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B. Neganov and V. Trofimov, Otkrytiya, Izobret 146
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P. Luke, J. Beeman, F. Goulding, S. Labov, and E. Silver, Nucl. Instrum. Meth. A 289
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K. Kubodera and S. Nozawa, Int. J. Mod. Phys. E 3
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2014

Solar neutrino physics with low-threshold dark matter detectors

Billard, J., Strigari, L., Figueroa-Feliciano, E.

Understand

Dark matter detectors will soon be sensitive to Solar neutrinos via two distinct channels: coherent neutrino-nucleus scattering and neutrino electron elastic scattering.

We establish an analysis method for extracting Solar model properties and neutrino properties from these measurements, including the possible effects of sterile neutrinos which have been hinted at by some reactor experiments and cosmological measurements.
Even including sterile neutrinos, through the coherent scattering channel a 1 ton-year exposure with a low-threshold Germanium detector could improve on the current measurement of the normalization of the $^8$B Solar neutrino flux down to 3% or less.
Combining with the elastic scattering data will provide constraints on both the high and low energy survival probability, and will improve on the uncertainty on the active-to-sterile mixing angle by a factor of two.

Built on

D. Z. Freedman, Phys. Rev., D 9
1974
Earlier work this paper cites.
D. Z. Freedman, D. N. Schramm, and D. L. Tubbs, Annu. Rev. Nucl. Part. Sci. 27
1977
Earlier work this paper cites.
D. Z. Freedman, Phys. Rev. D 9
1985
Earlier work this paper cites.
B. Neganov and V. Trofimov, Otkrytiya, Izobret 146
1985
Earlier work this paper cites.
P. Luke, J. Beeman, F. Goulding, S. Labov, and E. Silver, Nucl. Instrum. Meth. A 289
1990
Earlier work this paper cites.
K. Kubodera and S. Nozawa, Int. J. Mod. Phys. E 3
1994
Earlier work this paper cites.
J. D. Lewin and P. F. Smith, Astropart. Phys. 6
1996
Earlier work this paper cites.
N. Grevesse and A. J. Sauval, Space Sci. Rev. 85
1998
Earlier work this paper cites.
B. T. Cleveland, T. Daily, R. Davis, Jr., J. R. Distel, K. Lande, C. K. Lee, P. S. Wildenhain and J. Ullman, Astrophys. J. 496
1998
Earlier work this paper cites.
A. Aguilar-Arevalo et al
2001
Earlier work this paper cites.
W. J. Marciano and Z. Parsa, J. Phys. G 29
2003
Earlier work this paper cites.
A. Friedland, C. Lunardini and C. Pena-Garay, Phys. Lett. B 594
2004
Earlier work this paper cites.
C. Giunti and M. Laveder, Mod. Phys. Lett. A 22
2007
Earlier work this paper cites.
M. Asplund, N. Grevesse, A. J. Sauval and P. Scott, Ann. Rev. Astron. Astrophys. 47
Original
2009
Earlier work this paper cites.
J. N. Abdurashitov et al
Original
2009
Earlier work this paper cites.
C. Giunti and Y. F. Li, Phys. Rev. D 80
Original
2009
Earlier work this paper cites.
J. Monroe and P. Fisher, Phys. Rev. D 76
Original
2010
Earlier work this paper cites.