YNAO OpenIR  > 大样本恒星演化研究组
SNe Ia as a cosmological probe
Meng XC(孟祥存); Gao Y(高沿); Han ZW(韩占文)
Source PublicationINTERNATIONAL JOURNAL OF MODERN PHYSICS D
2015-12-01
Volume24Issue:14
DOI10.1142/S0218271815300293
Contribution Rank第1完成单位
Indexed BySCI
KeywordSne Ia Dark Energy
Abstract

Type Ia supernovae (SNe Ia) luminosities can be corrected in order to render them useful as standard candles that are able to probe the expansion history of the universe. This technique was successfully applied to discover the present acceleration of the universe. As the number of SNe Ia observed at high redshift increases and analysis techniques are perfected, people aim to use this technique to probe the equation-of-state of the dark energy (EOSDE). Nevertheless, the nature of SNe Ia progenitors remains controversial and concerns persist about possible evolution effects that may be larger and harder to characterize than the more obvious statistical uncertainties.

Funding ProjectNSFC[11473063] ; NSFC[11522327] ; NSFC[11390374] ; NSFC[11521303] ; Western Light Key Project of the Chinese Academy of Sciences ; Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences ; Strategic Priority Research Program "The Emergence of Cosmological Structures" of the Chinese Academy of Sciences[XDB09010202] ; Science and Technology Innovation Talent Programme of the Yunnan Province[2013HA005]
Funding OrganizationNSFC[11473063, 11522327, 11390374, 11521303] ; Western Light Key Project of the Chinese Academy of Sciences ; Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences ; Strategic Priority Research Program "The Emergence of Cosmological Structures" of the Chinese Academy of Sciences[XDB09010202] ; Science and Technology Innovation Talent Programme of the Yunnan Province[2013HA005]
Language英语
Subject Area天文学 ; 恒星与银河系
MOST Discipline Catalogue理学 ; 理学::天文学
SubtypeReview
PublisherWORLD SCIENTIFIC PUBL CO PTE LTD
Publication Place5 TOH TUCK LINK, SINGAPORE 596224, SINGAPORE
ISSN0218-2718
URL查看原文
Archive Date2015-10-23
WOS IDWOS:000369340900001
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS KeywordHUBBLE-SPACE-TELESCOPE ; SINGLE-DEGENERATE CHANNEL ; CHANDRASEKHAR MASS MODELS ; HIGH-REDSHIFT SUPERNOVAE ; HOST GALAXY PROPERTIES ; OXYGEN WHITE-DWARFS ; LIGHT-CURVE SHAPES ; DARK ENERGY ; DIFFERENT METALLICITIES ; ACCELERATING UNIVERSE
Citation statistics
Cited Times:10[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.ynao.ac.cn/handle/114a53/9329
Collection大样本恒星演化研究组
Corresponding AuthorMeng XC(孟祥存)
AffiliationBPS Group, Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, P. R. China
First Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Corresponding Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Meng XC,Gao Y,Han ZW. SNe Ia as a cosmological probe[J]. INTERNATIONAL JOURNAL OF MODERN PHYSICS D,2015,24(14).
APA Meng XC,Gao Y,&Han ZW.(2015).SNe Ia as a cosmological probe.INTERNATIONAL JOURNAL OF MODERN PHYSICS D,24(14).
MLA Meng XC,et al."SNe Ia as a cosmological probe".INTERNATIONAL JOURNAL OF MODERN PHYSICS D 24.14(2015).
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