New upper limit on the total neutrino mass from the 2 degree field galaxy redshift survey.

نویسندگان

  • Ø Elgarøy
  • O Lahav
  • W J Percival
  • J A Peacock
  • D S Madgwick
  • S L Bridle
  • C M Baugh
  • I K Baldry
  • J Bland-Hawthorn
  • T Bridges
  • R Cannon
  • S Cole
  • M Colless
  • C Collins
  • W Couch
  • G Dalton
  • R De Propris
  • S P Driver
  • G P Efstathiou
  • R S Ellis
  • C S Frenk
  • K Glazebrook
  • C Jackson
  • I Lewis
  • S Lumsden
  • S Maddox
  • P Norberg
  • B A Peterson
  • W Sutherland
  • K Taylor
چکیده

We constrain f(nu) identical with Omega(nu)/Omega(m), the fractional contribution of neutrinos to the total mass density in the Universe, by comparing the power spectrum of fluctuations derived from the 2 Degree Field Galaxy Redshift Survey with power spectra for models with four components: baryons, cold dark matter, massive neutrinos, and a cosmological constant. Adding constraints from independent cosmological probes we find f(nu)<0.13 (at 95% confidence) for a prior of 0.1<Omega(m)<0.5, and assuming the scalar spectral index n=1. This translates to an upper limit on the total neutrino mass m(nu,tot)<1.8 eV for "concordance" values of Omega(m) and the Hubble constant.

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عنوان ژورنال:
  • Physical review letters

دوره 89 6  شماره 

صفحات  -

تاریخ انتشار 2002