Built on

G. ’t Hooft, Predictions for neutrino - electron cross-sections in Weinberg’s model of weak interactions , Phys. Lett. B 37
1971
Earlier work this paper cites.
J.N. Bahcall, Neutrino Astrophysics , Cambridge University Press 1989
1989
Earlier work this paper cites.
G. G. Raffelt, Stars as Laboratories for Fundamental Physics , The University of Chicago Press, 1996
1996
Earlier work this paper cites.
J. N. Bahcall, S. Basu and M. H. Pinsonneault, How uncertain are solar neutrino predictions? , Phys. Lett. B 433
1998
Earlier work this paper cites.
J. Sulkimo et al. (Geant4 Collaboration) NIM Phys. Res. Sect. A 506
2003
Earlier work this paper cites.
J. N. Bachall and C. Pena-Garay, Solar models and solar neutrino oscillations New Journal of Physics 6 (2004)
2004
Earlier work this paper cites.
A. Friedland, C. Lunardini and C. Pena-Garay, Solar neutrinos as probes of neutrino matter interactions , Phys. Lett. B 594
2004
Earlier work this paper cites.
J. N. Bahcall, A. M. Serenelli and S. Basu, New solar opacities, abundances, helioseismology, and neutrino fluxes , Astrophys. J. 621
2005
Earlier work this paper cites.
M. C. Smith et al
2007
Earlier work this paper cites.
K. Arisaka, H. Wang, P. F. Smith, D. Cline, A. Teymourian, E. Brown, W. Ooi and D. Aharoni et al
Original
2009
Earlier work this paper cites.
L. Strigari, Neutrino Coherent Scattering Rates at Direct Dark Matter Detectors , New J. Phys. 11
2009
Earlier work this paper cites.
E. Aprile et al
Original
2010
Earlier work this paper cites.
A. Manalaysay, T. Marrodán Undagoitia, A. Askin, L. Baudis, A. Behrens, A. D. Ferella, A. Kish and O. Lebeda et al
Original
2010
Earlier work this paper cites.
P. M. McCowan and R. C. Barber, Q value for the double-beta decay of Xe-136 , Phys. Rev. C 82
2010
Earlier work this paper cites.

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2013

Neutrino physics with multi-ton scale liquid xenon detectors

Baudis, L., Ferella, A., Kish, A. et al.

Understand

We study the sensitivity of large-scale xenon detectors to low-energy solar neutrinos, to coherent neutrino-nucleus scattering and to neutrinoless double beta decay.

As a concrete example, we consider the xenon part of the proposed DARWIN (Dark Matter WIMP Search with Noble Liquids) experiment.
We perform detailed Monte Carlo simulations of the expected backgrounds, considering realistic energy resolutions and thresholds in the detector.
In a low-energy window of 2-30 keV, where the sensitivity to solar pp and $^7$Be-neutrinos is highest, an integrated pp-neutrino rate of 5900 events can be reached in a fiducial mass of 14 tons of natural xenon, after 5 years of data.

Built on

G. ’t Hooft, Predictions for neutrino - electron cross-sections in Weinberg’s model of weak interactions , Phys. Lett. B 37
1971
Earlier work this paper cites.
J.N. Bahcall, Neutrino Astrophysics , Cambridge University Press 1989
1989
Earlier work this paper cites.
G. G. Raffelt, Stars as Laboratories for Fundamental Physics , The University of Chicago Press, 1996
1996
Earlier work this paper cites.
J. N. Bahcall, S. Basu and M. H. Pinsonneault, How uncertain are solar neutrino predictions? , Phys. Lett. B 433
1998
Earlier work this paper cites.
J. Sulkimo et al. (Geant4 Collaboration) NIM Phys. Res. Sect. A 506
2003
Earlier work this paper cites.
J. N. Bachall and C. Pena-Garay, Solar models and solar neutrino oscillations New Journal of Physics 6 (2004)
2004
Earlier work this paper cites.
A. Friedland, C. Lunardini and C. Pena-Garay, Solar neutrinos as probes of neutrino matter interactions , Phys. Lett. B 594
2004
Earlier work this paper cites.
J. N. Bahcall, A. M. Serenelli and S. Basu, New solar opacities, abundances, helioseismology, and neutrino fluxes , Astrophys. J. 621
2005
Earlier work this paper cites.
M. C. Smith et al
2007
Earlier work this paper cites.
K. Arisaka, H. Wang, P. F. Smith, D. Cline, A. Teymourian, E. Brown, W. Ooi and D. Aharoni et al
Original
2009
Earlier work this paper cites.
L. Strigari, Neutrino Coherent Scattering Rates at Direct Dark Matter Detectors , New J. Phys. 11
2009
Earlier work this paper cites.
E. Aprile et al
Original
2010
Earlier work this paper cites.
A. Manalaysay, T. Marrodán Undagoitia, A. Askin, L. Baudis, A. Behrens, A. D. Ferella, A. Kish and O. Lebeda et al
Original
2010
Earlier work this paper cites.
P. M. McCowan and R. C. Barber, Q value for the double-beta decay of Xe-136 , Phys. Rev. C 82
2010
Earlier work this paper cites.