Assessing cosmic acceleration with the Alcock-Paczyński effect in the SDSS-IV quasar catalog

Fulvio Melia, Jin Qin, Tong Jie Zhang

Research output: Contribution to journalArticlepeer-review

Abstract

The geometry of the Universe may be probed using the Alcock-Paczynski ´ (AP) effect, in which the observed redshift size of a spherical distribution of sources relative to its angular size varies according to the assumed cosmological model. Past applications of this effect have been limited, however, by a paucity of suitable sources and mitigating astrophysical factors, such as internal redshift-space distortions and poorly known source evolution. In this Letter, we introduce a new test based on the AP effect that avoids the use of spatially bound systems, relying instead on sub-samples of quasars at redshifts z . 1.5 in the Sloan Digital Sky Survey IV, with a possible extension to higher redshifts and improved precision when this catalog is expanded by upcoming surveys. We here use this method to probe the redshift-dependent expansion rate in three pertinent Friedmann-Lemaître-Robertson-Walker (FLRW) cosmologies: ΛCDM, which predicts a transition from deceleration to acceleration at z ∼ 0.7; Einstein-de Sitter, in which the Universe is always decelerating; and the Rh = ct universe, which expands at a constant rate. ΛCDM is consistent with these data, but Rh = ct is favoured overall.

Original languageEnglish (US)
JournalUnknown Journal
StatePublished - Aug 28 2020

Keywords

  • Cosmological parameters
  • Cosmology: observations
  • Cosmology: theory
  • Distance scale
  • Galaxies: active
  • Quasars: supermassive black holes

ASJC Scopus subject areas

  • General

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