Other Readings on Neutrinos

References

[1-1]

Theory of neutral particles: McLennan-Case construct for neutrino, its generalization, and a fundamentally new wave equation, Ahluwalia, D. V., Int. J. Mod. Phys. A11 (1996) 1855-1874, arXiv:hep-th/9409134.

[2-1]

Neutrino Counter Nuclear Weapon, Alfred Tang, arXiv:0805.3991, 2008.

[2-2]

Detection of Antineutrinos for Non-Proliferation, Nieto, Michael Martin, Hayes, A. C., Teeter, Corinne M., Wilson, William B., Stanbro, William D., arXiv:nucl-th/0309018, 2003.

[2-3]

Destruction of Nuclear Bombs Using Ultra-High Energy Neutrino Beam, Hirotaka Sugawara, Hiroyuki Hagura, Toshiya Sanami, arXiv:hep-ph/0305062, 2003.
From the article: We have shown that it is possible to eliminate the nuclear bombs from the surface of the earth utilizing the extremely high energy neutrino beam. When the neutrino beam hits a bomb, it will cause the fizzle explosion with 3% of the full strength. It seems that it is not possible to decrease the magnitude of the explosion smaller than this number at this stage. It is important to decrease this number to destroy bombs safely. We are not sure what this means when the plutonium or uranium is used to ignite the hydrogen bomb. We may just break the bomb or may lead to a full explosion.
...
We are certainly aware of the fact that this kind of device can not only target the nuclear bombs but other kinds of weapons of mass destruction and also, unfortunately, any kind of living object including human. But we should emphasize that the device itself is not a weapon of mass destruction.

[2-4]

Neutrinos and Arms Control: Thinking Big about Detection of Neutrinos from Reactors at Long Distances, J. Learned, 2003. Neutrinos and Arms Control Workshop, 5-7 February 2004, University of Hawaii. http://www.phys.hawaii.edu/~jgl/gigaton_array.pdf.

[3-1]

Far Field Monitoring of Rogue Nuclear Activity with an Array of Large anti-neutrino Detectors, Eugene Guillian, arXiv:hep-ph/0607095, 2006. Neutrino Sciences 2005.

[3-2]

Reactor monitoring (near and far) with neutrinos, Learned, J. G., Nucl. Phys. Proc. Suppl. 143 (2005) 152-156. 21st International Conference On Neutrino Physics And Astrophysics (Neutrino 2004), 14-19 June 2004, Paris, France.

[4-1]

Remark on the studies of the muon-induced neutron background in the liquid scintillator detectors, Karim Zbiri, arXiv:0910.3714, 2009.

[4-2]

A two-phase argon avalanche detector operated in a single electron counting mode, A. Bondar et al., arXiv:physics/0611068, 2006.

[5-1]

Tritium beta-decay endpoint for a Tachyonic Neutrino that travels Faster than Light, Ngee-Pong Chang, arXiv:hep-ph/0410175, 2004.

[5-2]

Faster-than-light speeds, tachyons, and the possibility of tachyonic neutrinos, Ehrlich, R., Am. J. Phys. 71 (2003) 1109-1114.

[5-3]

Neutrino mass^2 inferred from the cosmic ray spectrum and tritium beta decay, Ehrlich, Robert, Phys. Lett. B493 (2000) 229-232, arXiv:hep-ph/0009040.

[5-4]

Implications for the cosmic ray spectrum of a negative electron neutrino (mass)^2, Ehrlich, Robert, Phys. Rev. D60 (1999) 17302, arXiv:astro-ph/9812336.

[5-5]

Are muon neutrinos faster than light particles?: possible consequences for neutrino oscillations, Giannetto, E., Maccarrone, G. D., Mignani, R., Recami, E., Phys. Lett. B178 (1986) 115.

[5-6]

The neutrino as a tachyon, Chodos, Alan, Hauser, Avi I., Kostelecky, V. Alan, Phys. Lett. B150 (1985) 431.

Neutrino Unbound

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