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[hep-ph]
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in Super-Kamiokande I. Phys. Rev. D 91, 072006 (2015)
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p → e + π 0 and p → μ + π 0 in 0.31 megaton·years exposure of the SuperKamiokande water Cherenkov detector. Phys. Rev. D 95(1), 012004 (2017)
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A.S. Joshipura, E. Masso, S. Mohanty, Constraints on decay plus oscillation
solutions of the solar neutrino problem. Phys. Rev. D 66, 113008 (2002)
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7. K. Agashe, P. Du, M. Ekhterachian, C.S. Fong, S. Hong, L. Vecchi, Natural
seesaw and leptogenesis from hybrid of high-scale type I and TeV-scale inverse.
JHEP 1904, 029 (2019);
F. Bazzocchi, D.G. Cerdeno, C. Munoz, J.W.F. Valle, Calculable inverse-seesaw
neutrino masses in supersymmetry. Phys. Rev. D 81, 051701 (2010)
8. V. Agrawal, S.M. Barr, J.F. Donoghue, D. Seckel, Viable range of the mass scale
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the India-based neutrino observatory (INO). Pramana 88(5), 79 (2017)
© The Editor(s) (if applicable) and The Author(s), under exclusive license to Springer
Nature Switzerland AG 2021
R. N. Mohapatra, The Neutrino Story: One Tiny Particle’s Grand Role in the Cosmos,
https://doi.org/10.1007/978-3-030-51846-2
209
1. K.N. Abazajian et al., Light sterile neutrinos: a white paper. arXiv:1204.5379
[hep-ph]
2. K. Abe et al., Super-Kamiokande Collaboration, The search for n − ¯
n oscillation
in Super-Kamiokande I. Phys. Rev. D 91, 072006 (2015)
3. K. Abe et al., Super-Kamiokande Collaboration, Search for proton decay via
p → e + π 0 and p → μ + π 0 in 0.31 megaton·years exposure of the SuperKamiokande water Cherenkov detector. Phys. Rev. D 95(1), 012004 (2017)
4. G.V. Achar et al. Phys. Lett. 18 , 196 (1965)
5. A. Acker, S. Pakvasa, Solar neutrino decay. Phys. Lett. B 320, 320 (1994);
A.S. Joshipura, E. Masso, S. Mohanty, Constraints on decay plus oscillation
solutions of the solar neutrino problem. Phys. Rev. D 66, 113008 (2002)
6. F.C. Adams, G. Laughlin, A dying universe: the long term fate and evolution of
astrophysical objects. Rev. Mod. Phys. 69, 337 (1997);
D.A. Dicus, J.T. Letaw, D.C. Teplitz, V.L. Teplitz, The future of the universe.
Sci. Am. 248, 74 (1983)
7. K. Agashe, P. Du, M. Ekhterachian, C.S. Fong, S. Hong, L. Vecchi, Natural
seesaw and leptogenesis from hybrid of high-scale type I and TeV-scale inverse.
JHEP 1904, 029 (2019);
F. Bazzocchi, D.G. Cerdeno, C. Munoz, J.W.F. Valle, Calculable inverse-seesaw
neutrino masses in supersymmetry. Phys. Rev. D 81, 051701 (2010)
8. V. Agrawal, S.M. Barr, J.F. Donoghue, D. Seckel, Viable range of the mass scale
of the standard model. Phys. Rev. D 57, 5480 (1998)
9. S. Ahmed et al., ICAL Collaboration, Physics potential of the ICAL detector at
the India-based neutrino observatory (INO). Pramana 88(5), 79 (2017)
© The Editor(s) (if applicable) and The Author(s), under exclusive license to Springer
Nature Switzerland AG 2021
R. N. Mohapatra, The Neutrino Story: One Tiny Particle’s Grand Role in the Cosmos,
https://doi.org/10.1007/978-3-030-51846-2
209