Cosmological tests using gamma-ray bursts, the star formation rate and possible abundance evolution

Jun Jie Wei, Xue Feng Wu, Fulvio Melia, Da Ming Wei, Long Long Feng

Research output: Contribution to journalArticle

41 Scopus citations

Abstract

The principal goal of this paper is to use attempts at reconciling the Swift long gamma-ray bursts (LGRBs) with the star formation history (SFH) to compare the predictions of δ cold dark matter (δCDM) with those in the Rh = ct Universe. In the context of the former, we confirm that the latest Swift sample of GRBs reveals an increasing evolution in the GRB rate relative to the star formation rate (SFR) at high redshifts. The observed discrepancy between the GRB rate and the SFR may be eliminated by assuming a modest evolution parametrized as (1 + z)0.8 - perhaps indicating a cosmic evolution in metallicity. However, we find a higher metallicity cut of Z = 0.52 Z than was seen in previous studies, which suggested that LGRBs occur preferentially in metal-poor environments, i.e. Z ̃ 0.1-0.3 Z. We use a simple powerlaw approximation to the high-z (>3.8) SFH, i.e. RSF α [(1 + z)/4.8]α, to examine how the high-z SFR may be impacted by a possible abundance evolution in the Swift GRB sample. For an expansion history consistent with δCDM, we find that the Swift redshift and luminosity distributions can be reproduced with reasonable accuracy if α = -2.41+1.87 -2.09. For the Rh = ct Universe, the GRB rate is slightly different from that in δCDM, but also requires an extra evolutionary effect, with a metallicity cut of Z = 0.44 Z. Assuming that the SFR and GRB rate are related via an evolving metallicity, we find that the GRB data constrain the slope of the high-z SFR in Rh = ct to be α = -3.60+2.45 -2.45. Both cosmologies fit the GRB/SFR data rather well. However, in a one-on-one comparison using the Akaike information criterion, the best-fitting Rh = ct model is statistically preferred over the best-fitting δCDM model with a relative probability of ̃70 per cent versus ̃30 per cent.

Original languageEnglish (US)
Pages (from-to)3329-3341
Number of pages13
JournalMonthly Notices of the Royal Astronomical Society
Volume439
Issue number4
DOIs
StatePublished - Apr 2014

Keywords

  • Cosmology: observations
  • Cosmology: theory
  • Gamma-ray burst: general
  • Methods: statistical
  • Stars: formation

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Fingerprint Dive into the research topics of 'Cosmological tests using gamma-ray bursts, the star formation rate and possible abundance evolution'. Together they form a unique fingerprint.

  • Cite this