Abstract
We consider the effect of three species of neutrinos with nearly degenerate mass on the cosmic structure formation in a low-matter-density universe within a hierarchical clustering scenario with a flat Gaussian initial perturbation spectrum. The matching condition for fluctuation powers at the COBE scale and at the cluster scale leads to a strong upper limit on neutrino mass. For a flat universe with matter density parameter , we obtain for the Hubble constant . Allowing for the more generous parameter space limited by and age , the limit is 0.9 eV.
- Received 23 August 1999
DOI:https://doi.org/10.1103/PhysRevLett.84.1082
©2000 American Physical Society