|
Author |
Title |
Year |
Publication |
Volume |
Pages |
Links |
|
Centelles Chulia, S.; Cepedello, R.; Peinado, E.; Srivastava, R. |
Scotogenic dark symmetry as a residual subgroup of Standard Model symmetries |
2020 |
Chinese Physics C |
44 |
083110 - 7pp |
|
|
Morisi, S.; Valle, J.W.F. |
Neutrino masses and mixing: a flavour symmetry roadmap |
2013 |
Fortschritte der Physik-Progress of Physics |
61 |
466-492 |
|
|
de Salas, P.F.; Gariazzo, S.; Mena, O.; Ternes, C.A.; Tortola, M. |
Neutrino Mass Ordering From Oscillations and Beyond: 2018 Status and Future Prospects |
2018 |
Frontiers in Astronomy and Space Sciences |
5 |
36 - 50pp |
|
|
Farzan, Y.; Tortola, M. |
Neutrino oscillations and non-standard Interactions |
2018 |
Frontiers in Physics |
6 |
10 - 34pp |
|
|
Cai, Y.; Herrero-Garcia, J.; Schmidt, M.A.; Vicente, A.; Volkas, R.R. |
From the Trees to the Forest: A Review of Radiative Neutrino Mass Models |
2017 |
Frontiers in Physics |
5 |
63 - 56pp |
|
|
Jimenez, R.; Kitching, T.; Pena-Garay, C.; Verde, L. |
Can we measure the neutrino mass hierarchy in the sky? |
2010 |
Journal of Cosmology and Astroparticle Physics |
05 |
035 - 14pp |
|
|
Reid, B.A.; Verde, L.; Jimenez, R.; Mena, O. |
Robust neutrino constraints by combining low redshift observations with the CMB |
2010 |
Journal of Cosmology and Astroparticle Physics |
01 |
003 - 21pp |
|
|
Gomez-Cadenas, J.J.; Martin-Albo, J.; Muñoz Vidal, J.; Pena-Garay, C. |
Discovery potential of xenon-based neutrinoless double beta decay experiments in light of small angular scale CMB observations |
2013 |
Journal of Cosmology and Astroparticle Physics |
03 |
043 - 17pp |
|
|
Villaescusa-Navarro, F.; Bird, S.; Pena-Garay, C.; Viel, M. |
Non-linear evolution of the cosmic neutrino background |
2013 |
Journal of Cosmology and Astroparticle Physics |
03 |
019 - 30pp |
|
|
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 |
|