Upper Bound of 0.28 eV on Neutrino Masses from the Largest Photometric Redshift Survey
Abstract
We present a new limit of ∑mν≤0.28 (95% CL) on the sum of the neutrino masses assuming a flat ΛCDM cosmology. This relaxes slightly to ∑mν≤0.34 and ∑mν≤0.47 when quasinonlinear scales are removed and w≠-1, respectively. These are derived from a new photometric catalogue of over 700 000 luminous red galaxies (MegaZ DR7) with a volume of 3.3(Gpch-1)3 and redshift range 0.45<z<0.65. The data are combined with WMAP 5-year CMB, baryon acoustic oscillations, supernovae, and a Hubble Space Telescope prior on h. When combined with WMAP these data are as constraining as adding all supernovae and baryon oscillation data available. The upper limit is one of the tightest constraints on the neutrino from cosmology or particle physics. Further, if these bounds hold, they all predict that current-to-next generation neutrino experiments, such as KATRIN, are unlikely to obtain a detection.
- Publication:
-
Physical Review Letters
- Pub Date:
- July 2010
- DOI:
- 10.1103/PhysRevLett.105.031301
- arXiv:
- arXiv:0911.5291
- Bibcode:
- 2010PhRvL.105c1301T
- Keywords:
-
- 98.80.Es;
- 14.60.Pq;
- 95.80.+p;
- 98.65.Cw;
- Observational cosmology;
- Neutrino mass and mixing;
- Astronomical catalogs atlases sky surveys databases retrieval systems archives etc.;
- Galaxy clusters;
- Astrophysics - Cosmology and Nongalactic Astrophysics;
- Astrophysics - High Energy Astrophysical Phenomena;
- High Energy Physics - Experiment
- E-Print:
- PRL Accepted: 4 pages, 3 figures. Added: varying w limits and gauge of scale dependent bias, plus implications for neutrino particle experiments