Detection of supernova neutrinos at spallation neutron sources

[1]
K. Kotake, K. Sato and K. Takahashi, Rept. Prog. Phys., 69:971-1143(2006)
[2]
A. Mirizzi, I. Tamborra, H. T. Janka et al, arXiv:1508. 00785
[3]
X. H. Guo, M. Y. Huang and B. L. Young, Chin. Phys. C, 34(2):257-261(2010)
[4]
K. Hirata, T. Kajita, M. Koshiba et al, Phys. Rev. Lett., 58:1490-1493(1987)
[5]
R. M. Bionta, G. Blewitt, C. B. Bratton et al, Phys. Rev. Lett., 58:1494-1496(1987)
[6]
K. Scholberg, Ann. Rev. Nucl. Part. Sci., 62:81-103(2012)
[7]
CSNS Project Team, China Spallation Neutron Source Feasi-bility Research Report, Institute of High Energy Physics and Institute of Physics, Chinese Academy of Sciences, 2009(in Chinese)
[8]
J. Wei, S. N. Fu, J. Y. Tang et al, Chin. Phys. C, 33(11):1033-1042(2009)
[9]
S. Wang, S. X. Fang, S. N. Fu et al, Chin. Phys. C, 33 (Suppl. II):1-3(2009)
[10]
M. Y. Huang, S. Wang, J. Qiu et al, Chin. Phys. C, 37 (6):067001(2013)
[11]
M. Y. Huang, Chin. Phys. C, 40(6):063002(2016)
[12]
J. R. Wilson, Numerical Astrophysics, edited by J. M. Centrella, J. M. LeBlanc, and R. L. Bowers (Boston:Jones and Bartlett, 1985), p. 422-434
[13]
R. C. Schirato and G. M. Fuller, arXiv:astro-ph/0205390
[14]
L. Hudepohl, B. Muller, H. T. Janka et al, Phys. Rev. Lett., 104:251101(2010)
[15]
S. Sarikas, G. G. Raffelt, L. Hudepohl et al, Phys. Rev. Lett., 108:061101(2012)
[16]
L. Wolfenstein, Phys. Rev. D, 17:2369-2374(1978)
[17]
S. P. Mikheyev and A. Y. Smirnov, Sov. J. Nucl. Phys., 42:913-917(1985)
[18]
T. K. Kuo and J. Pantaleone, Rev. Mod. Phys., 61:937-979(1989)
[19]
M. Blennow and A. Y. Smirnov, Adv. High Energy Phys., 2013:972485(2013)
[20]
B. Dasgupta, A. Dighe and A. Mirizzi, Phys. Rev. Lett., 101:171801(2008)
[21]
H. Y. Duan, G. M. Fuller and J. Carlson, Comp. Scie. Disc., 1:015007(2008)
[22]
H. Y. Duan, G. M. Fuller and Y. Z. Qian, Ann. Rev. Nucl. Part. Sci., 60:569-594(2010)
[23]
A. S. Dighe and A. Y. Smirnov, Phys. Rev. D, 62:033007(2000)
[24]
A. N. Ioannisian and A. Y. Smirnov, Phys. Rev. Lett., 93:241801(2004)
[25]
X. H. Guo, M. Y. Huang and B. L. Young, Phys. Rev. D, 79:113007(2009)
[26]
M. Y. Huang, X. H. Guo and B. L. Young, Phys. Rev. D, 82:033011(2010)
[27]
P. Antonioli, R. T. Fienberg, F. Fleurot et al, New J. Phys., 6:114(2004)
[28]
T. Totani, K. Sato, H. E. Dalhed et al, Astrophys. J., 496, 216-225(1998)
[29]
M. T. Keil, G. G. Raffelt and H. T. Janka, Astrophys. J., 590, 971-991(2003)
[30]
C. Giunti and C. W. Kim, Fundamentals of Neutrino Physics and Astrophysics (New York:Oxford, 2007), p. 511-539
[31]
R. N. Mohapatra and P. B. Pal, Massive Neutrino in Physics and Astrophysics (Singapore:World Scientific, 2004), p. 340-358
[32]
H. T. Janka and W. Hillebrandt, Astron. Astrophys., 224, 49-56(1989)
[33]
H. T. Janka and W. Hillebrandt, Astron. Astrophys. Suppl. Ser., 78:375-397(1989)
[34]
S. Chakraborty, S. Choubey, S. Goswami et al, J. Cosmol. Astropart. Phys., 1006:007(2010)
[35]
L. Cadonati, F. P. Calaprice and M C. Chen, Astropart. Phys., 16:361-372(2002)
[36]
J. Arafune and M. Fukugita, Phys. Rev. Lett., 59:367-369(1987)
[37]
M. Fukugita, Y. Kohyama and K. Kubodera, Phys Lett. B, 212:139-144(1988)
[38]
E. Kolbe, K. Langanke and P. Vogel, Nucl. Phys. A, 652:91-100(1999)
[39]
C. Athanassopulos, L. B. Auerbach, D. A. Bauer et al, Phys. Rev. Lett., 75:2650-2653(1995)
[40]
C. Athanassopulos, L. B. Auerbach, R. L. Burman et al, Phys. Rev. C, 54:2685-2708(1996)
[41]
R. C. Allen, H. H. Chen, P. J. Doe et al, Phys. Rev. D, 47:11-28(1993)
[42]
R. Imlay and G. J. VanDalen, J. Phys. G:Nucl. Part. Phys., 29:2647-2664(2003)
[43]
L. B. Auerbach, R. L. Burman, D. O. Caldwell et al, Phys. Rev. D, 66:015501(2002)
[44]
X. H. Guo et al (Daya Bay Collaboration), arXiv:hep-ex/0701029
[45]
K. Nakazato, Phys. Rev. D, 88:083012(2013)
[46]
H. Zhang, K. Abe, Y. Hayato et al, Astropart. Phys., 60:41-46(2015)
[47]
G. J. VanDalen, arXiv:nucl-ex/0309014
[48]
K. A. Olive, K. Agashe, C. Amsler et al, Chin. Phys. C, 38(9):090001(2014)
[49]
F. Gapozzi, G. L. Fogli, E. Lisi et al, Phys. Rev. D, 89:093018(2014)
[50]
I. Tamborra, G. G. Raffelt, F. Hanke et al, Phys. Rev. D, 90:045032(2014)
[51]
R. L. Burman and W. C. Louis, J. Phys. G:Nucl. Part. Phys., 29:2499-2512(2003)
[52]
C. Athanassopoulos, L. B. Auerbach, D. Bauer et al, Nucl. Instrum. Methods Phys. Res. A, 388:149-172(1997)
[53]
G. Drexlin, V. Eberhard, H. Gemmeke et al, Nucl. Instrum. Methods Phys. Res. A, 289:490-495(1990)
[54]
R. L. Burman, A. C. Dodd and P. Plischke, Nucl. Instrum. Methods Phys. Res. A, 368:416-424(1996)
[55]
B. Boardman, Spallation Neutron Source:Description of Accelerator and Target, RL-82-006, 1982
[56]
SNS Project Team, Spallation Neutron Source Design Manual, June, 1998
[57]
Boardman B. Spallation Neutron Source: Description of Accel-erator and Target. RL-82-006, 1982
[58]
ESS Central Project Team, ESS Technical Design Report, ESS-doc-274-v15, 2015
[59]
SNS Project Team. Spallation Neutron Source Design Manual. June, 1998
[60]
ESS Central Project Team. ESS Technical Design Report. ESS-doc-274-v15, 2015
[61]
M. Elnimr, I. Stancu, M. Yeh et al, arXiv:1307.7097
[62]
E. Baussan, M. Blennow, M. Bogomilov et al, Nucl. Phys. B, 885:127-149(2014)
[63]
Elnimr M, Stancu I, Yeh M et al. The OscSNS White Paper. arXiv:1307.7097 [physics.ins-det]
[64]
Baussan E, Blennow M, Bogomilov M et al. Nucl. Phys. B,2014, 885: 127-149
[65]
E. Kolbe, K. Langanke and P. Vogel, Phys. Rev. D, 66:013007(2002)
[66]
Kolbe E, Langanke K, Vogel P. Phys. Rev. D, 2002, 66: 013007
[67]
K. Langanke, P. Vogel and E. Kolbe, Phys. Rev. Lett., 76:2629-2632(1996)
[68]
Langanke K, Vogel P, Kolbe E. Phys. Rev. Lett., 1996, 76:2629-2632
[69]
S. Nussinov and R. Shrock, Phys. Rev. Lett., 86:2223-2226(2001) 1996, 368: 416-424
[70]
Nussinov S, Shrock R. Phys. Rev. Lett., 2001, 86: 2223-2226