Model-independent distance calibration of high-redshift gamma-ray bursts and constrain on the Lambda CDM model
Lin, HN; Li, X2; Chang, Z1
刊名MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2016
卷号455期号:2页码:2131-2138
关键词gamma-ray burst: general GREATER-THAN 1 cosmological parameters HUBBLE DIAGRAM COSMOLOGICAL IMPLICATIONS STANDARD CANDLES PEAK LUMINOSITY DARK-ENERGY SUPERNOVAE SPECTRA ENERGETICS UNIVERSE
DOIhttp://dx.doi.org/10.1093/mnras/stv2471
英文摘要Gamma-ray bursts (GRBs) are luminous enough to be detectable up to redshift z similar to 10. They are often proposed as complementary tools to Type Ia supernovae (SNe Ia) in tracing the Hubble diagram of the Universe. The distance calibrations of GRBs usually make use of one or some of the empirical luminosity correlations, such as iota(lag)-L, V-L, E-p-L, E-p-E-gamma, tau(RT)-L and E-p-E-iso relations. These calibrating methods are based on the underlying assumption that the empirical luminosity correlations are universal over all redshift range. In this paper, we test the possible redshift dependence of six luminosity correlations by dividing GRBs into low-z and high-z classes according to their redshift smaller or larger than 1.4. It is shown that the E-p-E-gamma relation for low-z GRBs is consistent with that for high-z GRBs within 1 sigma uncertainty. The intrinsic scatter of V-L relation is too large to make a convincing conclusion. For the rest four correlations, however, low-z GRBs differ from high-z GRBs at more than 3 sigma confidence level. As such, we calibrate GRBs using the E-p-E-gamma relation in a model-independent way. The constraint of high-z GRBs on the Lambda cold dark matter (Lambda CDM) model gives Omega(M) = 0.302 +/- 0.142(1 sigma), well consistent with the Planck 2015 results.
学科主题Astronomy & Astrophysics
语种英语
资助机构National Natural Science Fund of China [11375203, 11305181] ; State Key Laboratory of Theoretical Physics, Institute of Theoretical Physics, Chinese Academy of Sciences, China [Y5KF181CJ1]
内容类型期刊论文
源URL[http://ir.itp.ac.cn/handle/311006/23219]  
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, State Key Lab Theoret Phys, Beijing 100190, Peoples R China
2.Chongqing Univ, Dept Phys, Chongqing 401331, Peoples R China
3.Chinese Acad Sci, Inst High Energy Phys, Beijing 100049, Peoples R China
推荐引用方式
GB/T 7714
Lin, HN,Li, X,Chang, Z. Model-independent distance calibration of high-redshift gamma-ray bursts and constrain on the Lambda CDM model[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2016,455(2):2131-2138.
APA Lin, HN,Li, X,&Chang, Z.(2016).Model-independent distance calibration of high-redshift gamma-ray bursts and constrain on the Lambda CDM model.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,455(2),2131-2138.
MLA Lin, HN,et al."Model-independent distance calibration of high-redshift gamma-ray bursts and constrain on the Lambda CDM model".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 455.2(2016):2131-2138.
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