Galaxy clustering, CMB and supernova data constraints on ϕCDM model with massive neutrinos
We investigate a scalar field dark energy model (i.e., ϕCDM model) with massive neutrinos, where the scalar field possesses an inverse power-law potential, i.e., V(ϕ)∝ϕ−α (α>0). We find that the sum of neutrino masses Σmν has significant impacts on the CMB temperature power spectrum and on the ma...
| Main Authors: | , |
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| Format: | Article |
| Language: | English |
| Published: |
Elsevier
2016-01-01
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| Series: | Physics Letters B |
| Online Access: | http://www.sciencedirect.com/science/article/pii/S0370269315008709 |