Cosmological preference for a negative neutrino mass
University of California System · Southern Methodist University
Abstract
The most precise determination of the sum of neutrino masses from cosmological data, derived from analysis of the cosmic microwave background (CMB) and baryon acoustic oscillations (BAO) from the Dark Energy Spectroscopic Instrument (DESI), favors a value below the minimum inferred from neutrino flavor oscillation experiments. We explore which data are most responsible for this puzzling aspect of the current constraints on neutrino mass and whether they are related to other anomalies in cosmology. We demonstrate conclusively that the preference for negative neutrino masses is a consequence of larger-than-expected lensing of the CMB in both the two- and four-point lensing statistics. Furthermore, we show that…
Citation impact
- FWCI
- 45.39
- Percentile
- 100%
- References
- 99
Authors
2Topics & keywords
- Neutrino
- Preference
- Particle physics
- Physics
- Psychology
- Mathematics
- Statistics