Improvement of cosmological neutrino mass bounds
By E. Giusarma, M. Gerbino, O. Mena, S. Vagnozzi, Shirley Ho, K. Freese. 2016
157 citations recorded by the source corpus.
The most recent measurements of the temperature and low-multipole polarization anisotropies of the cosmic microwave background from the Planck satellite, when combined with galaxy clustering data f ...
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/c1cc0fad171493cdcc73978a662d9eeb9bc6d43b
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In Astronomy and Astrophysics
- T. Treu
- P. J. Marshall
- Dominique Sluse
- Leon V. E. Koopmans
- T. Collett
- M. Auger
- C. Fassnacht
- Sherry H. Suyu
In Nuclear and High Energy Physics
Citations in the corpus
- New physics in light of the H0 tension: An alternative view (2019, background): “06 eV, the minimum mass allowed within the normal ordering, given the current very tight upper limits onMν [14, 71, 225–237], which also mildly favour the normal ordering [71, 235,”
- MontePython 3: Boosted MCMC sampler and other features (2018, unknown): “For completeness, it is possible to use only one or two degenerate massive neutrinos and the rest massless, but this has been shown to be slightly inaccurate for the precision of current experiments [31].”
- Global constraints on absolute neutrino masses and their ordering (2017, background): “[69] E.”
- Modular A4 invariance and neutrino mixing (2018, background): “The sum of neutrino masses are restricted by the cosmological observations [37, 38].”
- 2020 global reassessment of the neutrino oscillation picture (2020, unknown): “[119–121] after considering very similar cosmological observations.”
- Updated results on neutrino mass and mass hierarchy from cosmology with Planck 2018 likelihoods (2019, unknown): “15 eV (95%) or better [15, 25–43].”
- H0LiCOW - V. New COSMOGRAIL time delays of HE 0435-1223: H0 to 3.8 per cent precision from strong lensing in a flat ΛCDM model (2016, background): “Given the above, it is important to consider a range of plausible extended cosmological models when investigating the information that can be gained from any specific cosmological probe (see e.g. Collett & Auger 2014; Giusarma et al. 2016).”