| |
Author |
Title |
Year |
Publication |
Volume |
Pages |
Links |
|
|
Reig, M.; Valle, J.W.F.; Yamada, M. |
Light majoron cold dark matter from topological defects and the formation of boson stars |
2019 |
Journal of Cosmology and Astroparticle Physics |
09 |
029 - 25pp |
|
|
|
Peinado, E.; Reig, M.; Srivastava, R.; Valle, J.W.F. |
Dirac neutrinos from Peccei-Quinn symmetry: A fresh look at the axion |
2020 |
Modern Physics Letters A |
35 |
2050176 - 9pp |
|
|
|
FCC Collaboration (Abada, A. et al); Aguilera-Verdugo, J.J.; Hernandez, P.; Ramirez-Uribe, N.S.; Renteria-Olivo, A.E.; Rodrigo, G.; Sborlini, G.F.R.; Valle, J.W.F. |
FCC Physics Opportunities: Future Circular Collider Conceptual Design Report Volume 1 |
2019 |
European Physical Journal C |
79 |
474 - 161pp |
|
|
|
Avila, I.M.; De Romeri, V.; Duarte, L.; Valle, J.W.F. |
Phenomenology of scotogenic scalar dark matter |
2020 |
European Physical Journal C |
80 |
908 - 19pp |
|
|
|
Bazzocchi, F.; Cerdeño, D.G.; Muñoz, C.; Valle, J.W.F. |
Calculable inverse-seesaw neutrino masses in supersymmetry |
2010 |
Physical Review D |
81 |
051701 - 5pp |
|
|
|
Chen, P.; Ding, G.J.; Gonzalez-Canales, F.; Valle, J.W.F. |
Classifying CP transformations according to their texture zeros: Theory and implications |
2016 |
Physical Review D |
94 |
033002 - 26pp |
|
|
|
Chen, P.; Ding, G.J.; Srivastava, R.; Valle, J.W.F. |
Predicting neutrino oscillations with “bi-large” lepton mixing matrices |
2019 |
Physics Letters B |
792 |
461-464 |
|
|
|
Centelles Chulia, S.; Ma, E.; Srivastava, R.; Valle, J.W.F. |
Dirac neutrinos and dark matter stability from lepton quarticity |
2017 |
Physics Letters B |
767 |
209-213 |
|
|
|
Leite, J.; Morales, A.; Valle, J.W.F.; Vaquera-Araujo, C.A. |
Dark matter stability from Dirac neutrinos in scotogenic 3-3-1-1 theory |
2020 |
Physical Review D |
102 |
015022 - 11pp |
|
|
|
Mandal, S.; Rojas, N.; Srivastava, R.; Valle, J.W.F. |
Dark matter as the origin of neutrino mass in the inverse seesaw mechanism |
2021 |
Physics Letters B |
821 |
136609 - 15pp |
|
