Large Distance Modification of Newtonian Potential and Structure Formation in Universe
arXiv:1712.08591 · doi:10.1016/j.dark.2018.02.001
Abstract
In this paper, we study the effects of super-light brane world perturbative modes on structure formation in our universe. As these modes modify the large distance behavior of Newtonian potential, they effect the clustering of a system of galaxies. So, we explicitly calculate the clustering of galaxies interacting through such a modified Newtonian potential. We use a suitable approximation for analyzing this system of galaxies, and discuss the validity of such approximations. We observe that such corrections also modify the virial theorem for such a system of galaxies.
13 pages, 3 captioned figures
References in corpus (19)
- Modified f(R) gravity unifying R^m inflation with \LambdaCDM epoch
- Observational constraints on self-accelerating cosmology
- The Bullet Cluster 1E0657-558 evidence shows Modified Gravity in the absence of Dark Matter
- Rotational Velocity Curves in the Milky Way as a Test of Modified Gravity
- The virial theorem and the dynamics of clusters of galaxies in the brane world models
- An Alternative to Particle Dark Matter
- Higher order corrections to the Newtonian potential in the Randall-Sundrum model
- Clustering of Galaxies with f(R) gravity
- Brane world corrections to Newton's law
- Generalizing MOND to explain the missing mass in galaxy clusters
- Effects of Cosmological Constant on Clustering of Galaxies
- The best fit for the observed galaxy Counts-in-Cell distribution function
- Clustering of Galaxies with Dynamical Dark Energy
- On the stability of a galactic disk in modified gravity
- On the universality of MOG weak field approximation at galaxy cluster scale
- Thermodynamics and galactic clustering with a modified gravitational potential
- No need for dark matter in galaxy clusters within Galileon theory
- Galaxy Cluster A1689 in Modified MOND, MOG and Emergent Gravity
- Shapes and Probabilities of Galaxy Clusters II: Comparisons with observations
Cited by in corpus (10)
- Finite Tsallis Gravitational Partition Function for a System of Galaxies
- Two approaches that prove divergence free nature of non-local gravity
- Galactic Clustering Under Power-law Modified Newtonian Potential
- Logarithmic corrections to Newtonian gravity and Large Scale Structure
- The large scale structure formation in an expanding universe
- Gravitational partition function modified by super-light brane world perturbative modes
- Effect of nonfactorizable background geometry on thermodynamics of clustering of galaxies
- Time dependent dark energy and the thermodynamics of many-body systems
- Study of the large scale structure through modified gravity theory using statistical mechanics
- Statistical description of galaxy clusters in Finzi model of gravity