期刊
PHYSICAL REVIEW D
卷 85, 期 8, 页码 -出版社
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.85.081101
关键词
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资金
- Danish Council for Independent Research\Natural Sciences
- Australian Research Council [DP0772084, DP1093738]
- CAASTRO
- AAOmega spectrograph
- Australian Research Council [DP0772084, DP1093738] Funding Source: Australian Research Council
The absolute neutrino mass scale is currently unknown, but can be constrained by cosmology. The WiggleZ high redshift, star-forming, and blue galaxy sample offers a complementary data set to previous surveys for performing these measurements, with potentially different systematics from nonlinear structure formation, redshift-space distortions, and galaxy bias. We obtain a limit of Sigma m(v) < 0.60 eV (95% confidence) for WiggleZ+Wilkinson Microwave Anisotropy Probe. Combining with priors on the Hubble parameter and the baryon acoustic oscillation scale gives Sigma m(v) < 0: 29 eV, which is the strongest neutrino mass constraint derived from spectroscopic galaxy redshift surveys.
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