New limits on neutrino decay from the Glashow resonance of high-energy cosmic neutrinos
- Published: 22 Jun 2020
- Publisher: Zenodo
- Niels Bohr Institute Denmark
mbustamante@nbi.ku.dk; ORCID: 0000-0001-6923-
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Related research
- Niels Bohr Institute Denmark
mbustamante@nbi.ku.dk; ORCID: 0000-0001-6923-
0865 [1] P. B. Pal and L. Wolfenstein, Phys. Rev. D 25, 766
(1982). [2] Y. Hosotani, Nucl. Phys. B 191, 411 (1981). [3] J. F. Nieves, Phys. Rev. D 28, 1664 (1983). [4] J. N. Bahcall, N. Cabibbo, and A. Yahil, Phys. Rev. [OpenAIRE]
Lett. 28, 316 (1972). [5] Y. Chikashige, R. N. Mohapatra, and R. D. Peccei,
Phys. Rev. Lett. 45, 1926 (1980). [6] G. B. Gelmini, S. Nussinov, and M. Roncadelli,
Nucl. Phys. B 209, 157 (1982). [7] R. Tomas, H. Pas, and J. W. F. Valle, Phys. Rev. D
64, 095005 (2001), arXiv:hep-ph/0103017. [8] S. Hannestad and G. Ra elt, Phys. Rev. D 72, 103514
(2005), arXiv:hep-ph/0509278 [hep-ph]. [9] S. Zhou, Phys. Lett. B 659, 336 (2008), arXiv:0706.0302
[hep-ph]. [10] S.-L. Chen, X.-G. He, and H.-C. Tsai, JHEP 11, 010
(2007), arXiv:0707.0187 [hep-ph]. [11] X.-Q. Li, Y. Liu, and Z.-T. Wei, Eur. Phys. J. C 56,
97 (2008), arXiv:0707.2285 [hep-ph]. [12] M. Escudero and M. Fairbairn, Phys. Rev. D 100,
103531 (2019), arXiv:1907.05425 [hep-ph]. [13] M. G. Aartsen et al. (IceCube), Phys. Rev. Lett. 111,
021103 (2013), arXiv:1304.5356 [astro-ph.HE]. [14] M. G. Aartsen et al. (IceCube), Science 342, 1242856
(2013), arXiv:1311.5238 [astro-ph.HE]. [15] M. G. Aartsen et al. (IceCube), Phys. Rev. Lett. 113,
101101 (2014), arXiv:1405.5303 [astro-ph.HE]. [16] M. G. Aartsen et al. (IceCube), Phys. Rev. Lett. 115, [OpenAIRE]