中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Comparison Between chi(2) and Bayesian Statistics with Considering the Redshift Dependence of Stretch and Color from JLA Data

文献类型:期刊论文

作者Zhao, Ze1,2
刊名COMMUNICATIONS IN THEORETICAL PHYSICS
出版日期2019
卷号71期号:9页码:1097-1108
关键词DARK ENERGY COSMOLOGICAL CONSTRAINTS LIGHT CURVES SUPERNOVAE
ISSN号0253-6102
DOI10.1088/0253-6102/71/9/1097
英文摘要In this work, we compare the impacts given by chi(2) statistics and Bayesian statistics. Bayesian statistics is a new statistical method proposed by [C. Ma, P. S. Corasaniti, and B. A. Bassett, arXiv:1603.08519[astro-ph.CO](2016)] recently, which gives a fully account for the standard-candle parameter dependence of the data covariance matrix. For this two statistical methods, we explore the possible redshift-dependence of stretch-luminosity parameter alpha and color-luminosity parameter beta by using redshift tomography. By constraining the ACDM model, we check the consistency of cosmology-fit results given by the SN sample of each redshift bin. We also adopt the linear parametrization to explore the possible evolution of alpha and beta and the deceleration parameter q(z) for CPL, JBP, BA and Wang models. We find that: (i) Using the full JLA data, at high redshift alpha has a trend of decreasing at more than 1.5 sigma confidence level (CL), and beta has a significant trend of decreasing at more than 19 sigma CL. (ii) Compared with chi(2) statistics (constant alpha, beta) and Bayesian statistics (constant alpha, beta), Bayesian statistics (linear alpha and beta) yields a larger best-fit value of fractional matter density Omega(m)(0) from JLA+CMB+GC data, which is much closer to slightly deviates from the best-fit result given by other cosmological observations. (iii) The figure of merit (FoM) given by JLA+CMB+GC data from Bayesian statistics is also larger than the FoM from chi(2) statistics, which indicates that former statistics has a better accuracy. (iv) q(z) given by both statistical methods favor an eternal cosmic acceleration at 1 sigma CL.
学科主题Physics
语种英语
源URL[http://ir.itp.ac.cn/handle/311006/26944]  
专题理论物理研究所_理论物理所1978-2010年知识产出
作者单位1.Chinese Acad Sci, Inst Theoret Phys, CAS Key Lab Theoret Phys, Beijing 100190, Peoples R China
2.Univ Chinese Acad Sci, Sch Phys Sci, 19A Yuquan Rd, Beijing 100049, Peoples R China
3.Chinese Acad Sci, Kavli Inst Theoret Phys China, Beijing 100190, Peoples R China
推荐引用方式
GB/T 7714
Zhao, Ze. Comparison Between chi(2) and Bayesian Statistics with Considering the Redshift Dependence of Stretch and Color from JLA Data[J]. COMMUNICATIONS IN THEORETICAL PHYSICS,2019,71(9):1097-1108.
APA Zhao, Ze.(2019).Comparison Between chi(2) and Bayesian Statistics with Considering the Redshift Dependence of Stretch and Color from JLA Data.COMMUNICATIONS IN THEORETICAL PHYSICS,71(9),1097-1108.
MLA Zhao, Ze."Comparison Between chi(2) and Bayesian Statistics with Considering the Redshift Dependence of Stretch and Color from JLA Data".COMMUNICATIONS IN THEORETICAL PHYSICS 71.9(2019):1097-1108.

入库方式: OAI收割

来源:理论物理研究所

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