|
Author |
Title |
Year |
Publication |
Volume |
Pages |
Links |
|
Bustamante, M.; Gago, A.M.; Pena-Garay, C. |
Energy-independent new physics in the flavour ratios of high-energy astrophysical neutrinos |
2010 |
Journal of High Energy Physics |
04 |
066 - 28pp |
|
|
Bergstrom, J.; Gonzalez-Garcia, M.C.; Maltoni, M.; Pena-Garay, C.; Serenelli, A.M.; Song, N.Q. |
Updated determination of the solar neutrino fluxes from solar neutrino data |
2016 |
Journal of High Energy Physics |
03 |
132 - 19pp |
|
|
Norena, J.; Verde, L.; Jimenez, R.; Pena-Garay, C.; Gomez, C. |
Cancelling out systematic uncertainties |
2012 |
Monthly Notices of the Royal Astronomical Society |
419 |
1040-1050 |
|
|
Serenelli, A.; Scott, P.; Villante, F.L.; Vincent, A.C.; Asplund, M.; Basu, S.; Grevesse, N.; Pena-Garay, C. |
Implications of solar wind measurements for solar models and composition |
2016 |
Monthly Notices of the Royal Astronomical Society |
463 |
2-9 |
|
|
Serenelli, A.; Pena-Garay, C.; Haxton, W.C. |
Using the standard solar model to constrain solar composition and nuclear reaction S factors |
2013 |
Physical Review D |
87 |
043001 - 9pp |
|
|
Borexino Collaboration (Bellini, G. et al); Pena-Garay, C. |
Final results of Borexino Phase-I on low-energy solar neutrino spectroscopy |
2014 |
Physical Review D |
89 |
112007 - 68pp |
|
|
Caputo, A.; Pena-Garay, C.; Witte, S.J. |
Looking for axion dark matter in dwarf spheroidal galaxies |
2018 |
Physical Review D |
98 |
083024 - 6pp |
|
|
Borexino Collaboration (Bellini, G. et al); Pena-Garay, C. |
Precision Measurement of the (7)Be Solar Neutrino Interaction Rate in Borexino |
2011 |
Physical Review Letters |
107 |
141302 - 5pp |
|
|
Jimenez, R.; Pena-Garay, C.; Verde, L. |
Is it possible to explore Peccei-Quinn axions from frequency-dependence radiation dimming? |
2011 |
Physics Letters B |
703 |
232-236 |
|
|
Borexino Collaboration (Bellini, G. et al); Pena-Garay, C. |
Absence of a day-night asymmetry in the Be-7 solar neutrino rate in Borexino |
2012 |
Physics Letters B |
707 |
22-26 |
|