|
Author |
Title |
Year |
Publication |
Volume |
Pages |
Links |
|
Bellomo, N.; Bellini, E.; Hu, B.; Jimenez, R.; Pena-Garay, C.; Verde, L. |
Hiding neutrino mass in modified gravity cosmologies |
2017 |
Journal of Cosmology and Astroparticle Physics |
02 |
043 - 12pp |
|
|
Vinyoles, N.; Serenelli, A.M.; Villante, F.L.; Basu, S.; Bergstrom, J.; Gonzalez-Garcia, M.C.; Maltoni, M.; Pena-Garay, C.; Song, N.Q. |
A New Generation of Standard Solar Models |
2017 |
Astrophysical Journal |
835 |
202 - 16pp |
|
|
Simpson, F.; Jimenez, R.; Pena-Garay, C.; Verde, L. |
Dark energy from the motions of neutrinos |
2018 |
Physics of the Dark Universe |
20 |
72-77 |
|
|
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 |
|
|
Pena-Garay, C.; Verde, L.; Jimenez, R. |
Neutrino footprint in large scale structure |
2017 |
Physics of the Dark Universe |
15 |
31-34 |
|
|
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 |
|
|
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 |
|
|
Villaescusa-Navarro, F.; Miralda-Escude, J.; Pena-Garay, C.; Quilis, V. |
Neutrino halos in clusters of galaxies and their weak lensing signature |
2011 |
Journal of Cosmology and Astroparticle Physics |
06 |
027 - 14pp |
|
|
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 |
|
|
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 |
|