TY - JOUR

T1 - Cosmological tests with the joint lightcurve analysis

AU - Melia, F.

AU - Wei, J. J.

AU - Maier, R. S.

AU - Wu, X. F.

N1 - Funding Information:
We thank the National Basic Research Program (“973” Program) of China (grants 2014CB845800 and 2013CB834900), the National Natural Science Foundation of China (grant Nos. 11322328 and 11373068), the One-Hundred-Talents Program, the Youth Innovation Promotion Association (2011231), the Strategic Priority Research Program “The Emergence of Cosmological Structures” (grant No. XDB09000000) of the Chinese Academy of Sciences, and the Natural Science Foundation of Jiangsu Province (grant No. BK20161096).
Publisher Copyright:
© EPLA, 2018.

PY - 2018/9

Y1 - 2018/9

N2 - We examine whether a comparison between wCDM and using merged Type-Ia SN catalogs produces results consistent with those based on a single homogeneous sample. Using the Betoule et al. (Astron. Astrophys., 568 (2014) 22). Joint Lightcurve Analysis (JLA) of a combined sample of 613 events from SNLS and SDSS-II, we estimate the parameters of the two models and compare them. We find that the improved statistics can alter the model selection in some cases, but not others. In addition, based on the model fits, we find that there appears to be a lingering systematic offset of ∼0.04-0.08 mag between the SNLS and SDSS-II sources, in spite of the cross-calibration in the JLA. Treating wCDM, ΛCDM and as separate models, we find in an unbiased pairwise statistical comparison that the Bayes Information Criterion (BIC) favors the Universe with a likelihood of vs. for wCDM, but the ratio of likelihoods is reversed ( vs. ) when (i.e., ΛCDM) and strongly reversed ( vs. ) if in addition k = 0 (i.e., flat ΛCDM). We point out, however, that the value of k is a measure of the net energy (kinetic plus gravitational) in the Universe and is not constrained theoretically, though some models of inflation would drive due to an expansion-enforced dilution. Since we here consider only the basic ΛCDM model, the value of k needs to be measured and, therefore, the pre-assumption of flatness introduces a significant bias into the BIC.

AB - We examine whether a comparison between wCDM and using merged Type-Ia SN catalogs produces results consistent with those based on a single homogeneous sample. Using the Betoule et al. (Astron. Astrophys., 568 (2014) 22). Joint Lightcurve Analysis (JLA) of a combined sample of 613 events from SNLS and SDSS-II, we estimate the parameters of the two models and compare them. We find that the improved statistics can alter the model selection in some cases, but not others. In addition, based on the model fits, we find that there appears to be a lingering systematic offset of ∼0.04-0.08 mag between the SNLS and SDSS-II sources, in spite of the cross-calibration in the JLA. Treating wCDM, ΛCDM and as separate models, we find in an unbiased pairwise statistical comparison that the Bayes Information Criterion (BIC) favors the Universe with a likelihood of vs. for wCDM, but the ratio of likelihoods is reversed ( vs. ) when (i.e., ΛCDM) and strongly reversed ( vs. ) if in addition k = 0 (i.e., flat ΛCDM). We point out, however, that the value of k is a measure of the net energy (kinetic plus gravitational) in the Universe and is not constrained theoretically, though some models of inflation would drive due to an expansion-enforced dilution. Since we here consider only the basic ΛCDM model, the value of k needs to be measured and, therefore, the pre-assumption of flatness introduces a significant bias into the BIC.

UR - http://www.scopus.com/inward/record.url?scp=85054651955&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85054651955&partnerID=8YFLogxK

U2 - 10.1209/0295-5075/123/59002

DO - 10.1209/0295-5075/123/59002

M3 - Article

AN - SCOPUS:85054651955

VL - 123

JO - Europhysics Letters

JF - Europhysics Letters

SN - 0295-5075

IS - 5

M1 - 59002

ER -