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research
Revised WMAP constraints on neutrino masses and other extensions of the minimal
Λ
\Lambda
Λ
CDM model
Authors
Oystein Elgaroy
Hans Kristian Eriksen
Jostein R. Kristiansen
Publication date
1 August 2006
Publisher
'American Physical Society (APS)'
Doi
Cite
View
on
arXiv
Abstract
Recently, two issues concerning the three-year WMAP likelihood code were pointed out. On large angular scales (
l
≲
30
l \lesssim 30
l
≲
30
), a sub-optimal likelihood approximation resulted in a small power excess. On small angular scales (
l
≳
300
l \gtrsim 300
l
≳
300
), over-subtraction of unresolved point sources produced a small power deficit. For a minimal six-parameter cosmological model, these two effects conspired to decrease the value of
n
s
n_s
n
s
​
by
∼
0.7
σ
\sim 0.7 \sigma
∼
0.7
σ
. In this paper, we study the change in preferred parameter ranges for more extensive cosmological models, including running of
n
s
n_s
n
s
​
, massive neutrinos, curvature, and the equation of state for dark energy. We also include large-scale structure and supernova data in our analysis. We find that the parameter ranges for
α
s
\alpha_s
α
s
​
,
Ω
k
\Omega_k
Ω
k
​
and
w
w
w
are not much altered by the modified analysis. For massive neutrinos the upper limit on the sum of the neutrino masses decreases from
M
ν
<
1.90
M_\nu < 1.90
M
ν
​
<
1.90
eV to
M
ν
<
1.57
M_\nu < 1.57
M
ν
​
<
1.57
eV when using the modified WMAP code and WMAP data only. We also find that the shift of
n
s
n_s
n
s
​
to higher values is quite robust to these extensions of the minimal cosmological model.Comment: 7 pages. Matching version published in Physical Review D. Figures changed, references added, additional comment
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Last time updated on 09/07/2019