Searching for the evidence of dynamical dark energy

Deng Wang (Department of Astronomy, School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai, 200240, China; Theoretical Physics Division, Chern Institute of Mathematics, Nankai University, Tianjin, 300071, China) ; Wei Zhang (Department of Physics, Nankai University, Tianjin, 300071, China) ; Xin-He Meng (Department of Physics, Nankai University, Tianjin, 300071, China)

In the statistical framework of model-independent Gaussian processes (GP), we search for the evidence of dynamical dark energy (DDE) using the “Joint Light-curve Analysis” (JLA) Type Ia supernovae (SNe Ia) sample, the 30 latest cosmic chronometer data points (H(z)), Planck’s shift parameter from cosmic microwave background (CMB) anisotropies, the 156 latest HII galaxy measurements and 79 calibrated gamma-ray bursts (GRBs). We find that the joint constraint from JLA + H(z) + CMB + HII + GRB supports the global measurement of $$H_0$$ H0 by Planck collaboration very much in the low redshift range $$z\in [0, 0.76]$$ z[0,0.76] at the $$2\sigma $$ 2σ confidence level (C.L.), gives a cosmological constant crossing (quintom-like) equation of state (EoS) of DE at the $$2\sigma $$ 2σ C.L. and implies that the evolution of the late-time Universe may be actually dominated by the DDE.

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      "value": "In the statistical framework of model-independent Gaussian processes (GP), we search for the evidence of dynamical dark energy (DDE) using the \u201cJoint Light-curve Analysis\u201d (JLA) Type Ia supernovae (SNe Ia) sample, the 30 latest cosmic chronometer data points (H(z)), Planck\u2019s shift parameter from cosmic microwave background (CMB) anisotropies, the 156 latest HII galaxy measurements and 79 calibrated gamma-ray bursts (GRBs). We find that the joint constraint from JLA + H(z) + CMB + HII + GRB supports the global measurement of $$H_0$$ <math><msub><mi>H</mi><mn>0</mn></msub></math>  by Planck collaboration very much in the low redshift range $$z\\in [0, 0.76]$$ <math><mrow><mi>z</mi><mo>\u2208</mo><mo>[</mo><mn>0</mn><mo>,</mo><mn>0.76</mn><mo>]</mo></mrow></math>  at the $$2\\sigma $$ <math><mrow><mn>2</mn><mi>\u03c3</mi></mrow></math>  confidence level (C.L.), gives a cosmological constant crossing (quintom-like) equation of state (EoS) of DE at the $$2\\sigma $$ <math><mrow><mn>2</mn><mi>\u03c3</mi></mrow></math>  C.L. and implies that the evolution of the late-time Universe may be actually dominated by the DDE."
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Published on:
08 March 2019
Publisher:
Springer
Published in:
European Physical Journal C , Volume 79 (2019)
Issue 3
Pages 1-10
DOI:
https://doi.org/10.1140/epjc/s10052-019-6726-3
Copyrights:
The Author(s)
Licence:
CC-BY-4.0

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