Cosmological neutrino mass limit and the dynamics of dark energy
arXiv:astro-ph/0609463 · doi:10.1103/PhysRevD.75.103505
Abstract
We investigate the correlation between the neutrino mass limit and dark energy with time evolving equation of state. Parameterizing dark energy as w=w_0+w_1*z/(1+z), we make a global fit using Markov Chain Monte Carlo technique to determine w_0, w_1, neutrino mass as well as other cosmological parameters simultaneously. We pay particular attention to the correlation between neutrino mass Σm_ν and w_1 using current cosmological observations as well as the future simulated datasets such as PLANCK, SNAP and LAMOST.
9 pages, 5 figures, 1 table
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