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R. D. Peccei and H. R. Quinn, Phys. Rev. Lett. 38
1978
Earlier work this paper cites.
A. M. Dziewonski and D. L. Anderson, Phys. Earth Planet. Interiors 25
1981
Earlier work this paper cites.
T. R. Taylor and G. Veneziano, Phys. Lett. B 213
1994
Earlier work this paper cites.
F. Vissani, hep-ph/9708483; V. D. Barger, S. Pakvasa, T. J. Weiler and K. Whisnant, Phys. Lett. B 437
1998
Earlier work this paper cites.
W. Hu, R. Barkana and A. Gruzinov, Phys. Rev. Lett. 85
2000
Earlier work this paper cites.
V. Barger, D. Marfatia and K. Whisnant, Phys. Rev. D 65
2002
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J. Yoo et al
2003
Earlier work this paper cites.
P. F. Harrison, D. H. Perkins and W. G. Scott, Phys. Lett. B 530
2003
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G. L. Fogli, E. Lisi, A. Palazzo and A. M. Rotunno, Phys. Lett. B 623
2005
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L. B. Auerbach et al
2005
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P. Huber, M. Lindner and W. Winter, Comput. Phys. Commun. 167
2007
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F. Piazza and M. Pospelov, Phys. Rev. D 82
Original
2010
Earlier work this paper cites.

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2018

Liao, Jiajun, Marfatia, Danny, Whisnant, Kerry

Couplings between light scalar dark matter (DM) and neutrinos induce a perturbation to the neutrino mass matrix.

If the DM oscillation period is smaller than ten minutes (or equivalently, the DM particle is heavier than $0.69\times10^{-17}$ eV), the fast-averaging over an oscillation cycle leads to a modification of the measured oscillation parameters.
We present a specific $\mu-\tau$ symmetric model in which the measured value of $\theta_{13}$ is entirely generated by the DM interaction, and which reproduces the other measured oscillation parameters.
For a scalar DM particle lighter than $10^{-15}$ eV, adiabatic solar neutrino propagation is maintained.

R. D. Peccei and H. R. Quinn, Phys. Rev. Lett. 38
1978
Earlier work this paper cites.
A. M. Dziewonski and D. L. Anderson, Phys. Earth Planet. Interiors 25
1981
Earlier work this paper cites.
T. R. Taylor and G. Veneziano, Phys. Lett. B 213
1994
Earlier work this paper cites.
F. Vissani, hep-ph/9708483; V. D. Barger, S. Pakvasa, T. J. Weiler and K. Whisnant, Phys. Lett. B 437
1998
Earlier work this paper cites.
W. Hu, R. Barkana and A. Gruzinov, Phys. Rev. Lett. 85
2000
Earlier work this paper cites.
V. Barger, D. Marfatia and K. Whisnant, Phys. Rev. D 65
2002
Earlier work this paper cites.
J. Yoo et al
2003
Earlier work this paper cites.
P. F. Harrison, D. H. Perkins and W. G. Scott, Phys. Lett. B 530
2003
Earlier work this paper cites.
G. L. Fogli, E. Lisi, A. Palazzo and A. M. Rotunno, Phys. Lett. B 623
2005
Earlier work this paper cites.
L. B. Auerbach et al
2005
Earlier work this paper cites.
P. Huber, M. Lindner and W. Winter, Comput. Phys. Commun. 167
2007
Earlier work this paper cites.
F. Piazza and M. Pospelov, Phys. Rev. D 82
Original
2010
Earlier work this paper cites.