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• W1989846839 abstract "At present, cosmology provides the nominally strongest constraint on the masses of standard model neutrinos. However, this constraint is extremely dependent on the nature of the dark energy component of the Universe. When the dark energy equation of state parameter is taken as a free (but constant) parameter, the neutrino mass bound is sigma m(v) < or = 1.48 eV (95% C.L.), compared with sigma m(v) < or = 0.65 eV (95% C.L.) in the standard model where the dark energy is in the form of a cosmological constant. This has important consequences for future experiments aimed at the direct measurement of neutrino masses. We also discuss prospects for future cosmological measurements of neutrino masses." @default.
• W1989846839 created "2016-06-24" @default.
• W1989846839 creator A5059867176 @default.
• W1989846839 date "2005-11-23" @default.
• W1989846839 modified "2023-09-24" @default.
• W1989846839 title "Neutrino Masses and the Dark Energy Equation of State:Relaxing the Cosmological Neutrino Mass Bound" @default.
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• W1989846839 doi "https://doi.org/10.1103/physrevlett.95.221301" @default.
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