Article ID Journal Published Year Pages File Type
1779588 New Astronomy 2009 8 Pages PDF
Abstract
Cosmological limits on neutrino masses are softened, by more than a factor 2, if Cold Dark Matter (CDM) and Dark Energy (DE) are coupled. In turn, a neutrino mass yielding Ων up to ∼0.20 allows coupling levels β≃0.15 or more, already easing the coincidence problem. The coupling, in fact, displaces both P(k) and Cl spectra in a fashion opposite to neutrino mass. Estimates are obtained through a Fisher-matrix technique.
Related Topics
Physical Sciences and Engineering Physics and Astronomy Astronomy and Astrophysics
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