On the Reality of the Accelerating Universe
arXiv:astro-ph/0207558 · doi:10.1086/343071
Abstract
Two groups recently deduced the positive value for the cosmological constant, concluding at a high (>= 99%) confidence level that the Universe should be accelerating. This conclusion followed from the statistical analysis of dozens of high-redshift supernovae. In this paper this conclusion is discussed. From the conservative frequentist's point of view the validity of null hypothesis of the zero cosmological constant is tested by the classical statistical chi^2 test for the 60 supernovae listed in Perlmutter et al. 1999 (ApJ, 517, 565). This sample contains 42 objects discovered in the frame of Supernova Cosmology Project and 18 low-redshift object detected earlier. Excluding the event SN1997O, which is doubtlessly an outlier, one obtains the result: The probability for seeing a worse chi^2 - if the null hypothesis is true - is in the 5% to 8% range, a value that does not indicate significant evidence againts the null. If one excludes further five possible outliers, proposed to be done by Perlmutter et al. 1999, then the sample of 54 supernovae is in an excellent accordance with the null hypothesis. It also seems that upernovae from the High-z Supernova Search Team does not change the acceptance of null hypothesis. This means that the rejection of the Einstein equations with zero cosmological constant - based on the supernova data alone - is still premature.
11 pages, no figures, accepted for publication in ApJ
References in corpus (2)
Cited by in corpus (9)
- Alternatives to Quintessence Model Building
- Constraints on Cardassian Scenario from the Expansion Turnaround Redshift and the Sunyaev-Zeldovich/X-ray Data
- Dynamical systems analysis of tachyon dark energy model from a new perspective
- Redshift distribution of gamma-ray bursts and star formation rate
- Interacting dark sector: a dynamical system perspective
- A curious relation between the flat cosmological model and the elliptic integral of the first kind
- A possible interrelation between the estimated luminosity distances and internal extinctions of type Ia supernovae
- Quintessence scalar field and cosmological constant: Dynamics of a multi-component dark energy model
- Perturbation in an interacting dark universe