| Author |
Title |
Year  |
Publication |
Volume |
Pages |
| Diamanti, R.; Ando, S.; Gariazzo, S.; Mena, O.; Weniger, C. |
Cold dark matter plus not-so-clumpy dark relics |
2017 |
Journal of Cosmology and Astroparticle Physics |
06 |
008 - 17pp |
| Gariazzo, S.; Mena, O.; Miralles, V.; Ramirez, H.; Boubekeur, L. |
Running of featureful primordial power spectra |
2017 |
Physical Review D |
95 |
123534 - 7pp |
| Gariazzo, S.; Escudero, M.; Diamanti, R.; Mena, O. |
Cosmological searches for a noncold dark matter component |
2017 |
Physical Review D |
96 |
043501 - 11pp |
| 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 |
| Lopez-Honorez, L.; Mena, O.; Palomares-Ruiz, S.; Villanueva-Domingo, P. |
Warm dark matter and the ionization history of the Universe |
2017 |
Physical Review D |
96 |
103539 - 14pp |
| Vagnozzi, S.; Giusarma, E.; Mena, O.; Freese, K.; Gerbino, M.; Ho, S.; Lattanzi, M. |
Unveiling nu secrets with cosmological data: Neutrino masses and mass hierarchy |
2017 |
Physical Review D |
96 |
123503 - 26pp |
| Gerbino, M.; Lattanzi, M.; Mena, O.; Freese, K. |
A novel approach to quantifying the sensitivity of current and future cosmological datasets to the neutrino mass ordering through Bayesian hierarchical modeling |
2017 |
Physics Letters B |
775 |
239-250 |
| Di Valentino, E.; Melchiorri, A.; Mena, O. |
Can interacting dark energy solve the H-0 tension? |
2017 |
Physical Review D |
96 |
043503 - 11pp |
| Gerbino, M.; Freese, K.; Vagnozzi, S.; Lattanzi, M.; Mena, O.; Giusarma, E.; Ho, S. |
Impact of neutrino properties on the estimation of inflationary parameters from current and future observations |
2017 |
Physical Review D |
95 |
043512 - 22pp |
| Di Valentino, E.; Giusarma, E.; Lattanzi, M.; Mena, O.; Melchiorri, A.; Silk, J. |
Cosmological axion and neutrino mass constraints from Planck 2015 temperature and polarization data |
2016 |
Physics Letters B |
752 |
182-185 |
