Neutrino mass limit from galaxy cluster number density evolution - INSPIRE

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Neutrino mass limit from galaxy cluster number density evolution

Tina Kahniashvili
(
- Kansas State U. and
- Abastumani Astrophys. Observ.
)
,
Eckhard von Toerne
(
- Kansas State U. and
- Bonn U.
)
,
Natalia A. Arhipova
(
- Lebedev Inst., Astro Space Ctr.
)
,
Bharat Ratra
(
- Kansas State U.
)

Mar, 2005

5 pages

Published in:

Phys.Rev.D 71 (2005) 125009

e-Print:

astro-ph/0503328 [astro-ph]

DOI:

10.1103/PhysRevD.71.125009

View in:

ADS Abstract Service

reference search11 citations

Citations per year

Abstract: (arXiv)

Measurements of the evolution with redshift of the number density of massive galaxy clusters are used to constrain the energy density of massive neutrinos and so the sum of neutrino masses

\sum m_\nu

. We consider a spatially-flat cosmological model with cosmological constant, cold dark matter, baryonic matter, and massive neutrinos. Accounting for the uncertainties in the measurements of the relevant cosmological parameters we obtain a limit of

\sum m_\nu

<

2.4 eV (95 % C.L.).

14.60.Pq
98.80.Es
98.65.Dx
neutrino: mass
upper limit
galaxy: cluster
galaxy: density
redshift: dependence
Hubble constant
numerical calculations: interpretation of experiments

References(72)

Figures(0)

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