Modeling the formation of galaxy clusters in MOND

Details Modeling the formation of galaxy clusters in MOND Modeling the formation of galaxy clusters in MOND

2005-05-05

arxiv.org/abs/astro-ph/0505095v1

Mon.Not.Roy.Astron.Soc. 366 (2006) 969-976

Astronomy and Astrophysics

Astrophysics

8 pages, 7 figures, MNRAS submitted

Scientific paper

10.1111/j.1365-2966.2005.09831.x

We use a one dimensional hydrodynamical code to study the evolution of spherically symmetric perturbations in the framework of Modified Newtonian Dynamics (MOND). The code evolves spherical gaseous shells in an expanding Universe by employing a MOND-type relationship between the fluctuations in the density field and the gravitational force, $g$. We focus on the evolution of initial density perturbations of the form $\delta_{i}\sim r_{i}^{-s}$ for $0

Affiliated with

Also associated with

No associations

Rating

Modeling the formation of galaxy clusters in MOND does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Modeling the formation of galaxy clusters in MOND, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Modeling the formation of galaxy clusters in MOND will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-114497