ITP OpenIR  > 理论物理所2013年知识产出
Planck constraints on holographic dark energy
Li, M; Li, XD; Ma, YZ; Zhang, X; Zhang, ZH; Li, M (reprint author), Chinese Acad Sci, Inst Theoret Phys, Beijing 100190, Peoples R China.
2013
发表期刊JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
ISSN1475-7516
期号9页码:21
摘要We perform a detailed investigation on the cosmological constraints on the holographic dark energy (HDE) model by using the Planck data. We find that HDE can provide a good fit to the Planck high-l (l greater than or similar to 40) temperature power spectrum, while the discrepancy at 20 40 found in the ACDM model remains unsolved in the HDE model. The Planck data alone can lead to strong and reliable constraint on the HDE parameter c. At the 68% confidence level (CL), we obtain c = 0.508 +/- 0.207 with Planck+WP-lensing, favoring the present phantom behavior of HDE at the more than 2 sigma CL. By combining Planck+WP with the external astrophysical data sets, i.e. the BAO measurements from 6dFGS-FSDSS DR7(R)+BOSS DR9, the direct Hubble constant measurement result (Ho = 73.8 +/- 2.4 km s(-1) Mpc(-1)) from the HST, the SNLS3 supernovae data set, and Union2.1 supernovae data set, we get the 68% CL constraint results c = 0.484 +/- 0.070, 0.474 +/- 0.049, 0.594 +/- 0.051, and 0.642 +/- 0.066, respectively. The constraints can be improved by 2%-15% if we further add the Planck lensing data into the analysis. Compared with the WMAP-9 results, the Planck results reduce the error by 30%-60%, and prefer a phantom-like HDE at higher significant level. We also investigate the tension between different data sets. We find no evident tension when we combine Planck data with BAO and HST. Especially, we find that the strong correlation between Omega(m)h(3) and dark energy parameters is helpful in relieving the tension between the Planck and HST measurements. The residual value of chi(2)Planck+WP+HST (-) chi(2)Planck+WP is 7.8 in the ACDM model, and is reduced to 1.0 or 0.3 if we switch the dark energy to w model or the holographic model. When we introduce supernovae data sets into the analysis, some tension appears. We find that the SNLS3 data set is in tension with all other data sets; for example, for the Planck+WP, WMAP-9 and BAO+HST, the corresponding Delta chi(2) is equal to 6.4, 3.5 and 4.1, respectively. As a comparison, the Union2.1 data set is consistent with these three data sets, but the combination Union2.1+BAO+HST is in tension with Pianck+WP-Flensing, corresponding to a large Delta chi(2) that is equal to 8.6 (1.4% probability). Thus, combining internal inconsistent data sets (SNIa+BAO+HST with Planck+WP+lensing) can lead to ambiguous results, and it is necessary to perform the HDE data analysis for each independent data sets. Our tightest self-consistent constraint is c = 0.495 0.039 obtained from Planck+WP+BAO-FHST-Flensing.
部门归属[Li, Miao; Zhang, Zhenhui] Chinese Acad Sci, Inst Theoret Phys, Beijing 100190, Peoples R China; [Li, Miao; Zhang, Zhenhui] Chinese Acad Sci, Kavli Inst Theoret Phys China, Beijing 100190, Peoples R China; [Li, Miao; Zhang, Zhenhui] Chinese Acad Sci, Key Lab Frontiers Theoret Phys, Beijing 100190, Peoples R China; [Li, Xiao-Dong] Korea Inst Adv Study, Seoul 130722, South Korea; [Ma, Yin-Zhe] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z1, Canada; [Ma, Yin-Zhe] Canadian Inst Theoret Astrophys, Toronto, ON M5S 3H8, Canada; [Zhang, Xin] Northeastern Univ, Coll Sci, Shenyang 110004, Peoples R China; [Zhang, Xin] Peking Univ, Ctr High Energy Phys, Beijing 100080, Peoples R China
关键词South-pole Telescope Microwave Background Anisotropies Hubble-space-telescope Cosmological Constant Black-holes Accelerating Universe Galaxy Clusters Power-spectrum Ia Supernovae Entropy
学科领域Physics
资助者National Natural Science Foundation of China [11275247, 10821504, 10705041, 10975032, 11175042]; Korea Dark Energy Search (KDES) grant; Natural Sciences and Engineering Research Council of Canada; Canadian Institute for Theoretical Astrophysics (CITA); National Ministry of Education of China [NCET-09-0276, N100505001, N120505003] ; National Natural Science Foundation of China [11275247, 10821504, 10705041, 10975032, 11175042]; Korea Dark Energy Search (KDES) grant; Natural Sciences and Engineering Research Council of Canada; Canadian Institute for Theoretical Astrophysics (CITA); National Ministry of Education of China [NCET-09-0276, N100505001, N120505003] ; National Natural Science Foundation of China [11275247, 10821504, 10705041, 10975032, 11175042]; Korea Dark Energy Search (KDES) grant; Natural Sciences and Engineering Research Council of Canada; Canadian Institute for Theoretical Astrophysics (CITA); National Ministry of Education of China [NCET-09-0276, N100505001, N120505003] ; National Natural Science Foundation of China [11275247, 10821504, 10705041, 10975032, 11175042]; Korea Dark Energy Search (KDES) grant; Natural Sciences and Engineering Research Council of Canada; Canadian Institute for Theoretical Astrophysics (CITA); National Ministry of Education of China [NCET-09-0276, N100505001, N120505003]
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收录类别SCI
语种英语
资助者National Natural Science Foundation of China [11275247, 10821504, 10705041, 10975032, 11175042]; Korea Dark Energy Search (KDES) grant; Natural Sciences and Engineering Research Council of Canada; Canadian Institute for Theoretical Astrophysics (CITA); National Ministry of Education of China [NCET-09-0276, N100505001, N120505003] ; National Natural Science Foundation of China [11275247, 10821504, 10705041, 10975032, 11175042]; Korea Dark Energy Search (KDES) grant; Natural Sciences and Engineering Research Council of Canada; Canadian Institute for Theoretical Astrophysics (CITA); National Ministry of Education of China [NCET-09-0276, N100505001, N120505003] ; National Natural Science Foundation of China [11275247, 10821504, 10705041, 10975032, 11175042]; Korea Dark Energy Search (KDES) grant; Natural Sciences and Engineering Research Council of Canada; Canadian Institute for Theoretical Astrophysics (CITA); National Ministry of Education of China [NCET-09-0276, N100505001, N120505003] ; National Natural Science Foundation of China [11275247, 10821504, 10705041, 10975032, 11175042]; Korea Dark Energy Search (KDES) grant; Natural Sciences and Engineering Research Council of Canada; Canadian Institute for Theoretical Astrophysics (CITA); National Ministry of Education of China [NCET-09-0276, N100505001, N120505003]
WOS记录号WOS:000326826000021
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文献类型期刊论文
条目标识符http://ir.itp.ac.cn/handle/311006/15286
专题理论物理所2013年知识产出
通讯作者Li, M (reprint author), Chinese Acad Sci, Inst Theoret Phys, Beijing 100190, Peoples R China.
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GB/T 7714
Li, M,Li, XD,Ma, YZ,et al. Planck constraints on holographic dark energy[J]. JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS,2013(9):21.
APA Li, M,Li, XD,Ma, YZ,Zhang, X,Zhang, ZH,&Li, M .(2013).Planck constraints on holographic dark energy.JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS(9),21.
MLA Li, M,et al."Planck constraints on holographic dark energy".JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS .9(2013):21.
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