Probing the anisotropic expansion from supernovae and GRBs in a model-independent way
arXiv:1406.6448 · doi:10.1093/mnras/stu1279
Abstract
In this paper, we study the anisotropic expansion of the universe using type Ia supernovae Union 2.1 sample and 116 long gamma-ray bursts. The luminosity distance is expanded with model-independent cosmographic parameters as a function of directly. Thus the results are independent of cosmology model. We find a dipolar anisotropy in the direction (, ) in galactic coordinates with a significant evidence (more than ). The magnitude is for the dipole, and for the monopole, respectively. This dipolar anisotropy is more significant at low redshift from the redshift tomography analysis. We also test whether this preferred direction is caused by bulk flow motion or dark energy dipolar scalar perturbation. We find that the direction and the amplitude of the bulk flow in our results are approximately consistent with the bulk flow surveys. Therefore, bulk flow motion may be the main reason for the anisotropic expansion at low redshift, but the effect of dipolar distribution dark energy can not be excluded, especially at high redshift.
17 pages, 5 figures, 5 tables, accepted for publication in MNRAS
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- The deceleration parameter in `tilted' universes: generalising the Friedmann background
- Testing cosmic anisotropy with Pade approximation and Pantheon+ sample
- Cosmography of the Local Universe by Multipole Analysis of the Expansion Rate Fluctuation Field
- Consistency of Pantheon+ supernovae with a large-scale isotropic universe
- Anisotropic universe with anisotropic dark energy
- Probing the Cosmological Principle with weak lensing shear
- The Two-Point Correlation Function of Gamma-ray Bursts
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- New Constraints on Anisotropic Expansion from Supernovae Type Ia
- Measuring cosmic dipole with the GRB luminosity-time relation