Energy density of massive neutrinos

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The discussion centers on seeking an updated reference for the energy density parameter of massive neutrinos, \Omega_{\nu}, with current estimates suggesting values around 10^{-3}. Participants note that recent constraints primarily derive from cosmic microwave background (CMB) data and galaxy power spectrum results, particularly from the SDSS catalogue. A key reference mentioned is a 2004 paper by Tegmark, but more recent findings are desired. The latest estimate provided indicates \Omega_{\nu} is less than 0.0065 at 95% confidence. This highlights the ongoing interest in refining measurements of neutrino masses and their implications for cosmology.
nicksauce
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Does anyone have an up-to-date reference for the best value of \Omega_{\nu}, given our current understanding of neutrino masses? Dodelson's cosmology book has \Omega_{\nu}\approx 10^{-3}, but something more recent would be nice.
 
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Not sure if the results get quoted like that these days, usually it's just the mass limits rather than translating that into a density parameter. I think the best constraints come from CMB plus galaxy power spectrum results, the biggest data set being the SDSS catalogue. I think there was a Tegmark paper in 2004 on this, though there is bound to be more recent work.
 
nicksauce said:
Does anyone have an up-to-date reference for the best value of \Omega_{\nu}, given our current understanding of neutrino masses? Dodelson's cosmology book has \Omega_{\nu}\approx 10^{-3}, but something more recent would be nice.
This is probably about the best current measure:
http://lambda.gsfc.nasa.gov/product/map/current/params/lcdm_sz_lens_mnu_wmap5_bao_snall.cfm

They estimate \Omega_\nu < 0.0065 at 95% confidence.
 
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Thanks a lot.
 
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