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Cosmological Constant
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Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant,10.1086/300499,Astronomical Journal,Adam G. Riess,Alex
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Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
(
Citations: 294
)
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Adam G. Riess
,
Alexei V. Filippenko
,
Peter Challis
,
Alejandro Clocchiatti
,
Alan Diercks
,
Peter M. Garnavich
,
Ron L. Gilliland
,
Craig J. Hogan
,
Saurabh Jha
,
Robert P. Kirshner
,
B. Leibundgut
,
M. M. Phillips
http://academic.research.microsoft.com/io.ashx?type=5&id=3476525&selfId1=0&selfId2=0&maxNumber=12&query=
We present spectral and photometric observations of 10 Type Ia supernovae (SNe Ia) in the redshift range 0.16 <= z 0) and a current acceleration of the expansion (i.e., q_0 = 0, the spectroscopically confirmed SNe Ia are statistically consistent with q_0 0 at the 3.0 sigma and 4.0 sigma confidence levels, for two different fitting methods, respectively. Fixing a ``minimal'' mass density, Omega_M = 0.2, results in the weakest detection, Omega_Lambda > 0 at the 3.0 sigma
confidence level
from one of the two methods. For a flat universe prior (Omega_M + Omega_Lambda = 1), the spectroscopically confirmed SNe Ia require Omega_Lambda > 0 at 7 sigma and 9 sigma formal
statistical significance
for the two different fitting methods. A universe closed by ordinary matter (i.e., Omega_M = 1) is formally ruled out at the 7 sigma to 8 sigma
confidence level
for the two different fitting methods. We estimate the dynamical age of the universe to be 14.2 +/- 1.7 Gyr including systematic uncertainties in the current Cepheid distance scale. We estimate the likely effect of several sources of systematic error, including progenitor and metallicity evolution, extinction,
sample selection
bias, local perturbations in the expansion rate, gravitational lensing, and sample contamination. Presently, none of these effects appear to reconcile the data with Omega_Lambda = 0 and q_0 >= 0.
Journal:
Astronomical Journal - ASTRON J
, vol. 116, no. 3, pp. 1009-1038, 1998
DOI:
10.1086/300499
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Citation Context
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...Going back to (230), we divide the integration range into the intervals [0,
1
] and [1, ∞]. After dividing by T , the contribution of the second interval is bounded by...
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References
(2)
Statistics in theory and practice
(
Citations: 133
)
Robert Lupton
Published in 1993.
Master Thesis
(
Citations: 42
)
Jong-Il Hwang
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Gaussian Process Modeling of Derivative Curves
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Bruno Sansó
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Herbert K. H. Lee
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