Rep., 6:33034(2016)
[85]	T. Araki et al (KamLAND Collaboration), Nature, 436:499(2005)
[86]	A. Gando et al (KamLAND Collaboration), Nature Geoscience, 4:647(2011)
[87]	A. Gando et al (KamLAND Collaboration), Phys. Rev. D, 88:033001(2013)
[88]	G. Bellini et al (Borexino Collaboration), Phys. Lett. B, 687:299(2010)
[89]	G. Bellini et al (Borexino Collaboration), Phys. Lett. B, 722:295(2013)
[90]	M. Agostini et al (Borexino Collaboration), Phys. Rev. D, 92:031101(R) (2015)
[91]	Y. Huang et al, Geochem. Geophys. Geosyst., 14:2003(2013).
[92]	C. Bassin, G. Laske, and T. G. Masters (2000), The current limits of resolution for surface wave tomography in North America, EOS Trans.
[93]	N. M. Shapiro, and M. H. Ritzwoller, Geophysical Journal International, 151:88(2002)
[94]	M. Negretti, M. Reguzzoni, and D. Sampietro, A web processing service for GOCE data exploitation, in First International GOCE Solid Earth workshop, edited, Enschede, The Netherlands (2012)
[95]	Y. Huang, V. Strati, F. Mantovani, S. B. Shirey, and W. F. McDonough, Geochem. Geophys. Geosyst., 15:3925(2014)
[96]	D. F. Hollenbach and J. M. Herndon, Proc. Nat. Acad. Sci., 98:11085(2001)
[97]	S. Enomoto, Neutrino geophysics and observation of geo-neutrinos at KamLAND, Ph.D. Thesis, Tohoku University (2005)
[98]	P. Vogel and J. F. Beacom, Phys. Rev. D, 60:053003(1999)
[99]	X. B. Ma et al, Phys. Rev. C, 88:014605(2013)
[100]	M. Baldoncini et al, Phys. Rev. D, 91:065002(2015)
[101]	K.S. Hirata et al, Phys. Rev. Lett., 58:1490(1987)
[102]	K.S. Hirata et al, Phys. Rev. D, 38:448(1988)
[103]	R.M. Bionta et al, Phys. Rev. Lett., 58:1494(1987)
[104]	C.B. Bratton et al, Phys. Rev. D, 37:3361(1988)
[105]	E.N. Alekseev et al, JETP Lett., 45:589(1987)
[106]	E.N. Alekseev et al, Phys. Lett. B, 205:209(1988)
[107]	G. G. Raffelt, Proc. Int. Sch. Phys. Fermi, 182:61(2012)[arXiv:1201.1637]
[108]	R.N. Mohapatra and P.B. Pal, Massive Neutrinos in Physics and Astrophysics, World Scientific Publishing Co. Pte. Ltd. 2004
[109]	C. Lunardini and A.Y. Smirnov, JCAP, 0306:009(2003)
[110]	P.D. Serpico, S. Chakraborty, T. Fischer et al, Phys. Rev. D, 85:085031(2012)
[111]	C.D. Ott, E.P. O'Connor, S. Gossan et al, Nucl. Phys. B (Proc. Suppl.), 235-236:381(2013)
[112]	S. Ando, J.F. Beacom, H. Yksel, Phys. Rev. Lett., 95:171101(2005)
[113]	K. Scholberg et al, New J. Phys., 6:114(2004)
[114]	S. M. Adams et al, J. Astrophys., 778:164(2013)
[115]	G. Raffelt, I. Tamborra, B. Mller and L. Hdepohl and H.T. Janka, Phys. Rev. D, 86:125031(2012)
[116]	K. Scholberg, Annu. Rev. Nucl. Part. Sci. 62:81(2012)
[117]	John F. Beacom, Will M. Farr and Petr Vogel, Phys. Rev. D, 66:033001(2002)
[118]	Basudeb Dasgupta and John F. Beacom, Phys. Rev. D, 83:113006(2011)
[119]	B. von Krosigk et al, Eur. Phys. J. C, 73:2390(2013)
[120]	Hanyu Wei et al, Astropart. Phys., 75:38(2016)
[121]	F. P. An et al (Daya Bay Collaboration), Phys. Rev. D (R), 90:071101(2014)
[122]	F. P. An et al (Daya Bay Collaboration), Phys. Rev. D, 93:072011(2016)
[123]	M. Ikeda et al (Super-Kamiokande Collaboration), Astrophys. J. 669:519(2007)
[124]	John F. Beacom and P. Vogel, Phys. Rev. D, 60:033007(1999)
[125]	M. Malek et al (Super-Kamiokande Collaboration), Phys. Rev. Lett., 90:061101(2003)
[126]	K. Bays et al (Super-Kamiokande Collaboration), Phys. Rev. D, 85:052007(2012)
[127]	H. Zhang et al (Super-Kamiokande Collaboration), Astropart. Phys., 60:41(2015)
[128]	A. Gando et al (KamLAND Collaboration), Astrophys. J. 745:193(2012)
[129]	G. Bellini et al (Borexino Collaboration), Phys. Lett. B, 696:191(2011)
[130]	B. Aharmim et al (SNO Collaboration), Astrophys. J. 653:1545(2006)
[131]	J. F. Beacom, Annu. Rev. Nucl. Part. Sci., 60:439(2010)
[132]	S. Ando, K. Sato and T. Totani, Astropart. Phys., 18:307(2003); J. Phys. Soc. Jpn. (Suppl. B), 77:9(2008)
[133]	T. Totani and K. Sato, Astropart. Phys., 3:367(1995)
[134]	R. A Malaney, Astropart. Phys., 7:125(1997)
[135]	D. H. Hartmann and S. E. Woosley, Astropart. Phys., 7:137(1997)
[136]	M. Kaplinghat, G. Steigman and T. P. Walker, Phys. Rev. D, 62:043001(2000)
[137]	L. Strigari, M. Kaplinghat, G. Steigman and T. Walker, JCAP, 0403:007(2004)
[138]	T. Totani, K. Sato and Y. Yoshii, Astrophys. J. 460:303(1996)
[139]	S. Horiuchi, J. F. Beacom and E. Dwek, Phys. Rev. D, 79:083013(2009)
[140]	M. Fukugita and M. Kawasaki, Mon. Not. Roy. Astron. Soc., 340:L7(2003)
[141]	C. Lunardini, Phys. Rev. Lett., 102:231101(2009)
[142]	J. F. Beacom and M. R. Vagins, Phys. Rev. Lett., 93:171101(2004)
[143]	M. Wurm, Astropart. Phys., 35:685(2012)
[144]	Jingyi Yu, Zhe Wang, and Shaomin Chen, Chin. Phys. C, 39:056102(2015)
[145]	F. P. An et al (Daya Bay Collaboration), Chin. Phys. C, 37:011001(2013)
[146]	S. Abe et al (KamLAND Collaboration), Phys. Rev. C, 81:025807(2010)
[147]	Shirley Weishi Li and John F. Beacom, Phys. Rev C, 89:045801(2014)
[148]	Shirley Weishi Li and John F. Beacom, Phys. Rev. D, 92:105033(2015)
[149]	Shirley Weishi Li and John F. Beacom, Phys. Rev. D, 91:105005(2015)
[150]	O. Peres and A. Smirnov, Phys. Rev. D, 79:113002(2009)
[151]	G. Battistoni, A. Ferrari, T. Montaruli and P.R. Sala, Astropart. Phys., 23:526(2005)
[152]	R. Moellenberg, Ph. D. thesis, Technische Universitmt Mmnchen (2009)
[153]	J. F. Navarro, C. S. Frenk and S. D. M. White, Astrophys. J. 462:563(1996)
[154]	B. Moore, T. R. Quinn, F. Governato, J. Stadel and G. Lake, Mon. Not. Roy. Astron. Soc., 310:1147(1999)
[155]	A. V. Kravtsov, A. A. Klypin, J. S. Bullock and J. R. Primack, Astrophys. J. 502:48(1998)
[156]	H. Yuksel, S. Horiuchi, J. F. Beacom and S. Ando, Phys. Rev. D, 76:123506(2007)
[157]	M. Wurm et al (LENA Collaboration), Astropart. Phys., 35:685(2012)
[158]	S. Palomares-Ruiz and S. Pascoli, Phys. Rev., D 77:025025(2008)
[159]	J. Silk, K. A. Olive and M. Srednicki, Phys. Rev. Lett., 55:257(1985)
[160]	L. M. Krauss, K. Freese, W. Press and D. Spergel, Astrophys. J. 299:1001(1985)
[161]	K. Freese, Phys. Lett. B, 167:295(1986)
[162]	L. M. Krauss, M. Srednicki and F. Wilczek, Phys. Rev. D, 33:2079(1986)
[163]	T. K. Gaisser, G. Steigman and S. Tilav, Phys. Rev. D, 34:2206(1986)
[164]	K. Griest and D. Seckel, Nucl. Phys. B, 283:681(1987)[Erratum-ibid. B, 296:1034(1988)]
[165]	A. Gould, Astrophys. J. 321:560(1987)
[166]	G. Wikstrom and J. Edsjo, JCAP, 0904:009(2009)
[167]	T. Tanaka et al (Super-Kamiokande Collaboration), Astrophys. J. 742:78(2011)
[168]	P. Gondolo, J. Edsjo, P. Ullio, L. Bergstrom, M. Schelke and E. A. Baltz, JCAP, 0407:008(2004)
[169]	K. Choi et al (Super-Kamiokande Collaboration), Phys. Rev. Lett., 114:141301(2015)
[170]	Nicols Bernal, Justo Martn-Albo and Sergio Palomares-Ruiz, JCAP, 1308:011(2013)
[171]	Carsten Rott, Jennifer M. Siegal-Gaskins, and John F. Beacom, Phys. Rev. D, 88:055005(2013)

[1]	Jiemiao Wang , Hulin Wang , Dongliang Zhang . Solar neutrino background in high-pressure gaseous ⁸²SeF₆ TPC neutrinoless double beta decay experiments. Chinese Physics C, 2024, 48(4): 043003. doi: 10.1088/1674-1137/ad2675
[2]	M. Novello , C. E. L. Ducap . How can the neutrino interact with the electromagnetic field?. Chinese Physics C, 2018, 42(1): 013102. doi: 10.1088/1674-1137/42/1/013102
[3]	Takuya Morozumi , Hideaki Okane , Hiroki Sakamoto , Yusuke Shimizu , Kenta Takagi , Hiroyuki Umeeda . Phenomenological aspects of possible vacua of a neutrino flavor model. Chinese Physics C, 2018, 42(2): 023102. doi: 10.1088/1674-1137/42/2/023102
[4]	Jing Xu , Ming Lu , Xin-Heng Guo , Li-Jun Hu . Effects of a reverse shock wave on neutrino oscillations in a new supernova model. Chinese Physics C, 2018, 42(11): 113103. doi: 10.1088/1674-1137/42/11/113103
[5]	Nai-Bo Zhang , Shou-Yu Wang , Bin Qi , Jian-Hua Gao , Bao-Yuan Sun . Neutrino emissivity of the nucleon direct URCA process for rotational traditional and hyperonic neutron stars. Chinese Physics C, 2017, 41(7): 075101. doi: 10.1088/1674-1137/41/7/075101
[6]	Zhi-zhong Xing , Jing-yu Zhu . Neutrino mass ordering and μ-τ reflection symmetry breaking. Chinese Physics C, 2017, 41(12): 123103. doi: 10.1088/1674-1137/41/12/123103
[7]	Shivaramakrishna Singirala . Implications of fermionic dark matter on recent neutrino oscillation data. Chinese Physics C, 2017, 41(4): 043102. doi: 10.1088/1674-1137/41/4/043102
[8]	Ming-Yang Huang . Study of accelerator neutrino detection at a spallation source. Chinese Physics C, 2016, 40(6): 063002. doi: 10.1088/1674-1137/40/6/063002
[9]	Ran Han , Yu-Feng Li , Liang Zhan , William F McDonough , Jun Cao , Livia Ludhova . Potential of geo-neutrino measurements at JUNO. Chinese Physics C, 2016, 40(3): 033003. doi: 10.1088/1674-1137/40/3/033003
[10]	LI Zhi-Hui , TANG Jing-Yu . A CW superconducting linac as the proton driver for a medium baseline neutrino beam in China. Chinese Physics C, 2014, 38(12): 127001. doi: 10.1088/1674-1137/38/12/127001
[11]	ZHAO Jie , YU Ze-Yuan , LIU Jiang-Lai , LI Xiao-Bo , ZHANG Fei-Hong , XIA Dong-Mei . ¹³C(α, n)¹⁶O background in a liquid scintillator based neutrino experiment. Chinese Physics C, 2014, 38(11): 116201. doi: 10.1088/1674-1137/38/11/116201
[12]	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
[13]	YANG Zhen-Wei , DING Ming-Ming , CHEN Shao-Min , WANG Zhe , ZHANG Feng , GAO Yuan-Ning . Simulation study of neutrino nucleus crosssection measurement in a segmented detectorat a spallation neutron source. Chinese Physics C, 2012, 36(6): 538-543 . doi: 10.1088/1674-1137/36/6/010
[14]	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
[15]	LÜ Lei , WANG Wen-Yu , XIONG Zhao-Hua . Can a non-unitary effect be prominent in neutrino oscillation measurements?. Chinese Physics C, 2010, 34(12): 1791-1796. doi: 10.1088/1674-1137/34/12/003
[16]	Young Bing-Lin . Current status of neutrino physics. Chinese Physics C, 2010, 34(2): 287-298. doi: 10.1088/1674-1137/34/2/026
[17]	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
[18]	AN Feng-Peng , TIAN Xin-Chun , ZHAN Liang , CAO Jun . Systematic impact of spent nuclear fuel on θ₁₃ sensitivity at reactor neutrino experiment. Chinese Physics C, 2009, 33(9): 711-716. doi: 10.1088/1674-1137/33/9/001
[19]	LIU Jing-Jing , LUO Zhi-Quan . Pair neutrino energy loss for nuclei ⁵⁶Fe at the late stages of stellar evolution. Chinese Physics C, 2008, 32(8): 617-619. doi: 10.1088/1674-1137/32/8/005
[20]	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

Access

Get Citation

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 and Kai Zuber. Physics prospects of the Jinping neutrino experiment[J]. Chinese Physics C, 2017, 41(2): 023002. doi: 10.1088/1674-1137/41/2/023002

RIS(for EndNote,Reference Manager,ProCite)

BibTex

Txt

Milestone

Received: 2016-09-13
Revised: 2016-10-26

Fund

Supported by the National Natural Science Foundation of China (11235006, 11475093, 11135009, 11375065, 11505301, and 11620101004), the Tsinghua University Initiative Scientific Research Program (20121088035, 20131089288, and 20151080432), the Key Laboratory of Particle Radiation Imaging (Tsinghua University), the CAS Center for Excellence in Particle Physics (CCEPP), U.S. National Science Foundation Grant PHY-1404311 (Beacom), and U.S. Department of Energy under contract DE-AC02-98CH10886 (Yeh).

Article Metric

Article Views(1591)
PDF Downloads(72)
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

Physics prospects of the Jinping neutrino experiment

Abstract：

References

Access

Article Metrics

Metrics

通讯作者: 陈斌, bchen63@163.com

Email This Article

Physics prospects of the Jinping neutrino experiment

Corresponding author: Shaomin Chen,

Corresponding author: Zhe Wang,

HTML

目录