Affiliation:
1. Department of Astronomy, Beijing Normal University, Beijing 100875, China
2. National Centre for Nuclear Research, Pasteura 7, PL-02-093 Warsaw, Poland
3. National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
Abstract
ABSTRACT
In this paper, we quantify the ability of multiple measurements of high-redshift quasars to constrain several theories of modified gravity, including the Dvali–Gabadadze–Porrati braneworld scenario, generalized Chaplygin gas, f(T) modified gravity, and modified polytropic Cardassian model. Recently released sample of 1598 quasars with X-ray and ultraviolet flux measurements in the redshift range of 0.036 ≤ z ≤ 5.1003, as well as a compilation of 120 intermediate-luminosity radio quasars covering the redshift of 0.46 < z < 2.76 are respectively used as standard probes at higher redshifts. For all considered modified gravity theories, our results show that there is still some possibility that the standard Λ cold dark matter (ΛCDM) scenario might not be the best cosmological model preferred by the current quasar observations. In order to improve cosmological constraints, the quasar data are also combined with the latest observations of baryon acoustic oscillations, which strongly complement the constraints. Finally, we discuss the support given by the data to modified gravity theories, applying different information theoretic techniques like the Akaike information criterion, Bayesian information criterion, and Jensen–Shannon divergence.
Funder
National Natural Science Foundation of China
National Key Research and Development Program of China
Chinese Academy of Sciences
Beijing Normal University
Opening Project of Key Laboratory of Computational Astrophysics
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Cited by
34 articles.
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