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A. I. Vainshtein, “To the problem of nonvanishing gravitation mass,” Phys. Lett. B39
1972
Earlier work this paper cites.
L. Wolfenstein, “Neutrino Oscillations in Matter,” Phys. Rev. D 17
1985
Earlier work this paper cites.
K. Hirata et al
1987
Earlier work this paper cites.
R. M. Bionta, G. Blewitt, C. B. Bratton, D. Casper, A. Ciocio, R. Claus, B. Cortez, M. Crouch et al
1987
Earlier work this paper cites.
K. Nomoto, “Evolution of 8 to 10 solar mass stars toward electron capture supernovae II,” Astro. Jour. 322
1987
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P. Anselmann et al
1998
Earlier work this paper cites.
A. Aguilar-Arevalo et al
2001
Earlier work this paper cites.
B. Armbruster et al
2002
Earlier work this paper cites.
P. Gu, X. Wang, X. Zhang, “Dark energy and neutrino mass limits from baryogenesis,” Phys. Rev. D68
2003
Earlier work this paper cites.

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R. Fardon, A. E. Nelson and N. Weiner, “Dark energy from mass varying neutrinos,” JCAP 0410
2004
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2004
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D. .N. Abdurashitov, V. N. Gavrin, S. V. Girin, V. V. Gorbachev, T. V. Ibragimova, A. V. Kalikhov, N. G. Khairnasov and T. V. Knodel et al
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2011

Neutrino Dispersion Relations from a Dark Energy Model

Ciuffoli, Emilio, Evslin, Jarah, Liu, Jie et al.

Understand

We consider a model in which the neutrino is kinetically coupled to a scalar field and study its implications for environmentally dependent neutrino velocities.

Following the usual effective field theory logic, this coupling is expected to arise in neutrino dark energy models.
It leads to a Lorentz violation in the neutrino sector.
The coupling of the scalar field to the stress tensor of the Earth yields terrestrial neutrino dispersion relations distinct from those in interstellar space.

Built on

A. I. Vainshtein, “To the problem of nonvanishing gravitation mass,” Phys. Lett. B39
1972
Earlier work this paper cites.
L. Wolfenstein, “Neutrino Oscillations in Matter,” Phys. Rev. D 17
1985
Earlier work this paper cites.
K. Hirata et al
1987
Earlier work this paper cites.
R. M. Bionta, G. Blewitt, C. B. Bratton, D. Casper, A. Ciocio, R. Claus, B. Cortez, M. Crouch et al
1987
Earlier work this paper cites.
K. Nomoto, “Evolution of 8 to 10 solar mass stars toward electron capture supernovae II,” Astro. Jour. 322
1987
Earlier work this paper cites.
P. Anselmann et al
1998
Earlier work this paper cites.
A. Aguilar-Arevalo et al
2001
Earlier work this paper cites.
B. Armbruster et al
2002
Earlier work this paper cites.
P. Gu, X. Wang, X. Zhang, “Dark energy and neutrino mass limits from baryogenesis,” Phys. Rev. D68
2003
Earlier work this paper cites.

Similar

R. Fardon, A. E. Nelson and N. Weiner, “Dark energy from mass varying neutrinos,” JCAP 0410
2004
Cited alongside, same era.
A. Nicolis, R. Rattazzi, “Classical and quantum consistency of the DGP model,” JHEP 0406
2004
Cited alongside, same era.
D. .N. Abdurashitov, V. N. Gavrin, S. V. Girin, V. V. Gorbachev, T. V. Ibragimova, A. V. Kalikhov, N. G. Khairnasov and T. V. Knodel et al
2006
Cited alongside, same era.
S. Abe et al
Original
2008
Cited alongside, same era.
A. A. Aguilar-Arevalo et al
Original
2009
Cited alongside, same era.