Gravitational theoretical development supporting MOND

Дата и время публикации : 2013-07-15T13:46:34Z

Авторы публикации и институты :
Edmund A. Chadwick
Timothy F. Hodgkinson
Graham S. McDonald

Ссылка на журнал-издание: Ссылка на журнал-издание не найдена
Коментарии к cтатье: 10 pages to appear in Physical Review D, vol. 88, July 2013. Copyright APS.
Первичная категория: gr-qc

Все категории : gr-qc, astro-ph.GA, 83D99

Краткий обзор статьи: Conformal geometry is considered within a general relativistic framework. An invariant distant for proper time is defined and a parallel displacement is applied in the distorted space-time, modifying Einstein’s equation appropriately. A particular solution is introduced for the covariant acceleration potential that matches the observed velocity distribution at large distances from the galactic centre, i.e. Modified Newtonian Dynamics (MOND). This explicit solution, of a general framework that allows both curvature and explicit local expansion of space-time, thus reproduces the observed flattening of galaxys’ rotation curves without the need to assume the existence of dark matter. The large distance expansion rate is found to match the speed of a spherical shock wave.

Category: Physics