Acquire information about neutrino parameters by detecting supernova neutrinos

Preprint English OPEN
Huang, Ming-Yang; Guo, Xin-Heng; Young, Bing-Lin;
(2010)
  • Related identifiers: doi: 10.1103/PhysRevD.82.033011
  • Subject: High Energy Physics - Phenomenology | Astrophysics - High Energy Astrophysical Phenomena | Astrophysics - Cosmology and Nongalactic Astrophysics
    arxiv: Astrophysics::Galaxy Astrophysics | Physics::Instrumentation and Detectors | High Energy Physics::Phenomenology | Astrophysics::High Energy Astrophysical Phenomena | High Energy Physics::Experiment

We consider the supernova shock effects, the Mikheyev-Smirnov-Wolfenstein (MSW) effects, the collective effects, and the Earth matter effects in the detection of type II supernova neutrinos on the Earth. It is found that the event number of supernova neutrinos depends o... View more
  • References (59)
    59 references, page 1 of 6

    [1] K. Kotake, K. Sato, and K. Takahashi, Rept. Prog. Phys. 69, 971 (2006) [arXiv:astro-ph/0509456].

    [2] K. Hirata et al., Phys. Rev. Lett. 58, 1490 (1987); R.M. Bionta et al., Phys. Rev. Lett. 58, 1494 (1987); V. Trimble, Rev. Mod. Phys. 60, 859 (1988); W.D. Arnett, J.N. Bahcall, R.P. Kirshner, and S.E. Woosley, Ann. Rev. Astron. Astrophys. 27, 629 (1989); W. Hillebrandt and P. Ho¨flich, Rep. Prog. Phys. 52, 1421 (1989); D.N. Schramm, Phys. Rep. 189, 89 (1990); M. Koshiba, Phys. Rep. 220, 229 (1992); R. McCray, Ann. Rev. Astron. Astrophys. 31, 175 (1993).

    [3] A. Dighe, J. Phys. Conf. Ser. 136, 022041 (2008) [arXiv:0809.2977], AIP Conf. Proc. 981, 75 (2008) [arXiv:0712.4386].

    [4] X.-H. Guo, M.-Y. Huang, and B.-L. Young, Chin. Phys. C 34, 257 (2010) [arXiv:0905.1534].

    [5] G.G. Raffelt, Stars as Laboratories for Fundamental Physics (The University of Chicago Press, Chicago 1996).

    [6] B. Dasgupta, A. Dighe, and A. Mirizzi, Phys. Rev. Lett. 101, 171801 (2008) [arXiv:0802.1481].

    [7] S. Skadhauge and R.Z. Funchal, J. Cosmol. Astropart. Phys. 04, 014 (2007) [arXiv:hep-ph/0611194].

    [8] J.F. Beacom, R.N. Boyd, and A. Mezzacappa, Phys. Rev. Lett. 85, 3568 (2000) [arXiv:hep-ph/0006015], Phys. Rev. D 63, 073011 (2001) [arXiv:astro-ph/0010398].

    [9] [Daya Bay Collaboration] X.-H. Guo et al., A precision measurement of the neutrino mixing angle θ13 using reactor antineutrinos at Daya Bay, arXiv:hep-ex/0701029.

    [10] P. Antonioli et al., New J. Phys. 6, 114 (2004) [arXiv:astro-ph/0406214].

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