Energy density of massive neutrinos

Join the discussion
Registration is free. Start your own thread to ask a follow-up.
3 replies · 3K views
Science Advisor
Homework Helper
Messages
1,270
Reaction score
8
Does anyone have an up-to-date reference for the best value of [itex]\Omega_{\nu}[/itex], given our current understanding of neutrino masses? Dodelson's cosmology book has [itex]\Omega_{\nu}\approx 10^{-3}[/itex], but something more recent would be nice.
 
Astronomy news on Phys.org
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 [itex]\Omega_{\nu}[/itex], given our current understanding of neutrino masses? Dodelson's cosmology book has [itex]\Omega_{\nu}\approx 10^{-3}[/itex], 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 [itex]\Omega_\nu < 0.0065[/itex] at 95% confidence.
 
Last edited by a moderator: