An analytic model for non-spherical lenses in covariant MOdified Newtonian Dynamics

Huan Yuan Shan, Martin Feix, Benoit Famaey, Hongsheng Zhao

Research output: Contribution to journalArticlepeer-review

26 Citations (Scopus)

Abstract

Strong gravitational lensing by galaxies in MOdified Newtonian Dynamics (MOND) has until now been restricted to spherically symmetric models. These models were able to account for the size of the Einstein ring of observed lenses, but were unable to account for double-imaged systems with collinear images, as well as four-image lenses. Non-spherical models are generally cumbersome to compute numerically in MOND, but we present here a class of analytic non-spherical models that can be applied to fit double-imaged and quadruple-imaged systems. We use them to obtain a reasonable MOND fit to 10 double-imaged systems, as well as to the quadruple-imaged system Q2237+030 which is an isolated bulge-disc lens producing an Einstein cross. However, we also find five double-imaged systems and three quadruple-imaged systems for which no reasonable MOND fit can be obtained with our models. We argue that this is mostly due to the intrinsic limitation of the analytic models, even though the presence of small amounts of additional dark mass on galaxy scales in MOND is also plausible.

Original languageEnglish
Pages (from-to)1303-1312
Number of pages10
JournalMonthly Notices of the Royal Astronomical Society
Volume387
Issue number3
Early online date23 May 2008
DOIs
Publication statusPublished - 1 Jul 2008

Keywords

  • gravitational lensing
  • cosmology : theory
  • dark matter
  • GRAVITATIONAL LENS
  • DARK-MATTER
  • SPHERICAL GALAXIES
  • EXTERNAL SHEAR
  • MASS
  • CLUSTERS
  • GRAVITY
  • TEVES
  • SPECTROSCOPY
  • Q0957+561

Fingerprint

Dive into the research topics of 'An analytic model for non-spherical lenses in covariant MOdified Newtonian Dynamics'. Together they form a unique fingerprint.

Cite this