Observational constraints on cosmological models with the updated long gamma-ray bursts

Hao Wei*

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

107 Citations (Scopus)

Abstract

In the present work, by the help of the newly released Union2 compilation which consists of 557 Type Ia supernovae (SNIa), we calibrate 109 long Gamma-Ray Bursts (GRBs) with the well-known Amati relation, using the cosmology-independent calibration method proposed by Liang et al.. We have obtained 59 calibrated high-redshift GRBs which can be used to constrain cosmological models without the circularity problem (we call them "Hymnium" GRBs sample for convenience). Then, we consider the joint constraints on 7 cosmological models from the latest observational data, namely, the combination of 557 Union2 SNIa dataset, 59 calibrated Hymnium GRBs dataset (obtained in this work), the shift parameter R from the WMAP 7-year data, and the distance parameter A of the measurement of the baryon acoustic oscillation (BAO) peak in the distribution of SDSS luminous red galaxies. We also briefly consider the comparison of these 7 cosmological models.

Original languageEnglish
Article number020
JournalJournal of Cosmology and Astroparticle Physics
Volume2010
Issue number8
DOIs
Publication statusPublished - Aug 2010

Keywords

  • Dark energy experiments
  • Dark energy theory
  • Gamma ray burst experiments
  • Supernova type ia - Standard candles

Fingerprint

Dive into the research topics of 'Observational constraints on cosmological models with the updated long gamma-ray bursts'. Together they form a unique fingerprint.

Cite this