2012/09/30 by Xin Li, Ming-Hua Li, Hai-Nan Lin +1
Physics and Astronomy · #Advanced Differential Geometry Research #Astrophysics #Astrophysics and Cosmic Phenomena #Circular symmetry #Classical mechanics #Cosmology and Gravitation Theories #Gravitation #Gravitational field #Mathematical physics #Physics #Quadrupole #Quantum mechanics #Schwarzschild radius #astro-ph.CO #astro-ph.GA #gr-qc
paper · pdf · doi:10.1093/mnras/sts237
published as Mon. Not. Roy. Astron. Soc. 430, 450 (2013) · 15 pages, 8 figures
openalex publication_date 2012/11/14 · arxiv created 2013/03/03 · arxiv updated 2013/03/05 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
It is known that theory of MOND with spherical symmetry cannot account for the convergence κ-map of Bullet Cluster 1E0657-558. In this paper, we try to set up a Finslerian MOND, a generalization of MOND in Finsler spacetime. We use Ric=0 to obtain the gravitational vacuum field equation in a four-dimensional Finsler spacetime. To leading order in the post-Newtonian approximation, we obtain the explicit form of the Finslerian line element. It is simply the Schwarzschild's metric except for the Finslerian rescaling coefficient f(v) of the radial coordinate r, i.e. R=f(v(r))r. By setting f(v(r))=(1-√(a0r2/GM))-1, we obtain the famous MOND in a Finslerian framework. Taking a dipole and a quadrupole term into consideration, we give the convergence κ in gravitational lensing astrophysics in our model. Numerical analysis shows that our prediction is to a certain extent in agreement with the observations of Bullet Cluster 1E0657-558. With the theoretical temperature T taking the observed value 14.8 keV, the mass density profile of the main cluster obtained in our model is the same order as that given by the best-fit King β-model.