TESTING COSMOLOGICAL MODELS WITH TYPE Ic SUPER LUMINOUS SUPERNOVAE
文献类型：期刊论文
| 作者 | Wei, Jun-Jie1,2; Wu, Xue-Feng1,5,6 ; Melia, Fulvio1,3,4
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| 刊名 | ASTRONOMICAL JOURNAL
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| 出版日期 | 2015-05-01 |
| 卷号 | 149期号:5页码:165 |
| 关键词 | cosmic background radiation cosmological parameters cosmology: observations cosmology: theory distance scale supernovae: general |
| 英文摘要 | The use of type Ic super luminous supernovae (SLSNe Ic) to examine the cosmological expansion introduces a new standard ruler with which to test theoretical models. The sample suitable for this kind of work now includes 11 SLSNe Ic, which have thus far been used solely in tests involving the. cold dark matter (Lambda CDM) model. In this paper, we broaden the base of support for this new, important cosmic probe by using these observations to carry out a one-on-one comparison between the R-h = ct and Lambda CDM cosmologies. We individually optimize the parameters in each cosmological model by minimizing the chi(2) statistic. We also carry out Monte Carlo simulations based on these current SLSNe Ic measurements to estimate how large the sample would have to be in order to rule out either model at a similar to 99.7% confidence level. The currently available sample indicates a likelihood of similar to 70-80% that the R-h = ct universe is the correct cosmology versus similar to 20-30% for the standard model. These results are suggestive, though not yet compelling, given the current limited number of SLSNe Ic. We find that if the real cLosmology is Lambda CDM, a sample of similar to 240 SLSNe Ic would be sufficient to rule out R-h = ct at this level of confidence, while similar to 480 SLSNe Ic would be required to rule out Lambda CDM if the real universe is instead R-h = ct. This difference in required sample size reflects the greater number of free parameters available to fit the data with Lambda CDM. If such SLSNe Ic are commonly detected in the future, they could be a powerful tool for constraining the dark-energy equation of state in Lambda CDM, and differentiating between this model and the R-h = ct universe. |
| 学科主题 | 天文和天体物理 |
| WOS标题词 | Science & Technology ; Physical Sciences |
| 类目[WOS] | Astronomy & Astrophysics |
| 研究领域[WOS] | Astronomy & Astrophysics |
| 关键词[WOS] | KULLBACKS SYMMETRIC DIVERGENCE ; HUBBLE-SPACE-TELESCOPE ; GAMMA-RAY BURSTS ; SUPERLUMINOUS SUPERNOVAE ; CT UNIVERSE ; R-H ; IA SUPERNOVAE ; ULTRALUMINOUS SUPERNOVAE ; LEGACY SURVEY ; DARK-ENERGY |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000354065200016 |
| 源URL | [http://libir.pmo.ac.cn/handle/332002/14886]  |
| 专题 | 紫金山天文台_南极天文中心 |
| 作者单位 | 1.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Jiangsu, Peoples R China 2.Univ Chinese Acad Sci, Beijing 100049, Peoples R China 3.Univ Arizona, Dept Phys, Program Appl Math, Tucson, AZ 85721 USA 4.Univ Arizona, Dept Astron, Tucson, AZ 85721 USA 5.Chinese Ctr Antarctic Astron, Nanjing 210008, Jiangsu, Peoples R China 6.Nanjing Univ, Purple Mt Observ, Joint Ctr Particle Nucl Phys & Cosmol, Nanjing 210008, Jiangsu, Peoples R China |
| 推荐引用方式 GB/T 7714 | Wei, Jun-Jie,Wu, Xue-Feng,Melia, Fulvio. TESTING COSMOLOGICAL MODELS WITH TYPE Ic SUPER LUMINOUS SUPERNOVAE[J]. ASTRONOMICAL JOURNAL,2015,149(5):165. |
| APA | Wei, Jun-Jie,Wu, Xue-Feng,&Melia, Fulvio.(2015).TESTING COSMOLOGICAL MODELS WITH TYPE Ic SUPER LUMINOUS SUPERNOVAE.ASTRONOMICAL JOURNAL,149(5),165. |
| MLA | Wei, Jun-Jie,et al."TESTING COSMOLOGICAL MODELS WITH TYPE Ic SUPER LUMINOUS SUPERNOVAE".ASTRONOMICAL JOURNAL 149.5(2015):165. |
入库方式： OAI收割
来源：紫金山天文台
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