CONSTRAINTS ON NON-FLAT COSMOLOGIES WITH MASSIVE NEUTRINOS AFTER PLANCK?2015
文献类型:期刊论文
作者 | Chen,Yun3; Ratra,Bharat2; Biesiada,Marek4,5; Li,Song1; Zhu,Zong-Hong4 |
刊名 | The Astrophysical Journal |
出版日期 | 2016-09-22 |
卷号 | 829期号:2 |
ISSN号 | 0004-637X |
关键词 | cosmology: miscellaneous cosmology: theory dark energy |
DOI | 10.3847/0004-637X/829/2/61 |
英文摘要 | ABSTRACT We investigate two dark energy cosmological models (i.e., the ΛCDM and ?CDM models) with massive neutrinos assuming two different neutrino mass hierarchies in both the spatially flat and non-flat scenarios, where in the ?CDM model the scalar field possesses an inverse power-law potential, V(?)?∝???α (α?>?0). Cosmic microwave background data from Planck?2015, baryon acoustic oscillation data from 6dFGS, SDSS-MGS, BOSS-LOWZ and BOSS CMASS-DR11, the joint light-curve analysis compilation of SNe Ia apparent magnitude observations, and the Hubble Space Telescope H0 prior, are jointly employed to constrain the model parameters. We first determine constraints assuming three species of degenerate massive neutrinos. In the spatially flat (non-flat) ΛCDM model, the sum of neutrino masses is bounded as Σmν?0.165(0.299) eV at 95% confidence level (CL). Correspondingly, in the flat (non-flat) ?CDM model, we find Σmν?0.164(0.301) eV at 95% CL. The inclusion of spatial curvature as a free parameter results in a significant broadening of confidence regions for Σmν and other parameters. In the scenario where the total neutrino mass is dominated by the heaviest neutrino mass eigenstate, we obtain similar conclusions to those obtained in the degenerate neutrino mass scenario. In addition, the results show that the bounds on Σmν based on two different neutrino mass hierarchies have insignificant differences in the spatially flat case for both the ΛCDM and ?CDM models; however, the corresponding differences are larger in the non-flat case. |
语种 | 英语 |
出版者 | The American Astronomical Society |
WOS记录号 | IOP:0004-637X-829-2-61 |
源URL | [http://ir.bao.ac.cn/handle/114a11/36179] |
专题 | 中国科学院国家天文台 |
作者单位 | 1.Department of Physics, Capital Normal University, Beijing 100048, China 2.Department of Physics, Kansas State University, 116 Cardwell Hall, Manhattan, KS 66506, USA 3.Key Laboratory for Computational Astrophysics, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100012, China; chenyun@bao.ac.cn 4.Department of Astronomy, Beijing Normal University, Beijing 100875, China 5.Department of Astrophysics and Cosmology, Institute of Physics, University of Silesia, Uniwersytecka 4, 40-007 Katowice, Poland |
推荐引用方式 GB/T 7714 | Chen,Yun,Ratra,Bharat,Biesiada,Marek,et al. CONSTRAINTS ON NON-FLAT COSMOLOGIES WITH MASSIVE NEUTRINOS AFTER PLANCK?2015[J]. The Astrophysical Journal,2016,829(2). |
APA | Chen,Yun,Ratra,Bharat,Biesiada,Marek,Li,Song,&Zhu,Zong-Hong.(2016).CONSTRAINTS ON NON-FLAT COSMOLOGIES WITH MASSIVE NEUTRINOS AFTER PLANCK?2015.The Astrophysical Journal,829(2). |
MLA | Chen,Yun,et al."CONSTRAINTS ON NON-FLAT COSMOLOGIES WITH MASSIVE NEUTRINOS AFTER PLANCK?2015".The Astrophysical Journal 829.2(2016). |
入库方式: OAI收割
来源:国家天文台
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