|
Author |
Title |
Year |
Publication |
Volume |
Pages |
Links |
|
Capozzi, F.; Ferreira, R.Z.; Lopez-Honorez, L.; Mena, O. |
CMB and Lyman-alpha constraints on dark matter decays to photons |
2023 |
Journal of Cosmology and Astroparticle Physics |
06 |
060 - 23pp |
|
|
Abdalla, E. et al; Mena, O. |
Cosmology intertwined: A review of the particle physics, astrophysics, and cosmology associated with the cosmological tensions and anomalies |
2022 |
Journal of High Energy Astrophysics |
34 |
49-211 |
|
|
Lopez-Honorez, L.; Mena, O.; Palomares-Ruiz, S.; Vincent, A.C. |
Constraints on dark matter annihilation from CMB observations before Planck |
2013 |
Journal of Cosmology and Astroparticle Physics |
07 |
046 - 26pp |
|
|
Gariazzo, S.; Martinez-Mirave, P.; Mena, O.; Pastor, S.; Tortola, M. |
Non-unitary three-neutrino mixing in the early Universe |
2023 |
Journal of Cosmology and Astroparticle Physics |
03 |
046 - 18pp |
|
|
Di Valentino, E.; Gariazzo, S.; Mena, O.; Vagnozzi, S. |
Soundness of dark energy properties |
2020 |
Journal of Cosmology and Astroparticle Physics |
07 |
045 - 45pp |
|
|
Gavela, M.B.; Lopez Honorez, L.; Mena, O.; Rigolin, S. |
Dark coupling and gauge invariance |
2010 |
Journal of Cosmology and Astroparticle Physics |
11 |
044 - 15pp |
|
|
Ramirez, H.; Passaglia, S.; Motohashi, H.; Hu, W.; Mena, O. |
Reconciling tensor and scalar observables in G-inflation |
2018 |
Journal of Cosmology and Astroparticle Physics |
04 |
039 - 20pp |
|
|
Stadler, J.; Boehm, C.; Mena, O. |
Is it mixed dark matter or neutrino masses? |
2020 |
Journal of Cosmology and Astroparticle Physics |
01 |
039 - 18pp |
|
|
Gariazzo, S.; Mena, O.; Ramirez, H.; Boubekeur, L. |
Primordial power spectrum features in phenomenological descriptions of inflation |
2017 |
Physics of the Dark Universe |
17 |
38-45 |
|
|
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 |
|